14:30
Internal instabilities in ice-sheets: thermally-induced runaways and their interactions with glacier mechanics
14:30
Devil in the detail: imaging sub-glacial landforms using high-resolution radar surveys of the Antarctic ice sheet
Constant scalar curvature orbifold metrics and stability of orbifolds through embeddings in weighted projective spaces
Abstract
There is a conjectural relationship due to Yau-Tian-Donaldson between stability of projective manifolds and the existence of canonical Kahler metrics (e.g. Kahler-Einstein metrics). Embedding the projective manifold in a large projective space gives, on one hand, a Geometric Invariant Theory stability problem (by changing coordinates on the projective space) and, on the other, a notion of balanced metric which can be used to approximate the canonical Kahler metric in question. I shall discuss joint work with Richard Thomas that extends this framework to orbifolds with cyclic quotient singularities using embeddings in weighted projective space, and examples that show how several obstructions to constant scalar curvature orbifold metrics can be interpreted in terms of stability.
Hidden symmetries and higher-dimensional rotating black holes
Abstract
The 4D rotating black hole described by the Kerr geometry possesses many of what was called by Chandrasekhar "miraculous" properties. Most of them can be related to the existence of a fundamental hidden symmetry called the principal conformal Killing-Yano (PCKY) tensor. In my talk I shall demonstrate that, in this context, four dimensions are not exceptional and that the (spherical horizon topology) higher-dimensional rotating black holes are very similar to their four-dimensional cousins. Namely, I shall present the most general spacetime admitting the PCKY tensor and show that is possesses the following properties: 1) it is of the algebraic type D, 2) it allows a separation of variables for the Hamilton-Jacobi, Klein-Gordon, Dirac, gravitational, and stationary string equations, 3) the geodesic motion in such a spacetime is completely integrable, 4) when the Einstein equations with the cosmological constant are imposed the metric becomes the Kerr-NUT-(A)dS spacetime. Some of these properties remain valid even when one includes the electromagnetic field.
Berry Phase and Supersymmetry
Abstract
Approximate groups
Abstract
Let $A$ be a finite set in some ambient group. We say that $A$ is a $K$-approximate group if $A$ is symmetric and if the set $A.A$ (the set of all $xy$, where $x$, $y$ lie in $A$) is covered by $K$ translates of $A$. I will illustrate this notion by example, and will go on to discuss progress on the "rough classification" of approximate groups in various settings: abelian groups, nilpotent groups and matrix groups of fixed dimension. Joint work with E. Breuillard.
11:00
Homological Mirror Symmetry for the 4-torus
Abstract
I will describe joint work with Mohammed Abouzaid, in which we complete the proof of homological mirror symmetry for the standard four-torus and consider various applications. A key tool is the recently-developed holomorphic quilt theory of Mau-Wehrheim-Woodward.