We study the global behavior of (weakly) stable constant mean
curvature hypersurfaces in general Riemannian manifolds. We show some
nonexistence of complete and noncompact hypersurfaces with
constant mean curvaure. By using harmonic function theory, we prove
some one-end theorems which are new even for constant mean curvature
hypersurfaces in space forms.
A Einstein metric is stable if the second variation of the total scalar curvature functional is nonpositive in the direction of changes in conformal structures. Using spin^c structure we prove that a compact Einstein metric with nonpositive scalar curvature admits a nonzero parallel spin$^c$ spinor is stable. In particular, all metrics with nonzero parallel spinor (these are Ricci flat with special holonomy such as Calabi-Yau and $G_2$) and Kahler-Einstein metrics with nonpositive scalar curvature are stable. In fact we show that metrics with nonzero parallel spinor are local maxima for the Yamabe invariant and any metric of positive scalar curvature cannot lie too close to them. Similar results also hold for Kahler-Einstein metrics with nonpositive scalar curvature. This is a joint work with Xianzhe Dai and Xiaodong Wang.
Let G be a finite abelian group. A zero-sum problem on G asks for
the smallest positive integer k such that for any sequence a_1,...,a_k
of elements of G there exists a subsequence of required length the sum of
whose terms vanishes. In this talk we will give a survey of problems and
results in this field. In particular, we will talk about Olson's theorem
on the Davenport constanst of an abelian p-group and Reiher's celebrated
proof of the Kemnitz conjecture.
The Euler-Poincare formula gives a relation between the local
properties of an l-adic sheaf (like ramification) and its global
properties (like the Euler characteristic). In this talk we will see how
to apply it to compute the rank of some pure exponential sums.
We introduce the constraint equations for the Einstein-scalar field system on compact manifolds. Using the conformal method we reformulate these equations as a determined system of nonlinear partial differential equations. By introducing a new conformal invariant, which is sensitive to the presence of the initial data for the scalar field, we are able to divide the set of free conformal data into subclasses depending on the possible signs for the coefficients of terms in the resulting Einstein-scalar field Lichnerowicz equation. For most of these subclasses we determine whether or not a solution exists. In contrast to other well studied field theories, there are certain cases, depending on the mean curvature and the potential of the scalar field, for which we are unable to resolve the question of existence of a solution. We consider this system in such generality so as to include the vacuum constraint equations with an arbitrary cosmological constant, the Yamabe equation and even (all cases of) the prescribed scalar curvature problem as special cases.
This is joint work with Yvonne Choquet-Bruhat and Jim Isenberg.
We are going to consider the general problem whether the sum of
two closed operators on a Banach space is closed on the
intersection of their domains. We introduce absolute functional
calculus for sectorial operators, which is stronger than
$H^\infty$-calculus. Using this technique, we prove a theorem of
Dore-Venni type for sums of closed operators. There, we are able
to remove any assumptions such as R-boundedness or BIP on one of
the operators given that the second operator has absolute
calculus. Moreover, we show that any sectorial operator has
absolute calculus on the real interpolation spaces between its
domain and the space itself.