1 Introduction
The classical sharp
$ L^{p} $
Sobolev inequality in
$ \mathbb {R}^n $
is stated for functions from the homogeneous Sobolev space
$\dot {W}^{1,p}(\mathbb {R}^n)$
(see, e.g.,[Reference Leoni19, Chapter 11]) defined by
where
$1\le p< n $
and
$p^*=\frac {np}{n-p}$
. That is, for any
$f \in \dot {W}^{1,p}(\mathbb {R}^n)$
, there exists an optimal constant
$a_{n, p}$
such that
where
$ \left \| \cdot \right \| _{p} $
denotes the
$ L^{p} $
norm of the Euclidean norm of functions, and
$ \nabla f $
is the gradient of
$ f $
. Here,
$\omega _n=\pi ^{n/2} / \Gamma (1+n/2)$
denotes the volume of the Euclidean unit ball
$B^n$
in
$\mathbb {R}^n$
, and
$\Gamma (\cdot )$
is the Gamma function. Inequality (1.1) goes back to Federer and Fleming [Reference Federer and Fleming9] and Maz’ya[Reference Maz’ya28] for
$ p=1 $
, and to Aubin[Reference Aubin2] and Talenti[Reference Talenti35] for
$ 1<p<n $
. The sharp
$L^1$
Sobolev inequality is known to be equivalent to the isoperimetric inequality.
A major advance regarding (1.1) was achieved by Lutwak, Yang, and Zhang [Reference Lutwak, Yang and Zhang26], which built upon the foundational work of Zhang [Reference Zhang43] for the case
$p=1$
. They established the first affine-invariant form of the
$ L^p $
Sobolev inequality, now called the sharp
$ L^p $
affine Sobolev inequality, which replaces the
$L^p$
norm of gradient in (1.1) by the
$L^p$
affine energy (a suitable average of the norm of one-dimensional gradient projections). More precisely, if
$ 1 \leq p < n $
and
$ f \in \dot {W}^{1, p}(\mathbb {R}^n) $
, then
Here, we write
$c_{n,p}$
as
for convenience and explicit expressions for the optimal constant in (1.2) were found in [Reference Zhang43] (for
$p = 1$
) and in [Reference Lutwak, Yang and Zhang26] (for
$p> 1$
). The functional
$\mathcal {E}_p(f)$
is usually called the
$L^p$
affine energy of f defined by
where we denote by
$G_{n, m}$
the Grassmann manifold of m-dimensional subspaces in
$\mathbb {R}^n$
(
$1\leq m\leq n$
),
$ \text {P}_{\xi }(\nabla f(x)) $
the orthogonal projection of
$ \nabla f(x) $
onto
$ \xi \in G_{n, m} $
, and
$ d\xi $
is the rotationally invariant probability measure on
$ G_{n, m} $
. Note that
$G_{n,1}$
can be identified as the hemisphere of the unit sphere
$S^{n-1} $
and
$G_{n,n}$
can be identified as
$\mathbb {R}^n$
. As the name suggests, inequality (1.2) is invariant under affine transformations of
$ \mathbb {R}^n $
, whereas inequality (1.1) is invariant only under rotations and translations. Subsequently, Wang [Reference Wang37] and, independently, Nguyen [Reference Nguyen32] characterized the equality conditions in (1.2) for
$1 < p < n$
if and only if
with
$\phi \in \mathrm {GL}(n)$
(the group of general linear transformations),
$a>0$
, and
$x_0 \in \mathbb {R}^n$
. For
$p=1$
, Wang [Reference Wang36] showed that the extremals are precisely the characteristic functions of ellipsoids when functions are from BV(
$\mathbb {R}^n$
) (the set of functions of bounded variation on
$ \mathbb {R}^n $
). Moreover, the Hölder inequality immediately implies that (see [Reference Lutwak, Yang and Zhang26])
which shows that the affine form (1.2) provides a significantly stronger inequality than (and directly implies) the classical one (1.1). The
$L^p$
affine Sobolev inequality has its basis in the
$L^p$
affine isoperimetric inequalities [Reference Lutwak, Yang and Zhang25] and has had significant impact in both convex geometry and analysis (see, e.g., [Reference Cianchi, Lutwak, Yang and Zhang3, Reference De Nápoli, Haddad, Jiménez and Montenegro5, Reference Fang, Xu, Zhou and Zhu7, Reference Haberl and Schuster11–Reference Kniefacz and Schuster18, Reference Nguyen33, Reference Wang and Wang38–Reference Xiao41]).
Let
$ C_0^\infty (\mathbb {R}^n) $
denote the set of functions on
$ \mathbb {R}^n $
that are infinitely differentiable and have compact support. It is well known that
$ \dot {W}^{1,p}(\mathbb {R}^n) $
is the closure of
$ C_0^\infty (\mathbb {R}^n) $
under the norm
$\|\nabla f\|_p$
. Another important development for (1.1) is the sharp Lorentz–Sobolev inequality [Reference Alvino1]: if
$ 1 \leq p < n $
and
$ f \in C_0^\infty (\mathbb {R}^n) $
, then
where
$ [f]_t = \{ x \in \mathbb {R}^n : |f(x)| \geq t \} $
is the level set of f and
$V(\cdot )$
denotes the n-dimensional volume (Lebesgue measure). Actually, the Lorentz–Sobolev inequality (1.5) implies (1.1) but without sharp constant unless
$ p = 1 $
(see, e.g., [Reference Ludwig, Xiao and Zhang23]).
Note that level sets in general are not convex. However, a powerful technique of the
$ L^p $
convexification introduced by Lutwak, Yang, and Zhang [Reference Lutwak, Yang and Zhang26, Reference Zhang43] via the solution of the
$ L^p $
Minkowski problem makes level sets always convex. Using the
$ L^p $
convexification of level sets
$ \langle f \rangle _t$
(an origin-symmetric convex body in
$\mathbb {R}^n$
; see (2.6)), instead of
$ [f]_t $
, Ludwig, Xiao, and Zhang [Reference Ludwig, Xiao and Zhang23] established a reinforcing version of inequality (1.5), named the sharp convex Lorentz–Sobolev inequality: if
$1\leq p<n$
and
$f\in C_{0}^{\infty }(\mathbb {R}^{n})$
, then
The sharp convex Lorentz–Sobolev inequality (1.6) immediately implies the
$ L^{p} $
Sobolev inequality with the best constant by using the following sharp inequality due to Lutwak, Yang, and Zhang [Reference Lutwak, Yang and Zhang26]:
and the equality case corresponds to inequality (1.2). It was shown in [Reference Ludwig, Xiao and Zhang23] that the convex version (1.6) is stronger than the classical one (1.5). Furthermore, as noted in [Reference Ludwig, Xiao and Zhang23], inequality (1.6) can also be derived from the proof of the
$L^{p}$
affine Sobolev inequality (1.2).
In fact, the sharp convex Lorentz–Sobolev inequality (1.6) can be strengthened in the following two inequalities [Reference Ludwig, Xiao and Zhang23]: if
$ f \in C_0^{\infty }(\mathbb {R}^n)$
and
$ 1 \leq p < n $
, then
and
Here,
$C_p(K)$
is the
$L^{p}$
variational capacity for a compact set K in
$\mathbb {R}^n$
(see, e.g., [Reference Colesanti and Salani4, Reference Evans and Gariepy6, Reference Maz’ya29, Reference Maz’ya31]) defined by
where
$\textbf {1}_K$
stands for the characteristic function of K. The functional
$\Phi _p(K)$
is the
$L^{p}$
integral affine surface area [Reference Lutwak, Yang and Zhang25] for a Lipschitz star body K (see Section 2) in
$\mathbb {R}^n$
defined by
where
$V_p(\cdot ,\cdot )$
is the
$L^p$
mixed volume defined in (2.3). Moreover, (1.8) and (1.9) are sharp in the sense that all inequalities approach an equality as f tends to the characteristic function of an origin-centered ball for
$ p = 1 $
, and as
$ f $
tends to
$(a +b|x|^{\frac {p}{p-1}})^{\frac {p-n}{p}} $
with
$a, b>0$
for
$ 1 < p < n $
.
Recently, Xiao [Reference Xiao40] introduced an affine version of the
$L^{p}$
variational capacity – the p-affine capacity (denoted by
$C_{p,d}(\cdot )$
). In this article, we prefer to use the notation
$ C_{1,p}(\cdot ) $
rather than
$C_{p,d}(\cdot )$
for convenience. That is, for
$1 \le p < n$
and a compact set K in
$\mathbb {R}^n$
,
It is derived from [Reference Lutwak, Yang and Zhang26, inequality (7.1)] and [Reference Zhang43, inequality (4.8)] that if K is an origin-symmetric convex body in
$\mathbb {R}^n$
, then
The
$ p$
-affine capacity strengthens both the
$L^p$
isocapacitary inequality [Reference Maz’ya30] and the
$L^{p} $
affine isoperimetric inequality [Reference Lutwak, Yang and Zhang25] in Xiao’s p-affine capacity inequality [Reference Xiao40]:
with equality if K is an origin-centered ball in
$\mathbb {R}^n$
. Naturally, together with inequality (1.4), Xiao [Reference Xiao40] derived the following Lutwak–Xiao–Yang–Zhang’s (abbreviated as LXYZ’s)
$L^p$
affine Sobolev inequality chain: if
$f \in \dot {W}^{1,p}(\mathbb {R}^n)$
and
$1 \leq p < n$
, then
with equality if f tends to the characteristic function of an origin-centered ball for
$ p = 1 $
, and
$ f $
tends to
$(a +b|x|^{\frac {p}{p-1}})^{\frac {p-n}{p}} $
with
$a, b>0$
for
$ 1 < p < n $
. The above inequality chain was also restated by Li and Zhu [Reference Li and Zhu22], who used
$L^{p}$
polar projection bodies to provide a new proof for the second inequality in (1.12). A more general version of the chain (1.12) was established by Wang and Wang [Reference Wang and Wang38] by using the general
$ L^p $
affine capacity [Reference Hong and Ye17] and integral surface area, together with the asymmetric
$ L^{p} $
convexification of level sets.
The aim of this article is to establish the Grassmannian form of LXYZ’s
$L^p$
affine Sobolev inequality chain. To do this, we will first introduce some definitions related to Grassmann manifolds.
The Grassmannian
$L^p$
affine energy
$ \mathcal {E}_{m,p}(\cdot ) $
was introduced by Kniefacz and Schuster [Reference Kniefacz and Schuster18] defined by, for
$ 1\le p<n $
,
$ 1\le m\le n $
, and
$f \in \dot {W}^{1,p}(\mathbb {R}^n)$
,
where
$c_{m,p}$
is given in (1.3). They subsequently proved the sharp Grassmannian
$L^p$
Sobolev inequality, extending the classical
$ L^{p} $
affine Sobolev inequality (1.2) to the following Grassmannian form:
When
$ 1<p<n$
, equality in (1.14) holds for
$ m>1 $
if and only if
$ f(x) = \pm (a + |b(x - x_0)|^{\frac {p}{p-1}})^{\frac {p-n}{p}}$
with
$ a,b>0 $
and
$ x_{0}\in {\mathbb {R}^{n}} $
; for
$ m=1 $
if and only if
$f(x) = \pm (a + |\phi (x - x_0)|^{\frac {p}{p-1}})^{\frac {p-n}{p}}$
with
$ \phi \in \mathrm {GL}(n) $
,
$ a>0 $
, and
$ x_{0}\in {\mathbb {R}^{n}} $
. When
$p = 1$
, the authors [Reference Kniefacz and Schuster18] further extended (1.14) to functions from
$\mathrm {BV}(\mathbb {R}^n)$
and showed that equality in (1.14) if and only if f is a multiple of the characteristic function of a ball when
$m> 1$
and an ellipsoid when
$m = 1$
. Actually, the case
$m = 1$
of inequality (1.14) immediately reduces to the
$L^p$
affine Sobolev inequality (1.2).
The Grassmannian
$L^{p}$
integral affine surface area
$\Phi _{m,p}(\cdot )$
, recently introduced by Ye, Lu, and Huang [Reference Ye, Lu and Huang42], extends the
$L^{p}$
integral affine surface area from the case of one-dimensional subspaces to arbitrary m-dimensional subspaces. Specifically, for
$p\geq 1$
,
$1 \leq m \leq n$
, and a Lipschitz star body K in
$\mathbb {R}^n$
,
The normalization above is chosen so that
$\Phi _{m,p}(B^n) = n\omega _n$
(see (4.2)). By using inequality (1.14), the authors of [Reference Ye, Lu and Huang42] extended inequalities (1.9) to the following Grassmannian form: for
$ 1\le p<n $
,
$ 1\le m\le n $
, and
$f \in C_0^\infty (\mathbb {R}^n)$
,
with equality when f tends to the characteristic function of an origin-centered ball for
$ p = 1 $
, and when
$ f $
tends to
$(a +b|x|^{\frac {p}{p-1}})^{\frac {p-n}{p}} $
with
$a, b>0$
for
$ 1 < p < n $
.
In this article, we will introduce the following Grassmannian form of p-affine capacities defined by, for
$ 1\le p<n $
,
$ 1\le m\le n $
, and a compact subset
$ K \subset \mathbb {R}^{n}$
,
The case
$m=1$
of
$C_{m,p}(\cdot )$
is just the
$ p$
-affine capacity. The case
$m=n-1$
of
$C_{m,p}(\cdot )$
can be seen as the sine version (the orthogonal projection of
$\nabla f$
onto the
$(n-1)$
-dimensional subspace) of p-affine capacities.
Firstly, we have the following reinforcing geometric inequalities, which split and then strengthen the
$ L ^{p} $
affine isoperimetric inequality.
Theorem 1.1 Let
$ 1\le p<n $
and
$ 1\le m\le n $
. If
$ K $
is a Lipschitz star body in
$\mathbb {R}^n $
, then
with equality if
$ K $
is a ball containing the origin in its interior for
$ p=1 $
, and
$ K $
is an origin-centered ball for
$ 1<p<n $
.
Secondly, based on Theorem 1.1 and (1.7), we establish the Grassmannian form of LXYZ’s
$L^p$
affine Sobolev inequality chain in the following theorem.
Theorem 1.2 Let
$ 1\le p<n $
and
$ 1\le m\le n $
. If
$ f\in \dot {W}^{1,p}(\mathbb {R}^n) $
, then
with equality when f tends to the characteristic function of an origin-centered ball for
$ p = 1 $
, and when
$ f $
tends to
$(a +b|x|^{\frac {p}{p-1}})^{\frac {p-n}{p}} $
with
$a, b>0$
for
$ 1 < p < n $
.
Clearly, the case
$ m=1 $
of (1.19) is just the inequality chain (1.12). The case
$m= n-1$
is the sine counterpart of (1.12) since
$\mathcal {E}_{n-1,p}(\cdot )$
,
$\Phi _{n-1,p}(\cdot ),$
and
$C_{n-1,p}(\cdot )$
are all the corresponding sine versions (see, e.g., [Reference Li, Xi and Zhang21] for more information).
The rest of this article is organized as follows: In Section 2, the background materials are provided. Basic properties for the newly defined
$C_{m,p}(\cdot )$
are listed in Section 3. The proofs of Theorems 1.1 and 1.2 are presented in Section 4.
2 Background materials
In this section, we list some basic facts about convex bodies and star bodies. The books [Reference Gardner10, Reference Schneider34] are good references.
Throughout, we shall work in the Euclidean space
$ \mathbb {R}^n $
with
$n\geq 2$
. For
$ x, y \in \mathbb {R}^n $
, we denote their inner product by
$ x \cdot y $
and the Euclidean norm of
$ x $
by
$ |x| = \sqrt {x \cdot x} $
. Denote by
$S^{n-1}$
the unit sphere and by
$ B^n $
the Euclidean unit ball in
$\mathbb {R}^n$
. A convex body is a compact convex set in
$ \mathbb {R}^{n} $
which is throughout assumed to contain the origin in its interior. We write
$\mathcal {K}_o^n$
for the class of convex bodies. Each convex body
$ K $
is uniquely determined by its support function
$ h_{K}:\mathbb {R}^{n}\to [0,\infty ) $
defined by
For
$ p \geq 1$
,
$ K,L\in \mathcal {K}_o^n $
, and
$ \varepsilon>0 $
, the Minkowski–Firey
$ L^p $
sum
$ K +_p \varepsilon \cdot L \in \mathcal {K}_o^n$
is defined by
The
$ L^p $
mixed volume
$ V_p(K, L) $
of
$ K, L \in \mathcal {K}_0^n $
was defined in [Reference Lutwak24] by
In his prominent work, Lutwak [Reference Lutwak24] showed the existence of the limit and derived the following variational formula:
where
$S_p(K, \cdot ) = h_K^{1-p} S_K $
is the
$L^p$
surface area measure of K and
$S_K$
is the classical surface area measure of K. In particular,
The variational formula (2.1) led to an embryonic
$L^p$
Brunn–Minkowski theory, which has expanded rapidly thereafter. For further details, as well as detailed bibliography on the topic, we refer the reader to [Reference Schneider34, Chapter 9] and the references therein.
A subset
$M \subseteq \mathbb {R}^n$
is said to be star-shaped with respect to the origin o if the intersection of every straight line through the origin with M is a line segment. Its radial function
$\rho _M:\mathbb R^n \backslash \left \{o\right \}\rightarrow [0,\infty )$
is defined by
for each
$x\in \mathbb R^n \backslash \left \{o\right \}$
. A star-shaped set M is called a star body in
$\mathbb {R}^n$
if the radial function restricted on
$S^{n-1}$
is positive and continuous. We say that
$ M $
is a Lipschitz star body, that is,
$ M $
has Lipschitz boundary
$ \partial M $
. Then the unit outer normal
$ \nu _M(x) $
to
$ M $
exists for almost all
$ x \in \partial M $
. Note that the radial function
$\rho _M$
is locally Lipschitz continuous when restricted to its core
Thus, if
$ M $
is a Lipschitz star body and
$ L \in \mathcal {K}_o^n $
, the
$ L^p $
mixed volume
$ V_p(M, L) $
can be reformulated as (see [Reference Ludwig, Xiao and Zhang23])
In particular, for
$ \xi \in G_{n,m} $
,
where we use the fact that
$ h_{B^n \cap \xi }(x) = |\text {P}_\xi (x)| $
for any
$ x \in \mathbb {R}^n $
. When
$ \xi = \mathbb {R}^n $
, the
$ L^p $
surface area
$ S_p(M) $
for a Lipschitz star body M can be given by
The following co-area formula (see, e.g.,[Reference Federer8, p. 258]) will be needed. If
$ f : \mathbb {R}^n \to \mathbb {R} $
is Lipschitz and
$ g : \mathbb {R}^n \to [0, \infty ) $
is integrable, then
where
$ \partial [f]_t = \{ x \in \mathbb {R}^n : |f(x)| = t \} $
for some
$ t> 0 $
.
The
$ L^p $
convexification of level sets was defined in [Reference Ludwig, Xiao and Zhang23] as follows (a local version of
$K_{p}f$
in [Reference Lutwak, Yang and Zhang27]). Let
$ U $
be an open subset of
$ \mathbb {R}^n $
and
$ f : U \to \mathbb {R} $
be a locally Lipschitz continuous function. Suppose
$ \nabla f(x) \neq 0 $
a.e. on
$ \partial [f]_t$
for some
$ t> 0 $
. For
$ 1 \leq p < n $
, the
$ L^p $
convexification
$ \langle f \rangle _t $
of the level set
$ [f]_t $
is the unique origin-symmetric convex body in
$\mathbb {R}^n$
such that
holds for any even
$ g \in C(S^{n-1}) $
, where
$ \nu (x) = -\frac {\nabla f(x)}{|\nabla f(x)|} $
. Note that if
${f \in C_0^\infty (\mathbb {R}^n)} $
, by Sard’s theorem,
$ \nabla f \neq 0 $
on
$ \partial [f]_t $
for a.e.
$ t> 0 $
, and hence the assumptions on
$ f $
are fulfilled. By a simple continuity argument, the
$L^p $
mixed volume
$ V_p(K,L)$
can be extended to the case that L is a compact convex set containing the origin in its relative interior (see, e.g., [Reference Lutwak, Yang and Zhang26]). In particular, when
$L=B^n \cap \xi $
for
$\xi \in G_{n,m}$
, by (2.1) and (2.6), we have
Let
$\mathrm {Sim}(n)$
denote the group of similarities (a similarity is a composition of a dilation and a rotation followed by a translation) of
$ \mathbb {R}^n $
. An inequality
$ L[f] \leq R[f] $
for a class of functions
$ f : \mathbb {R}^n \rightarrow \mathbb {R} $
is called similarity invariant if
for each
$ (s, \Psi ) \in \mathbb {R} \backslash \{0\} \times \text {Sim}(n) $
.
3 Basic properties of
$ C_{m,p}(\cdot )$
Recall that the Grassmannian
$ p$
-affine capacity
$ C_{m,p}(K)$
is defined by, for
$ 1\le p<n $
,
$ 1\le m\le n $
, and a compact subset
$ K \subset \mathbb {R}^{n}$
,
The basic properties of
$C_{m,p}(\cdot )$
are listed as follows. Some proofs can be found in [Reference Xiao39–Reference Xiao41]; for completeness, we provide the details.
Proposition 3.1 Suppose that
$ 1\le p<n $
and
$ 1\le m\le n $
. Let
$ K \subset \mathbb {R}^{n}$
be a compact subset.
-
(i) $C_{m,p}(rK) = r^{n-p} C_{m,p}(K)$
, where
$ rK = \{rx : x \in K\} $
,
$ r>0 $
. -
(ii) $C_{m,p}(\phi {K}) = C_{m,p}({K})$
for each rotation or translation
$ \phi $
. -
(iii) If compact sets $K_1$
and
$K_2$
satisfy
$K_1 \subset K_2 \subset \mathbb {R}^n$
, then
$C_{m,p}(K_1) \leq C_{m,p}(K_2)$
. -
(iv) $C_{m,p}(\cdot )$
is upper-semi-continuous; that is, for any
$\epsilon> 0$
there is an open set
$O \supset K$
such that
$C_{m,p}(F) \leq C_{m,p}(K) + \epsilon $
for every compact
$F \subset \mathbb {R}^n$
with
$O \supset F \supset K$
. -
(v) If $\{K_j\}_{j=1}^{\infty }$
is a sequence of compact subsets with
$K_{j+1} \subseteq K_j \subseteq \mathbb {R}^n, j = 1, 2, 3, \ldots~ $
, then
$C_{m,p}(\cap _{j=1}^{\infty } K_j) = \lim _{j \rightarrow \infty } C_{m,p}(K_j)$
. -
(vi) $C_{m,p}(\partial K) = C_{m,p}(K)$
. -
(vii) $C_{m,p}(K)^{\frac {1}{n-p}}$
is quasi-increasing on
$[1, n)$
with respect to p; that is, for any
$1 \leq p \leq q < n$
, there exists a positive constant
$\lambda $
depending on
$p, q, m, n$
such that
$C_{m,p}(K)^{\frac {1}{n-p}}\leq \lambda C_{m,q}(K)^{\frac {1}{n-q}}$
. -
(viii) For $ {f \in C_0^{\infty }(\mathbb {R}^n)}$
, $$\begin{align*}\Big( \int_0^{\infty} C_{m,p}(\langle f \rangle_t) dt \Big) \Big/ \Big( \int_0^{\infty} V(\langle f \rangle_t)^{\frac{n-p}{n}} dt \Big) \end{align*}$$and
$$\begin{align*}\Big( \int_0^{\infty} \Phi_{m,p}(\langle f \rangle_t) dt \Big )\Big /\Big( \int_0^{\infty} C_{m,p}(\langle f \rangle_t) dt \Big) \end{align*}$$are $\mathrm {Sim}(n)$
-invariant.
Proof (i)–(iii) The results follow from the definition (3.1) and a simple calculation.
(iv) Let
$\mathcal {B}(K) = \{f \in \dot {W}^{1,p}(\mathbb {R}^n) : f =1 \text { in a neighborhood of } K \text { and } 0 \leq f \leq 1 \text { in } \mathbb {R}^n\}$
. We first show
To see this, it is enough to verify
For each
$j \in \mathbb {N}$
, define
$\psi _j \in C^\infty (\mathbb {R})$
by
satisfying
$0 \leq \psi _j' \leq 1 + j^{-1}$
everywhere. Thus, for any
$f \in \dot {W}^{1,p}(\mathbb {R}^n)$
with
$f \geq \textbf {1}_K$
,
$\psi _j \circ f$
belongs to
$\mathcal {B}(K)$
. Applying the chain rule yields
Taking
$j \to \infty $
gives (3.3).
Therefore, by (3.2), for any
$\epsilon> 0$
, there exists
$f \in \mathcal {B}(K)$
satisfying
Let O be a neighborhood of K with
$f = 1$
in O. Then for any compact
$F \subset \mathbb {R}^n$
with
$K \subset F \subset O$
, by (3.2) again, we have
(v) It is obvious from the monotonicity of capacity that
and it is enough to show that
By (3.1), for any
$\varepsilon \in (0, 1)$
, there is a function
$f \in \dot {W}^{1,p}(\mathbb {R}^n)$
with
$f \ge \textbf {1}_{\cap _{j=1}^{\infty } K_j}$
such that
By compactness, there exists
$N \in \mathbb {N}$
such that for all
$j \geq N$
, the inclusion
$K_j \subseteq \{x \in \mathbb {R}^n : f(x) \geq 1-\varepsilon \}$
holds. So by Property (iii), we have
Letting
$\varepsilon \rightarrow 0$
yields the desired result.
(vi) It is enough to show that
For any
$f \in \dot {W}^{1,p}(\mathbb {R}^n)$
with
$f \geq \textbf {1}_{\partial K}$
, let
Thus,
$g \in \dot {W}^{1,p}(\mathbb {R}^n)$
with
$g \geq \textbf {1}_{K}$
and
$| \text {P}_{\xi } \nabla g| \leq | \text {P}_{\xi } \nabla f|$
for all
$\xi \in G_{n,m}$
. Hence,
holds for any
$f \in \dot {W}^{1,p}(\mathbb {R}^n)$
with
$f \geq \textbf {1}_{\partial K}$
, and (3.4) follows.
(vii) Consider the test function
By the Hölder inequality and the sharp Grassmannian
$L^p$
Sobolev inequality (1.14), we have
Thus, a straightforward computation yields
Taking the infimum over
$ f $
and using the definitions of
$ C_{m,q}(K) $
give the desired result.
(viii) Let
$ s> 0 $
and
$ \Psi (x) =\phi (x) + x_0 $
(
$ \phi $
is a rotation followed by a dilation and
$ x_0 \in \mathbb {R}^n $
). In [Reference Ludwig, Xiao and Zhang23], Lemma 13 states that if
$ {f \in C_0^{\infty }(\mathbb {R}^n)}$
and
$\nabla f(x)\neq 0$
on
$\partial [f]_t$
for
$t>0$
, then
Note that by [Reference Li, Xi and Huang20, Lemma 7.2] and the definition of
$ \Phi _{m,p}(K) $
, we have
Thus, the desired results follow by combining (3.5), Proposition 3.1(i) and (ii), and (3.6), (3.7).
4 Proofs of the main results
We split inequalities (1.18) into two parts to prove. Firstly, we will show the following lemma. The case
$ m=1 $
of inequality (4.1) is just (1.10).
Lemma 4.1 Let
$ 1\le p<n $
and
$ 1\le m\le n $
. For a compact set
$ K$
in
$\mathbb {R}^n$
,
Proof It was shown in [Reference Ye, Lu and Huang42, Lemma 4.2] that for any
$u\in S^{n-1}$
,
$ 1\le m\le n $
, and
$ 1\le p<\infty $
,
Thus, for
$f\in {\dot {W}^{1,p}}(\mathbb {R}^n)$
with
$f \ge \textbf {1}_{K} $
, by Fubini’s theorem and (4.2), we obtain
where
$ \nu (x) = -\frac {\nabla f(x)}{|\nabla f(x)|}$
. Now, it follows from (1.17), (1.13), and Jensen’s inequality that
Taking the infimum over
$f\in {\dot {W}^{1,p}}(\mathbb {R}^n)$
with
$f \ge \textbf {1}_{K} $
immediately gives (4.1).
Theorem 4.2 Let
$ 1\le p<n $
and
$ 1\le m\le n $
. For a compact set
$ K$
in
$\mathbb {R}^n$
,
with equality if
$ K $
is a ball.
Proof It suffices to prove the inequality for
$f \in C_0^\infty (\mathbb {R}^n)$
with
$f \ge \textbf {1}_{K}$
. By Sard’s theorem, for almost all
$t> 0$
, the boundary
$ \partial [f]_t $
of the level set is a
$C^1$
submanifold which has everywhere nonzero normal vector
$\nabla f$
. Thus, it follows from (2.5) and (2.7) that
where
$ \nu (x) = -\frac {\nabla f(x)}{|\nabla f(x)|}$
. By (4.5), the Minkowski inequality for integrals, (1.15), and (1.16), we further have
For
$1 \le p < n$
, it was proved in [Reference Ye, Lu and Huang42, Lemma 3.2] that if
$f \in C_0^\infty (\mathbb {R}^n)$
with
$f \geq \mathbf {1}_K$
, then
which yields (4.4) by using (4.7) and taking the infimum over f.
For the equality condition of inequality (4.4), we choose a closed ball
$\overline {B(x_0, r_0)} = \{x \in \mathbb {R}^n : |x - x_0| \leq r_0, \ \ r_0>0\}$
. Note that the
$L^{p}$
variational capacity
$C_p(K)$
is invariant for translations and is homogeneous of degree
$n-p$
(see, e.g., [Reference Ludwig, Xiao and Zhang23, p. 183]). Then
where the fact that
$C_p(B^n)=n\omega _n\Big ( \frac {n-p}{p-1} \Big )^{p-1}$
can be found in [Reference Maz’ya31, p. 148]. Therefore, Lemma 4.1, Theorem 4.2, and (4.8) ensure that
The identity above shows that equality in (4.4) holds for balls.
Lemma 4.3 [Reference Ludwig, Xiao and Zhang23, Lemmas 5 and 6]
If K is a Lipschitz star body in
$\mathbb {R}^n$
, then
and
for almost all
$x \in \partial K \cap D_K$
, where
$D_K = \{tx : t> 0, x \in \partial K, \ |x \cdot \nu _K(x)| > 0\}$
is the core of K.
The left side inequality of (1.18) is obtained by choosing an appropriate test function for a Lipschitz star body.
Theorem 4.4 Let
$ 1\le p<n $
and
$ 1\le m\le n $
. If
$ K $
is a Lipschitz star body in
$\mathbb {R}^n $
, then
When
$1 < p < n$
, equality in (4.11) holds if and only if K is an origin-centered ball for
$1 < m \leq n$
, and K is an origin-centered ellipsoid for
$m = 1$
. When
$p = 1$
, equality in (4.11) always holds.
Proof
Case
$ {1 < p < n}$
: For the Lipschitz star body
$ K $
in
$\mathbb {R}^n$
and
$s>0$
, let
Then
$ f(x)\geq \mathbf {1}_K$
and
$f\in {\dot {W}^{1,p}}(\mathbb {R}^n)$
(see [Reference Ludwig, Xiao and Zhang23, p. 187]). From the fact that g is strictly decreasing on
$s \in (1, \infty ) $
, it follows that, for all
$t \in (0, 1)$
with
$t = g(s) = s^{\frac {n-p}{1-p}}$
,
That is,
$[f]_t=[f]_{g(s)}=sK$
for any
$s>1$
. Note that
$1/\rho _{K}(x)$
is homogeneous of degree 1. Therefore, by the co-area formula (2.5), (4.9), (4.10), and (2.3), we get
Together with the definition of
$C_{m,p}(K)$
and
$ \Phi _{m,p}(K) $
, we further have
as desired.
Case
$ {p = 1:}$
We always have
$ C_{m,1}(K)=\Phi _{m,1}(K) $
whenever
$ K $
is a Lipschitz star body. In fact, for sufficiently small
$\varepsilon>0$
, let
where
$\text {dist}(x,K)$
is the Euclidean distance x to K. Consider
and its closure
$\bar {K}_{\varepsilon }$
. Following [Reference Zhang43, p. 195], we have
where
$x'$
is a unique point in
$\partial K$
such that
$ \text {dist}(x,K) = |x' - x|$
and
$ \nu (x') = \frac {x' - x}{|x' - x|}. $
Let
$t = \text {dist}(x,K)\in (0,\varepsilon )$
. Then,
$dx = dS_K dt + o(\Delta t)$
. Therefore, by (2.3), as
$\varepsilon \to 0$
, we have
This, along with the definitions of
$C_{m,1}(K)$
and
$\Phi _{m,1}(K)$
, yields
On the other hand, if
$f \geq \textbf {1}_K$
with K being a Lipschitz star body and
$t \in (0,1)$
, then
$K \subset [f]_t$
. Thus, by (2.3) and (2.7), we now conclude that
By the co-area formula (2.5) with
$ \nu (x) = -\frac {\nabla f(x)}{|\nabla f(x)|}$
and (2.7), we further have
which gives
By the definitions of
$C_{m,1}(K)$
and
$ \Phi _{m,1}(K) $
again, we obtain
The equality conditions for (4.11) are immediately from that of Theorem 4.2 and [Reference Ye, Lu and Huang42, Theorem 4.4], which in turn follows from the equality case of [Reference Kniefacz and Schuster18, Theorem 1].
Finally, we are in a position to prove Theorem 1.2.
Proof of Theorem 1.2.
We split inequality (1.19) into four inequalities as follows:
It is only to prove inequality (4.14). Inequality (4.12) can be obtained in (4.3) with the equality conditions by using Jensen’s inequality, which occurs precisely when f is such that
$ \|\text {P}_{\xi }\nabla f\|_{p} $
is independent of
$\xi \in G_{n,m}$
. Inequality (4.13) is just (4.6), and inequality (4.15) can be found in (1.7).
To obtain inequality (4.14), we take
$ K = \langle f \rangle _t $
in (1.18), which yields that
Integrating three terms with respect to t yields (4.14).
The equality conditions of (1.19) immediately follow from those of the Grassmannian convex Lorentz–Sobolev inequality(1.14) and the Grassmannian
$L^p$
Sobolev inequalities (1.16).




