Online learning is a popular framework for sequential prediction
problems. The standard approach to analyzing an algorithm's
(learner's) performance in online learning is in terms of its
empirical regret defined to be the excess loss suffered by
the...
We make the case that over the coming decade, computer assisted
reasoning will become far more widely used in the mathematical
sciences. This includes interactive and automatic theorem
verification, symbolic algebra, and emerging technologies
such...
The importance of analyzing big data and in particular very
large networks has shown that the traditional notion of a fast
algorithm, one that runs in polynomial time, is often insufficient.
This is where property testing comes in, whose goal is to...
Given an increasing family F in {0,1}^n, its measure according
to mu_p increases and often exhibits a threshold behavior, growing
quickly as p increases from near 0 to near 1 around a specific
value p_c. Thresholds of families have been of great...
In this talk I will outline recent work in collaboration with
Pierre Germain, Zaher Hani and Jalal Shatah regarding a rigorous
derivation of the kinetic wave equation. The proof presented will
rely of methods from PDE, statistical physics and number...
Due to its importance in materials science where it models the
slow relaxation of grain boundaries, multiphase mean curvature flow
has received a lot of attention over the last decades.
In this talk, I want to present two theorems. The first one
is...
Symplectic geometry, and its close relative contact geometry,
are geometries closely tied to complex geometry, smooth topology,
and mathematical physics. The h-principle is a general method used
for construction of smooth geometric objects...
We develop a framework for graph sparsification and sketching,
based on a new tool, short cycle decomposition -- a decomposition
of an unweighted graph into an edge-disjoint collection of short
cycles, plus a small number of extra edges. A simple...
I will discuss an upcoming result proving the full
finite-codimension non-linear asymptotic stability of the
Schwarzschild family as solutions to the Einstein vacuum equations
in the exterior of the black hole region.