1. Introduction
1.1 Background/motivation
Enumerating curves on compact Calabi–Yau 4-folds has been drawing increasing interest in recent years. A key feature distinguishing Calabi–Yau manifolds of dimension 4 and above is that Gromov–Witten invariants vanish for genus greater than one.Footnote 1 Inspired by this observation and drawing from heuristic arguments in ideal geometries, researchers have proposed Gromov–Witten/Donaldson–Thomas correspondence for compact Calabi–Yau 4-folds [Reference Klemm and PandharipandeKP08, Reference Cao, Maulik and TodaCMT18, Reference Cao, Maulik and TodaCMT22, Reference Cao and TodaCT21, Reference Cao and KoolCK20].
However, the picture becomes considerably more complex for non-compact (e.g., local) Calabi–Yau 4-folds. Their invariants, defined via torus localization, can encompass all genera and are rational functions of equivariant parameters, making the aforementioned correspondences highly elusive in this setting. In an attempt to gain a better understanding of (non-compact) Calabi–Yau 4-folds, we draw inspiration from the realm of enumerative geometry for 3-folds. On 3-folds, the degeneration formula for the Donaldson–Thomas and Pandharipande–Thomas theories stands as a formidable tool [Reference Li and WuLW15] (see also [Reference ZhouZho18] for the case of orbifolds). Its elegance has been instrumental in numerous groundbreaking computations; see, for example, [Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06b, Reference Maulik, Oblomkov, Okounkov and PandharipandeMOO+11, Reference Okounkov and PandharipandeOP10b, Reference OkounkovOko17, Reference Pandharipande and PixtonPP13, Reference Pandharipande and PixtonPP14, Reference Pandharipande and PixtonPP17].
Parallel to the relationship between the Donaldson–Thomas (DT) theory of 3-folds and the quantum cohomology of Nakajima quiver varieties [Reference Okounkov and PandharipandeOP10a, Reference Okounkov and PandharipandeOP10b], curve counting theory on non-compact Calabi–Yau 4-folds is connected to the quantum critical cohomology of quivers with potentials and also the theory of gauged linear sigma models [Reference Cao and ZhaoCZ26]. The latter provides representation theoretical and physical motivations and contexts for studying the degeneration formula, where integrable systems related to cohomological Hall algebras [Reference Kontsevich and SoibelmanKS11] and quantum groups [Reference Li and YamazakiLY20, Reference Rapcak, Soibelman, Yang and ZhaoRSY+20, Reference Varagnolo and VasserotVV23] emerge.
The present paper extends the degeneration formula framework to the Donaldson–Thomas theory of Calabi–Yau 4-folds. We remark that such an extension is a difficult, albeit potentially fruitful, venture. The difficulty comes from two sources. (1) Because of the nature of the moduli spaces involved in the 4-fold case, the use of derived algebraic geometry, and shifted symplectic geometry, is crucial. A detailed explanation is given in Remark 1.4. (2) The invariants of 4-folds depend on the choice of orientation [Reference Cao, Gross and JoyceCGJ20, Reference Cao, Gross and JoyceCGJ25], and behave in a more complicated way than those of 3-folds.
Below, we give a summary of the results obtained in this paper.
1.2 Expanded degenerations and family invariants
Let
$\pi : X \to {\mathbb A}^1$
be a Calabi–Yau simple degeneration of relative dimension n (Definitions 2.6 and 2.10). There is an associated stack
${\mathcal C}$
of expanded degeneration (Definition 2.9) and a universal family
which is a Calabi–Yau family (Proposition 2.11). Let
$\operatorname{{Hilb}}^{}(X/{\mathbb A}^1)$
be the Hilbert stack of stable subschemes on the family
${\mathcal X} \to {\mathcal C}$
(Definition 2.18). Fixing compactly supported numerical K-theory classes
$P_t \in K_{c, \leqslant n - 2}^\mathrm{num} (X_t)$
for all
$t\in {\mathbb A}^1$
, we have an open substack (Lemma 2.21)
of stable subschemes on the decorated expanded degeneration
${\mathcal X}^{P_t} \to {\mathcal C}^{P_t}$
with class
$P_t$
for
$t\in {\mathbb A}^1$
(see § 2.4 for the details). A version of the Alexandrov–Kontsevich–Schwarz–Zaboronsky-type argument, similar to [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Reference PreygelPre], yields the following.
Theorem 1.1 (Theorem 3.2).
$\operatorname{{Hilb}}^{P_t }(X/{\mathbb A}^1)$
has a derived enhancement
$\mathbf{Hilb}^{P_t }(X/{\mathbb A}^1)$
with a canonical
$(2-n)$
-shifted symplectic structure over
${\mathcal C}^{P_t}$
.
In the present paper, we focus on the case when
$n=4$
, where
$\textbf{Hilb}^{P_t }(X/{\mathbb A}^1)\to {\mathcal C}^{P_t}$
has a
$(-2)$
-shifted symplectic structure. Subject to the isotropic condition (verified in Proposition 5.11), there is a well-defined square root virtual pullback [Reference ParkPar21].
Theorem 1.2 (Family invariants, Proposition 5.11, Theorem 5.13). Fix K-theory classes
$P_t \in K_{c, \leqslant 2}^\mathrm{{num}} (X_t)$
for all
$t\in \mathbb{A}^1$
.
-
(1) The map
(1.1)has a canonical symmetric obstruction theory in sense of Definition 5.2, which is isotropic if
\begin{equation}\pi: \operatorname{{Hilb}}^{P_t}(X/{\mathbb A}^1)\to {\mathcal C}^{P_t} \end{equation}
$P_t\in K_{c, \leqslant 1}^{\mathrm{num}} (X_t)$
for all
$t\in \mathbb{A}^1$
, i.e. their support has dimension not bigger than one.
-
(2) In the presence of an orientation on
$\pi$
in the sense of Definition 4.1, there is a square root virtual pullback (1.2)where
\begin{equation} \sqrt{\pi^!} : A_*({\mathcal C}^{P_t})\to A_*(\operatorname{{Hilb}}^{P_t}(X/{\mathbb A}^1)), \end{equation}
$A_*(-)$
denotes the Chow group with rational coefficients.
-
(3) In the further presence of a torus T action on the family
$X\to {\mathbb A}^1$
, preserving Calabi–Yau volume forms on fibers, the above pullback map lifts to a map between T-equivariant Chow groups.
The above pullback map captures the virtual counting for the family
$\pi$
whose base change to a general element in
${\mathcal C}^{P_t}$
recovers the virtual counting of the general fiber of
$X/\mathbb{A}^1$
. The base change to the special fiber can be linked with relative invariants, which we introduce now.
1.3 Expanded pairs and relative invariants
Let (Y,D) be a smooth log Calabi–Yau pair (Definition 2.4) with
$\dim_{\mathbb{C}}Y=n$
, and
be the associated universal expanded pairs over the stack
${\mathcal A}$
of expanded pairs (Definition 2.3), which is a log Calabi–Yau pair (relative to
${\mathcal A}$
) (Proposition 2.5).
There exists a Hilbert stack
$\operatorname{{Hilb}} (Y, D)$
parameterizing families of stable subschemes in the universal family
${\mathcal Y} / {\mathcal A}$
(Definition 2.18) and a restriction map
Fix
$P\in K_{c, \leqslant n-2}^{\mathrm{num}} (Y)$
with
$P|_D\in K_c^{\mathrm{num}} (D)$
as the K-theoretic Gysin pullback (2.8) to D. We have open substacks
and a similar restriction map
As in Theorem 1.1, the target of (1.3) has a derived enhancement with a canonical
$(3-n)$
-shifted symplectic structure relative to
${\mathcal A}^P$
. By a family argument as in [Reference CalaqueCal15], we obtain the following.
Theorem 1.3 (Theorem 3.3). The restriction map
$r_{{\mathcal D}\to {\mathcal Y}}$
has a derived enhancement
which has a
$(3-n)$
-shifted Lagrangian structure relative to
${\mathcal A}^P$
.
We restrict ourselves to the case when
$n=4$
and hence D is a Calabi–Yau 3-fold.
Remark 1.4. The question of extracting ‘correct’ relative invariants from the
$({-}1)$
-shifted Lagrangian structure on (1.4) is illusive. Indeed, there is a conjecture by Joyce [Reference JoyceJoy18] asserting the existence of a map
with the prescribed properties. Here
$\varphi_{\operatorname{{Hilb}}^{P|_D} (D)\times {\mathcal A}^P}$
is a certain perverse sheaf coming from gluing local sheaves of vanishing cycles. However, there are layers of difficulties in proving this conjecture, partially involving gluing in infinity categories (see also [Reference Khan and KinjoKK23], which addresses other difficulties).
Note that by the Darboux theorem [Reference Bouaziz and GrojnowskiBG13, Reference Brav, Bussi and JoyceBBJ19], derived critical loci of regular functions on smooth schemes provide local charts of the
$({-}1)$
-shifted symplectic derived scheme
$\textbf{Hilb}^{P|_D} (D)$
. In this paper, we focus on such local charts and make the following assumption.
Assumption 1.5. Fix
$P_D\in K_c^\mathrm{{num}}(D)$
. We assume there is an equivalence
of the
$({-}1)$
-shifted symplectic derived scheme, where W is a quasi-projective smooth scheme and
$\phi$
is a regular function.
Let
$P\in K_{c,\leqslant 2}^{\mathrm{num}} (Y)$
and
$P_D:=P|_D\in K_c^{\mathrm{num}} (D)$
. Denote the inclusion to the ambient space by
By an abuse of notation, we also denote its product with
$\operatorname{id}_{{\mathcal A}^P}$
by p. The way this paper takes to define relative invariants is then motivated by the study on quasimaps to quivers with potentials [Reference Cao and ZhaoCZ26], where we observe that the composition map
has a (relative)
$\textit{(-2)}$
-shifted symplectic structure (Proposition 3.8).
As in Theorem 1.2, we check the isotropic condition (Proposition 5.6), and obtain a virtual pullback map (by abuse of notation, p and
$r_{{\mathcal D}\to {\mathcal Y}}$
also denote their classical truncations).
Theorem 1.6 (Relative invariants, Proposition 5.6, Theorem 5.7). Let
$P\in K_{c, \leqslant 2}^{\mathrm{num}} (Y)$
.
-
(1) Under Assumption 1.5, the map
(1.8)has a canonical symmetric obstruction theory in sense of Definition 5.2. If
\begin{equation}p\circ r_{{\mathcal D}\to {\mathcal Y}}: \operatorname{{Hilb}}^P(Y,D) \to W\times {\mathcal A}^P \end{equation}
$P\in K_{c,\leqslant 1}^{\mathrm{num}} (Y)$
, the obstruction theory is isotropic after base change to the zero locus
$Z(\phi)\hookrightarrow W$
of
$\phi: W\to \mathbb{C}$
.
-
(2) In the presence of an orientation on (1.8) in the sense of Definition 4.1, there is a square root virtual pullback
(1.9)
\begin{equation}\sqrt{(p\circ r_{{\mathcal D}\to {\mathcal Y}})^!} : A_*(Z(\phi)\times {\mathcal A}^P)\to A_*(\operatorname{{Hilb}}^P(Y,D)). \end{equation}
-
(3) In the further presence of a torus T action on the pair (Y,D) and the equivalence (1.6), the above pullback lifts to a map between T-equivariant Chow groups.
Remark 1.7. It is expected that our relative invariant (1.9) encodes the effect of (1.5) on algebraic cycles, i.e. we should have the commutative diagram (see also [Reference Cao and ZhaoCZ26, Diagram (1.6)])

where the left vertical map is given by the composition of the cycle map with the canonical map from the Borel–Moore homology of
$Z(\phi)$
to the vanishing cycle cohomology (refer to [Reference Cao and ZhaoCZ26, Equation (A.8)]).
There is a version of Theorem 1.6 where Chow groups are replaced by Grothendieck groups
$K_0(-)$
of coherent sheaves, with similar proof. Moreover, we expect an analogue of diagram (1.10), where the cohomology of the vanishing cycle is replaced by the Grothendieck group of the matrix factorization category
$MF(W,\phi)$
. In this setting, the canonical map
is surjective (e.g. [Reference Pavic and ShinderPS21, Lemma 1.10], [Reference SchlichtingSch11]). Therefore, the K-theoretic version of (1.9) contains all information about the K-theoretic version of the provisional map (1.5). The K-theoretic analogue of diagram (1.10) has recently been addressed in [Reference Cao, Toda and ZhaoCTZ25].
1.4 Local (log) Calabi–Yau 4-folds
In general, we do not know whether the maps (1.1) and (1.7) are orientable. It is an even more difficult question to find a canonical orientation suitable for calculations (see Remark 4.2 for details). Local (log) Calabi–Yau 4-folds provide a large class of examples where we can obtain canonical orientation for the maps mentioned above.
Let
$U\to {\mathbb A}^1$
be a simple degeneration of 3-folds (Definition 2.6) whose fiber over
$0\in {\mathbb A}^1$
is a union
$U_+\cup_S U_-$
of two smooth 3-folds
$U_\pm$
along a common smooth divisor S. Let
be the associated Calabi–Yau simple degeneration, where the generic fibers are total spaces of canonical bundles of smooth 3-folds and the central fiber is a union of log Calabi–Yau 4-folds (Definition 2.4), i.e. the fiber
$X_c$
over
$c\in {\mathbb A}^1$
satisfies
-
–
$X_c=\operatorname{Tot}(\omega_{U_c})$
if
$c\neq 0$
, -
–
$X_0=Y_+\cup_D Y_-$
, where
$Y_{\pm}=\operatorname{Tot}(\omega_{U_\pm}(S))$
and
$D=\operatorname{Tot}(\omega_S)$
.
Theorem 1.8 (Theorem 4.3, Remark 4.4). For (1.11), the map
$\pi: \operatorname{{Hilb}}^{P_t }(X/{\mathbb A}^1)\to {\mathcal C}^{P_t}$
(1.1) has a canonical orientation.
Let (U,S) be a smooth pair with
$\dim_{\mathbb{C}} U=3$
. Consider the log Calabi–Yau pair (Definition 2.4):
In this case, there is a line bundle
$K^{-1/2}_{\operatorname{{Hilb}}(D)}$
(4.25) constructed using the fact that a derived moduli stack of compactly supported sheaves on
$D=\operatorname{Tot}(\omega_S)$
is the
$({-}1)$
-shifted cotangent bundle of a derived moduli stack of sheaves on S.
Assumption 1.9. Let
$\mathbf{Hilb}^{P_D} (D)\cong \textbf{Crit}(\phi:W\to \mathbb{C})$
be as in Assumption 1.5. Assume
Equation (1.13) is a compatibility condition between the square root provided using S and the one provided using the ambient space W of the Hilbert scheme. There are many cases where (1.13) is satisfied (Example 4.11). Examples where Assumption 1.9 is satisfied are discussed in § 1.6.
1.5 Degeneration formulae
Given
$X/{\mathbb A}^1$
as in (1.11) and (Y,D) as in (1.12), by combining Theorems 1.2 and 1.8, and Theorems 1.6 and 1.10, we define the following invariants using the canonical orientations of § 1.4.
-
– Fix
$P_t \in K_{c,\leqslant 1}^\mathrm{{num}} (X/\mathbb{A}^1)$
for all
$t\in {\mathbb A}^1$
. The family invariant (Definition 5.14) is given by the pullback map (1.2) :
\begin{equation*}\Phi^{P_t}_{X/{\mathbb A}^1}:=\sqrt{\pi^!}: A_*({\mathcal C}^{P_t}) \to A_*(\operatorname{{Hilb}}^{P_t}(X/{\mathbb A}^1)). \end{equation*}
-
– Fix
$P \in K_{c,\leqslant 1}^\mathrm{{num}} (Y)$
. The relative invariant (Definition 5.9) is a map where
\begin{equation*} \Phi^{P}_{Y,D}:=\sqrt{(p\circ r_{{\mathcal D}\to {\mathcal Y}})^!}\circ \boxtimes : A_*(Z(\phi))\otimes A_{*}({\mathcal A}^{P}) \to A_*(\operatorname{{Hilb}}^P(Y,D)), \end{equation*}
$\sqrt{(p\circ r_{{\mathcal D}\to {\mathcal Y}})^!}$
is given by (1.9) and
$\boxtimes$
is the exterior product for Chow cycles,
-
– Fix
$P_{\pm} \in K_{c,\leqslant 1}^\mathrm{{num}} (Y_\pm)$
. The product version (5.35) of the above relative invariant is
\begin{equation*}\Phi^{P_-}_{Y_-,D}\otimes\Phi^{P_+}_{Y_+,D}:A_*(Z(\phi\boxplus \phi))\otimes A_{*}({\mathcal A}^{P_-}\times {\mathcal A}^{P_+}) \to A_*(\operatorname{{Hilb}}^{P_-}(Y_-,D)\times \operatorname{{Hilb}}^{P_+}(Y_+,D) ). \end{equation*}
Theorem 1.11. (Degeneration formula, Theorem 5.22). For invariants defined above using the canonical orientations of § 1.4, we have
\begin{align*}i_r^!(\Phi^{P_t}_{X/{\mathbb A}^1}[{\mathcal C}^{P_t}])&=[\operatorname{{Hilb}}^{P_r} (X_r)]^{\mathrm{vir}}, \quad\forall\,\,r\in \mathbb{A}^1\backslash \{0\},\\i_{0}^!(\Phi^{P_t}_{X/{\mathbb A}^1}[{\mathcal C}^{P_t}])&= n_*\,\sum_{(P_-, P_+)\in \Lambda^{P_0}_{\rm spl}}i_{(P_-, P_+)}^!(\Phi^{P_t}_{X/{\mathbb A}^1}[{\mathcal C}^{P_t}]). \end{align*}
Moreover, for each splitting data
$(P_-, P_+)\in \Lambda^{P_0}_{\rm spl}$
(2.10), we have
In the presence of a torus action, the above equalities hold in equivariant Chow groups.
Here
$i_{(-)}^!$
is the Gysin pullback of
$i_{(-)}$
in (5.34),
$i_{\bar{\Delta}}$
is given in (5.19),
$\bar{\sigma}$
is the involution (5.20),
$\bar{\Delta}$
is the anti-diagonal embedding (5.18), and n is the normalization map in (5.21).
Remark 1.12. Our degeneration formula is stated on the total space
$X=K_U$
of the canonical bundle of a 3-fold U. It can by no means be reduced to the degeneration formula of the 3-fold U [Reference Li and WuLW15] for the following two reasons. (1) For general curve classes, the stable subschemes (or stable pairs) on X do not necessarily scheme theoretically lie on the 3-fold U, so in general there is not even a map between Hilbert stacks on X and U. (2) Even for an irreducible curve class
$\beta$
, where a moduli
$P(K_U,\beta)$
of Pandharipande–Thomas (PT) stable pairs on the total space
$K_U$
can be identified with a moduli
$P(U,\beta)$
of PT stable pairs on U, our degeneration formula does not follow from the 3-fold one. This is because under the above identification, the 4-fold virtual class reduces to a virtual class on
$P(U,\beta)$
, defined by pair-deformation obstruction theory
$\operatorname{{Ext}}^*(I,F)$
(e.g. [Reference Cao, Maulik and TodaCMT22, Proposition 4.3]), different from the sheaf obstruction theory
$\operatorname{{Ext}}^*(I,I)_0$
used in [Reference Li and WuLW15].
1.6 Applications
Next we mention examples where Assumption 1.9 is satisfied, and discuss applications. The first one is given by relative Hilbert schemes of one-dimensional subschemes on local
$\mathbb{P}^1$
(which are total spaces of rank three bundles on
$\mathbb{P}^1$
) with their restriction maps to Hilbert schemes of points on
$\mathbb{C}^3$
(Examples 3.10, 4.11). We expect this to be helpfulFootnote
2
for understanding the structure of Donaldson–Thomas/Pandharipande–Thomas type curve counting invariants on such non-compact Calabi–Yau 4-folds.
The other example which satisfies Assumption 1.9 is the main focus of this paper, and is given by relative Hilbert schemes of points on the pair (1.12) with their restriction maps to a point. By using a variant of the theory of expanded pairs, called rubber theory [Reference Okounkov and PandharipandeOP10b], we are able to prove the conjectural tautological Donaldson–Thomas formula on
$\mathbb{C}^4$
[Reference Cao and KoolCK18, Conjecture 1.6] by following the magical pole analysis as in the 3-fold case [Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06b].
Theorem 1.13 (Theorem 6.8). Let
$T\subset (\mathbb{C}^*)^4$
be the Calabi–Yau subtorus (6.1) and
$L\in \mathop{\rm Pic}\nolimits^{(\mathbb{C}^*)^4}(\mathbb{C}^4)$
be an equivariant line bundle on
$\mathbb{C}^4$
. With the canonical choice of orientation (in Definition 6.1), we have
\begin{equation}1+\sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^n ({\mathbb C}^4)]_T^\mathrm{vir}}e_T(L^{[n]})=M(q)^{\int_{\mathbb{C}^4} c^T_1(L)\cdot c^T_3(\mathbb{C}^4) }, \end{equation}
where
is the MacMahon function and
$\int_{\mathbb{C}^4}$
denotes equivariant pushforward to a point.
As a special case of the above result, we prove a conjecture of Nekrasov.
Corollary 1.14 (Corollary 6.9). We have
\begin{align*}\displaystyle 1+\sum_{n=1}^\infty q^n\int_{[\operatorname{{Hilb}}^n ({\mathbb C}^4)]_T^\mathrm{vir}} 1 = \exp \bigg[{-}\frac{(s_1 + s_2 )(s_1 + s_3) (s_2 + s_3) }{s_1 s_2 s_3 (s_1 + s_2 + s_3) } q \bigg], \end{align*}
where
$s_1,s_2,s_3$
are equivariant parameters of T.
We recall the basics of rubber theory in Appendix A, and prove the above theorem in § 6. We remark that, compared with the 3-fold case,
$\mathop{\rm DT}\nolimits_4$
invariants are much more difficult to compute because of the difficulty in the choice of orientation. The canonical orientations of § 1.4, used in Theorem 1.11, are compatible with the degeneration formula. We also prove the compatibility of this canonical orientation with the orientation used in the work of Kool and Rennemo [Reference Kool and RennemoKR25]; see Proposition B.2. Based on these observations, the proof of Theorem 1.13 follows from Theorem 1.11, the pole analysis, and Kool and Rennemo’s explicit sign formula for those zero-dimensional subschemes in
$\mathbb{C}^4$
, which are scheme theoretically supported on a
$\mathbb{C}^3$
. See the proof of Theorem 6.8 for more details.
By using the degeneration formula, we are also able to compute zero-dimensional
$\mathop{\rm DT}\nolimits_4$
-invariants for some non-toric Calabi–Yau 4-folds. Consider the following smooth quasi-projective 4-fold
where C is a smooth connected projective curve of genus g, and
$L_1$
,
$L_2$
,
$L_3$
are line bundles on C. Let
$p_1, \ldots, p_r \in C$
be r distinct points and
$D_i := \{p_i\} \times {\mathbb C}^3\subset X$
be the fibers over
$p_i$
. We impose the (log) CY condition
which implies that
\begin{equation}D:=\bigsqcup_{i=1}^r D_i \end{equation}
is an anti-canonical divisor of X. Let
$({\mathbb C}^*)^3$
be the torus which acts on the fibers of the projection
$X\to C$
and consider the subtorus
As in the
$\mathbb{C}^4$
case, one can define the tautological relative invariants and their generating series
$Z (X, \bigsqcup_{i=1}^r D_i; L_m)$
(refer to Definition 6.12, where the orientations are canonically chosen).
Theorem 1.15 (Theorem 6.16). Let X be a local curve (1.15) and
$\bigsqcup_{i=1}^r D_i$
(1.16) be its anti-canonical divisor. Then
\begin{align*}Z \bigg(\!X, \bigsqcup_{i=1}^r D_i; L_m\!\bigg) = M(q)^{\int_X c_1^{T \times {\mathbb C}^*_m} (L_m)\, \cdot \,c_3^T (T_X[-D])},\end{align*}
where
$T_X[-D]$
is the sheaf of tangent vectors with logarithmic zeros along D (Definition 6.13).
1.7 Related works and some future directions
Nekrasov conjectured a K-theoretic analogue of the formula (1.14) [Reference NekrasovNek20], which is proved in a recent work of Kool and Rennemo [Reference Kool and RennemoKR25]. While our proof of (1.14) uses a degeneration formula and pole analysis, their proof uses a totally different idea and is based on a factorizable sequence of sheaves developed by Okounkov [Reference OkounkovOko17]. Note that the formula of [Reference NekrasovNek20] is K-theoretic and reproduces the cohomological formula of the present paper under the cohomological limit studied in [Reference Cao, Kool and MonavariCKM22a]. The advantage of using the degeneration method in this paper is that one can also deal with non-toric Calabi–Yau 4-folds, see e.g. (1.15).
In future work, we hope to apply the degeneration formula developed in this paper to formulate and prove Gromov–Witten/Donaldson–Thomas correspondence (as in [Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06a, Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06b]) on general Calabi–Yau 4-folds.
We also remark that the study of the degeneration formula of
$\mathop{\rm DT}\nolimits_4$
theory (in its most general form) should be put in the context of logarithmic geometry (see [Reference Maulik and RanganathanMR20] for a study in this direction on 3-folds). It will be interesting to explore this perspective more in the future.
2. Reminder of expanded pairs and degenerations
In this section, we review the foundations on moduli stacks of expanded pairs and degenerations as developed by Jun Li [Reference LiLi01]. In the present paper, we are mainly interested in those moduli stacks associated to (log) Calabi–Yau 4-folds. Nevertheless, this section works in arbitrary dimension.
2.1 Expanded pairs
Definition 2.1. A smooth pair (Y, D) consists of a smooth quasi-projective variety Y and a smooth connectedFootnote
3
divisor
$D\subset Y$
. More generally, a locally smooth pair (Y’, D’) consists of a quasi-projective variety Y’ and a connected divisor D’, so that étale locally around D’ the pair is a smooth pair.
Let (Y, D) be a smooth pair. The associated bubble component is the following
${\mathbb P}^1$
-bundle over D:
It comes with two canonical sections
$D_0 = {\mathbb P}_D ( {\mathcal O}_D )$
and
$D_\infty = {\mathbb P}_D (N_{D/Y})$
.
For an integer
$k\geqslant 0$
, let
where the divisor
$D_\infty$
of the ith
$\Delta$
is glued to the
$D_0$
of the
$(i+1)$
th
$\Delta$
. The normal bundle of
$D_0$
and that of
$D_\infty$
in
$\Delta$
are inverse to each other, making the singularity of
$Y[k]_0$
smoothable in the first order.
Let
$D[k]_0$
be the
$D_\infty$
of the last bubble component
$\Delta$
. Then
is a locally smooth pair, which we call the expanded pair of length k.
There is a projective map
which contracts all the bubble components, and maps the divisor
$D[k]_0$
isomorphically to D.
In [Reference LiLi01], for each k, a family of expanded pairs is explicitly constructed whose properties are given below. In particular, the generic fiber is Y and the most special fiber is
$Y[k]_0$
. This family is called the standard family.
Proposition 2.2 ([Reference LiLi01, Reference Li and WuLW15], [Reference ZhouZho18, Proposition 2.16]). There is a flat family
together with a smooth connected divisor
$D[k] \subset Y[k]$
, and a projective map
$p_k: Y[k] \to Y \times {\mathbb A}^k$
which satisfy the following properties.
-
(1) The pair (Y[k], D[k]) is a smooth pair, with Y[k] a smooth quasi-projective variety of dimension
$\dim Y + k$
. There is an isomorphism
$D[k] \cong D \times {\mathbb A}^k$
under which
$\pi_k |_{D[k]}$
coincides with a projection to
${\mathbb A}^k$
. -
(2) Let
$t = (t_1, \ldots, t_k) \in {\mathbb A}^k$
be a closed point. Let
$l = \sharp \{ i \mid t_i =0 \}$
. The fiber of
$\pi_k$
over t is isomorphic to
$Y[l]_0$
. The restriction of
$p_k$
to this fiber is the contraction map p (2.1).
-
(3) There is a
$({\mathbb C}^*)^k$
-action on Y[k], such that
$\pi_k$
and
$p_k$
are equivariant, where
$({\mathbb C}^*)^k$
acts on
${\mathbb A}^k$
in the standard way. For a closed point
$t\in {\mathbb A}^k$
as above, the stabilizer group
$\operatorname{Stab}_t ({\mathbb A}^k) \cong ({\mathbb C}^*)^l$
acts on the fiber
$Y[l]_0$
by scaling the l bubble components
$\Delta$
.
There is a smooth equivalence relation
$\sim$
on both Y[k] and
${\mathbb A}^k$
[Reference ZhouZho18, § 2.5], induced by the
$({\mathbb C}^*)^k$
-action above and permutations of the coordinates of
${\mathbb A}^k$
off diagonal. Moreover, for
$l\leqslant k$
, the family
$Y[l] \to {\mathbb A}^l$
has standard embeddings into
$Y[k] \to {\mathbb A}^k$
. The direct limit of the families, up to the equivalence relations, define the stacks of interest.
Definition 2.3 ([Reference LiLi01], [Reference Li and WuLW15, § 2.3], [Reference ZhouZho18, Definition 2.20]). The stack of expanded pairs is defined as
${\mathcal A} := \underrightarrow\lim \ [{\mathbb A}^k / \sim]$
, with universal expanded pair
${\mathcal Y} := \underrightarrow\lim \ [Y[k] / \sim]$
, and universal relative divisor
${\mathcal D} := \underrightarrow\lim \ [D[k] / \sim]$
.
${\mathcal A}$
is a smooth Artin stack of dimension 0, and
${\mathcal Y}$
is a smooth Artin stack of dimension
$\dim Y$
. There is a representable, projective map
whose composition with the projection to
${\mathcal A}$
gives the family map
which is flat and also representable. The universal relative divisor
${\mathcal D}$
satisfies
such that the restriction of p to
${\mathcal D}$
coincides with the base change of
$D \hookrightarrow Y$
over
${\mathcal A}$
. For a scheme S, a family of expanded pairs over S is a map
$S \to {\mathcal A}$
. Pulling back the universal family
$\pi$
gives a family
endowed with a divisor
${\mathcal D}_S\subset {\mathcal Y}_S$
obtained by pulling back the universal divisor
${\mathcal D}$
. We also refer to
$({\mathcal Y}_S,{\mathcal D}_S)$
as a family of expanded pairs over S.
Definition 2.4. Let (Y, D) be a locally smooth pair, such that Y is Gorenstein with canonical line bundle
$\omega_Y$
. Let S be a scheme, and
$({\mathcal Y}_S, {\mathcal D}_S)$
a family of expanded pairs over S:
-
–
$({\mathcal Y}_S, {\mathcal D}_S)$
is log Calabi–Yau (log CY) over S if
$\omega_{{\mathcal Y}_S / S} ({\mathcal D}_S) \cong {\mathcal O}_{{\mathcal Y}_S}$
; -
– in particular, if
$S = \operatorname{{Spec}} \mathbb{C}$
, where
$({\mathcal Y}_S, {\mathcal D}_S) = (Y[k]_0, D[k]_0)$
for some
$k\geqslant 0$
, we say that
$(Y[k]_0, D[k]_0)$
is log CY if it is log CY over
$\operatorname{{Spec}} \mathbb{C}$
.
If (Y, D) is log CY, the adjunction formula implies that
$\omega_D \cong {\mathcal O}_D$
.
Proposition 2.5.
If (Y, D) is a smooth log CY pair, then any family
${\mathcal Y}_S \to S$
of expanded pairs with pullback divisor
${\mathcal D}_S$
is log CY over S. In particular, the standard families (Y[k], D[k]) are log CY over
${\mathbb A}^k$
; the universal pair
$({\mathcal Y}, {\mathcal D})$
is log CY over the base
${\mathcal A}$
; and the expanded pairs
$(Y[k]_0, D[k]_0)$
are log CY.
Proof. Since
${\mathcal Y}_S \to S$
is flat, the log CY property is preserved under arbitrary base change. It suffices to prove the log CY property for the standard families (Y[k], D[k]) over
${\mathbb A}^k$
. Obviously,
Hence it suffices to prove (Y[k], D[k]) is log CY. We prove this by induction on k. Recall (see [Reference LiLi01, p. 521]) that Y[k] is constructed as
When
$k=1$
,
$Y[1] = \operatorname{Bl}_{D \times \{0\} } (Y \times {\mathbb A}^1)$
. The map
$p: Y[1] \to Y \times {\mathbb A}^1$
is the blow-up, and D[1] is the proper transform of
$D\times {\mathbb A}^1$
. Let E be the exceptional divisor. We have
\begin{eqnarray*}\omega_{Y[1]} &\cong& p^* \omega_{Y\times {\mathbb A}^1} \otimes {\mathcal O} (E) \\&\cong& p^* {\mathcal O} (-D \times {\mathbb A}^1 ) \otimes {\mathcal O} (E) \qquad\quad \text{(since }(\textit{Y, D})\text{ is log CY)} \\&\cong& {\mathcal O} (-D[1]) \otimes {\mathcal O} (-E) \otimes {\mathcal O} (E) \\&\cong& {\mathcal O} (-D[1]) .\end{eqnarray*}
Therefore, (Y[1], D[1]) is log CY and the proposition follows. The inductive process is obtained by replacing Y by
$Y[k-1]$
in the
$k=1$
case above.
2.2 Expanded degenerations
Definition 2.6. Let X be a smooth quasi-projective variety over
${\mathbb C}$
. A map
is a simple degeneration if it is flat, with smooth fiber
$X_c=\pi^{-1}(c)$
for
$c\neq 0$
, and central fiber
where
$(Y_\pm, D)$
are smooth pairs (Definition 2.1), and
$Y_\pm$
intersect transversally at the singularFootnote
4
divisor
$D=Y_- \cap Y_+ $
in the sense that étale locally around
$0\in {\mathbb A}^1$
, the map
$\pi$
is of the form
where
$Y_\pm$
are cut out by the equations
$(x=0)$
and
$(y=0)$
respectively.
By definition, we automatically have
For
$k\geqslant 0$
, consider the following expanded degeneration of length k:
Similarly, these arise as central fibers of standard families. There is a projective map
which contracts all the
$\Delta$
.
Define the multiplication map
Let
$({\mathbb C}^*)^k$
act on
${\mathbb A}^1$
trivially and on
${\mathbb A}^{k+1}$
such that m is equivariant.
Proposition 2.7 ([Reference LiLi01, Reference Li and WuLW15], [Reference ZhouZho18, Proposition 2.13]). There is a standard family
which satisfies the following properties.
-
(1) The total space X[k] is a smooth quasi-projective variety of dimension
$(\dim X + k)$
. There is a projective map
$p_k: X[k] \to X \times_{{\mathbb A}^1} {\mathbb A}^{k+1}$
. -
(2) Let
$t = (t_0, \ldots, t_k) \in {\mathbb A}^{k+1}$
be a closed point. If
$c = t_0 \cdots t_k\neq 0$
, then the fiber of
$\pi_k$
over t is isomorphic to
$X_c$
, to which the restriction of
$p_k$
is the identity map; if
$t_0 \cdots t_k = 0$
, and hence
$l := \sharp \{i \mid t_i = 0 \} \geqslant 1$
, then the fiber of
$\pi_k$
over t is isomorphic to
$X[l-1]_0$
, to which the restriction of
$p_k$
is the contraction map p (2.2). -
(3) There is a
$({\mathbb C}^*)^k$
-action on X[k], such that
$\pi_k$
and
$p_k$
are equivariant. For a closed point
$t\in {\mathbb A}^{k+1}$
as above with
$t_0 \cdots t_k = 0$
, the stabilizer group
$\operatorname{Stab}_t ({\mathbb A}^{k+1} ) \cong ({\mathbb C}^*)^{l-1}$
acts on the fiber
$X[l-1]_0$
by scaling
$(l-1)$
bubble components.
An expanded degeneration can be obtained by gluing two expanded pairs:
for any
$0\leqslant i\leqslant k$
. The following proposition is a description of this fact in terms of standard families.
Proposition 2.8 ([Reference LiLi01, Reference Li and WuLW15], [Reference ZhouZho18, Proposition 2.18]). The composition
$\operatorname{pr}_i \circ\, \pi_k: X[k] \to {\mathbb A}^1$
is a simple degeneration, with singular divisor
$D_i[k]$
and central fiber
$X[k] \times_{{\mathbb A}^1} 0 = X[k]_-^i \cup_{D_i[k]} X[k]_+^i$
, where
Footnote 5
As before, one can define the stack of expanded degenerations by quotienting out the
$({\mathbb C}^*)^k$
together with the discrete symmetries, and then taking the direct limit.
Definition 2.9 ([Reference LiLi01], [Reference Li and WuLW15, §§ 2.1 and 2.2], [Reference ZhouZho18, Definition 2.22]). The stack of expanded degenerations is defined as
${\mathcal C}:= \underrightarrow\lim \ [{\mathbb A}^{k+1} / \sim]$
, with universal expanded degeneration
${\mathcal X} :=\underrightarrow\lim \ [X[k] / \sim]$
.
${\mathcal C}$
is a smooth Artin stack of dimension 1, and
${\mathcal X}$
is a smooth Artin stack of dimension
$\dim X$
. They both admit a map to
${\mathbb A}^1$
. There is a representable and projective map
whose composition with the projection to
${\mathcal C}$
is the family map
which is flat and also representable.
In general, let
$S \to {\mathbb A}^1$
be a scheme over
${\mathbb A}^1$
. Given a
${\mathbb A}^1$
-morphism
$S \to {\mathcal C}$
, the pullback of the universal family
$\pi$
gives a family
which we call a family of expanded degenerations over S.
Definition 2.10. Let
$\pi: X\to {\mathbb A}^1$
be a simple degeneration and let
$\pi_S: {\mathcal X}_S \to S$
be a family of expanded degenerations:
-
–
$\pi_S: {\mathcal X}_S \to S$
is called Calabi–Yau (CY), if the relative canonical bundle is trivial:
$\omega_{{\mathcal X}_S / S} \cong {\mathcal O}_{{\mathcal X}_S}$
; -
– in particular,
$\pi: X \to {\mathbb A}^1$
is called Calabi–Yau (CY) if it is CY over
${\mathbb A}^1$
; any expanded degeneration
$X[k]_0$
is CY if it is CY in the usual sense, i.e.
$\omega_{X[k]_0} \cong {\mathcal O}_{X[k]_0}$
.
Proposition 2.11.
Let
$\pi: X\to {\mathbb A}^1$
be a CY simple degeneration. Then:
-
(1) the smooth pairs
$(Y_\pm, D)$
in Definition 2.6 are log CY; -
(2) any family
${\mathcal X}_S \to S$
of expanded degenerations is CY. In particular, the standard families
$\pi_k: X[k] \to {\mathbb A}^{k+1}$
are CY; the universal family
$\pi: {\mathcal X} \to {\mathcal C}$
is CY; any expanded degeneration
$X[k]_0$
is CY.
Proof. For (1), it is straightforward to see that
By the definition of simple degeneration, we have
The adjunction formula then implies that
The case for
$Y_-$
is similar.
For (2), as in the proof of Proposition 2.5, it suffices to show that the standard family X[k] is CY. Recall (see [Reference LiLi01]) that X[k] is constructed inductively from
$X[k-1]$
. We prove this by induction on k. When
$k=1$
, X[1] is constructed in two steps. First, one takes the blow-up
$\operatorname{Bl}_{D \times \{0\} } (X \times_{{\mathbb A}^1} {\mathbb A}^2)$
, where the map
${\mathbb A}^2 \to {\mathbb A}^1$
is the multiplication. The exceptional divisor is
$\Delta \times_D \Delta$
, with normal bundle
${\mathcal O}_{\Delta \times_D \Delta} (-1, -1)$
. One then blows down a factor of
${\mathbb P}^1$
and obtains X[1]. The resulting map
is a resolution of singularities, with exceptional divisor
$\Delta$
, whose normal bundle is
${\mathcal O}_\Delta ({-}1)^{\oplus 2}$
. Therefore, it is a crepant resolution, and X[1] is CY. Replacing X by
$X[k-1]$
in the
$k=1$
case gives the inductive process.
Next we describe the central fiber of the universal family
${\mathcal X}$
. The multiplication map (2.3) gives a map
whose fiber over 0 is denoted by
By construction, this is a limit of the standard smooth charts
$[{\mathbb A}^{k+1} \times_{{\mathbb A}^1} 0 / \sim] = [\,\bigcup_{i=1}^{k+1} H_i / \sim]$
, where
$H_i = (t_i=0) \subset {\mathbb A}^{k+1}$
is the ith standard hyperplane. Let
be the normalization, which means that
${\mathcal C}_0^\dagger := \underrightarrow\lim\, [\,\coprod_{i=1}^{k+1} H_i / \sim]$
. Let
be the fiber product, which by definition is
$\underrightarrow\lim\, [\,\coprod_{i=1}^{k+1} X[k] |_{H_i} / \sim]$
.
A geometric interpretation of
${\mathcal X}^\dagger_0$
and
${\mathcal C}^\dagger_0$
can be obtained from Proposition 2.8, which implies that
${\mathcal C}_0^\dagger$
classifies expanded degenerations with a marked nodal divisor, and
${\mathcal X}^\dagger_0$
is the universal divisor. This marking then makes it possible to split the expanded degeneration at the marked nodal divisor, resulting in two expanded pairs.
Corollary 2.12. There is a canonical isomorphism
${\mathcal C}_0^\dagger \cong {\mathcal A} \times {\mathcal A}$
, such thatFootnote
6
2.3 Topological data
Let B be a scheme and
$\pi: V \to B$
be a quasi-projective scheme over B. Let
$K_c (V / B)$
be the fiberwise compactly supported K-group, i.e. the Grothendieck group of coherent sheaves F on V, whose supports
$\mathop{\rm Supp}\nolimits F$
are proper over B. In particular, there is a well-defined K-theoretic pushforward map
to the Grothendieck group
$K_0 (B)$
of coherent sheaves on B.
Definition 2.13.
$F_1$
,
$F_2 \in K_c (V / B)$
are called fiberwise numerically equivalent and are denoted by
$F_1 \sim_{\mathrm{num}} F_2$
, if
for any locally free sheaf E on V. Define the fiberwise compactly supported numerical K-theory as
When
$B = \text{pt}$
, we simply denote it by
$K_c^\mathrm{{num}} (V)$
.
Let
$\pi: X\to {\mathbb A}^1$
be a simple degeneration, with central fiber
$X_0 = Y_- \cup_D Y_+$
and smooth fibers
$X_t$
(for any
$t\neq 0$
). Denote the closed embeddings as follows:
Lemma 2.14. The K-theoretic Gysin pullback [Reference FultonFul98, Example 15.1.8]
descends to the corresponding numerical K-theories
Proof. We prove the case for
$i_t^*$
; the other proof is similar. Take
$[F_i]\in K_c(X/ {\mathbb A}^1)$
(
$i=1,2$
) such that
for any locally free E on X. Then for any locally free sheaf V on
$X_t$
,
Since X is smooth,
$i_{t*} V$
has a resolution by a perfect complex
$E^\bullet$
of locally free sheaves. By (2.9) and a proper pushforward to a point, we know that
$\chi(X,F_1\otimes i_{t*}V)=\chi(X,F_2\otimes i_{t*} V)$
.
Using the above Gysin pullback, we define the following.
Definition 2.15. Given
$P_0\in K_c^{\mathrm{num}} (X_0)$
, a splitting datum for
$P_0$
is a pair
$(P_-, P_+)$
, with
$P_\pm \in K_c^\mathrm{{num}} (Y_\pm)$
, such that
where
$(-)|_D$
denotes the K-theoretic Gysin pullback from
$Y_\pm$
to D (2.8). We denote the set of all splitting data of
$P_0$
by
$\Lambda^{P_0}_{\rm spl}$
.
Recall that a K-group has a topological filtration
which consists of classes [F] whose support has dimension at most i. The filtration restricts to give corresponding compactly supported classes and descends to numerical K-theory classes:
2.4 Relative Hilbert stacks
Definition 2.16. Let W be a quasi-projective scheme,
$D \subset W$
be a closed subscheme, and F be a coherent sheaf on W. F is said to be normal to D if
$\operatorname{{Tor}}_1^{{\mathcal O}_W} (F, {\mathcal O}_D) = 0$
.
Let (Y, D) be a smooth pair and
$\pi: X \to {\mathbb A}^1$
be a simple degeneration. Let Z be a properly supported closed subscheme on the expanded pair
$Y[k]_0$
or the expanded degeneration
$X[k]_0$
. We treat Z as an object in the Hilbert scheme by considering the quotient sheaf
$ {\mathcal O}_{Y[k]_0} \twoheadrightarrow {\mathcal O}_Z$
. An automorphism of Z is understood as an automorphism induced by the
$({\mathbb C}^*)^k$
-action.
Definition 2.17. A properly supported closed subscheme Z in
$Y[k]_0$
or
$X[k]_0$
is called stable if:
-
–
${\mathcal O}_Z$
is normal to every singular divisor D in
$Y[k]_0$
or
$X[k]_0$
, as well as the relative divisor
$D[k]_0$
(in the case of
$Y[k]_0$
); and -
– the automorphism group
$\operatorname{Aut} ({\mathcal O}_{Y[k]_0} \twoheadrightarrow {\mathcal O}_Z)$
or
$\operatorname{Aut} ({\mathcal O}_{X[k]_0} \twoheadrightarrow {\mathcal O}_Z)$
is finite.
The same definition can be made for families of expanded pairs and expanded degenerations, where we require the stable condition on geometric fibers and the flatness of Z over the base. In particular, one can consider stable subschemes on the universal families
${\mathcal Y} \to {\mathcal A}$
and
${\mathcal X} \to {\mathcal C}$
.
Definition 2.18. Denote by
$\operatorname{{Hilb}} (Y, D)$
the stack parameterizing families of stable subschemes Z in the universal family
${\mathcal Y} / {\mathcal A}$
. Similarly, denote by
$\operatorname{{Hilb}} (X/{\mathbb A}^1)$
the corresponding stack for
${\mathcal X} / {\mathcal C}$
.
-
(1) Given a numerical K-theory class
$P \in K_c^{\mathrm{num}} (Y)$
, let
$\operatorname{{Hilb}}^P (Y, D)$
be the substack parameterizing stable subschemes Z such that
$p^K_*[{\mathcal O}_Z] = P$
. Here
$p^K_*$
is the K-theoretic proper pushforward (2.7) of the contraction map
$p: Y[k]_0 \to Y$
. -
(2) Suppose that we are given numerical K-theory classes
$P_t \in K_c^\mathrm{num} (X_t)$
for all
$t\in {\mathbb A}^1$
. Recall that the standard families
$X[k] \to {\mathbb A}^{k+1}$
have fibers either of the form
$X[k]_0$
(
$k\geqslant 0$
), or isomorphic to
$X_t$
with
$t\neq 0$
. Let
$\operatorname{{Hilb}}^{P_t} (X/{\mathbb A}^1)$
be the substack parameterizing stable subschemes Z such that the following hold. -
– If Z is a subscheme in a fiber of the form
$X[k]_0$
(
$k\geqslant 0$
), then
$p^K_* [{\mathcal O}_Z] =P_0$
. Here
$p^K_*$
is the K-theoretic proper pushforward (2.7) of the contraction map
$p: X[k]_0 \to X_0$
. -
– If Z is a subscheme in a fiber isomorphic to
$X_t$
with
$t\in {\mathbb A}^1 \backslash \{0\}$
, then
$[{\mathcal O}_Z] = P_t$
.
Remark 2.19. To have nonempty moduli stack
$\operatorname{{Hilb}}^P (X/{\mathbb A}^1)$
, there is necessarily a
$P_\eta\in K_c^{\mathrm{num}}(X_\eta)$
where
$\eta$
is the generic point of
${\mathbb A}^1$
, so that for any closed point
$t\in{\mathbb A}^1$
,
$P_t\in K_c^\mathrm{num} (X_t)$
is the K-theoretic specialization of
$P_\eta$
.
Remark 2.20. Although we focus on the case of Hilbert stacks, most of the constructions also work for moduli of stable quotients as in [Reference Li and WuLW15, Definition 4.2] and [Reference ZhouZho18, Definition 3.18]. These include many other interesting moduli stacks of objects in derived categories (e.g.
$Z_t$
-stable pairs, considered in [Reference Cao and TodaCT22a, Reference Cao and TodaCT22b, Reference Cao and TodaCT23]).
Lemma 2.21.
The relative Hilbert stack
$\operatorname{{Hilb}}^P (Y, D)$
(respectively
$\operatorname{{Hilb}}^{P_t} (X/{\mathbb A}^1))$
is an open and closed substack of
$\operatorname{{Hilb}} (Y, D)$
(respectively
$\operatorname{{Hilb}}(X/{\mathbb A}^1))$
.
Proof. We prove the statement for
$\operatorname{{Hilb}}^{P_t} (X/{\mathbb A}^1)$
; the case for
$\operatorname{{Hilb}}^P (Y, D)$
is simpler. Let
${\mathcal X}_S \to S$
be a family of expanded degenerations, and
${\mathcal Z}_{\mathcal S}$
be a family of stable subschemes in
${\mathcal X}_S$
. Up to an étale base change, we may assume that
${\mathcal X}_S \to S$
is the base change of a standard family of
$X[k] \to {\mathbb A}^{k+1}$
, i.e. the classifying map
$S\to \mathcal{C}$
factors through
$S\stackrel{\xi}{\to} {\mathbb A}^{k+1} \to \mathcal{C}$
. Let
$m: {\mathbb A}^{k+1} \to {\mathbb A}^1$
be the multiplication map.
For any geometric point
$s\in S$
, the fiber
${\mathcal X}_s$
satisfies
\begin{align*}{\mathcal X}_s\cong\Bigg\{\begin{array}{l@{\quad \ }l}X[k]_0 \ \mathrm{for}\ \mathrm{some}\ k\geqslant 0 &\mathrm{if} \ s\in (m \circ \xi)^{-1} (0), \\[3pt] X_t & \mathrm{if} \ s\in (m \circ \xi)^{-1} (t), t\neq 0.\end{array}\end{align*}
Let
${\mathcal Z}_s$
be the corresponding stable subscheme in the fiber
${\mathcal X}_s$
. It suffices to prove that for all
$s\in (m \circ \xi)^{-1} (0)$
(respectively
$s\in (m \circ \xi)^{-1} (t)$
), the numerical K-theory class
$p^K_* [{\mathcal O}_{{\mathcal Z}_s}] \in K_c^\mathrm{num} (X_0)$
(respectively
$[{\mathcal O}_{{\mathcal Z}_s}] \in K_c^\mathrm{num} (X_t)$
) is locally constant in s. By definition, it suffices to prove that for any locally free sheaf E on
${\mathcal X}_s \cong X [k]_0 $
(respectively
${\mathcal X}_s \cong X_t$
), the function
is locally constant in s. But this follows from the flatness of
${\mathcal Z}_S$
over S.
Proposition 2.22 [Reference Li and WuLW15, Theorems 4.14, 4.15].
-
(1) The relative Hilbert stack
$\operatorname{{Hilb}} (Y, D)$
(respectively
$\operatorname{{Hilb}} (X/{\mathbb A}^1))$
is a Deligne–Mumford stack, locally of finite type (respectively locally of finite type over
${\mathbb A}^1)$
. -
(2) If Y is proper (respectively
$\pi: X\to {\mathbb A}^1$
is proper), then
$\operatorname{{Hilb}}^P (Y, D)$
(respectively
$\operatorname{{Hilb}}^{P_t} (X/{\mathbb A}^1))$
is proper (respectively proper over
${\mathbb A}^1)$
.
Remark 2.23. In practice, the following cases are often of particular interest, where neither the target spaces nor the moduli spaces are proper:
-
– local curves (see Equation (6.12)); and
-
– toric varieties (see e.g. [Reference Cao and KoolCK18, Reference Cao and KoolCK20] for discussions on toric Calabi–Yau 4-folds).
The standard way out in such situations is to find a torus T acting on (Y,D) (respectively T acting on X, trivially on
${\mathbb A}^1$
and
$\pi: X\to {\mathbb A}^1$
being equivariant), such that the fixed loci
$\operatorname{{Hilb}}^P (Y, D)^T$
(respectively
$\operatorname{{Hilb}}^{P_t} (X/{\mathbb A}^1)^T$
) are proper. Enumerative invariants can then be defined via T-equivariant localization. This is indeed the case in the two situations mentioned above. The reason is that one can then find a natural smooth T-equivariant compactification
$\bar Y$
of Y, where the closure
$\bar D$
of D is still smooth, such that the T-fixed loci
$\operatorname{{Hilb}}^P (Y, D)^T$
form a union of connected components of the T-fixed locus
$\operatorname{{Hilb}}^P (\bar Y, \bar D)^T$
, which is proper by Proposition 2.22, and similarly for the
$X/\mathbb{A}^1$
case.
For example, in the case of local curves, we can take T to be the torus which acts on fibers, or its Calabi–Yau subtorus.
Several variants are needed for applications in the present paper. For
$P \in K_c^{\mathrm{num}} (Y)$
, there is a stack
${\mathcal A}^P$
parameterizing expanded pairs with a weight structure, whose total continuous weight is P. A weight structure on an expanded pair assigns each irreducible component and each singular divisor an element in
$K_c^\mathrm{{num}}(Y)$
, so that the summation of all weights is the fixed K-theory class P. The assignment is subject to a continuity condition. We refer an interested reader to [Reference ZhouZho18, Definition 7.2] and [Reference Li and WuLW15, Definition 2.14] for details. Similarly, one has the stack
${\mathcal C}^{P_t}$
. There are étale maps forgetting the weight structure:
Denote the universal families over
${\mathcal A}^P$
and
${\mathcal C}^{P_t}$
by
${\mathcal Y}^P$
and
${\mathcal X}^{P_t}$
, with family maps
The Hilbert stack
$\operatorname{{Hilb}}^P (Y, D)$
in Definition 2.18 can also be described as the stack parameterizing families of stable subschemes Z in the universal family
${\mathcal Y}^P / {\mathcal A}^P$
satisfying
$p^K_*[{\mathcal O}_Z] = P$
. This is because objects in
$\operatorname{{Hilb}}^P (Y, D)$
have fixed topological data P, so
$\operatorname{{Hilb}}^P (Y, D)\to {\mathcal A}$
factors through
${\mathcal A}^P$
. The argument is similar for
$\operatorname{{Hilb}}^{P_t} (X/{\mathbb A}^1)$
.
We also have the weighted versions of (2.4), (2.5), and (2.6):
For each splitting datum
$(P_-, P_+)$
of
$P_0$
in Definition 2.15, there is an open and closed substack
${\mathcal C}_0^{\dagger, (P_-, P_+)} \subset {\mathcal C}_0^{\dagger, P_0}$
, and we let
Corollary 2.12 can be refined as follows.
Corollary 2.24 ([Reference Li and WuLW15, Proposition 2.13], [Reference ZhouZho18, Proposition 7.4]). Given a splitting datum
$(P_-, P_+)$
of
$P_0$
, there is a canonical isomorphism
${\mathcal C}_0^{\dagger, (P_-, P_+)} \cong {\mathcal A}^{P_-} \times {\mathcal A}^{P_+}$
, such that
Denote by
$\Lambda^P_{\rm spl}$
the set of all splitting data of P.
Lemma 2.25 ([Reference Li and WuLW15, Proposition 2.19], [Reference ZhouZho18, Proposition 7.5]). There are canonically constructed line bundles with sections
$(L_{P_-, P_+}, s_{P_-, P_+} )$
over
${\mathcal C}^{P_t}$
, indexed by splitting data
$(P_-, P_+) \in \Lambda_{\rm spl}^{P_0}$
, such that:
-
– we have
where
\begin{align*}\bigotimes_{(P_-, P_+) \in \Lambda^{P_0}_{\rm spl} } L_{P_-, P_+} \cong {\mathcal O}_{{\mathcal C}^{P_t}}, \quad \prod_{(P_-, P_+) \in \Lambda^{P_0}_{\rm spl} } s_{P_-, P_+} \cong \pi^{*} t,\end{align*}
$\pi: \mathcal{C}^{P_t} \to {\mathbb A}^1 = \operatorname{{Spec}} {\mathbb C}[t]$
is the canonical map; and
-
–
$\mathcal{C}_0^{\dagger, (P_-, P_+)}$
is the closed substack in
$\mathcal{C}^{P_t}$
defined by
$s_{P_-, P_+} = 0$
.
The lemma leads to a similar decomposition of Hilbert stacks. More precisely, the Hilbert stack
parameterizes stable closed subschemes on singular expanded degenerations. We can consider its normalization
$\operatorname{{Hilb}}^{P_0} (X/{\mathbb A}^1 )_0^\dagger$
, which parameterizes stable closed subschemes in the family
${\mathcal X}_0^{\dagger, P_0} \to {\mathcal C}_0^{\dagger, P_0}$
. There are open and closed stacks
indexed by all possible splitting data of
$P_0$
, whose union is
$\operatorname{{Hilb}}^{P_0} (X/{\mathbb A}^1 )_0^\dagger$
. Since
$\operatorname{{Hilb}}^{P_t} (X/{\mathbb A}^1)$
is of finite type, so is
$\operatorname{{Hilb}}^{P_0} (X/{\mathbb A}^1 )_0^\dagger$
, and therefore the above union is a finite union.
For each splitting datum, we have the following decomposition.
Proposition 2.26 ([Reference Li and WuLW15, Proposition 2.20], [Reference ZhouZho18, Proposition 7.4]). The decomposition in Corollary 2.24 induces the following commutative diagram.

An alternative viewpoint for the Hilbert scheme is to consider it as a moduli of ideal sheaves. The following lemma shows that this also works in the relative setting.
Lemma 2.27.
Let F be a torsion-free sheaf of rank 1 with trivial determinant on
$X[k]_0$
, which is normal to all singular divisors D. Then there exists a closed subscheme
$Z \subset X[k]_0$
of codimension
$\geqslant 2$
, normal to all singular divisors, such that
$F \cong I_Z$
is its ideal sheaf.
Proof. We first prove this on a smooth quasi-projective variety W. Given a torsion-free sheaf F of rank 1, consider its embedding into the double dual
$F \hookrightarrow F^{\vee\vee}$
. Being a reflexive sheaf of rank 1,
$F^{\vee\vee}$
is a line bundle up to codimension 3, which implies that it is actually a line bundle by the proof of [Reference KollárKol90, Lemma 6.13]. It follows that
$F = I_Z$
for some Z with
$\operatorname{codim} Z \geqslant 2$
, since
$\det F = {\mathcal O}_W$
, and
$F \hookrightarrow F^{\vee\vee}$
is an isomorphism up to codimension 2.
Now consider F on
$X[k]_0$
. For simplicity, we may assume that
$k=0$
, i.e.
$X[k]_0 = X_0 = Y_- \cup_D Y_+$
. The case for a general k is similar. Since F is normal to D, we have a short exact sequence
Now by [Reference ZhouZho18, Lemma 3.4], both
$F |_{Y_\pm }$
are torsion-free (and also of rank 1 with trivial determinant). Therefore, there exists
$Z_\pm \subset Y_\pm$
, such that
$F |_{Y_\pm} \cong I_{Z_\pm}$
. It is straightforward to see that the normality of
$Z_\pm$
to D is equivalent to that of
$I_{Z_\pm}$
to D. The
$Z_\pm$
then glue up to
$Z \subset X_0$
, and we have
$F \cong I_Z$
.
3. Shifted symplectic structures
We construct shifted symplectic structures and Lagrangian structures (in the sense of [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Reference Calaque, Pantev, Toën, Vaquié and VezzosiCPT+17]) on the derived enhancement of (relative) Hilbert stacks constructed in the previous section. These will be used to construct virtual structures on those moduli stacks in later sections.
From now on, we will always impose the ‘codimension
$\geqslant 2$
’ assumption. More precisely, we consider the open and closed substack
$\mathrm{Hilb}_{\operatorname{codim} \geqslant 2} (X/{\mathbb A}^1)$
(respectively
$\mathrm{Hilb}_{\operatorname{codim} \geqslant 2} (Y, D)$
) parameterizing subschemes Z with codimension
$\geqslant 2$
. To avoid heavy notation, we will omit the subscripts and denote them just by
$\mathrm{Hilb} (X/{\mathbb A}^1)$
(respectively
$\mathrm{Hilb} (Y, D)$
).
3.1 Shifted symplectic structure on
$\mathbf{Hilb}(X/{\mathbb A}^1)/\mathcal{C}$
Let
$\pi : X \to {\mathbb A}^1$
be a Calabi–Yau simple degeneration (Definitions 2.6, 2.10) and
be the induced map from the universal expanded degeneration
${\mathcal X}$
to the stack
${\mathcal C}$
of expanded degenerations. By Proposition 2.11, we know that
Let
$\textbf{RPerf}$
be the derived (classifying) stack of perfect complexes of quasi-coherent sheaves, and
$\Omega_{\textbf{RPerf}}$
be the natural 2-shifted symplectic form on
$\textbf{RPerf}$
[Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Theorem 0.3]. Consider the derived mapping stack over
${\mathcal C}$
:
where we treat classical stacks
${\mathcal X}$
and
${\mathcal C}$
as derived stacks by the natural inclusion functor.
There is a determinant map (e.g. [Reference Schürg, Toën and VezzosiSTV15, § 3.1])
to the derived moduli stack of line bundles on
${\mathcal X}/{\mathcal C}$
. The homotopy pullback diagram

defines the derived moduli stack
$\textbf{RPerf}({\mathcal X}/{\mathcal C})_{0}$
of perfect complexes on
${\mathcal X}/{\mathcal C}$
with trivial determinant. Let
$\textbf{RPerf}({\mathcal X}/{\mathcal C})_{0, \mathop{\rm rk}\nolimits=1}$
be the open and closed substack of perfect complexes with (virtual) rank 1.
Lemma 3.1. The classical truncation
contains
$\operatorname{{Hilb}} (X/{\mathbb A}^1)$
as an open substack.
Proof. Let
$\mathrm{Perf}({\mathcal X} / {\mathcal C})^{\geqslant 0}_{0, \mathop{\rm rk}\nolimits=1}$
be the open substack of
$\mathrm{RPerf}({\mathcal X}/{\mathcal C})_{0, \mathop{\rm rk}\nolimits=1}$
consisting of perfect complexes F, such that
$\mathrm{Ext}^i (F, F) = 0$
for
$i\lt0$
. We will prove that
$\mathrm{Perf}({\mathcal X} / {\mathcal C})^{\geqslant 0}_{0, \mathop{\rm rk}\nolimits=1}$
contains
$\operatorname{{Hilb}} (X/{\mathbb A}^1)$
as an open substack. Let
${\mathcal X} \to S$
be a family of expanded degenerations over S, and
$Z \subset {\mathcal X}$
be a family of stable subschemes, which gives an object in
$\operatorname{{Hilb}} (X/{\mathbb A}^1) (S)$
. According to [Reference WuWu07a, Corollary 5.9] (see also [Reference WuWu07b, Corollary 2.9]), the ideal sheaf
$I_Z$
is a fiberwise perfect complex. Since we have assumed that
$\operatorname{codim} Z \geqslant 2$
, we obtain a map
sending Z to
$I_Z$
. By Lemma 2.27, an ideal sheaf
$I_Z$
in
$\operatorname{{Hilb}} (X/{\mathbb A}^1)$
can be characterized as a torsion-free sheaf of rank 1 with trivial determinant. Choosing a relatively ample line bundle on
$X/C$
, we may replace the ‘torsion-free’ condition by ‘Gieseker stable’. The substack
$\operatorname{{Hilb}} (X/{\mathbb A}^1)$
then consists of perfect complexes whose Tor-amplitudes concentrate at degree 0, i.e. they are actually coherent sheaves, as well as being properly supported, Gieseker stable and stable (in the sense of Definition 2.17). However, these are all open conditions.Footnote
7
Hence we obtain an open embedding.
There is a derived enhancement
$\mathbf{Hilb} (X/{\mathbb A}^1)$
of
$\operatorname{{Hilb}} (X/{\mathbb A}^1)$
making the diagram

a homotopy pullback diagram [Reference Schürg, Toën and VezzosiSTV15, Proposition 2.1].
Similarly, fixing K-theory classes
$P_t\in K_{c, \leqslant n -2}^{\mathrm{num}} (X_t)$
for all
$t\in \mathbb{A}^1$
, we also have the open substack
$\mathbf{Hilb}^{P_t}(X/{\mathbb A}^1)$
of
$\mathbf{Hilb}(X/{\mathbb A}^1)$
which gives a derived enhancement of
$\operatorname{{Hilb}}^{P_t} (X/{\mathbb A}^1)$
(Definition 2.18).
Theorem 3.2.
Write
$\dim_{\mathbb{C}} X=n+1$
and choose a trivialization
$\mathrm{vol}_{{\mathcal X}/{\mathcal C}}: \mathcal{O}_{{\mathcal X}}\stackrel{\cong}{\to} \omega_{{\mathcal X}/{\mathcal C}}$
. Then as a derived stack over
${\mathcal C}$
,
$\mathbf{Hilb}(X/{\mathbb A}^1)$
has a canonical
$(2-n)$
-shifted symplectic structure
$\Omega_{\mathbf{Hilb}(X/{\mathbb A}^1)/{\mathcal C}}$
. Similarly,
$\mathbf{Hilb}^{P_t}(X/{\mathbb A}^1)/{\mathcal C}^{P_t}$
has a canonical
$(2-n)$
-shifted symplectic structure.
This follows from a family version of the construction of Preygel, [Reference PreygelPre],Footnote
8
which adapts the construction of [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Theorem 2.5] to a moduli of perfect complexes
$(\mathcal{O}\to F)$
on a quasi-projective Calabi–Yau variety, with fixed determinant and the support of F being proper. We sketch the argument and adapt it to our case.
Proof. We deal with
$\textbf{Hilb}(X/{\mathbb A}^1)/{\mathcal C}$
; the decorated case follows in a similar way. We use differential calculus on derived stacks following [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Reference Calaque, Pantev, Toën, Vaquié and VezzosiCPT+17, Reference PreygelPre].
Step 1: Pullback. Let
$\mathcal{E}$
be the universal family over
$\textbf{RPerf}$
. By [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Theorem 2.12], the 2-shifted symplectic form on
$\textbf{RPerf}$
is
Here NC denotes the weighted negative cyclic complex, i.e.
$NC^{w}$
used in [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Theorem 2.12], and
$\operatorname{ch}_2$
denotes the second Chern character (see [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, p. 317]).
Consider the evaluation map
and the pullback form
By an abuse of notation, we denote its image in the negatively cyclic complex (relative to
${\mathcal C}$
) by
Step 2: Lift to a compactly supported form. Let
$\mathcal{F}:=\mathop{\rm ev}\nolimits^*\mathcal{E}$
and
$\mathcal{Z}\subset {\mathcal X}\times_{{\mathcal C}}\mathbf{Hilb}(X/{\mathbb A}^1)$
be the universal substack. This is the support of the cone of the trace map
which is proper over
$\mathbf{Hilb}(X/{\mathbb A}^1)$
. In other words, outside the support
$\mathcal{Z}$
, the trace map is an isomorphism:
We now construct a lift of
$\mathop{\rm ev}\nolimits^*\Omega_{\textbf{RPerf}}$
to a form which is supported on
$\mathcal{Z}$
.
Recall that, for a map
$M_X\to M$
of derived stacks over some base derived stack B and a closed derived substack
$K\subset M_X$
with open immersion
$i: M_X\setminus K\to M_X$
, we define
A section of
$NC_{K}(M_X/B)(p)$
is called a closed p-form on
$M_X/B$
supported on K.
Let
$M_X={\mathcal X}\times_{{\mathcal C}}\mathbf{Hilb}(X/{\mathbb A}^1)$
,
$M=\mathbf{Hilb}(X/{\mathbb A}^1)$
and
$B={\mathcal C}$
in the above. There is a canonical null-homotopy
$\operatorname{ch}_2(\mathcal{O}_{\text{pt}})\sim 0$
in
$NC(\text{pt})(2)$
. Pulling it back along the natural projection
$p: ({\mathcal X}\times_{{\mathcal C}}\mathbf{Hilb}(X/{\mathbb A}^1))\setminus \mathcal{Z}\to \text{pt}$
gives a null-homotopy in
$NC(({\mathcal X}\times_{{\mathcal C}}\mathbf{Hilb}(X/{\mathbb A}^1))\setminus \mathcal{Z})(2)$
:
The fiber sequence
then turns the null-homotopy above into a canonical lift
By an abuse of notation, we write this lift in the relative negatively cyclic homology as
Step 3: Integration. For any quasi-coherent complex F on
$\mathbf{Hilb}(X/{\mathbb A}^1)$
, there is a trace map:Footnote
9
where
$\pi_M: {\mathcal X}\times_{{\mathcal C}}\mathbf{Hilb}(X/{\mathbb A}^1)\to \mathbf{Hilb}(X/{\mathbb A}^1)$
is the projection and
is the functorFootnote
10
of the section with support
$\mathcal{Z}$
. By the argument in [Reference PreygelPre, Proof of Corollary A. 0.12], the complex F may be taken to be the de Rham complex. The same construction as in [Reference PreygelPre, Theorem 3.0.6] shows that the map
$\operatorname{tr}_{{\mathcal X}/{\mathcal C}}$
and a trivialization
defines an integration map
We define
The verification of non-degeneracy is a routine check using Grothendieck–Serre duality.
3.2 Lagrangian structure on
$(\mathbf{Hilb} (Y, D)\to \mathbf{Hilb} ({\mathcal D}))/{\mathcal A}$
Let (Y,D) be a smooth log Calabi–Yau pair (Definition 2.4) so that D is a Calabi–Yau variety. Consider the induced map
from the universal expanded pair
${\mathcal Y}$
to the stack
${\mathcal A}$
of expanded pairs, with universal relative divisor
as in Definition 2.3.
Consider the restriction map between derived mapping stacks:
This map is compatible with determinant maps, i.e. the diagram

is commutative. Therefore we have an induced restriction map
of derived moduli stack of perfect complexes with trivial determinant.
As in Lemma 3.1,
$\mathbf{Hilb}(Y,D)$
is an open substack in
$\textbf{RPerf}({\mathcal D}/{\mathcal A})_{0, \mathop{\rm rk}\nolimits=1}$
. Further restriction to the open substack
$\mathbf{Hilb}(Y,D)$
gives
For a fixed K-theory class
$P\in K_{c, \leqslant \dim_{\mathbb{C}}Y-2}^{\mathrm{num}} (Y)$
, we also have the open substack
$\mathbf{Hilb}^P(Y,D)$
of
$\mathbf{Hilb}(Y,D)$
which gives a derived enhancement of
$\operatorname{{Hilb}}^P (Y,D)$
(Definition 2.18). There is a similar restriction map
Fixing a trivialization
$\mathrm{vol}_D: \mathcal{O}_D \stackrel{\cong}{\to} \omega_{D}$
, by a base change to
${\mathcal D}\cong D\times{\mathcal A}$
, we obtain a trivialization
As in Theorem 3.2,
$\mathrm{vol}_D$
induces a
$(2-\dim_{\mathbb{C}}D)$
-shifted symplectic structure on
$\mathbf{Hilb}(D)$
. Pulling back to
$(\mathbf{Hilb}(D)\times {\mathcal A})/{\mathcal A}$
, we obtain a
$(2-\dim_{\mathbb{C}}D)$
-shifted symplectic structure on
$(\mathbf{Hilb}(D)\times {\mathcal A})/{\mathcal A}$
.
We have a commutative diagram

where
$\mathop{\rm ev}\nolimits_{Y,D} and \mathop{\rm ev}\nolimits_{D}$
are evaluation maps. By Proposition 2.5,
${\mathcal D}\in|\omega_{{\mathcal Y}/{\mathcal A}}^{-1}|$
is an anticanonical divisor of
${\mathcal Y}/{\mathcal A}$
, and therefore we have the following fiber sequence:
Theorem 3.3.
The sequence (3.10) induces a Lagrangian structure on the map (3.6) relative to
${\mathcal A}$
. Similarly, it induces a Lagrangian structure on the map (3.7) relative to
${\mathcal A}^P$
.
This follows from adapting the argument of [Reference CalaqueCal15, §§ 2.2.3 and 3.2.1]Footnote 11 to the family case.
Proof. We prove the claim for (3.6). The other case follows in a similar way. Let
be the universal substack. It is the support of the cone of the trace map (
$\mathcal{F}_{Y,D}:=\mathop{\rm ev}\nolimits_{Y,D}^*\mathcal{E}$
):
which is proper over
$\mathbf{Hilb}(Y,D)$
. We have the following commutative diagrams (with the three boxes being homotopy pullback diagrams).

The vertical maps in the lower half of the diagram are natural projections,
$\mathcal{Z}_{D}\subset {\mathcal D}\times_{{\mathcal A}} (\mathbf{Hilb}(D)\times {\mathcal A})$
is the universal substack of
$\mathbf{Hilb}(D)\times {\mathcal A}$
and
${\mathcal Z}$
is given by the pullback diagram.
A base change implies that for any
$F\in\mathop{\rm QCoh}\nolimits(\mathbf{Hilb}(Y,D))$
,
$G\in \mathop{\rm QCoh}\nolimits(\mathbf{Hilb}(D)\times{\mathcal A})$
, we have
\begin{align}\pi^{{\mathcal Y}}_{M_{Y,D}*}\underline{\mathbf{R}\Gamma_{\mathcal{Z}_{Y,D}}}(i_{{\mathcal D}\to {\mathcal Y}*}\mathcal{O}_{{\mathcal D}}\boxtimes F)&\cong\pi^{{\mathcal Y}}_{M_{Y,D}*}i_{{\mathcal D}\to {\mathcal Y}*}\underline{\mathbf{R}\Gamma_{\mathcal{Z}_{}}}(\mathcal{O}_{{\mathcal D}}\boxtimes F)\nonumber \\&\cong \pi^{{\mathcal D}}_{M_{Y,D}*}\underline{\mathbf{R}\Gamma_{\mathcal{Z}_{}}}(\mathcal{O}_{{\mathcal D}}\boxtimes F), \nonumber\\\pi^{{\mathcal D}}_{M_{Y,D}*}\underline{\mathbf{R}\Gamma_{\mathcal{Z}_{}}}(\mathcal{O}_{{\mathcal D}}\boxtimes r_{{\mathcal D}\to {\mathcal Y}}^*G) &\cong\pi^{{\mathcal D}}_{M_{Y,D}*}\underline{\mathbf{R}\Gamma_{\mathcal{Z}_{}}}\,r_{{\mathcal D}\to {\mathcal Y}}^*(\mathcal{O}_{{\mathcal D}}\boxtimes G) \nonumber\\&\cong \pi^{{\mathcal D}}_{M_{Y,D}*}\,r_{{\mathcal D}\to {\mathcal Y}}^*\,\underline{\mathbf{R}\Gamma_{\mathcal{Z}_{D}}}(\mathcal{O}_{{\mathcal D}}\boxtimes G) \nonumber\\&\cong r_{{\mathcal D}\to {\mathcal Y}}^*\,\pi_{M_{D}*}\,\underline{\mathbf{R}\Gamma_{\mathcal{Z}_{D}}}(\mathcal{O}_{{\mathcal D}}\boxtimes G)\end{align}

Applying
$\pi^{{\mathcal Y}}_{M_{Y,D}*}\underline{\mathbf{R}\Gamma_{\mathcal{Z}_{Y,D}}}$
to (3.10), we obtain, for any
$G\in \mathop{\rm QCoh}\nolimits(\mathbf{Hilb}(D)\times{\mathcal A})$
a commutative diagram

where
$\operatorname{tr}_{(-)}$
is the trace map (3.4). The top and bottom row of the diagram are both fiber sequences.
Let
$\mathcal{E}$
be the universal family over
$\textbf{RPerf}$
. Then
The pullback of the shifted symplectic form of
$\mathbf{Hilb}(D)\times {\mathcal A}$
to
$\mathbf{Hilb}(Y,D)$
is
\begin{align}r_{{\mathcal D}\to {\mathcal Y}}^*\int_{{\mathcal D}/{\mathcal A}}\mathrm{vol}_{{\mathcal D}/{\mathcal A}}\wedge(\mathop{\rm ev}\nolimits_D^*\Omega_{\textbf{RPerf}})&=\int_{{\mathcal D}/{\mathcal A}}(\operatorname{id}\times r_{{\mathcal D}\to {\mathcal Y}})^*(\mathrm{vol}_{{\mathcal D}/{\mathcal A}}\wedge(\mathop{\rm ev}\nolimits_D^*\Omega_{\textbf{RPerf}})) \nonumber\\&=\int_{{\mathcal D}/{\mathcal A}}\mathrm{vol}_{{\mathcal D}/{\mathcal A}}\wedge i_{{\mathcal D}\to {\mathcal Y}}^*(\mathop{\rm ev}\nolimits_{Y,D}^*\Omega_{\textbf{RPerf}})\end{align}
where the second equality uses the commutativity of diagram (3.9), and the upper boxes in diagram (3.11) (which ensures the compactly supported lifts also coincide).
To construct a null-homotopy of (3.15), it suffices to construct a null-homotopy of the map (in the equation below,
$d=\dim_{\mathbb C} D$
):
This is provided by
$\operatorname{tr}_{{\mathcal Y}/{\mathcal A}}$
in diagram (3.14) following the argument in [Reference CalaqueCal15, §§ 3.2.1 and 2.2.3].
3.3 Composition with a Lagrangian fibration
The restriction map
$r_{{\mathcal D}\to {\mathcal Y}}$
has a Lagrangian structure (Theorem 3.3). Fix a numerical K-theory class
$P_D\in K_{c,\leqslant \dim_{\mathbb{C}}D-2}^\mathrm{{num}}(D)$
and consider the open substack
$\mathbf{Hilb}^{P_D}(D)$
of
$\mathbf{Hilb} (D)$
. We are interested in the case when
$\mathbf{Hilb}^{P_D}(D)$
has a Lagrangian fibration structure in the following sense.
Definition 3.4 [Reference CalaqueCal19, Definition 1.9]. Let
$\pi:M\to N$
be a map of derived Artin stacks locally of finite presentations. The structure of an n-shifted Lagrangian fibration on
$\pi$
is an n-shifted symplectic structure
$\Omega_{M}$
on M together with a null-homotopy of its image under the natural map
$\mathcal{A}^{2,\textit{cl}}(M,n)\to \mathcal{A}^{2,\textit{cl}}(M/N,n)$
, such that the induced sequence
is a fiber sequence.
Remark 3.5. For a map
$\pi$
relative to a base B, one defines it similarly, replacing
${\mathbb T}_M$
by
${\mathbb T}_{M/B}$
.
Here is an example of Lagrangian fibration (in the
$n=-1$
case).
Example 3.6 Let W be a smooth complex algebraic variety and
$\phi$
a regular function. We define its derived critical locus
$\textbf{Crit}(\phi)$
by the following homotopy pullback diagram.

$\textbf{Crit}(\phi)$
has a canonical
$({-}1)$
-shifted symplectic structure by the Lagrangian intersection theorem of [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Theorem 0.5]. The natural embedding
is a
$({-}1)$
-shifted Lagrangian fibration [Reference GrataloupGra22, Remark 3.12].
Lemma 3.7.
Let A be a derived Artin stack and
$L \stackrel{f}{\to} M \stackrel{\pi}{\to} B$
be maps of derived Artin stacks (over A), locally of finite presentations. Assume that f has an n-shifted Lagrangian structure relative to A and
$\pi$
has an n-shifted Lagrangian fibration structure relative to A. Then
$\pi\circ f: L\to B$
has an induced
$(n-1)$
-shifted symplectic structure.
Proof. This is a relative version of [Reference SafronovSaf23, Proposition 1.10]. We have the following homotopy pullback diagram.

Note that
$L\times_A B \to M\times_A B $
and
$M\to M\times_A B$
have n-shifted Lagrangian structures relative to B. As a Lagrangian intersection, we know that
$L\to B$
has an induced
$(n-1)$
-shifted symplectic structure.
As a consequence, we have the following proposition.
Proposition 3.8.
Fix
$P\in K_{c, \leqslant \dim_{\mathbb{C}}Y-2}^{\mathrm{num}} (Y)$
and
$P_D:=P|_D\in K_c^{\mathrm{num}} (D)$
. Assume that the shifted symplectic stack
$\mathbf{Hilb}^{P_D}(D)$
admits a Lagrangian fibration structure
$\mathbf{Hilb}^{P_D} (D)\to W$
. Then its composition with
$r_{{\mathcal D}\to {\mathcal Y}}$
(3.7),
has an induced
$(1-\dim_{\mathbb{C}}D)$
-shifted symplectic structure.
Remark 3.9. There are many quasi-projective Calabi–Yau 3-folds D satisfying the condition that the classical truncation
$\operatorname{{Hilb}}^{P_D} (D):=t_0(\mathbf{Hilb}^{P_D} (D))$
is a global critical locus and the ambient space and regular function have canonical choice given by the so-called quivers with potentials [Reference Derksen, Weyman and ZelevinskyDWZ08, Reference GinzburgGin06, Reference Kontsevich and SoibelmanKS11].
Example 3.10. When
$D=\mathbb{C}^3$
, it is believed that one has an equivalence of the
$({-}1)$
-shifted symplectic derived scheme
Here W is the non-commutative Hilbert scheme
and
$\phi$
is the potential function:
By Example 3.6,
$\mathbf{Hilb}^n(D)\to W$
then has a Lagrangian fibration structure.
4. Orientations on moduli stacks
In this section, we collect notions of orientations associated with shifted symplectic stacks and shifted Lagrangians. We prove that canonical orientation exists on local CY 4-folds (1.11).
4.1 Orientation on
$(\operatorname{{Hilb}}(X/{\mathbb A}^1)\to {\mathcal C})$
Recall that a Calabi–Yau simple degeneration (Definitions 2.6 and 2.10) of quasi-projective n-folds is a family
where the generic fibers of
$\pi$
are smooth quasi-projective Calabi–Yau n-folds. Associated to this data, using § 2.2, we have the stack
${\mathcal C}$
of expanded degeneration with universal family
By Theorem 3.2,
$\mathbf{Hilb}(X/{\mathbb A}^1)/{\mathcal C}$
has a
$(2-n)$
-shifted symplectic structure, which induces an isomorphism
When n is even, taking the determinant induces an isomorphism
Here
$\det({\mathbb T}_{\mathbf{Hilb}(X/{\mathbb A}^1)/{\mathcal C}})$
is the determinant line bundle. Restricting to the classical truncation
$\operatorname{{Hilb}}(X/{\mathbb A}^1)=t_0(\mathbf{Hilb}(X/{\mathbb A}^1))$
, we obtain
By the construction of the shifted symplectic structure in Theorem 3.2, this isomorphism agrees with the one provided by the Grothendieck–Serre duality.
As in [Reference Borisov and JoyceBJ17, § 2.4], [Reference Cao, Gross and JoyceCGJ20, § 1.4], and [Reference Cao and LeungCL14, Reference Cao and LeungCL17a], we define the following.
Definition 4.1. Assume n is even. An orientation on
$\operatorname{{Hilb}}(X/{\mathbb A}^1)/{\mathcal C}$
is a square root of the isomorphism (4.2).
Remark 4.2. In this paper, we focus on the case of
$n=4$
, and a generic fiber of
is the Hilbert scheme on a smooth quasi-projective Calabi–Yau 4-fold. The restriction of the isomorphism (4.2) to such a fiber has a square root under some assumptions [Reference Cao, Gross and JoyceCGJ20, Reference Cao, Gross and JoyceCGJ25, Reference Joyce and UpmeierJU25].Footnote 12 The argument in the papers cited in the previous sentence is differential geometric in nature and uses gauge theoretic moduli spaces. Although it might be possible to adapt the argument to a family, here we provide a canonical orientation that is useful for calculations on (1.11). This is motivated by [Reference CaoCao20] and [Reference Cao, Kool and MonavariCKM22b, § 4.2].
Theorem 4.3.
Let
$U\to {\mathbb A}^1$
be a simple degeneration of 3-folds, and
the associated simple degeneration of 4-folds. Then
$\operatorname{{Hilb}}(X/{\mathbb A}^1)/{\mathcal C}$
has an orientation. Similarly,
$\operatorname{{Hilb}}^{P_t}(X/{\mathbb A}^1)/{\mathcal C}^{P_t}$
has an orientation.
Proof. Let
$M_{\mathrm{cpt}}({\mathcal X}/{\mathcal C})$
be the moduli stack of sheaves on
${\mathcal X}$
with support proper over
$ {\mathcal C}$
. Consider the forgetful map
Let
$\bar{f}:=f\times_{\operatorname{id}_{{\mathcal C}}} \operatorname{id}_{{\mathcal X}}$
, and let
be the natural projections.
Let
${\mathbb F}$
be the universal sheaf on
$M_{\mathrm{cpt}}({\mathcal X}/{\mathcal C})\times_{{\mathcal C}} {\mathcal X}$
and
${\mathbb I}=(\mathcal{O}_{\operatorname{{Hilb}}(X/{\mathbb A}^1)\times_{{\mathcal C}} {\mathcal X}}\to \bar{f}^*{\mathbb F})$
be the universal pair. Then we have the natural isomorphism
\begin{align}\det({\mathbb T}_{\mathbf{Hilb}(X/{\mathbb A}^1)/{\mathcal C}}|_{\operatorname{{Hilb}}(X/{\mathbb A}^1)})&\cong \det(\pi_{H_X*}\mathbf{R}{\mathcal H} om({\mathbb I},{\mathbb I})_0[1]) \nonumber\\&\cong \det(\pi_{H_X*}\mathbf{R}{\mathcal H} om(\bar{f}^*{\mathbb F},\bar{f}^*{\mathbb F})[1]) \nonumber\\&\cong f^*\det(\pi_{M_X*}\mathbf{R}{\mathcal H} om({\mathbb F},{\mathbb F})[1]),\end{align}
where the second isomorphism uses the distinguished triangles (e.g. [Reference Cao, Maulik and TodaCMT22, § 3.2])
and Grothendieck–Serre duality
As in (4.2), we also have
given by Grothendieck–Serre duality on
$\pi_{M_X*}\mathbf{R}{\mathcal H} om({\mathbb F},{\mathbb F})[1]$
. Notice that a choice of square root of (4.5) gives a choice of square root of (4.2) under the pullback map (4.4) (e.g. [Reference Cao, Maulik and TodaCMT22, Theorem 6.3]).
We provide two (equivalent) constructions of a square root of (4.5). As in Theorem 3.2 (see also [Reference Brav and DyckerhoffBD21]), by adapting [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Theorem 2.5] to (relatively) compactly supported sheaves, the natural derived enhancement
$\textbf{M}_{\mathrm{cpt}}({\mathcal X}/{\mathcal C})$
of
$M_{\mathrm{cpt}}({\mathcal X}/{\mathcal C})$
has a shifted symplectic structure relative to
${\mathcal C}$
. Since
${\mathcal X}=\operatorname{Tot}(\omega_{{\mathcal U}/{\mathcal C}})$
,
$\textbf{M}_{\mathrm{cpt}}({\mathcal X}/{\mathcal C})$
is equivalent to the
$(-2)$
-shifted symplectic cotangent bundle (relative to
${\mathcal C}$
) of the derived moduli stack
$\textbf{M}_{\mathrm{cpt}}({\mathcal U}/{\mathcal C})$
of compactly supported sheaves on
${\mathcal U}/{\mathcal C}$
[Reference Bozec, Calaque and ScherotzkeBCS24, Theorem 6.17]. Let
$\textbf{p}$
be the projection
Then there is a fiber sequence
Restricting to the classical truncation and taking the determinant, we obtain
by Grothendieck–Serre duality.
Alternatively, let
$\pi: {\mathcal X}=\operatorname{Tot}(\omega_{{\mathcal U}/{\mathcal C}}) \to {\mathcal U}$
be the projection, and consider the following diagram.

Spectral construction gives a distinguished triangle
Taking the determinant gives an isomorphism
where the second isomorphism is given by Grothendieck–Serre duality. It is easy to see that (4.9) and (4.7) are the same. Up to a constant determined in (4.10) below, the square of this isomorphism gives (4.5). The case of
$\operatorname{{Hilb}}^{P_t}(X/{\mathbb A}^1)/{\mathcal C}^{P_t}$
is similar, by replacing
${\mathcal X}^{}/{\mathcal C}$
in the above by
${\mathcal X}^{P_t}/{\mathcal C}^{P_t}$
.
Remark 4.4. The orientation on
$\operatorname{{Hilb}}(X/{\mathbb A}^1)/{\mathcal C}$
is constructed using the pullback of an orientation on the moduli stack
$M_{\mathrm{cpt}}({\mathcal X}/{\mathcal C})$
of compactly supported sheaves on
${\mathcal X}/{\mathcal C}$
via the forgetful map (4.3). By spectral construction (4.8), the symmetric obstruction complex on
$M_{\mathrm{cpt}}({\mathcal X}/{\mathcal C})$
is of the form
where
$\mathbb{V}$
is a perfect complex and
$\varphi$
is self-dual under the symmetric pairing on
${\mathbb E}$
(defined by Grothendieck–Serre duality). Therefore there is a canonical isomorphism
$\det({\mathbb E})\cong {\mathcal O}$
and orientations of
${\mathbb E}$
are given by
on each connected component of
${\mathcal X}$
(as [Reference Oh and ThomasOT23, Equations (59) and (63)]). We choose the plus sign in the above as the canonical choice of orientation. Similarly,
$\operatorname{{Hilb}}^{P_t}(X/{\mathbb A}^1)/{\mathcal C}^{P_t}$
has a canonical choice of orientation.
4.2 Orientation on
$(\operatorname{{Hilb}}(Y,D)\to\operatorname{{Hilb}}({\mathcal D}))/{\mathcal A}$
Given a smooth log Calabi–Yau pair (Y,D) (Definition 2.4) so that D is a Calabi–Yau variety, we have a stack
${\mathcal A}$
of expanded pairs, a universal expanded pair
${\mathcal Y}$
, and a universal divisor
${\mathcal D}$
(Definition 2.3):
By Theorem 3.3, the restriction map
has a Lagrangian structure relative to
${\mathcal A}$
. Hence there is an isomorphism [Reference Pantev, Toën, Vaquie and VezzosiPTV+13, Definition 2.8]:
Combining with the fiber sequence
we obtain an isomorphism of determinant line bundles:
and
$r_{{\mathcal D}\to {\mathcal Y}}^*\det({\mathbb T}_{(\mathbf{Hilb}(D)\times {\mathcal A})/{\mathcal A)}}\cong \mathcal{O}$
if
$\dim_{\mathbb{C}}D$
is even, which reduces to Definition 4.1.
Restricting (4.12) to the classical truncation, we obtain
where
$r_{{\mathcal D}\to {\mathcal Y}}$
denotes its classical truncation by an abuse of notation.
As in [Reference Cao and LeungCL17a, Definition 4.4] and [Reference Cao and LeungCL17b, Definition 6.1], we use the following definition.
Definition 4.5. Assume
$\dim_{\mathbb{C}}D$
is odd. A relative orientation on the map
is the following data: a line bundle
$K^{-1/2}_{\operatorname{{Hilb}}(D)}$
, an isomorphism
and an isomorphism
whose square is the isomorphism (4.13).
As in Theorem 4.3, we have the following.
Theorem 4.6.
Let (U,S) be a smooth pair (Definition 2.1) with
$\dim_{\mathbb{C}} U=3$
and let
be the (associated) log Calabi–Yau pair (Definition 2.4). Then
has a relative orientation. Similarly,
$\operatorname{{Hilb}}^P(Y,D)\to \operatorname{{Hilb}}^{P|_D}(D)\times {\mathcal A}^P$
has a relative orientation.
The proof is similar to the proof of Theorem 4.3.
Proof. Let
$M_{\mathrm{cpt}}({\mathcal Y}/{\mathcal A})$
be the moduli stack of compactly supported sheaves on
${\mathcal Y}/{\mathcal A}$
which are normal to
${\mathcal D}$
in the sense of Definition 2.16. Let
$M_{\mathrm{cpt}}(D)$
be the moduli stack of compactly supported sheaves on D. We have a commutative diagram

where r is the restriction map, and both
$f_Y$
and
$f_D$
are forgetful maps sending
$(\mathcal{O}\to F)$
to F. Let
$\bar{f}_Y:=f_Y\times_{\operatorname{id}_{{\mathcal A}}} \operatorname{id}_{{\mathcal Y}}$
, and
be the projections. The embedding
$i:{\mathcal D}\hookrightarrow {\mathcal Y}$
induces
$\bar{i}: M_{\mathrm{cpt}}({\mathcal Y}/{\mathcal A})\times_{{\mathcal A}} {\mathcal D}\hookrightarrow M_{\mathrm{cpt}}({\mathcal Y}/{\mathcal A})\times_{{\mathcal A}} {\mathcal Y}$
. Let
${\mathbb F}$
be the universal sheaf on
$M_{\mathrm{cpt}}({\mathcal Y}/{\mathcal A})\times_{{\mathcal A}} {\mathcal Y}$
and
${\mathbb I}=(\mathcal{O}_{\operatorname{{Hilb}}(Y,D)\times_{{\mathcal A}} {\mathcal Y}}\to \bar{f}_Y^*{\mathbb F})$
be the universal pair. As in (4.4), we have
Consider the natural projection and the inclusion of a divisor:
We have the commutative diagram

where
$\pi_{\dagger}$
denotes the pushforward map from
${\mathcal Y}$
to
${\mathcal U}$
by
$\pi$
and
$j_{\dagger}$
denotes the pullback map from
${\mathcal U}$
to
${\mathcal S}$
by j. Note that we have
where
${\mathbb F}_U\to M_{\mathrm{cpt}}({\mathcal U}/{\mathcal A})\times_{{\mathcal A}} {\mathcal U}$
is the universal object of the moduli stack
$M_{\mathrm{cpt}}({\mathcal U}/{\mathcal A})$
of compactly supported sheaves on
${\mathcal U}/{\mathcal A}$
(which are normal to
${\mathcal S}$
) and
${\mathbb F}_S\to M_{\mathrm{cpt}}({\mathcal S}/{\mathcal A})\times_{{\mathcal A}} {\mathcal S}$
is the universal object of the moduli stack
$M_{\mathrm{cpt}}({\mathcal S}/{\mathcal A})=M_{\mathrm{cpt}}(S)\times {\mathcal A}$
of compactly supported sheaves on
$(S\times{\mathcal A})/{\mathcal A}$
.
As with (4.9), by using Serre duality and diagrams (4.16) and (4.17), we obtain
Combining (4.15) and (4.18), we obtain
\begin{equation}\det({\mathbb T}_{\mathbf{Hilb}(Y,D)/{\mathcal A}}|_{\operatorname{{Hilb}}(Y,D)})\cong \frac{f_Y^*\det(\pi_{M_Y*} \bar{i}_*\bar{i}^*{\mathbb F})}{f_Y^*\pi_{\dagger}^*j_{\dagger}^*\det(\pi_{M_S*}\mathbf{R}{\mathcal H} om({\mathbb F}_S,{\mathbb F}_S))}. \end{equation}
Consider the projection and the embedding:
We have a commutative diagram

where
$p_{\dagger}$
is the pushforward of sheaves via p and r is the restriction map via i. As in (4.17), we have
where
${\mathbb F}_D$
(respectively
${\mathbb F}_S$
) is the universal sheaf on
$M_{\mathrm{cpt}}({\mathcal D}/{\mathcal A})\times_{{\mathcal A}}{\mathcal D}$
(respectively on
$M_{\mathrm{cpt}}({\mathcal S}/{\mathcal A})\times_{{\mathcal A}}{\mathcal S}$
).
As in (4.15) and (4.18), with
$f_D$
defined in diagram (4.14), we have

where the second isomorphism is derived as in (4.8). We define
Then, (4.22) provides an isomorphism
Finally, we compute
$r_{{\mathcal D}\to {\mathcal Y}}^*K^{-1/2}_{\operatorname{{Hilb}}(D)}$
:

where the last equality is by base change along the following Cartesian diagram.

Comparing with (4.19), we conclude that
It is straightforward to show that this provides a relative orientation.
The case of
$\operatorname{{Hilb}}^P(Y,D)\to \operatorname{{Hilb}}^{P|_D}(D)\times {\mathcal A}^P$
is similar, by replacing
${\mathcal Y}^{}/{\mathcal A}$
in the above by
${\mathcal Y}^{P}/{\mathcal A}^{P}$
.
Remark 4.7. We have isomorphisms

which is written using data purely on S.
4.3 Orientation on
$(\operatorname{{Hilb}}(Y,D)\to W\times {\mathcal A}) $
Definition 4.8. Let S be a quasi-projective surface and
$D=\operatorname{Tot}(\omega_S)$
, and fix
$P_D\in K_{c,\leqslant 2}^\mathrm{{num}}(D)$
. A Lagrangian fibration
is S-compatible if the line bundle (4.25) satisfies
where p also denotes its classical truncation by an abuse of notation.
Recall from Proposition 3.8 that the composition map
has a (relative)
$(-2)$
-shifted symplectic structure. By an abuse of notation, we denote its classical truncation by
Proposition 4.9.
Let (U,S) be a smooth pair (Definition 2.1) with
$\dim_{\mathbb{C}} U=3$
and
If p is the S-compatible Lagrangian fibration given in Definition 4.8, then the map
$p\circ r_{{\mathcal D}\to {\mathcal Y}}$
has an orientation in the sense of Definition 4.1.
Proof. The diagram

induces a fiber sequence
Therefore
\begin{align*}\det{\mathbb L}_{p\circ r_{{\mathcal D}\to {\mathcal Y}}}&\cong r_{{\mathcal D}\to {\mathcal Y}}^*\det {\mathbb L}_{p}\otimes \det{\mathbb L}_{r_{{\mathcal D}\to {\mathcal Y}}} \\&\cong r_{{\mathcal D}\to {\mathcal Y}}^*\bigg(\frac{\det {\mathbb L}_{\mathbf{Hilb}^{P|_D}(D)\times {\mathcal A}^{P}}}{p^*\det {\mathbb L}_{W\times {\mathcal A}^{P}}}\bigg)\otimes\bigg(\frac{\det {\mathbb L}_{\mathbf{Hilb}^{P}(Y,D)}}{r_{{\mathcal D}\to {\mathcal Y}}^*\det({\mathbb L}_{\mathbf{Hilb}^{P|_D}(D)\times {\mathcal A}^{P}})}\bigg) \\&\cong \frac{\det {\mathbb L}_{\mathbf{Hilb}^{P}(Y,D)}}{r_{{\mathcal D}\to {\mathcal Y}}^*p^*\det {\mathbb L}_{W\times {\mathcal A}^{P}}} \cong \frac{\det {\mathbb L}_{\mathbf{Hilb}^{P}(Y,D)/{\mathcal A}^{P}}}{r_{{\mathcal D}\to {\mathcal Y}}^*p^*\det {\mathbb L}_{(W\times {\mathcal A}^{P})/{\mathcal A}^{P}}}.\end{align*}
By (4.24) in Theorem 4.6 and Definition 4.8, we know that
which can be checked to be an orientation.
Remark 4.10. In this remark, we explain how to construct a canonical orientation on
$p\circ r_{{\mathcal D}\to {\mathcal Y}}$
.
Let (Y,D) be the log Calabi–Yau pair given by (4.27) and
be the universal expanded pair over the stack
${\mathcal A}$
of expanded pairs. Denote by
$\textbf{M}_{\mathrm{cpt}}(-)$
the derived moduli stack of compactly supported sheaves on
$(-)={\mathcal Y}/{\mathcal A}$
,
${\mathcal U}/{\mathcal A}$
,
${\mathcal D}/{\mathcal A}$
,
${\mathcal S}/{\mathcal A}$
. Then we have a pushforward map
and a restriction map
Note that
$\textbf{M}_{\mathrm{cpt}}({\mathcal D}/{\mathcal A})$
is the
$({-}1)$
-shifted cotangent bundle of
$\textbf{M}_{\mathrm{cpt}}({\mathcal S}/{\mathcal A})$
over
${\mathcal A}$
:
with projection
As in Theorem 3.3, the map r has a Lagrangian structure (over
${\mathcal A}$
). By [Reference CalaqueCal19, Theorem 2.2],
$p_\dagger$
has a Lagrangian fibration structure (over
${\mathcal A}$
). Therefore the composed map
has a
$(-2)$
-shifted symplectic structure (Lemma 3.7). In particular, there is an isomorphism
As in (4.6), there is a fiber sequence
which is self-dual under the pairing (4.28). Its restriction to the classical truncation
$M_{\mathrm{cpt}}({\mathcal Y}/{\mathcal A})$
provides a canonical isomorphism:
Define
$\mathbb{V}:=\pi_\dagger^*{\mathbb T}_{\textbf{M}_{\mathrm{cpt}}({\mathcal U}/{\mathcal A})/\textbf{M}_{\mathrm{cpt}}({\mathcal S}/{\mathcal A})}|_{M_{\mathrm{cpt}}({\mathcal Y}/{\mathcal A})}$
. As in Remark 4.4, we choose
as the canonical choice of orientation on
$M_{\mathrm{cpt}}({\mathcal Y}/{\mathcal A}) \to M_{\mathrm{cpt}}({\mathcal S}/{\mathcal A})$
.
There is a forgetful map
By comparing (4.15), (4.18), (4.22), (4.23) and using (4.26), the above canonical orientation on
induces a canonical orientation on
We give examples in which (4.26) in Definition 4.8 is satisfied.
Example 4.11. Consider the smooth pair
where the associated log Calabi–Yau pair is
By Example 3.10, we have an inclusion into the non-commutative Hilbert scheme:
Then (4.26) holds, i.e.
$p^*\det({\mathbb T}_W)\cong K^{-1/2}_{\operatorname{{Hilb}}^n(D)}$
for the square root
$K^{-1/2}_{\operatorname{{Hilb}}^n(D)}$
in (4.23). Therefore
has an orientation by Proposition 4.9.
Proof. As
$S=\mathbb{C}^2$
is symplectic, we have that
is the determinant of the tautological bundle of
$\operatorname{{Hilb}}^n(D)$
. By (3.19), we have
where the right-hand side (RHS) is written as a
$\operatorname{GL}(n)$
-equivariant complex. Then
where the RHS is the determinant of the tautological bundle. After restricting to
$\operatorname{{Hilb}}^n(D)$
, we know that (4.31) and (4.32) are isomorphic.
5. Relative invariants and degeneration formulae
We recall the general theory of virtual pullbacks [Reference ParkPar21] arising from
$(-2)$
-shifted symplectic structures, and then apply this to our setting to define relative invariants and family invariants. Finally we prove a degeneration formula relating relative and family invariants.
5.1 Virtual pullback via symmetric obstruction theory
Definition 5.1 [Reference ParkPar21, Proposition 1.7, § A.2]. A symmetric complex
${\mathbb E}$
on an algebraic stack
${\mathcal X}$
consists of the following data:
-
(1) a perfect complex
${\mathbb E}$
of tor-amplitude
$[-2,0]$
on
${\mathcal X}$
; -
(2) a non-degenerate symmetric form
$\theta$
on
${\mathbb E}$
, i.e. a morphism in the derived category of
\begin{align*}\theta : {\mathcal O}_{{\mathcal X}} \to ({\mathbb E} \otimes{\mathbb E})[-2]\end{align*}
${\mathcal X}$
, invariant under the transposition
$\sigma : {\mathbb E} \otimes {\mathbb E} \to {\mathbb E} \otimes {\mathbb E}$
, with the induced map
$\iota_{\theta} : {\mathbb E}^\vee\to{\mathbb E}[-2]$
being an isomorphism;
-
(3) an orientation o of
${\mathbb E}$
, i.e. an isomorphism
$o:{\mathcal O}_{\mathcal X} \to \det({\mathbb E})$
of line bundles such that
$\det(\iota_\theta)=o\circ o^\vee$
.
For a symmetric complex
${\mathbb E}$
, there is a quadratic function [Reference ParkPar21, § A.2] from the virtual normal cone
$\frak{C}_{{\mathbb E}}$
of
${\mathbb E}$
,
characterized by some naturality conditions.
Definition 5.2 [Reference ParkPar21, Definition 1.9, § A.2]. A symmetric obstruction theory for a Deligne–Mumford morphism
$f : {\mathcal X}\to {\mathcal Y}$
between algebraic stacks is a morphism
$\phi : {\mathbb E} \to {\mathbf L}_f$
in the derived category of
${\mathcal X}$
such that:
-
(1)
${\mathbb E}$
is a symmetric complex; and -
(2)
$\phi$
is an obstruction theory in the sense of Behrend and Fantechi [Reference Behrend and FantechiBF97], i.e.
$h^0(\phi)$
is an isomorphism and
$h^{-1}(\phi)$
is surjective, where
${\mathbf L}_f := \tau^{\geqslant -1}{\mathbb L}_f$
is the truncated cotangent complex.
The obstruction theory
$\phi$
induces a closed embedding of the intrinsic normal cone
Definition 5.3. A symmetric obstruction theory
$\phi : {\mathbb E} \to {\mathbf L}_f$
is isotropic if the intrinsic normal cone
$\frak{C}_f$
is isotropic in the virtual normal cone
$\frak{C}_{{\mathbb E}}$
, i.e. the restriction
$\frak{q}_{{\mathbb E}}|_{\frak{C}_f}: \frak{C}_f\hookrightarrow \frak{C}_{{\mathbb E}}\to {\mathbb A}^1$
vanishes.
Isotropic symmetric obstruction theory implies the existence of square root virtual pullback which we now briefly recall. For a symmetric complex
${\mathbb E}$
on an algebraic stack
${\mathcal X}$
, let
$\frak{Q}({\mathbb E})$
be the zero locus of the quadratic function
$\frak{q}_{{\mathbb E}}:\frak{C}_{\mathbb E}\to {\mathbb A}^1_{\mathcal X}$
. There is a square root Gysin pullback [Reference ParkPar21, Definition A.2]
if
${\mathcal X}$
is a quotient of a separated Deligne–Mumford stack by an algebraic group.
Definition 5.4. Assume that
$f:{\mathcal X}\to{\mathcal Y}$
is a Deligne–Mumford morphism between algebraic stacks with an isotropic symmetric obstruction theory
$\phi:{\mathbb E}\to{\mathbf L}_f$
. It induces a closed embedding
$a:\frak{C}_f\to \frak{Q}({\mathbb E})$
. The square root virtual pullback is the composition
where
$sp_f:A_*({\mathcal Y})\to A_*(\frak{C}_f)$
is the specialization map [Reference ManolacheMan12, Construction 3.6].
The map
$\sqrt{f^!}$
commutes with projective pushforwards, smooth pullbacks, and Gysin pullbacks for regular immersions and can be used to define the square root virtual pullback for any base change of f (e.g. [Reference ParkPar21, Equation (1.14)]). Moreover, it has a functoriality with respect to morphisms compatible with symmetric obstruction theories [Reference ParkPar21, Theorem A.4] as explained below.
Let
$f:{\mathcal X}\to{\mathcal Y}$
be a Deligne–Mumford (DM) morphism of algebraic stacks having reductive stabilizer groups and affine diagonals,Footnote
13
which are satisfied if
${\mathcal X}$
and
${\mathcal Y}$
are quotient stacks of separated DM stacks by algebraic tori. Let
$g:{\mathcal Y}\to{\mathcal Z}$
be a DM morphism of algebraic stacks. Assume
$\phi_g:{\mathbb E}_g\to {\mathbf L}_g$
,
$\phi_{g\circ f}:{\mathbb E}_{g\circ f}\to {\mathbf L}_{g\circ f}$
are isotropic symmetric obstruction theories,
$\phi_f:{\mathbb E}_f\to {\mathbf L}_f$
is a perfect obstruction theory [Reference Behrend and FantechiBF97] and they are compatible, i.e. there exists a perfect complex
${\mathbb D}$
and morphisms
$\alpha:{\mathbb E}_{g\circ f}\to {\mathbb D}$
and
$\beta:f^*{\mathbb E}_g\to {\mathbb D}$
fitting into the diagram of exact triangles

where the orientation of
${\mathbb E}_{g\circ f}$
is compatible with the orientation of
${\mathbb E}_{g}$
[Reference ParkPar21, Definition 2.1]. Here
$\phi_{g\circ f}=\phi_{g\circ f}'\circ\alpha$
,
$\phi_f=r\circ \phi'_f$
with
${\mathbf L}'_f$
is the cone of
$\tau^{\geqslant -1}f^*{\mathbf L}_g\to{\mathbf L}_{g\circ f}$
and
$r:{\mathbf L}'_f\to {\mathbf L}_f$
the truncation. Then we have
where
$f^!$
is the virtual pullback of Manolache [Reference ManolacheMan12]. In the presence of a torus action, the above extends to the torus equivariant setting.
5.2 Relative invariants
Let (Y,D) be a smooth log Calabi–Yau pair (Definition 2.4) so that D is a Calabi–Yau 3-fold. Fixing a K-theory class
$P\in K_{c, \leqslant 2}^{\mathrm{num}, } (Y)$
, we have a restriction map (3.7):
which has a Lagrangian structure (Theorem 3.3).
In this section, we work under the following assumption.
Assumption 5.5. We assume that there is a quasi-projective smooth scheme W, and a regular functionFootnote
14
$\phi$
on W, such that there is an equivalence
of the
$({-}1)$
-shifted symplectic derived scheme.
Under the above assumption, the composition (where p denotes the inclusion deduced by (5.6))
has a
$(-2)$
-shifted symplectic structure (Proposition 3.8).
Restricting the cotangent complex of
$p\circ r_{{\mathcal D}\to {\mathcal Y}}$
to the classical truncation, which, by an abuse of notation, we still write as
we get a canonical symmetric obstruction theory in the sense of Definition 5.2:
By the footnote to Assumption 5.5, we have
$\operatorname{Crit}(\phi)\subseteq Z(\phi)$
. By the construction,
$p\circ r_{{\mathcal D}\to {\mathcal Y}}$
factors through
$\operatorname{Crit}(\phi)$
. Therefore we obtain the following Cartesian diagram of classical stacks.

Hence we can pull back (5.8) to the upper line and get a canonical symmetric obstruction theory
The following isotropic result will be proven in Appendix C.
Proposition 5.6.
The symmetric obstruction theory (5.9) is isotropic in the sense of Definition 5.3 if
$P\in K_{c, \leqslant 1}^{\mathrm{num}} (Y)$
.
Therefore, we have the following theorem.
Theorem 5.7.
Let
$P\in K_{c,\leqslant 1}^{\mathrm{num}} (Y)$
. Assume that Assumption 5.5 holds and the classical truncation of (5.7) has an orientation. Then there is a square root virtual pullback
which satisfies the usual bivariance properties and functoriality spelled out in § 5.1.
Given a smooth pair (Definition 2.1) (U,S) with
$\dim_{\mathbb{C}} U=3$
, let
be the (associated) log Calabi–Yau 4-fold pair. Recall the line bundle
$K^{-1/2}_{\operatorname{{Hilb}}^{P|_D}(D)}$
(4.25).
Assumption 5.8. Given
$\mathbf{Hilb}^{P|_D}(D)\cong \textbf{Crit}(\phi:W\to \mathbb{C})$
as in Assumption 5.5, we assume that
By Proposition 4.9, the classical truncation of (5.7) then has an orientation in the sense of Definition 4.1 and we choose the canonical orientation as specified in Remark 4.10.
Definition 5.9. Let
$Y=\operatorname{Tot}(\omega_{U}(S))$
,
$D=\operatorname{Tot}(\omega_S)$
be as above. Fix a K-theory class
$P \in K_{c,\leqslant 1}^\mathrm{{num}} (Y)$
. Under Assumption 5.8, we define relative invariants:
where
$\boxtimes$
is the exterior product
5.3 Family invariants
Let
$\pi : X \to {\mathbb A}^1$
be a simple degeneration of Calabi–Yau 4-folds. Fixing K-theory classes
$P_t\in K_{c, \leqslant 2}^{\mathrm{num}}(X_t)$
for all
$t\in \mathbb{A}^1$
, the map
has a (relative)
$(-2)$
-shifted symplectic structure (Theorem 3.2). By restricting the cotangent complex of
$\mathbf{Hilb}^{P_t}(X/{\mathbb A}^1)/{\mathcal C}^{P_t}$
to the classical truncation, we obtain a canonical symmetric obstruction theory
The following isotropic result will be proven in Appendix C.
Proposition 5.11.
The symmetric obstruction theory (5.13) is isotropic in the sense of Definition 5.3 if
$P_t\in K_{c, \leqslant 1}^{\mathrm{num}} (X_t)$
for all
$t\in \mathbb{A}^1$
.
Remark 5.12. Here we restrict to curves/points classes on Calabi–Yau 4-folds. One can consider surface classes and other cases by a more detailed study of Hodge filtrations as in [Reference Bae, Kool and ParkBKP22, Remark 5.2].
Therefore, we have the following theorem.
Theorem 5.13.
Fix K-theory classes
$P_t \in K_{c,\leqslant 1}^\mathrm{{num}} (X_t)$
for all
$t\in \mathbb{A}^1$
and assume that the classical truncation of (5.12) has an orientation. Then there is a square root virtual pullback
which satisfies the usual bivariance properties and functoriality spelled out in § 5.1.
Let
$U\to {\mathbb A}^1$
be a simple degeneration of 3-folds and
be the associated simple degeneration of Calabi–Yau 4-folds. By Theorem 4.3, the classical truncation of (5.12) has an orientation in the sense of Definition 4.1. We choose the canonical orientation as specified in Remark 4.4.
Definition 5.14. Let
$X=\operatorname{Tot}(\omega_{U/{\mathbb A}^1})\to {\mathbb A}^1$
be as above. Given K-theory classes
$P_t \in K_{c,\leqslant 1}^\mathrm{{num}} (X_t)$
for all
$t\in {\mathbb A}^1$
, we define family invariants:
Remark 5.15. When there is a torus T acting on the family
$U\to {\mathbb A}^1$
, it naturally induces an action on
$X\to {\mathbb A}^1$
preserving Calabi–Yau volume forms on fibers, and the above pullback map (5.15) lifts to a map between T-equivariant Chow groups (where the T-action on
${\mathcal C}^{P_t}$
is trivial).
5.4 Degeneration formulae
In this section, we will relate relative invariants (Definition 5.9) of
$(Y_\pm,D)$
and family invariants (Definition 5.14) of
$X/ {\mathbb A}^1$
in a degeneration formula. We work in the following setting.
Setting 5.16.
Let
$U\to {\mathbb A}^1$
be a simple degeneration of 3-folds (Definition 2.6) with central fiber
$U_0=U_+\cup_S U_-$
. Consider
This is a CY simple degeneration (Definition 2.10) whose fiber satisfies:
-
–
$X_c=\operatorname{Tot}(\omega_{U_c})$
if
$c\neq 0$
; and
-
–
$X_0=Y_+\cup_D Y_-$
, where
$Y_{\pm}=\operatorname{Tot}(\omega_{U_\pm}(S))$
and
$D=\operatorname{Tot}(\omega_S)$
.
Data 5.17. In Setting 5.16 with Assumption 5.8, assume there is an automorphism
which preserves fibers of
$X\to {\mathbb A}^1$
and also
$Y_{\pm}$
, D in
$X_0$
, and there is an automorphism
on the W in (5.6) such that:
-
–
$\sigma^{*}\phi=-\phi$
; -
– the induced automorphism
$(\bar{\sigma}|_{D})_*: \operatorname{{Hilb}}^{P_D}(D)\to \operatorname{{Hilb}}^{P_D}(D)$
coincides with
$\sigma|_{\operatorname{{Hilb}}^{P_D}(D)}$
.
Example 5.18. As
$X=\operatorname{Tot}(\omega_{U/{\mathbb A}^1})$
, we can choose the order two element in the
$\mathbb{C}^*$
-action on fibers of
$X\to U$
as a candidate for
$\bar{\sigma}$
(5.16). We refer to [Reference Cao and ZhaoCZ26, Remark 4.18] for the choice of automorphism (5.17) in examples given by quivers with potentials. In particular, in Example 3.10, we can take
where the third coordinate corresponds to the fiber of
$\mathbb{C}^3=D\to S=\mathbb{C}^2$
. Then
$\sigma$
is homotopic to the identity map and compatible with
$\bar{\sigma}$
as required in Data 5.17.
We define the sum function
\begin{align*}\boxplus^n \phi: W^n\to \mathbb{C}, \quad (x_1,x_2,\ldots,x_n)\mapsto \sum_{i=1}^n\phi(x_i), \end{align*}
and denote by
$Z(\boxplus^n \phi)$
its zero locus.
Consider the diagonal embedding
and the anti-diagonal embedding
We have the commutativity of the diagrams

where the automorphism
is induced by the automorphism (5.17). The bottom square commutes because automorphisms
$\sigma$
and
$\bar{\sigma}$
are compatible in Data 5.17. where the map
$r_{{\mathcal D}\to {\mathcal Y}_-}\times r_{{\mathcal D}\to {\mathcal Y}_+}$
goes to
$\operatorname{{Hilb}}^{P_D}(D) \times \operatorname{{Hilb}}^{P_D}(D)$
(where
$P_D=P_-|_D=P_+|_D$
) and we omit the natural inclusion
in the above diagram. By diagram chasing along (5.19), we obtain the following lemma.
Lemma 5.19.
There is a canonical isomorphism
$\bar{\sigma}$
making the following diagram commutative.

Recalling the notions in § 2.4, we get the following Cartesian diagrams.

Using the shorthand
diagram (5.19) and Lemma 5.19 lead to the commutative diagram

where the lower square is Cartesian. Here
$ev_\Delta$
is the composition of the restriction map (at the common divisor) and the embedding
$\operatorname{Crit}(\phi)\hookrightarrow W$
.
By Theorem 5.13, the map
$\pi$
in diagram (5.21) admits a square root virtual pullback whose base change (via diagrams (5.21) and (5.22)) defines
$\sqrt{(\pi_{\mathrm{node}}\times\operatorname{id}_W)^!}$
. As in Theorem 5.7, the map
$r_{{\mathcal D}\to {\mathcal Y}_+}\times r_{{\mathcal D}\to {\mathcal Y}_-}$
in diagram (5.19) admits a square root virtual pullback (see also (5.33)) whose base change defines
$\sqrt{r_{\bar{\Delta}}^!}$
. The map
$\operatorname{id}_{{\mathcal H}}\times ev_\Delta$
is a regular embedding [Reference VistoliVis89, Definition 1.20], [Reference FultonFul98, Appendix B.7.3], so there is a Gysin pullback
$(\operatorname{id}_{{\mathcal H}}\times ev_\Delta)^!$
.
We have the following compatibility between the above pullbacks.
Proposition 5.20. Using the notation above, we have
Proof. The proof follows the same approach as the proof of [Reference Cao and ZhaoCZ26, Proposition 4.22]. It is enough to construct diagram (5.3) for the maps
As
$\bar{\sigma}$
is an isomorphism, one is reduced to construct diagram (5.3) for maps
Consider the derived enhancement of diagram (5.21)

where
$\mathbf{Hilb}^{P_t} (X/{\mathbb A}^1)$
is defined using diagram (3.2) and
$\mathbf{Hilb}^{(P_-, P_+)} (X/{\mathbb A}^1)_0^\dagger $
is defined by the above homotopy pullback diagram. Further homotopy pullback via diagram (5.22) defines a derived enhancement of
$h:=\pi_{\mathrm{node}}\times\operatorname{id}_W$
. Let
${\mathbb E}_h$
be the restriction of the derived cotangent complex to its classical truncation, then we obtain a symmetric obstruction theory (since
$\pi$
has a symmetric obstruction theory by Theorem 5.13):
Consider two derived enhancements of
$g:=r_{\Delta}$
. One of them is constructed via the following derived enhancement of part of diagram (5.19).

The restriction of the cotangent complex of
$\bf r_{\Delta}$
to the classical truncation gives rise to a symmetric obstruction theory
The other derived enhancement of
$g=r_{\Delta}$
is given by the following homotopy pullback diagram.

These two derived enhancements are related by the commutative diagram of derived stacks

where
$\iota$
is induced by the inclusion
$p:\mathbf{Hilb}^{P_- |_D}(D)\to W$
. The classical truncation of
$\bf j$
induces an isomorphism of classical stacks
\begin{align*}& t_0(\mathbf{Hilb}^{P_-}(Y_-,D)\times_{\mathbf{Hilb}^{P_-|_D}(D)}\mathbf{Hilb}^{P_+}(Y_+,D) )\\&\quad\cong t_0(\mathbf{Hilb}^{P_-}(Y_-,D)\times_{\Delta(W)} \mathbf{Hilb}^{P_+}(Y_+,D) )={\mathcal H}, \end{align*}
because the (classical) restriction map already lies in
$\operatorname{{Hilb}}^{P_- |_D}(D)$
.
By Lemma 5.21, we have the following commutative diagram.

Restricting the cotangent complexes to the classical truncations and using the fact that
$t_0(\textbf{r})$
is an isomorphism and
${\mathbb L}_{\bf e\circ \bf r}|_{\mathcal{H}}\cong {\mathbb L}_{\bf e}|_{\mathcal{H}}$
, we obtain the commutativity of the lower 3-by-3 block in (5.28). The middle column of (5.28) is given by the classical truncation of the cotangent complexes of (5.26). The commutativity of the other parts of (5.28) is a direct calculation, similar to the proof of [Reference Cao and ZhaoCZ26, Proposition 4.22].

The above diagram gives diagram (5.3) for the maps
One can check that the orientations chosen in Remarks 4.4 and 4.10 induce compatible orientations of
${\mathbb E}_g$
and
${\mathbb E}_h$
in diagram (5.28), as mentioned in § 5.1.
Finally notice that we have
where
${\mathbb E}_{r_{\bar{\Delta}}}$
is the symmetric obstruction theory used to define
$\sqrt{r_{\bar{\Delta}}^!}$
. Here the last isomorphism is due to the following commutative diagram of derived stack.

Considering the pullback of (5.28) by the map
$\bar{\sigma}$
, we obtain the desired diagram (5.3) for maps
$(\operatorname{id}_{{\mathcal H}}\times ev_\Delta)\circ \bar{\sigma}$
,
$(\pi_{\mathrm{node}}\times\operatorname{id}_W)$
,
$r_{\bar{\Delta}}$
. Therefore we are done.
Lemma 5.21.
Let
$\mathbf{Hilb}^{(P_-, P_+)} (X/{\mathbb A}^1)_0^\dagger$
and
$\mathbf{Hilb}^{P_-}(Y_-,D)\times_{\mathbf{Hilb}^{P_-|_D}(D)} \mathbf{Hilb}^{P_+}(Y_+,D)$
be the derived stacks defined by diagrams (5.23) and (5.25), respectively. Then there is an isomorphism of derived stacks
Proof. Consider the homotopy pushout diagram of derived stacks

whose classical truncation recovers the following isomorphism (refer to Equation (2.13)):
As the inclusion functor preserves colimits, so it preserves pushout diagrams, and we have
So we obtain an isomorphism of derived stacks
Using as shorthand
${\mathcal A}_{P}:={\mathcal A}^{P_-}\times {\mathcal A}^{P_+}$
and applying
$\textbf{Map}_{\mathrm{dst}/{\mathcal A}_{P}}(-,\textbf{RPerf}\times {\mathcal A}_{P})$
to diagram (5.30), we obtain a homotopy pullback diagram.

For any derived stack T over a base stack S, base change implies a canonical equivalence:
where
$\bullet_T=\bullet\times_ST$
. Combined with diagram (5.32), we obtain
\begin{align}& \textbf{Map}_{\mathrm{dst}/{\mathcal A}_{P}}({\mathcal X}_{0,\mathrm{der}}^{\dagger, (P_-, P_+)},\textbf{RPerf}\times {\mathcal A}_{P})\nonumber\\&\quad \cong \textbf{Map}_{\mathrm{dst}/{\mathcal A}^{P_-}}( {\mathcal Y}_-^{P_-},\textbf{RPerf}\times {\mathcal A}^{P_-})\times_{\textbf{Map}_{\mathrm{dst}/\text{pt}}( D,\textbf{RPerf})} \textbf{Map}_{\mathrm{dst}/{\mathcal A}^{P_+}}({\mathcal Y}_+^{\circ, P_+},\textbf{RPerf} \times_{} {\mathcal A}^{P_+} ).\end{align}
In (5.31) and (5.33), by fixing the determinant using diagram (3.1) and restricting to the open (relative) Hilbert substacks (3.2) and (3.6), we obtain the desired isomorphism
$\textbf{r}$
of (5.29).
Recalling Lemma 2.25 and Proposition 2.26, we have the following commutative diagram.

In a similar way to
$\Phi^{P_\pm}_{Y_\pm,D}$
(5.11), under Assumption 5.8, we define
Recall also that the base change of (5.35) defines
$\sqrt{r_{\bar{\Delta}}^!}$
in the above diagram.
Now we are ready to state our degeneration formula in the cycle version. In the below, we denote by
$[\operatorname{{Hilb}}^{P_r} (X_r)]^{\mathrm{vir}}$
the virtual class of
$\operatorname{{Hilb}}^{P_r} (X_r)$
for a smooth Calabi–Yau 4-fold
$X_r$
(
$r\neq 0$
) with choice of orientation given by the restriction of the orientation in Remark 4.4 to the fiber of
$\pi$
.
Theorem 5.22.
Let
$X\to {\mathbb A}^1$
be as given in Setting 5.16 and
$P_t\in K_{c,\leqslant 1}^\mathrm{{num}} (X_t)$
for all
$t\in \mathbb{A}^1$
. Let
$\Phi^{P_t}_{X/{\mathbb A}^1}$
be the family invariant (5.15) and
$\Phi^{P_-}_{Y_-,D}\otimes\Phi^{P_+}_{Y_+,D}$
be defined as in (5.35) under Assumption 5.8. Then
\begin{align*}i_r^!(\Phi^{P_t}_{X/{\mathbb A}^1}[{\mathcal C}^{P_t}])&=[\operatorname{{Hilb}}^{P_r} (X_r)]^{\mathrm{vir}}, \quad \forall\,\,r\in \mathbb{A}^1\backslash \{0\},\\i_{0}^!(\Phi^{P_t}_{X/{\mathbb A}^1}[{\mathcal C}^{P_t}])&= n_*\,\sum_{(P_-, P_+)\in \Lambda^{P_0}_{\rm spl}}i_{(P_-, P_+)}^!(\Phi^{P_t}_{X/{\mathbb A}^1}[{\mathcal C}^{P_t}]), \end{align*}
where n is the normalization map in (5.21). For each
$(P_-, P_+)$
, we have
where
$\bar{\sigma}$
is the automorphism in Data 5.17. Moreover, we have
Furthermore, in the presence of a torus action, the above equalities hold in equivariant Chow groups.
Proof. The first equality is by the base change property of square root virtual pullbacks [Reference ParkPar21, Proposition 1.15, Definition A.3]. A similar base change implies that

Recall that
$\sqrt{r_{\bar{\Delta}}^!}$
is defined by the base change of (5.35) via anti-diagonal embedding, and therefore
Finally, we have

In the special case when W in Assumption 5.8 is a point, the inclusions
$i_{\bar{\Delta}}$
,
$\bar{\Delta}$
and the automorphism
$\bar{\sigma}$
in Theorem 5.22 are identities, and therefore we have the following.
Corollary 5.23.
Let
$X\to {\mathbb A}^1$
be as given in Setting 5.16 and
$P_t\in K_{c,\leqslant 1}^\mathrm{{num}} (X_t)$
for all
$t\in \mathbb{A}^1$
. Assume that for any splitting datum
$(P_-,P_+)$
of
$P_0$
, we have
$\mathbf{Hilb}^{P_-|_D}(D)=\operatorname{{Spec}} \mathbb{C}$
. Then we have
\begin{align*}i_0^!(\Phi^{P_t}_{X/{\mathbb A}^1}[{\mathcal C}^{P_t}])=n_*\sum_{(P_-, P_+)\in \Lambda^{P_0}_{\rm spl}} \Phi^{P_-}_{Y_-,D}\otimes\Phi^{P_+}_{Y_+,D} \,[{\mathcal C}_0^{\dagger, (P_-, P_+)}]. \end{align*}
Moreover, in the presence of a torus action, the above equalities hold in equivariant Chow groups.
When we consider (relative) Hilbert stacks of points on
$X/\mathbb{A}^1$
and
$(Y_{\pm},D)$
, the above assumption holds. In particular, using (5.11), we define
In the following section, we will use the above degeneration formula (and a variant of it) to calculate tautological integrals on
$[\operatorname{{Hilb}}^{P_r} (X_r)]^{\mathrm{vir}}$
(
$r\neq 0$
) when
$X_r$
is
$\mathbb{C}^4$
or a local curve
$\operatorname{Tot}_C (L_1 \oplus L_2 \oplus L_3)$
.
6. Applications to Hilbert schemes of points
In this section, we study equivariant
$\mathop{\rm DT}\nolimits_4$
theory for Hilbert schemes of points on (log) Calabi–Yau 4-folds. As an application of our degeneration formula, we compute tautological integrals on virtual classes
$[\operatorname{{Hilb}}^n(\mathbb{C}^4)]^{\mathrm{vir}}$
and prove the conjectural formula proposed in [Reference Cao and KoolCK18]. We also compute zero-dimensional (relative)
$\mathop{\rm DT}\nolimits_4$
invariants for all local curves.
6.1 Virtual classes of
$\operatorname{{Hilb}}^n(\mathbb{C}^4)$
Consider
${\mathbb C}^4$
with torus action by
$({\mathbb C}^*)^4$
,
and also the three-dimensional CY subtorus
The ring of equivariant parameters is
As the T-fixed locus of
$\operatorname{{Hilb}}^n ({\mathbb C}^4)$
is proper [Reference Cao and KoolCK18, Lemma 3.1], the Hilbert scheme
$\operatorname{{Hilb}}^n ({\mathbb C}^4)$
of n points admits a T-equivariant virtual class [Reference Oh and ThomasOT23]
which depends on the choice of orientation [Reference Cao, Gross and JoyceCGJ20]. As
$\operatorname{{Hilb}}^n ({\mathbb C}^4)$
is connected [Reference FogartyFog68, Proposition 2.3], reversing an orientation affects the virtual class by a minus sign.
To fix the orientation of virtual classes, we fix a presentation of
$\mathbb{C}^4$
(refer to Theorem 4.3) as
and then use the convention specified by Remark 4.4. Here
$\mathbb{C}^3_{x_1,x_2,x_3}$
denotes the first three coordinate planes of
$\mathbb{C}^4_{x_1,x_2,x_3,x_4}$
.
6.2 Tautological insertions
Let
$L\in \mathop{\rm Pic}\nolimits^{(\mathbb{C}^*)^4}(\mathbb{C}^4)$
be a
$(\mathbb{C}^*)^4$
-equivariant line bundle on
$\mathbb{C}^4$
. The tautological rank n bundle of L is
where
$\pi_M: \operatorname{{Hilb}}^n(\mathbb{C}^4)\times \mathbb{C}^4\to \operatorname{{Hilb}}^n(\mathbb{C}^4)$
and
$\pi_X: \operatorname{{Hilb}}^n(\mathbb{C}^4)\times \mathbb{C}^4\to \mathbb{C}^4$
are projections and
$\mathcal{Z}\hookrightarrow \operatorname{{Hilb}}^n(\mathbb{C}^4)\times \mathbb{C}^4$
is the universal subscheme.
As in [Reference Cao, Kool and MonavariCKM22a], we take an extra one-dimensional torus
${\mathbb C}^*_m$
acting trivially on
$\mathbb{C}^4$
(and also on
$\operatorname{{Hilb}}^n(\mathbb{C}^4)$
), and let
denote the trivial line bundle on
$\mathbb{C}^4$
with
${\mathbb C}^*_m$
-equivariant weight m, and its tautological bundle.
Definition 6.1. Choose the orientation on
$\operatorname{{Hilb}}^n(\mathbb{C}^4)$
(
$n\geqslant 1$
) as specified by Equation (6.2) and Remark 4.4. We define the generating function of
$(T \times {\mathbb C}^*_m)$
-equivariant zero-dimensional
$\mathop{\rm DT}\nolimits_4$
invariants with tautological insertions,
\begin{align*} Z_{} ({\mathbb C}^4) :=1+\sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^n ({\mathbb C}^4)]_T^\mathrm{vir}} e_{T \times {\mathbb C}^*_m }(L_m^{[n]}),\end{align*}
which lies in
$(\operatorname{Frac} H^*_{T} (\text{pt}) \otimes H^*_{{\mathbb C}^*_m} (\text{pt}) ) [\![q]\!] \cong {\mathbb C} (s_1, s_2, s_3 )[m] [\![ q ]\!]$
, where q is the degree-counting parameter.
Remark 6.2. As
${\mathbb C}^*_m$
acts trivially on
${\mathbb C}^4$
, virtual normal bundles appearing in localization formulae of
$\operatorname{{Hilb}}^n ({\mathbb C}^4)$
do not involve m, and hence the coefficients of the above generating series are polynomials in m.
If we assign parameters with gradings as
the generating function
$ Z({\mathbb C}^4)$
will be homogeneous of degree 0.
6.3 Relative and rubber geometry
In the approach of [Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06b], zero-dimensional
$\mathop{\rm DT}\nolimits_3$
invariants are computed via the relative
$\mathop{\rm DT}\nolimits_3$
invariants of
$( {\mathbb P}^1 \times {\mathbb C}^2, \{\infty\} \times {\mathbb C}^2)$
. The naive four-dimensional analogue
$( {\mathbb P}^1 \times {\mathbb C}^3, \{\infty\} \times {\mathbb C}^3)$
does not have a well-defined
$\mathop{\rm DT}\nolimits_4$
analogy, as it fails to be (log)
$\mathrm{CY}_4$
. Instead, using the constructions in § 5.2 and their rubber analogue, we study T-equivariant versions of the following invariants (more basics about rubber theory are recalled in Appendix A).
-
(1)
$\mathop{\rm DT}\nolimits_4$
invariants of
$(X, D_\infty)$
, where and
\begin{align*}X = X_{-1, 0, 0} := \operatorname{Tot} ({\mathcal O}_{{\mathbb P}^1} ({-}1) \oplus {\mathcal O}_{{\mathbb P}^1} \oplus {\mathcal O}_{{\mathbb P}^1}), \quad D_\infty := \{\infty\} \times {\mathbb C}^3,\end{align*}
$({\mathbb C}^*)^4$
acts on X with the following tangent weights at fixed points: We take a three-dimensional subtorus
\begin{align*}\text{at } 0: \,\,\, -s_1, -s_2, -s_3, -s_4; \quad\text{at } \infty: \,\,\,s_1, -(s_2 + s_1), -s_3, -s_4.\end{align*}
$T\subset ({\mathbb C}^*)^4$
as follows. Recall that X can be constructed as
$ ({\mathbb C}^2 \backslash \{0\} ) \times_{{\mathbb C}^*} {\mathbb C}^3$
, where
${\mathbb C}^*$
acts on
${\mathbb C}^3$
by weights
$(-1, 0, 0)$
. Then we takeFootnote
15
where the second
\begin{align*}T = ({\mathbb C}^*)^2 \times_{{\mathbb C}^*} ({\mathbb C}^*)^2, \end{align*}
$({\mathbb C}^*)^2 \subset ({\mathbb C}^*)^3$
is the CY torus on
${\mathbb C}^3$
. In other words, T is a twisted product of the
${\mathbb C}^*$
on
${\mathbb P}^1$
and the CY torus on the fiber
${\mathbb C}^3$
. Equivariant parameters for T are given by the condition
\begin{align*}s_1 + s_2 + s_3 + s_4 = 0. \end{align*}
-
(2)
$\mathop{\rm DT}\nolimits_4$
invariants of
$(\Delta, D_0 \sqcup D_\infty)$
, where and
\begin{align*}\Delta = X_{0,0, 0} := {\mathbb P}^1 \times {\mathbb C}^3, \quad D_0 := \{0\} \times {\mathbb C}^3,\quad D_\infty := \{\infty\} \times {\mathbb C}^3,\end{align*}
$({\mathbb C}^*)^4$
acts on
$\Delta$
with tangent weights
$\mp s_1, -s_2, -s_3, -s_4$
at 0 and
$\infty$
. As before, we take where the second factor is the CY torus on
\begin{align*}T ={\mathbb C}^* \times ({\mathbb C}^*)^2, \end{align*}
$\mathbb{C}^3$
. The equivariant parameters of the CY torus T are given by the equation
\begin{align*}s_2 + s_3 + s_4 = 0.\end{align*}
-
(3) Rubber invariants of
$(\Delta, D_0 \sqcup D_\infty)$
, where the
${\mathbb C}^*$
-action on
${\mathbb P}^1$
is considered as an automorphism in the relative Hilbert stack. In this case, is the CY torus on the fiber
\begin{align*}T = ({\mathbb C}^*)^2\end{align*}
$\mathbb{C}^3$
, whose equivariant parameters satisfy
\begin{align*}s_2 + s_3 + s_4 = 0. \end{align*}
To fix the orientation of virtual classes, we need to fix the presentation of the log Calabi–Yau pair (refer to Theorem 4.6 Footnote 16 ) as
and then use the convention specified by Remark 4.10. In the above three cases, we fix
\begin{align}&\text{(1):}\,\, U= \operatorname{Tot} ({\mathcal O}_{{\mathbb P}^1} ({-}1)\oplus {\mathcal O}_{{\mathbb P}^1}), S= \{\infty\} \times {\mathbb C}^2_{x_2,x_3};\nonumber\\& \text{(2) and (3):}\,\, U= {\mathbb P}^1 \times {\mathbb C}^2_{x_2,x_3}, S= \{0,\infty\} \times {\mathbb C}^2_{x_2,x_3},\end{align}
where
$\mathbb{C}^2_{x_2,x_3}$
denotes the first two coordinate planes of
$\mathbb{C}^3_{x_2,x_3,x_4}$
.
As in Definition 6.1, we define relative invariants in the above geometries.
Definition 6.3. Choose the orientation specified by Equation (6.5) and Remark 4.10. We define generating functions of those relative
$\mathop{\rm DT}\nolimits_4$
invariants with tautological insertions by:
-
(1)
$(X, D_\infty)$
: where
\begin{align*}Z (X, D_\infty):=1+\sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^n (X, D_\infty)]_T^\mathrm{vir}} e_{T \times {\mathbb C}^*_m }(L_m^{[n]}), \end{align*}
$[\operatorname{{Hilb}}^n (X, D_\infty)]_T^\mathrm{vir}$
is the T-equivariant virtual class (5.37);
-
(2)
$(\Delta, D_0 \sqcup D_\infty)$
: where
\begin{align*}Z (\Delta, D_0 \sqcup D_\infty):=1+\sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^n (\Delta, D_0 \sqcup D_\infty)]_T^\mathrm{vir}} e_{T \times {\mathbb C}^*_m }(L_m^{[n]}), \end{align*}
$[\operatorname{{Hilb}}^n (\Delta, D_0 \sqcup D_\infty)]_T^\mathrm{vir}$
is the T-equivariant virtual class (5.37); and
-
(3) rubber theory for
$(\Delta, D_0 \sqcup D_\infty)$
: where
\begin{align*}Z^\sim (\Delta, D_0 \sqcup D_\infty):=1+\sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^{\sim, n} (\Delta ,D_0 \sqcup D_\infty )]_T^\mathrm{vir}} e_{T \times {\mathbb C}^*_m }(L_m^{[n]}), \end{align*}
$[\operatorname{{Hilb}}^{\sim, n} (\Delta ,D_0 \sqcup D_\infty )]_T^\mathrm{vir}$
is the rubber T-equivariant virtual class (Definition A.1).
We follow [Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06b] to compute these invariants.
Lemma 6.4.
The q-coefficients of
$Z (X, D_\infty)$
only have poles in monomials of
$s_2, s_1 + s_2, s_3, s_1+s_2 + s_3$
.
Proof. There is a projective map
where
$\operatorname{Tot} ({\mathcal O}_{{\mathbb P}^1} ({-}1) ) \to {\mathbb C}^2$
is the blowup of
${\mathbb C}^2$
at the origin. With our convention of T-action,
$\pi$
is T-equivariant if T acts on
${\mathbb C}^2 \times {\mathbb C}^2$
with tangent weights
$-s_2, -(s_1+s_2), -s_3, -s_4 = (s_1 + s_2 + s_3)$
.
The rest of the argument is the same as [Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06b, Lemma 3]. The Hilbert–Chow morphism, together with the contraction of bubbles, yields a proper and T-equivariant map
\begin{align*}\operatorname{{Hilb}}^n (X, D_\infty) \to \operatorname{Sym}^n X \to \operatorname{Sym}^n {\mathbb C}^4 \to \bigoplus_{i=1}^n {\mathbb C}^4,\end{align*}
where the last map is
The lemma then follows by pushing forward the virtual class to
$\bigoplus_{i=1}^n {\mathbb C}^4$
.
Lemma 6.5.
Let
$\psi_0 = \psi_0 ({\mathcal A}^{\sim})$
be the cotangent line bundle class introduced in Definition A.4,
where
\begin{equation}W_{\infty} := 1 + \sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^{\sim, n} (\Delta, D_0 \sqcup D_\infty)]_T^\mathrm{vir}}\frac{e_{T \times {\mathbb C}^*_m }(L_m^{[n]})}{s_1 - \psi_0 }.\end{equation}
Proof. This is standard (cf. [Reference Graber and VakilGV05]). Consider the subtorus
By
${\mathbb C}^*$
-localization, we have
The result then follows from a comparison of obstruction theories, where the denominator
$s_1 - \psi_0$
comes from splitting the node.
For
$l\geqslant 0$
, we introduce
\begin{align}F_{\infty, l }:=& \sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^{\sim, n} (\Delta, D_0 \sqcup D_\infty)]_T^\mathrm{vir}} e_{T \times {\mathbb C}^*_m }(L_m^{[n]}) \cdot \psi_0^l \\ \nonumber& \in {\operatorname{Frac}} \bigg( \frac{{\mathbb C} [s_1 + s_2 , s_3,s_4] }{ (s_1 + s_2 + s_3 + s_4) } \bigg) \otimes H^*_{{\mathbb C}^*_m} (\text{pt}) [\![q]\!] \cong {\mathbb C} (s_1 + s_2, s_3) [m] [\![q]\!] .\end{align}
Note that here, for the rubber theory, the bubble components
$\Delta$
come from the chart of X containing
$D_\infty$
, where the torus on the fiber has equivariant weights
$-(s_1 + s_2), -s_3, -s_4$
.
Lemma 6.6.
We have
$\log W_{\infty} = {1}/{s_1} F_{\infty,0}$
.
Proof. This is similar to [Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06b, Lemma 4]. Consider the universal substack
which is flat and finite of degree n over
$\operatorname{{Hilb}}^{\sim, n} (\Delta, D_0 \sqcup D_\infty)$
. We define
For
$l\geqslant 1$
, the projection formula implies that
\begin{align*}q \frac{d}{dq} F_{\infty, l}&= \sum_{n=1}^\infty q^n \int_{ [{\mathcal Z}^{\sim, n}]^\mathrm{vir}}\pi_{{\mathcal Z}^\sim}^*e_{T \times {\mathbb C}^*_m }(L_m^{[n]}) \cdot \pi_{{\mathcal Z}^\sim}^* \psi_0^l \\&= \sum_{n=1}^\infty q^n \int_{ [{\mathcal Z}^{\sim, n}]^\mathrm{vir}}\pi_{{\mathcal Z}^\sim}^*e_{T \times {\mathbb C}^*_m }(L_m^{[n]}) \cdot \pi^* \psi_0^l \\&= \sum_{n=1}^\infty q^n \int_{[{\mathcal Z}^{\sim, n}]^\mathrm{vir}} \pi_{{\mathcal Z}^\sim}^*e_{T \times {\mathbb C}^*_m }(L_m^{[n]}) \cdot \pi^* \psi_0^{l-1} \cdot \psi_0 ({\mathcal R}^\sim),\end{align*}
where
$\psi_0$
is the tautological psi-class on
$\operatorname{{Hilb}}^{\sim, n} (\Delta, D_0 \sqcup D_\infty)$
, pulled back from
$\psi_0({\mathcal A}^\sim)$
, and
$\psi_0 ({\mathcal R}^\sim)$
is the tautological psi-class on the universal family
$\pi: {\mathcal R}^\sim \to {\mathcal A}^\sim$
(see Remark A.6). The last identity follows from
which holds in the zero-dimensional case, since, base changed over
${\mathcal Z}^\sim$
, the universal section
$\Sigma_1$
is always disjoint from the relative divisor
$D_0$
.
For any
$l\geqslant 1$
, we have
\begin{align} q \frac{d}{dq} F_{\infty, l} &= \sum_{n=1}^\infty q^n \int_{ [{\mathcal Z}^{\sim, n}]^\mathrm{vir}} \pi_{{\mathcal Z}^\sim}^*e_{T \times {\mathbb C}^*_m }(L_m^{[n]}) \cdot \pi^* \psi_0^{l-1} \cdot \psi_0 ({\mathcal R}^\sim) \nonumber\\& = \sum_{n=1}^\infty q^n \sum_{\begin{subarray}{c}n_- + n_+ = n \\ n_-,n_+\gt0 \end{subarray} } \int_{ [\operatorname{{Hilb}}^{\sim, n_-} (\Delta, D_0 \sqcup D_\infty) ]_T^\mathrm{vir} } e_{T \times {\mathbb C}^*_m }(L_m^{[n_-]}) \cdot \psi_0^{l-1} \cdot \int_{ [{\mathcal Z}^{\sim, n_+} ]^\mathrm{vir}}\pi_{{\mathcal Z}^\sim}^*e_{T \times {\mathbb C}^*_m }(L_m^{[n_+]})\nonumber \\& = F_{\infty, l-1} \cdot q \frac{d}{dq} F_{\infty, 0}.\end{align}
In the second equality, we use the decomposition
where a similar argument as in Corollary 5.23 shows that the virtual classes coincide. We also use the splitting (according to the above isomorphism)
Note that
$\psi_0^{l-1}$
is distributed to the left integral as the marked point 0 is given from
$\operatorname{{Hilb}}^{\sim, n_-}(\Delta, D_0 \sqcup D_\infty)$
, and
$n_-,n_+$
in the above are positive by Remark A.2.
Solving (6.9), we obtain
By expanding the RHS of (6.7) and using the above equation, we obtain
\begin{equation*}W_{\infty}=1 + \sum_{l=0}^\infty \frac{F_{\infty,l}}{s_1^{l+1}}=1 + \sum_{l=0}^\infty\frac{F_{\infty,0}^{l+1}}{(l+1)!s_1^{l+1}}=\exp\bigg(\frac{F_{\infty, 0}}{s_1}\bigg). \end{equation*}
6.4 Zero-dimensional
$\mathop{\rm DT}\nolimits_4$
invariants of
${\mathbb C}^4$
Lemma 6.7.
For
$n\geqslant 1$
,
$\int_{[\operatorname{{Hilb}}^n ({\mathbb C}^4)]_T^\mathrm{vir}} e_{T \times {\mathbb C}^*_m} (L_m^{[n]})$
is divisible by m.
Proof. By the vertex formalism [Reference Cao and KoolCK18, Proposition 3.17],
can be written as a summation over solid partitions
$\pi$
of size n. Let
$\pi = \{\pi_{ijk}\}_{i, j, k\geqslant 1}$
be a solid partition ([Reference Cao and KoolCK18, Definition 3.3]), and Z be the T-fixed point in
$\operatorname{{Hilb}}^n ({\mathbb C}^4)$
corresponding to
$\pi$
. Then the contribution from the tautological insertion is
where
\begin{align*}H^0 ({\mathbb C}^4, \mathcal{O}_Z)\otimes e^m= \sum_{i, j, k\geqslant 1} \sum_{l=1}^{\pi_{ijk} } e^m t_1^{ i-1} t_2^{j-1} t_3^{k-1} t_4^{l-1}.\end{align*}
In particular, if
$n\geqslant 1$
, the solid partition
$\pi$
must contain the box with
$(i,j,k,l) = (1,1,1,1)$
. Therefore,
$H^0 ({\mathbb C}^4, \mathcal{O}_Z)\otimes e^m=e^m+\cdots$
, which contributes to a factor m in
$e_{T \times {\mathbb C}^*_m} (L_m^{[n]}|_Z)$
.
Theorem 6.8. With the canonical choice of orientation (in Definition 6.1),
where
is the MacMahon function and
$\int_{\mathbb{C}^4}$
denotes equivariant pushforward to a point.
As a consequence, for any
$L\in \mathop{\rm Pic}\nolimits^{(\mathbb{C}^*)^4}(\mathbb{C}^4)$
, we have
\begin{align*}1+ \sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^n ({\mathbb C}^4)]_T^\mathrm{vir}}e_T(L^{[n]}) = M(q)^{\int_{\mathbb{C}^4} c^T_3(\mathbb{C}^4)\cdot c^T_1(L)},\end{align*}
i.e. [Reference Cao and KoolCK18, Conjecture 1.6] holds on
$\mathbb{C}^4$
.
Proof. Identity (6.6) implies that
By Lemma 6.4,
$\log Z (X, D_\infty)$
only has poles in monomials of
$s_2, s_1 + s_2, s_3, s_1+s_2 + s_3$
. By Lemma 6.6 and Equation (6.8),
has a simple pole at
$s_1$
and the coefficients of
$F_{\infty, 0}$
are rational functions in
$s_1+s_2, s_3$
.
Combining with Lemma 6.7, we know that the
$q^n$
-coefficients (
$n\geqslant 1$
) of
$\log Z ({\mathbb C}^4)$
must be of the form (after applying
$s_4 = -s_1 - s_2 - s_3$
):
where
$a,b,c\in \mathbb{Z}$
are integers (possibly depending on n), and
$P_n$
and
$Q_n$
are homogeneous polynomials, such that (6.10) is homogeneous of degree 0. We may also assume that
$P_n$
and
$Q_n$
are not divisible by
$s_1, s_2, s_3, s_1 + s_2 + s_3$
.
By symmetry, we have
for some invariant function
$F \in \mathbb{C} (s_1, s_2, s_3, s_4,q)^{S_4}$
, where
$S_4$
is the symmetric group of
$s_1, s_2, s_3, s_4$
. In particular,
$Z(\mathbb{C}^4)$
is symmetric in
$s_1, s_2, s_3$
, and hence the order of poles at
$s_1, s_2, s_3$
are the same. Therefore
$a = b = 1$
. As symmetric rational functions are quotients of symmetric polynomials, we may further assume that
$P_n$
and
$Q_n$
are symmetric in
$s_1, s_2, s_3$
.
Since
$Q_n (s_1 + s_2, s_3)$
is symmetric in
$s_1, s_2, s_3$
, we have
By setting
$s_3 = 0$
, we see that the 2-variable polynomial
$Q_n (x,y)$
satisfies
which implies that
$Q_n (s_1+ s_2, s_3) = Q_n (s_1 + s_2 + s_3, 0)$
. By homogeneity, we have
However,
$Q_n(s_1 + s_2, s_3)$
is not divisible by
$s_1 + s_2 + s_3$
by assumption, so it must be a constant.
By the
$S_4$
-invariance, the function F is invariant under
By investigating the order of
$s_1$
and
$-s_1 -s_2 -s_3$
, we know
$c=1$
. After applying
$s_4 = -s_1 - s_2 - s_3$
, (6.10) is of the form
where the polynomials
$f_i$
are symmetric in
$s_1,s_2,s_3,s_4$
(depending on n) and homogeneous of degree
$4-i$
(so that the expression is homogeneous of degree 0 by the convention in Remark 6.2).
It follows that
\begin{align*}f_1 (s_1, s_2, s_3, s_4) &= a_3 \, e_3 (s) + a_{2,1} \, e_2 (s)\, e_1(s) + a_{1,1,1} \, e_1 (s)^3,\\ f_2 (s_1, s_2, s_3, s_4) &= a_2 \, e_2 (s) + a_{1,1} \, e_1(s)^2,\\f_3 (s_1, s_2, s_3, s_4) &= a_1 \, e_1 (s), \quad f_4 (s_1, s_2, s_3, s_4) = a_0,\end{align*}
for some
$a_3, a_{2,1}, a_{1,1,1}, a_2, a_{1,1}, a_1, a_0 \in {\mathbb C}$
and
are the elementary symmetric polynomials.
Under the CY condition
$s_1 + s_2 + s_3 + s_4 = 0$
, we have that
$e_1(s)=0$
, and thus we may take
Therefore (6.10) must be of the form
Note that
$a_3, a_2, a_0$
actually also depend on n, which we omit to avoid cumbersome notation. Summing over n, we conclude that there exists some
$g_3 (q) , g_2 (q), g_0 (q) \in q\cdot {\mathbb C}[\![q]\!]$
such that
To determine the formula, by taking
$m=-s_4 =s_1 + s_2 + s_3$
(refer to [Reference Cao and KoolCK18, Lemma 3.14]), we specialize to the case when
$L = {\mathcal O}\otimes t_4^{-1}$
, i.e. the line bundle associated to the smooth
$({\mathbb C}^*)^4$
-invariant divisor
$D=\mathbb{C}^3\subset \mathbb{C}^4$
cut out by
$x_4=0$
. This case has been calculated by 4-fold vertex in [Reference Cao and KoolCK18, Theorem 1.7]. To be precise, the invariant in [Reference Cao and KoolCK18, Theorem 1.7] is defined at the level of the torus fixed locus (i.e. solid partitions). It is related to our globally defined invariant by torus localization formula [Reference Oh and ThomasOT23], with the sign rule proven in [Reference Kool and RennemoKR25]. By Proposition B.2 and the sign rule in [Reference Kool and RennemoKR25], we know that, for torus fixed zero-dimensional subschemes which are scheme theoretically supported on D, we can take the 4-fold vertex (with the induced sign) to be the same as the 3-fold vertex given in [Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06a] up to a sign
$({-}1)^n$
depending on the number n of points. For other torus fixed subschemes, their contributions to the invariants are zero by [Reference Cao and KoolCK18, Equation (3.8)].
Let
$\bar e_k(s_1, s_2, s_3)$
be the specialization
which is a homogeneous polynomial in
$s_1, s_2, s_3$
of degree k. Then we have
By the MNOP formula [Reference Maulik, Nekrasov, Okounkov and PandharipandeMNO+06a], (6.11) is equal to
By expanding (6.11) using
$s_4 = - s_1 - s_2 - s_3$
and comparing with the above formula, we conclude that
The theorem then follows from the identity
where
$s_4 = - s_1 - s_2 - s_3$
.
By a similar degeneration argument or directly applying a specialization argument (e.g. [Reference Cao, Kool and MonavariCKM22a, Appendix A], [Reference Cao, Kool and MonavariCKM23, § 6.2]), we can obtain the following invariants without insertions, which confirms a conjecture of Nekrasov [Reference Cao and KoolCK18, Conjecture B.1].
Corollary 6.9. We have
\begin{equation*} 1+\sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^n({\mathbb C}^4)]_T^\mathrm{vir}} 1 = \exp \bigg[{-}\frac{(s_1 + s_2 )(s_1 + s_3) (s_2 + s_3) }{s_1 s_2 s_3 (s_1 + s_2 + s_3) } q \bigg]. \end{equation*}
We can also extract relative and rubber invariants from a similar pole analysis.
Corollary 6.10. We have:
-
(1)
$\displaystyle W_{\infty} =M(q)^{{m }/{s_1}}$
; and -
(2)
$\displaystyle Z (X, D_\infty) = M(q)^{- ({m (s_2 s_3 + s_3 s_4 + s_2 s_4 ) })/{ s_2 s_3 s_4} }$
.
Proof. The second equation follows from the first equation, Equation (6.6) and Theorem 6.8. We prove the first one. We have
where
$\log Z (X, D_\infty)$
only has poles in monomials of
$s_2, s_1 + s_2, s_3, s_1+s_2 + s_3$
(Lemma 6.4). Therefore,
$-F_{\infty, 0}$
is the residue of
$\log Z({\mathbb C}^4)$
at
$s_1$
, which is
$-m \log M(q)$
.
This corollary allows us to compute relative tautological invariants on
for topologically nontrivial line bundle (i.e. not just
$L_m=\mathcal{O} \otimes e^m$
). Consider a
$({\mathbb C}^*)^4 \times {\mathbb C}^*_m$
-equivariant line bundle
such that
In other words, L[l] is an equivariant enhancement of the pullback of the line bundle
${\mathcal O}_{{\mathbb P}^1} (-l)$
to X.
As in Definition 6.3, we define
\begin{align*}Z_{L[l]} (X, D_\infty):=1+\sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^n (X, D_\infty)]_T^\mathrm{vir}} e_{T \times {\mathbb C}^*_m }(L[l]^{[n]}). \end{align*}
Corollary 6.11.
We have
$Z_{L[l]} (X, D_\infty) = Z_{} (X, D_\infty) \cdot M(q)^l$
.
Proof. Similarly to (6.6), we have
where
\begin{align*}W_{\infty,t_1^l \cdot e^m} := 1 + \sum_{n=1}^\infty q^n \int_{[\operatorname{{Hilb}}^{\sim, n} (\Delta, D_0 \sqcup D_\infty)]_T^\mathrm{vir}}\frac{e_{T \times {\mathbb C}^*_m }(\mathcal{O}^{[n]}\otimes t_1^l\cdot e^m)}{s_1 - \psi_0} \end{align*}
is defined in a similar way to (6.7). Then the conclusion follows from Corollary 6.10(1) and (6.6).
6.5 Zero-dimensional
$\mathop{\rm DT}\nolimits_4$
invariants of log CY local curves
Let C be a smooth connected projective curve of genus g, and
$L_1$
,
$L_2$
,
$L_3$
be line bundles on C. Consider the smooth quasi-projective 4-fold
Let
$p_1, \ldots, p_r \in C$
be r distinct points and
$D_i := \{p_i\} \times {\mathbb C}^3$
be the fibers over
$p_i$
in X, which we will take as relative divisors. We impose the (log) CY condition:
which implies that
\begin{equation}D:=\bigsqcup_{i=1}^r D_i \end{equation}
is an anti-canonical divisor of X and
Let
$({\mathbb C}^*)^3$
be the torus acting on the fibers of
$X\to C$
, with CY subtorus
The ring of equivariant parameters is
Let L be a line bundle on C. By an abuse of notation, we still denote its pullback to X by L. Let
${\mathbb C}^*_m$
be an extra one-dimensional torus acting trivially on X and Hilbert schemes on X. Consider the
${\mathbb C}^*_m$
-equivariant line bundle on X,
with
$\mathbb{C}^*_m$
-weight set to be m. The T-fixed locus of
$\operatorname{{Hilb}}^n (X, \bigsqcup_{i=1}^r D_i)$
is proper (Remark 2.23), and its virtual class can be defined as in the previous sections.
To fix the orientation of virtual classes, we need to fix the presentation of the log Calabi–Yau pair (refer to Theorem 4.6) as
\begin{align*}\bigg(\!X,\bigsqcup_{i=1}^rD_i\!\bigg)=(\operatorname{Tot}(\omega_{U}(S)),\operatorname{Tot}(\omega_S)), \end{align*}
and then use the convention specified by Remark 4.10. Here we take
\begin{equation}U=\operatorname{Tot}_C(L_1\oplus L_2), \quad S= \bigsqcup_{i=1}^r\{p_i\}\times \mathbb{C}^2_{x_2,x_3}.\end{equation}
Definition 6.12. Choose the orientation specified by Equation (6.16) and Remark 4.10. The
$(T \times {\mathbb C}^*_m)$
-equivariant relative
$\mathop{\rm DT}\nolimits_4$
generating function of
$(X, \bigsqcup_{i=1}^r D_i)$
with tautological insertions is
\begin{align*} Z \bigg(\!X, \bigsqcup_{i=1}^r D_i; L_m\!\bigg) :=1+\sum_{n=1}^\infty q^n \int_{[ \operatorname{{Hilb}}^n (X, \bigsqcup_{i=1}^r D_i) ]^\mathrm{vir}_T } e_{T \times {\mathbb C}^*_m} (L_m^{[n]}) \in \frac{{\mathbb C} (s_2, s_3, s_4 )}{(s_2 + s_3 + s_4)}[m] [\![ q ]\!].\end{align*}
Our approach to compute
$ Z (X, \bigsqcup_{i=1}^r D_i; L_m)$
is an analogue of the application of the degeneration formula in the 3-fold case [Reference Bryan and PandharipandeBP05, Reference Bryan and PandharipandeBP08, Reference Okounkov and PandharipandeOP10b]. Consider a simple degeneration of the curve C into a union
where the line bundles
$L_i$
(
$1\leqslant i\leqslant 3$
) and L degenerate to
$L_i^\pm$
and
$L^\pm$
on
$C_\pm$
. The topological data are required to satisfy
We define
Let
$p_1, \ldots, p_{r_-}$
be the points that degenerate into
$C_-$
, and
$p_{r_- +1}, \ldots, p_{r_- + r_+}$
be those degenerating into
$C_+$
, where
$r_- + r_+ = r$
.
$Y_\pm$
then carries the corresponding divisors
$D_i$
. The node p also introduces an extra divisor
$D_p^\pm$
on
$Y_\pm$
. We require Equation (6.14) also to hold for
$Y_\pm$
.
The degeneration formula, i.e. Corollary 5.23, implies that
\begin{align*} Z \bigg(\!X, \bigsqcup_{i=1}^r D_i; L_m\!\bigg) = Z\bigg(\!Y_-, \bigsqcup_{i=1}^{r_-} D_i \sqcup D_p^- ; L^-_m\!\bigg) \cdot Z\bigg(\!Y_+, \bigsqcup_{i=r_- +1}^{r} D_i \sqcup D_p^+ ; L^+_m\!\bigg),\end{align*}
where the orientation on the RHS is chosen as in Definition 6.12.
Definition 6.13. For a smooth divisor
$D \subset X$
, let
$\Omega_X[D]$
denoteFootnote
17
the locally free sheaf of 1-forms on X with logarithmic poles along D and let
$T_X[-D]$
be its dual sheaf of tangent vectors with logarithmic zeros along D.
Example 6.14. For the divisor D in
${\mathbb C}^4$
defined by
$x_1 = 0$
,
$T_{{\mathbb C}^4}[-D]$
is generated by tangent vectors
$x_1 \partial_{x_1}$
and
$\partial_{x_i}$
(
$2\leqslant i\leqslant 4$
). As
$({\mathbb C}^*)^4$
-representations, we have
In particular,
$c_3 (T_{{\mathbb C}^4}[-D]) = -s_2 s_3 s_4$
.
Lemma 6.15.
Let
$D:= \bigsqcup_{i=1}^r D_i$
. Then
Proof. Recall that L is the pullback of a line bundle from C. By T-localization, we have
Then the result follows from the short exact sequence
\begin{align*}0 \to L_1 \oplus L_2 \oplus L_3 \to T_X[-D] |_C \to T_C\bigg({-}\sum_{i=1}^r p_i\! \bigg) \to 0,\end{align*}
and a direct calculation.
Now we state our main theorem on zero-dimensional
$\mathop{\rm DT}\nolimits_4$
invariants for any log CY local curve.
Theorem 6.16.
Let X be a local curve (6.12),
$\bigsqcup_{i=1}^r D_i$
(6.13) be its anti-canonical divisor and
$L_m$
be the line bundle (6.15). Then
\begin{align*}Z \bigg(\!X, \bigsqcup_{i=1}^r D_i; L_m\!\bigg) = M(q)^{\int_X c_1^{T \times {\mathbb C}^*_m} (L_m) \cdot c_3^T (T_X[-D])},\end{align*}
where
$M(q):=\prod_{n\geqslant 1}{1}/({(1-q^n)^n})$
is the MacMahon function, and
$T_X[-D]$
is given in Definition 6.13.
Proof. The moduli space of complex structures on a curve C and the Picard groups of line bundles on C with fixed degrees are connected. The equivariant Euler class of the tautological bundle of
$L_m$
depends only on the degree of L by the Grothendieck–Riemann–Roch theorem. With the orientation chosen canonically in Definition 6.12, our generating function is deformation invariant and hence depends only on the data g,
$\deg L_i$
,
$\deg L$
and r; we denote this by
\begin{align*} Z (g; l_1, l_2, l_3; l):=Z \bigg(\!X, \bigsqcup_{i=1}^r D_i; L_m\!\bigg),\end{align*}
where
$l_i := \deg L_i$
,
$l:= \deg L$
, and r is determined by Equation (6.14). The degeneration formula implies
where the relations between all the topological data are given in (6.17). Therefore the invariants for
$g\geqslant 1$
can be reduced to products of invariants on
$g =1$
. As for a
$g=1$
curve C, we can consider a degeneration of C into
$C_- \cup_{\{p, p'\}} C_+$
, where
$C_\pm \cong {\mathbb P}^1$
, and hence the invariants can then be further reduced to the
$g=0$
case.
On the other hand, Lemma 6.15 shows that the RHS of the theorem also satisfies a similar gluing formula. Hence, it suffices to prove the theorem for
$g=0$
.
The formula (6.19) for
$(0; 0, 0, 0; 0)$
is
which implies that
$Z (0; 0, 0, 0; 0) = 1$
, and hence
Combining with a further decomposition of the
$l_i$
and l using (6.19), it suffices to prove the theorem for the following four cases:
In the first case, the theorem reduces to Corollary 6.10 and Lemma 6.15. The second and third cases should follow from the first case by symmetry, but one must be careful about the choice of orientation: by the orientation convention (6.16) and the invariance of Corollary 6.10 (2) under variable change
$s_2\leftrightarrow s_3$
, we know the second case follows from the first case. As for the third case, we can redo § 6.3 by using the orientation fixed by presenting the log Calabi–Yau pairs in Definition 6.3 as (6.4) with
in each individual case (compared with the previous choice given in (6.5)). Since the formula of Theorem 6.8 (and therefore also Corollary 6.10 (2)) is invariant under the permutation
$(s_1,s_2,s_3,s_4)\to (s_1,s_3,s_4,s_2)$
, this case can also be reduced to the first case.
The last case
$(0; -1, 0, 0; 1)$
follows from Corollary 6.11 and Lemma 6.15. The theorem is therefore proved.
Appendix A. Rubber moduli stacks
A very useful variant of the construction in §§ 2.1 and 2.2 is the rubber moduli stacks (refer to [Reference Okounkov and PandharipandeOP10b, §§ 4.8 and 4.9]). We briefly describe their construction here, focusing on moduli of zero-dimensional subschemes. With a view toward the applications in § 6, we consider only the following case:
-
–
$D=\operatorname{Tot}(\omega_S)$
for a smooth surface S, with a torus T-action on D which preserves the Calabi–Yau volume form on D.
A.1 Rubber expanded pairs
Let
$\Delta:= D \times {\mathbb P}^1$
, whichFootnote
18
comes with two canonical divisors
$D_0 = D\times \{0\}$
and
$D_\infty := D \times \{\infty\}$
. As in Proposition 2.7, for each
$k\in{\mathbb N}$
, there is a standard family
$\Delta[k] \to {\mathbb A}^k$
, whose central fiber is
The standard families for the different k fit together. The family
$\Delta[k] \to {\mathbb A}^k$
is
$({\mathbb C}^*)^{k+1}$
-equivariant. Together with the discrete symmetries containing permutations of the coordinates, we obtain a smooth equivalence relation
$\sim$
. The difference between this setting and that in § 2.1 is that here we also turn on the
$\mathbb{C}^*$
-action on the first
$\Delta$
in
$\Delta[k]_0$
.
We are primarily interested in Hilbert stacks of points, where the topological data are of the form
with
$\text{pt} \in D$
a closed point. In numerical K-theory, the class
$[{\mathcal O}_{\text{pt}}]$
is independent of the choice of
$\text{pt}\in D$
by the connectedness of D. The transversality condition then forces
$P_- |_D = 0$
and
$\operatorname{{Hilb}}^{P_- |_D} (D) = \operatorname{{Spec}} \mathbb{C}$
. In what follows, we denote the topological datum by n instead of
$n [{\mathcal O}_{\text{pt}}]$
.
Analogous to Definitions 2.3 and 2.18, we have the following.
Definition A.1 Let Y, D,
$\Delta$
be as above, and
$n \geqslant 0$
be an integer.
-
– The stack of rubber expanded pairs is defined as
It is a smooth Artin stack of dimension
\begin{align*}{\mathcal A}^\sim := \underrightarrow\lim\, [{\mathbb A}^k / \sim].\end{align*}
$-1$
. As before, we denote by
${\mathcal A}^{\sim, n}$
the stack of rubber expanded pairs with total continuous weight
$P=n [{\mathcal O}_{\text{pt}}] $
.
-
– The rubber universal family is defined as
Similarly, let
\begin{align*}{\mathcal R}^\sim := \underrightarrow\lim\, [\Delta[k] / \sim]. \end{align*}
${\mathcal R}^{\sim, n}$
be the universal family over
${\mathcal A}^{\sim, n}$
.
-
– Consider closed subschemes on the stack of rubber expanded pairs (and with total continuous weight n), whose dimensions relative to the base are 0. Denote the corresponding rubber relative Hilbert stacks (and the weighted version) by
\begin{align*}\operatorname{{Hilb}}^\sim (\Delta, D_0 \sqcup D_\infty), \quad (\operatorname{{Hilb}}^{\sim, n} (\Delta, D_0 \sqcup D_\infty)). \end{align*}
-
– All the constructions in § 5.2 carry through in a straightforward way for rubber relative Hilbert stacks. In particular, we have a rubber analogue to Theorem 5.7 for the rubber relative Hilbert stack of zero-dimensional subschemes. The map
admits a canonical (T-equivariant) isotropic symmetric obstruction theory in sense of Definition 5.2. Hence, with orientation specified by Equation (6.5) and Remark 4.4, there is a (T-equivariant) square root virtual pullback
\begin{align*}r_{{\mathcal D}\to {\mathcal R}^\sim} : \operatorname{{Hilb}}^{\sim, n} (\Delta, D_0 \sqcup D_\infty) \to {\mathcal A}^{\sim, n}\end{align*}
The rubber T-equivariant virtual class is
\begin{align*}\Phi^{\sim, n}_{(\Delta ,D_0 \sqcup D_\infty )} := \sqrt{ r_{{\mathcal D}\to {\mathcal R}^\sim}^!} : A_{*}({\mathcal A}^{\sim, n}) \to A_*^T(\operatorname{{Hilb}}^{\sim, n} (\Delta ,D_0 \sqcup D_\infty )).\end{align*}
\begin{align*}[\operatorname{{Hilb}}^{\sim, n} (\Delta ,D_0 \sqcup D_\infty )]_T^\mathrm{vir} := \Phi^{\sim, n}_{(\Delta ,D_0 \sqcup D_\infty )} [{\mathcal A}^{\sim, n}]. \end{align*}
Remark A.2. As the
${\mathbb C}^*$
-action is turned on, we need
$n\geqslant 1$
to have nonempty Hilbert stacks.
As observed by Graber and Vakil [Reference Graber and VakilGV05] (see also [Reference Abramovich, Cadman, Fantechi and WiseACF+13, Proposition 4.2]), the stack
${\mathcal A}^\sim$
can be identified with a moduli stack of curves. Let
$\frak{M}_{0,2}^{\rm ss}$
be the Artin stack parameterizing semistable nodal curves of genus 0 with two markings, and
${\mathcal C}_{0,2}$
be its universal curve.
Proposition A.3.
There is an isomorphism
${\mathcal A}^\sim \cong \frak{M}^{\rm ss}_{0,2}$
. Moreover, if
$\Delta = {\mathbb P}^1 \times D$
, i.e.
$N_{D/Y} \cong {\mathcal O}_D$
, then the isomorphism above induces an isomorphism
${\mathcal R}^\sim \cong {\mathcal C}_{0,2} \times D$
.
Let
$s_0: {\mathcal D}_0 \cong {\mathcal A}^\sim \times D \hookrightarrow {\mathcal R}^\sim\cong {\mathcal C}_{0,2} \times D$
be the inclusion of the universal relative divisor. The universal cotangent line bundle at
${\mathcal D}_0$
is defined as the line bundle
${\mathcal L}_0 := s_0^* \omega_{{\mathcal R}^\sim / {\mathcal A}^\sim}$
over
${\mathcal A}^\sim \times D $
. When
$\Delta = D \times {\mathbb P}^1$
, we have
where
$\operatorname{pr}_{{\mathcal C}}: {\mathcal C}_{0,2} \times D\to {\mathcal C}_{0,2}$
and
$\operatorname{pr}_{{\mathcal A}}: {\mathcal A}^\sim \times D\to {\mathcal A}^\sim$
are projections and
${\mathcal L}_0 (\frak{M}_{0,2}^{ss})$
is the tautological cotangent line bundle of
$\frak{M}_{0,2}^{ss}\cong{\mathcal A}^\sim$
at the marked point 0.
Definition A.4. Assume
$\Delta = D \times{\mathbb P}^1$
. The pullback of the psi-class
$\psi_0 = c_1 ({\mathcal L}_0 (\frak{M}_{0,2}^{ss}))$
of
$\frak{M}^{\rm ss}_{0,2}$
under the isomorphism
${\mathcal A}^\sim \cong \frak{M}^{\rm ss}_{0,2}$
is called the psi-class
$\psi_0 ({\mathcal A}^\sim)$
at
${\mathcal D}_0$
.
A.2 Moduli interpretations of
${\mathcal R}^\sim$
By definition, for a scheme S, a family of rubber expanded pairs is a map
$S\to{\mathcal A}^\sim$
. Let
${\mathcal R}^\sim_S \to S$
be the pullback of the universal family. A map
$S \to {\mathcal R}^\sim$
is then equivalent to a pair
$({\mathcal R}^\sim_S, \Sigma_{1, S})$
, where
${\mathcal R}^\sim_S \to S$
is a family of rubber expanded pairs, and
$\Sigma_{1, S}$
is a section
$S \to {\mathcal R}^\sim_S$
, whose image in
${\mathcal R}^\sim_S$
is also denoted by
$\Sigma_{1, S}$
. Let
$D_{0, S}$
and
$D_{\infty, S}$
be the relative divisors in
${\mathcal R}^\sim_S$
. Note that
$\Sigma_{1, S}$
is allowed to intersect the nodal and relative divisors.
In particular, over a geometric point
$s\in S$
, we have
${\mathcal R}^\sim_s \cong \Delta [k_s]_0$
for some
$k_s \geqslant 0$
, where
The relative divisors in the rubber expanded pair are denoted by
$D_{0, s}$
,
$D_{\infty, s}$
, and
$\Sigma_{1, s}$
is a point in
$\Delta [k_s]_0$
. We denote by
$\Delta_{1,s}$
the first component
$\Delta$
in
$\Delta[k_s]_0$
, which contains
$D_{0,s}$
, and denote by
$D_{1,s}$
the nodal divisor where
$\Delta_{1,s}$
meets the other irreducible components.
Definition A.5. Let
$D(0 |1, \infty)$
be the divisor in
${\mathcal R}^\sim$
whose set of S-points consists of pairs
$({\mathcal R}^\sim_S, \Sigma_{1, S})$
where
$\Sigma_{1, s}$
does not lie in
$\Delta_{1,s} \backslash D_{1,s}$
for any geometric point s in S.
From now until the end of this section, we work under the additional assumption that the bundle
$N_{D/Y}$
is trivial.
Remark A.6. The stack
${\mathcal R}^\sim$
and the divisor
$D(0|1, \infty)$
has another moduli interpretation, parallel to Proposition A.3, which we now explain. By a standard construction, analogous to the case of the moduli of curves,
${\mathcal R}^\sim$
is isomorphic to a moduli stack whose S-points consists of pairs
$(\widetilde{\mathcal R}_S \to S, \widetilde \Sigma_{1, S})$
, where
$\widetilde{\mathcal R}_S \to S$
is a family of rubber expanded pairs, with relative divisors
$D_{0, S}$
and
$D_{\infty, S}$
, and
$\widetilde \Sigma_{1, S}: S\to \widetilde{\mathcal R}_S$
is a section which avoids all nodal and relative divisors. Under this isomorphism,
$D(0| 1, \infty)$
is then the divisor in
${\mathcal R}^\sim$
, where
$\widetilde \Sigma_{1, S}$
lies in a different irreducible component from
$D_{0, S}$
. From this point of view,
${\mathcal R}^\sim$
can be identified with an open substackFootnote
19
in
$\frak{M}_{0,3}^{ss} \times D$
, with markings 0, 1,
$\infty$
, where the curves are chains of rational curves; the divisor
$D(0|1, \infty)$
can then be identified with the closed substack where the marking 0 is required to lie on a different irreducible component from 1 and
$\infty$
. We also have a cotangent line bundle class
which can be identified with the pullback of
$\psi_0$
on
$\frak{M}_{0,3}^{ss}$
.
A generic point in
$D(0 |1, \infty)$
classifies an object
$\Delta \cup_D \Delta$
, where the point
$\Sigma_{1,s}$
lies generically on the second
$\Delta$
which contains
$D_\infty$
. Given a splitting datum
$n_- + n_+ = n$
, we denote by
$D(0 |1, \infty)^{n_-, n_+}$
the divisor in
${\mathcal R}^{\sim, n}$
for a generic point of which the first
$\Delta$
(i.e. containing
$D_0$
) carries weight
$n_-$
and the second
$\Delta$
(i.e. containing
$\Sigma_{1,s}$
and
$D_\infty$
) carries weight
$n_+$
.
Appendix B. Comparison of orientations on
$\operatorname{{Hilb}}^n(\mathbb{C}^4)$
In this section, we consider Hilbert schemes
$\operatorname{{Hilb}}^n(\mathbb{C}^4)$
of points on
$\mathbb{C}^4$
. We compare the orientation specified by Remark 4.4 and Equation (6.2) with the orientation chosen in the work of Kool and Rennemo [Reference Kool and RennemoKR25].
Let
$U=\mathbb{C}^3$
and
$X=\operatorname{Tot}(\omega_U)=\mathbb{C}^4$
with the projection
Let
$\bullet=X$
or U, and
$M_n(\bullet)$
be the moduli stack of zero-dimensional sheaves of length n on
$\bullet$
with closed embedding
the image of which is characterised by the commuting relations in endomorphisms of
$\mathbb{C}^n$
:
Recall the embedding of Hilbert schemes into non-commutative Hilbert schemes (Example 3.10):
the image of which is characterized by the commuting relations (B.2). We have the forgetful map
whose restriction to
$\operatorname{{Hilb}}^n(X)$
gives
$f: \operatorname{{Hilb}}^n(X)\to M_n(X)$
. Let us consider the projection
and its restriction
$\pi_\dagger: M_n(X)\to M_n(U)$
to
$M_n(X)$
. There is a commutative diagram

where the vertical maps are the closed embeddings mentioned above.
For
$\bullet=X$
or U, let
$\mathbb{F}_{\bullet}\to M_n(\bullet)\times \bullet$
be the universal object and
$\pi_{M_{\bullet}}: M_n(\bullet)\times \bullet\to M_n(\bullet)$
be the projection. By (4.8), (4.17) and a base change, we have a map
which is the restriction of the tangent map of the derived enhancement of
$\pi_\dagger: M_n(X)\to M_n(U)$
to the classical truncation. We give a description of this map using data on ambient stacks
$NM_n(\bullet)$
.
Lemma B.1.
There exists a map of
$\operatorname{GL}(n)$
-equivariant complexes on
$\operatorname{End}(\mathbb{C}^n)^{4}$

whose descent to
$NM_n(X)=[\operatorname{End}(\mathbb{C}^n)^{4}/{\operatorname{GL}}(n)]$
defines a map of complexes of vector bundles. Its restriction to
$M_n(X)$
is a resolution of the map (B.4) in the derived category.
When restricted to
$M_n(X)$
, the complex
$(\frak{g} \frak{l}_n\otimes \bigwedge^*\mathbb{C}^4\otimes \mathcal{O})$
has a natural pairing given by
which coincides with the Grothendieck–Serre duality pairing on
$\pi_{M_X*}\mathbf{R}{\mathcal H} om(\mathbb{F}_X,\mathbb{F}_X)[1]$
.
Proof. The description of the complex
$\pi_{M_U*}\mathbf{R}{\mathcal H} om(\mathbb{F}_U,\mathbb{F}_U)[1]$
in (B.4) using the complex
$(\frak{g} \frak{l}_n\otimes \bigwedge^*\mathbb{C}^3\otimes\mathcal{O})$
on
$NM_n(U)$
is given by [Reference Ricolfi and SavvasRS21, § 3.2], which uses a quasi-free dg resolution
$Q_3$
of
$\mathbb{C}[x_1,x_2,x_3]$
. One can do the
$\mathbb{C}^4$
case by the quasi-free dg resolution
$Q_4$
of
$\mathbb{C}[x_1,x_2,x_3,x_4]$
given in [Reference LamLam15, p. 55 and Example 6.3.1]. There is an explicit map between dg-algebra
$Q_3\to Q_4$
(see e.g. [Reference Adhikari and ShiAS24, Example 3.4]), which induces a map of derived stacks of zero-dimensional sheaves on X and U:
Its tangent map (described using
$Q_4$
and
$Q_3$
) defines (B.5). The statement on the identification of pairings is made because both are derived from the Calabi–Yau 4-algebra structure on
$\mathbb{C}[x_1,x_2,x_3,x_4]$
.
One can construct orientations on
$\operatorname{{Hilb}}^n(X)$
in the sense of Definition 4.1, by pulling back orientations on
$M_n(X)$
(see (4.4)). On
$M_n(X)$
, orientations can be constructed using isotropic quotient complexes
$V^\bullet$
of
$E^\bullet=\pi_{M_X*}\mathbf{R}{\mathcal H} om(\mathbb{F}_X,\mathbb{F}_X)[1]$
. Here recall that an isotropic quotient complex is a map
$E^\bullet\stackrel{d}{\to} V^\bullet$
such that
is a distinguished triangle. The orientation used in this paper (see (B.4), and Theorem 4.3) is when
with an explicit description given by the bottom line of (B.5).
The orientation used by Kool and Rennemo in [Reference Kool and RennemoKR25] is given by choosing a maximal isotropic quotient
and formally adding the automorphism and tangent part of
$M_n(X)$
, i.e. considering the following diagram.

Note that although the vertical map in the above diagram is not a map of complexes, one can use it to induce an orientation.
Proposition B.2. The two choices of orientations above coincide.
Proof. Recall that for a quadratic vector bundle
$E=V\oplus V^\vee$
(with
$V=A\oplus B$
) on a connected scheme (where the pairing on E is given by the natural pairing between V and
$V^\vee$
), if we choose its orientations induced by isotropic subbundles
$A\oplus B$
,
$A\oplus B^\vee$
, the orientations are the same if
$\mathop{\rm rk}\nolimits B$
is even and are opposite otherwise (e.g. [Reference Oh and ThomasOT23, Equations (7) and (8)]).
Similarly we can compare the difference of orientations determined by (B.5) and (B.6). Their difference happens on the terms
$\frak{g} \frak{l}_n\otimes \mathbb{C}\otimes \mathcal{O}$
versus
$\frak{g} \frak{l}_n\otimes \bigwedge^4 \mathbb{C}^4 \otimes \mathcal{O}$
, and
$\frak{g} \frak{l}_n\otimes \mathbb{C}^3\otimes \mathcal{O}$
versus
$\frak{g} \frak{l}_n\otimes \bigwedge^2\mathbb{C}^3\otimes \mathcal{O}$
(where we use
$\bigwedge^3\mathbb{C}^4=\bigwedge^3\mathbb{C}^3\oplus \bigwedge^2\mathbb{C}^3$
). Since the rank of
$(\frak{g} \frak{l}_n\otimes \mathbb{C}\otimes \mathcal{O})\oplus (\frak{g} \frak{l}_n\otimes \mathbb{C}^3\otimes \mathcal{O})$
is even, these two orientations coincide.
Appendix C. Proof of Propositions 5.6 and 5.11
Proof of Proposition 5.11. The proof adapts Park’s proof of the deformation invariance of
$\mathop{\rm DT}\nolimits_4$
invariants [Reference ParkPar24]. The infinitesimal criterion of isotropic condition in [Reference ParkPar24] yields that the isotropic condition claimed in Proposition 5.11 is equivalent to the following. For any local Artinian scheme
${\mathcal B}:=\operatorname{{Spec}} B$
with a map
${\mathcal B}\to {\mathcal C}^{P_t}$
, the base-change of the obstruction theory (5.13) to the homotopy pullback
is isotropic. Here
${\mathcal X}_{{\mathcal B}}:={\mathcal X}^{P_t}\times_{{\mathcal C}^{P_t}} {\mathcal B}$
is the base change of
${\mathcal X}^{P_t}\to {\mathcal C}^{P_t}$
to
${\mathcal B}$
. Let
$\Omega_{\mathbf{Hilb}^{P_t}({\mathcal X}_{{\mathcal B}}/{\mathcal B})/{\mathcal B}}\in HN^{-4}(\mathbf{Hilb}^{P_t}({\mathcal X}_{{\mathcal B}}/{\mathcal B})/{\mathcal B})(2)$
be the pullback of the shifted symplectic form in Theorem 3.2. By the relative local Darboux theorem [Reference ParkPar24, Theorem B], the isotropic condition follows if the image
of
$\Omega_{\mathbf{Hilb}^{P_t}({\mathcal X}_{{\mathcal B}}/{\mathcal B})/{\mathcal B}}$
in the periodic cyclic homology is zero. We use as shorthand
Since B is local Artinian, define
${\mathcal B}_{red}=\{b\}$
. Let
$[I_Z]\in \textbf{M}$
be a closed point. Necessarily,
$[I_Z]$
lies in the fiber
$\textbf{M}_b$
of
$\textbf{M}$
over
$b\in {\mathcal B}$
. Note that the classical truncation
$M_b$
of
$\textbf{M}_b$
is a scheme. Without loss of generality, we assume that its associated analytic space
$M_b(\mathbb{C})$
is connected. We have the following fiber diagram.

By the functoriality of the integration map, we have a commutative diagram

where
${\mathcal Z}_{\mathcal B}\subset {\mathcal X}_{{\mathcal B}}\times_{{\mathcal B}}\textbf{M}$
is the universal substack, and
$HP_{{\mathcal Z}_{\mathcal B}}$
denotes the cohomology of the periodic cyclic complex with support on
${\mathcal Z}_{\mathcal B}$
, defined in a similar way to (3.3).
We claim that in the lower-right horizontal map above, the restriction map to
$\{I_Z\}$
, is an isomorphism. Recall the following two facts.
-
– Nil-invariance of
$HP^*$
shown by Goodwillie [Reference GoodwillieGoo85]: for any derived stack
$\textbf{M}$
over
${\mathcal B}$
, the restriction map to the reduced part of the classical truncation (C.2)is an isomorphism.
\begin{equation}HP^*(\textbf{M}/{\mathcal B})(*) \to HP^*((t_0(\textbf{M}))_{red}/{\mathcal B})(*) \end{equation}
-
– The isomorphism between
$HP^*$
and the singular cohomology [Reference EmmanouilEmm95, Theorem 2.2] and [Reference HartshorneHar75, p. 89, Theorem IV. 1.1]: for any
$\mathbb{C}$
-scheme
$M_b$
, we have a canonical isomorphism (C.3)where
\begin{equation}HP^k(M_b)(p)\cong H^{k+2p}_{\mathrm{sing}}(M_b(\mathbb{C})), \,\,\, \forall\,\, k,p\in \mathbb{Z}, \end{equation}
$M_b(\mathbb{C})$
is the associated analytic space of
$M_b$
.
Combining (C.2) and (C.3), we have
\begin{align*}& HP^{-4}(\textbf{M}/{\mathcal B})(2)\cong HP^{0}(\textbf{M}/{\mathcal B})(0) \cong HP^{0}(M_b/{\mathcal B})(0)\cong HP^{0}((M_b\times {\mathcal B})/{\mathcal B})(0) \\&\quad \cong HP^{0}(M_b)(0)\otimes HP^{0}({\mathcal B}/{\mathcal B})(0) \cong HP^{0}(M_b)(0)\otimes B \cong H_{\mathrm{sing}}^{0}(M_b(\mathbb{C}))(0)\otimes B \cong B,\end{align*}
where the first isomorphism uses the periodicity of
$HP^*$
(which follows directly from the definition), the fourth isomorphism uses the fact that
$(M_b\times {\mathcal B})\to {\mathcal B}$
factors as
$M_b\times {\mathcal B}\to \mathrm{Spec}\,\mathbb{C}\times {\mathcal B}\cong {\mathcal B}$
, and the last one uses the connectedness assumption on
$M_b(\mathbb{C})$
. Since all the isomorphisms above are functorial in
$\textbf{M}$
, the restriction map is an isomorphism:
Recall that
$\Omega_{\mathbf{Hilb}^{P_t}({\mathcal X}_{{\mathcal B}}/{\mathcal B})/{\mathcal B}}$
is obtained by applying the integration map
$\int_{{\mathcal X}_{{\mathcal B}}/{\mathcal B}}\mathrm{vol}_{{\mathcal X}_{{\mathcal B}}/{\mathcal B}}\wedge(-)$
to
$\widetilde{\operatorname{ch}_2}(I_{{\mathcal Z}_{\mathcal B}})$
, where
$I_{{\mathcal Z}_{\mathcal B}}$
is the universal complex on
${\mathcal X}_{{\mathcal B}}\times_{{\mathcal B}}\textbf{M}$
, and
$\widetilde{\operatorname{ch}_2}(I_{{\mathcal Z}_{\mathcal B}})$
is the compactly supported lift of
${\operatorname{ch}_2}(I_{{\mathcal Z}_{\mathcal B}})$
from the proof of Theorem 3.2. The restriction of
$I_{{\mathcal Z}_{\mathcal B}}$
to
${\mathcal X}_{b}\times_{}\{I_Z\}$
is
$I_Z$
. By the commutative diagram (C.1), we have
Thanks to the isomorphism
$|_{\{I_Z\}}$
, to conclude the proof it is enough to show the vanishing of
$\widetilde{\operatorname{ch}_2}(I_Z)$
.
Notice that the isomorphism in [Reference EmmanouilEmm95, Theorem 2.2] is constructed on the chain level. Taking into account [Reference HartshorneHar75, p. 92, Corollary IV. 2.2], we have an isomorphism
Since
$\dim_{\mathbb C} Z\leqslant 1$
, we have
$H_{\mathrm{sing}}^{4}({\mathcal X}_b,{\mathcal X}_b\setminus Z)=0$
. Therefore
Proof of Proposition 5.6. The obstruction theory (5.9) is obtained by the base change of
along the map
$Z(\phi)\hookrightarrow W$
. Here (C.5) comes from the derived enhancement (5.7). As in the proof of Theorem 5.11, we may replace
${\mathcal A}^P$
by
${\mathcal B}=\operatorname{{Spec}} B$
where B is a local Artinian
$\mathbb{C}$
-algebra. For simplicity, we use the same notation for a derived
${\mathcal A}^P$
-stack (e.g.
${\mathcal D}, {\mathcal Y}$
,
$\mathbf{Hilb}^{P}(Y,D)$
and universal substacks
${\mathcal Z}_{Y,D}$
,
${\mathcal Z}$
,
${\mathcal Z}_{D}$
) to denote its base change to
${\mathcal B}$
.
By the relative Darboux theorem [Reference ParkPar24, Theorem B], it suffices to show that the composition of
and the canonical map
is null-homotopic.
For this purpose, we describe
$\Omega_{\mathbf{Hilb}^{P}(Y,D)/(W\times {\mathcal B})}$
. We introduce in this proof the following shorthand:
We have the following commutative diagram of complexes.

The map
has two null-homotopies. The shifted symplectic structure
is the loop formed by the concatenation of these two null-homotopies.
First, recall the null-homotopy coming from the Lagrangian structure in Theorem 3.3 on the map
The lower-left square in the diagram above fits into diagram (3.14). In particular, the map
${\mathbb C}\to NC_{ }(M_{{\mathcal Y}}/({\mathcal B}\times W))[-3](2)$
factors through a contractible space 0, and hence has a null-homotopy in this contractible space, which then projects to a null-homotopy in
$NC_{ }(M_{{\mathcal Y}}/({\mathcal B}\times W))[-3](2)$
. We denote this null-homotopy by
$\gamma_1$
.
The other null-homotopy, denoted by
$\gamma_2$
, comes from the Lagrangian fibration structure (Assumption 5.8) on the map
We introduce a third null-homotopy of
$\mathbb{C}\to PC_{}(M_{{\mathcal Y}}/({\mathcal B}\times W))[-3](2)$
, coming from the null-homotopy of a map
as in [Reference Cao and ZhaoCZ26, Proposition 3.27]. By the same calculation on the local Darboux chart as in [Reference Cao and ZhaoCZ26, Proposition 3.27], the loop formed by
$\gamma_0$
and
$\gamma_2$
in
$PC_{ }(M_{{\mathcal Y}}/({\mathcal B}\times W))[-3](2)$
is trivial after base change along the map
$Z(\phi)\hookrightarrow W$
. Here and below, we denote the image of
$\gamma_2$
under
$PC: NC(-)(2)\to PC(-)(2)$
by the same notation, and do the same for
$\gamma_1.$
To conclude the argument, it suffices to show that
$\gamma_0$
and
$\gamma_1$
form a trivial loop. Note that both
$\gamma_0$
and
$\gamma_1$
come from null-homotopies in
$PC_{ }(M_{{\mathcal Y}}/{\mathcal B})[-3](2)$
, which are still denoted by
$\gamma_0$
and
$\gamma_1$
by an abuse of notation, so we are reduced to showing that the loop they form is trivial. For this purpose, we use a similar argument as in the proof of Proposition 5.11. Let b be the closed point in
${\mathcal B}$
and
${\mathcal Y}_b$
the fiber of
${\mathcal Y}$
at the point b. Let
$p=\{I_{Z_Y}\}$
be a closed point of
$M_{\mathcal Y}$
sitting over b, where
$Z_Y\hookrightarrow{\mathcal Y}_b$
is a closed subscheme. By an abuse of notation, we also denote by p its image under the composition
$M_{\mathcal Y} \xrightarrow{r_{{\mathcal D}\to{\mathcal Y}}} M_{\mathcal D} \to M_D$
, where the second map is the projection. The p in the image is represented by
$I_{Z_D}$
with
$Z_D=Z_Y\cap D$
.
Then we have the commutative diagram

where all the maps from the back side to the front side are restriction maps.
By the same argument used in (C.4), the restriction from
$M_{\mathcal Y}$
to
$\{p\}$
induces an isomorphism on
$\pi_1$
. To show that the loop formed by
$\gamma_0$
and
$\gamma_1$
is trivial in
$PC(M_{\mathcal Y}/{\mathcal B})[-3](2)$
, it suffices to show that the image of this loop in
$PC(\{p\}/{\mathcal B})[-3](2)$
is trivial.
In the diagram above, the composition
${\mathbb C}\to PC_{Z_D}(D\times \{p\})(2)$
is given by
$\widetilde{\operatorname{ch}_2}(I_{Z_D})$
, and
${\mathbb C}\to PC_{Z_{Y}}({\mathcal Y}_b\times \{p\}/{\mathcal B})(2)$
is given by
$\widetilde{\operatorname{ch}_2}(I_{Z_Y})$
. As in Proposition 5.11,
$\widetilde{\operatorname{ch}_2}(I_{Z_Y})=0$
. Taking its image in
$PC(\{p\}/{\mathcal B})[-3](2)$
, we obtain yet another null-homotopy of
$\int_D\mathrm{vol}_D\wedge\widetilde{\operatorname{ch}_2}(I_{{\mathcal Z}})|_{\{p\}}$
when restricted to
$\{p\}$
. Notice that, on the one hand, this null-homotopy factors through the contractible space 0 at the bottom left corner and hence is homotopic in
$PC(\{p\}/{\mathcal B})[-3](2)$
to the image of
$\gamma_1$
. On the other hand, restricting to D gives
$\widetilde{\operatorname{ch}_2}(I_{Z_D})=0$
and hence a null-homotopy of the restriction of
$PC(\Omega_{M_D})$
in
$PC(\{p\})[-3](2)$
. We claim that this null-homotopy is homotopic to the restriction of
$\gamma_0$
in
$PC(\{p\})[-3](2)$
. Taking the image in
$PC(\{p\}/{\mathcal B})[-3](2)$
of the homotopy from the claim, we conclude that
$\gamma_0$
and
$\gamma_1$
are homotopic.
It remains to show the claim. Using the presentation of
$PC(M_D)[-3](2)\to PC(\{p\})[-3](2)$
given by [Reference Brav, Bussi and JoyceBBJ19, Example 2.8],
$\gamma_0$
goes to
$\phi|_{\{p\}}$
which is 0 by the footnote of Assumption 5.8. Similarly, recall that the null-homotopy
$\widetilde{\operatorname{ch}_2}(I_{Z_D})\sim 0$
is constructed using the equivalence
$PC_{Z_D}(D)(2)\simeq DR_{Z_D}(D)[4]$
. Hence, we do calculations in
$DR_{Z_D}(D)$
, where we have the map
Any de Rham differential form
$\beta$
on D with
$d_{dR}\beta=\widetilde{\operatorname{ch}_2}(I_{Z_D})$
, has to be a sum of (2,1) and (1,2)-forms and hence goes to 0 under
$\int_D\mathrm{vol}_D\wedge(-)$
.
Acknowledgements
We are grateful to Tasuki Kinjo, Martijn Kool, Xiaolong Liu, Sergej Monavari, Hiraku Nakajima, Andrei Okounkov, Rahul Pandharipande, Hyeonjun Park, Pavel Safronov and Yukinobu Toda for many helpful discussions and communications during the preparation of this work. We particularly thank Martijn Kool for explaining the sign rule and the orientation on Hilbert schemes of points on
$\mathbb{C}^4$
used in his upcoming work with Rennemo, and Hyeonjun Park for several very helpful discussions on virtual pullbacks and shifted symplectic structures. We thank the referee for several helpful suggestions which improved the exposition of the paper.
Conflicts of interest
None.
Financial support
The work of YC was partially supported by RIKEN Interdisciplinary Theoretical and Mathematical Sciences Program (iTHEMS), JSPS KAKENHI Grant Number JP19K23397 and Royal Society Newton International Fellowships Alumni 2022 and 2023. GZ is partially supported by the Australian Research Council via DE190101222 and DP210103081. ZZ is supported by NSFC grant 12401077 and a startup grant from Shanghai Jiao Tong University.
Journal information
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