1 Introduction
In [Reference Stong8], Stong proved the following characterisation of geodesic spheres in Euclidean space.
Theorem (Stong [Reference Stong8]).
Let
$n\geqslant 2$
and
$s\in \{2,\ldots ,n\}$
be two integers and let
$\Sigma $
be a closed, oriented hypersurface embedded into Euclidean space. If
$\Sigma $
is star-shaped,
$H_s$
is positive everywhere, and if there exists a constant c so that
then
$\Sigma $
is a geodesic sphere.
Star-shaped is to be understood in this statement as meaning that the support function
$\langle X,\nu \rangle $
has fixed sign, where X is the position vector field and
$\nu $
a global normal unit vector field. Further,
$H_k$
denotes the higher-order mean curvature of order k (the definition will be recalled in Section 2).
Very recently, Li and Peng [Reference Li and Peng6] proved an isotropic analogue of this result, thus giving a new characterisation of Wulff shapes.
The aim of this short paper is to extend Stong’s result to a particular class of warped products. To be precise, the geometric setting is the following. Let
$n\geqslant 2$
be an integer and
$(M^n,g_M)$
be a compact Riemannian manifold of dimension n and constant sectional curvature K. Let
$h:[0,t_0)\longrightarrow \mathbb {R}$
be a positive function satisfying the two conditions:
where
$t_0$
is either a positive number or
$+\infty $
. We consider the warped product P defined by
$P=[0,t_0)\times M$
endowed with the metric
$g_P=dt^2\oplus h(t)g_M$
, and the vector
$X=h(r){\partial }/{\partial r}$
which is a conformal vector field and plays a crucial role in the theory of hypersurfaces in these warped products (see, for instance, [Reference Brendle2]). We say that an oriented submanifold
$\Sigma $
in P is star-shaped if
$\langle X,\nu \rangle $
has fixed sign. The main result of this note is the following characterisation of a slice.
Theorem 1.1. Let
$n\geqslant 2$
,
$r\in \{2,\ldots ,n\}$
and
$s\in \{2,\ldots ,r-1\}$
be three integers and let
$\Sigma $
be a closed, oriented hypersurface embedded into the warped product
$(P^{n+1},g_P)$
satisfying conditions (H1) and (H2). If
$\Sigma $
is star-shaped,
$H_r$
is positive everywhere and there exists a constant c so that
then
$\Sigma $
is a slice
$\{t_1\}\times M$
.
2 Preliminaries
We consider the warped product
$(P,g_p)$
of the form given in the introduction and satisfying the two conditions (H1) and (H2).
Let
$\Sigma $
be a closed, connected and oriented hypersurface of
$(P^{n+1}, g_P)$
. We consider the function
$f=h'$
and the vector field
$X=h{\partial }/{\partial t}$
. We will also assume that
$\Sigma $
is star-shaped, that is, the function
$\langle X,\nu \rangle $
is nonnegative everywhere on
$\Sigma $
, where
$\nu $
is the outward normal unit vector field. In [Reference Brendle2], Brendle used the fact that X is a conformal vector field, that is,
$\mathcal {L}_Xg=2fg$
, to obtain the following Hsiung–Minkowski formula for hypersurfaces of these warped products:
where g is the induced metric on
$\Sigma $
and H the mean curvature of
$\Sigma $
.
More generally, there are similar formulas involving higher-order mean curvatures. Before giving these formulas, we recall some results about higher-order mean curvatures. They are extrinsic quantities defined from the second fundamental form and generalising the notion of mean curvature. Up to a normalisation the mean curvature H is the trace of the second fundamental form B,
In other words, the mean curvature is
where
$S_1$
is the first elementary symmetric polynomial and
$\kappa _1,\ldots ,\kappa _n$
are the principal curvatures. Higher-order mean curvatures are defined in a similar way for
$r\in \{1,\ldots ,n\}$
by
where
$S_r$
is the rth elementary symmetric polynomial, that is, for any n-tuple
$(x_1,\ldots ,x_n)$
,
Note that, of course,
$H_1$
is nothing more than the mean curvature H.
We now recall some well-known classical inequalities between the higher-order mean curvatures. First, if
$H_r>0,$
then
$H_j>0$
for any
$j\in \{1,\ldots ,s-1\}$
and
These classical inequalities can be found, for instance, in Li et al. [Reference Li, Wei and Xiong7] where the proof of Barbosa and Colares [Reference Barbosa and Colares1] for space forms is extended to warped products.
Moreover, we also have the classical Newton–Maclaurin inequalities
Therefore, since
$H_i>0$
and
$H_j>0$
,
Moreover, equality in (2.2) as well as in (2.3) occurs if and only if
$\Sigma $
is totally umbilical.
In particular, for
$s\in \{1,\ldots ,r\}$
,
which, since
$H_s>0$
and
$H_r>0$
, gives
Note at this point that the assumption of Theorem 1.1 says that a constant c can be included between those two quantities
${H_{s-1}}/{H_{r-1}}$
and
${H_{s}}/{H_r}$
.
We now recall the following general Hsiung–Minkowski formula in warped products. Namely, if conditions (H1) and (H2) are satisfied and
$\Sigma $
is star-shaped, then
This inequality was first proved by Brendle and Eichmair [Reference Brendle and Eichmair3] if
$\Sigma $
is convex. It turned out that the convexity assumption is not necessary and can be replaced by s-convexity [Reference Li, Wei and Xiong7], that is,
$H_s$
is positive everywhere, which is a weaker assumption than convexity (which means that all the principal curvatures are positive).
Note that (2.1) and (2.4) are the generalisations in this class of warped products of the so-called Hsiung–Minkowski formulas [Reference Hsiung5] for space forms (see, for instance, [Reference Li, Wei and Xiong7]). A crucial difference is that, in space forms, they are equalities, which is not the case here except for identity (2.1). However, the error term is well known (see [Reference Brendle and Eichmair3, Reference Li, Wei and Xiong7, Reference Wu and Xia9]). In order to give this error term explicitly, we need to introduce additional quantities. For
$j\in \{1,\ldots ,n\}$
, we set
$\Lambda _j=(\kappa _1,\ldots ,\kappa _{j-1},\kappa _{j+1},\ldots ,\kappa _n)$
, that is, the ordered set of principal curvatures without the jth one
$\kappa _j$
, and we define
for any
$j,r\in \{1,\ldots ,n\}$
. It is well known (see, for instance, [Reference Chen, Guan, Li and Scheuer4]) that if
$H_r>0$
, then
$H_{r;j}>0$
for any
$j\in \{1,\ldots ,n\}$
. We can now recall the Hsiung–Minkowski formula with explicit error term in (2.4). To be precise (see [Reference Brendle and Eichmair3, Reference Li, Wei and Xiong7]),
where
$A_j=-{(n(n-1))}^{-1}\langle X,e_j\rangle \mathrm {Ric}(e_j,\nu ).$
Moreover,
so that if M is star-shaped and assumption (H2) holds, then
$A_j\geqslant 0$
for any
$j\in \{1,\ldots ,n\}$
.
We finish this section by recalling the following inequalities whose proof can be found in [Reference Wu and Xia9]: for any
$k,l\in \{2,\ldots ,r\}$
with
$l<k$
and any
$j\in \{1\ldots ,n\}$
,
We now have all the ingredients to prove Theorem 1.1.
3 Proof of Theorem 1.1
Proof. From the assumptions,
$H_{s-1}\leqslant cH_{r-1}$
so that
where we have used the Hsiung–Minkowski formula (2.5) involving
$H_{r-1}$
and
$H_r$
. By assumption, we also have
$cH_r\leqslant H_s$
and since
$\langle X,\nu \rangle $
is nonnegative, (3.1) yields
We now use the Hsiung–Minkowski formula a second time, but involving
$H_{s-1}$
and
$H_s$
, to obtain
On the other hand, from (2.6),
From the assumption
$H_{s-1}\leqslant cH_{r-1}$
and the fact that
$H_{r-2;j}>0$
, we have
and so, since
$H_{r-1}>0$
,
Moreover, since all the
$A_j$
are nonnegative,
On the other hand, (3.2) gives
Hence, (3.4) is an equality, that is,
But from (3.3) and
$A_j\geqslant 0$
for any
$j\in \{1,\ldots ,n\}$
, each term of the sum in the integral of (3.5) is nonnegative, so that for any
$j\in \{1,\ldots ,n\}$
,
Finally, since
$(s-1)H_{s-2;j}-c(r-1)H_{r-2;j}<0$
and
$A_j\geqslant 0$
, we deduce that
$A_j=0$
for any
$j\in \{1,\ldots ,n\}$
.
We now recall that
$A_j=-{(n(n-1))}^{-1} \langle X,e_j\rangle \mathrm {Ric}(e_j,\nu )$
with
that is,
From (3.6),
$A_j=0$
for any
$j\in \{1,\ldots ,n\}$
implies that, at any point
$x\in \Sigma $
, the vector
$X(x)$
is either normal or tangent. Since X does not vanish, by continuity, X is tangent everywhere or normal everywhere. But, if X is tangent, then the support function
$\langle X,\nu \rangle $
vanishes and so the Hsiung–Minkowski (2.5) formula becomes
which is a contradiction since f and
$H_{r-1}$
are positive. Hence,
$\nu $
is parallel to
${\partial }/{\partial t}$
and so
$\Sigma $
is a slice
$\{t_1\}\times N$
, which concludes the proof.
We finish by noting that
$t_1$
can be explicitly given by the constant c. Indeed, since
$\Sigma $
is a slice, we have equality in the sequence of inequalities in (2.2), that is,
Hence, the assumption
gives
$c={1}/{H^{r-s}}$
. Moreover, the Brendle identity (2.4) becomes
and so
$t_1$
is the unique positive real number so that