Stanford University

Upcoming Events

Friday, April 26, 2024
11:00 AM
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384I
Selim Amar (Stanford)

We will move from the local to the global theory of FIOs, providing invariant definitions of relevant notions such as operator symbols. The necessary tools from symplectic geometry will be introduced. If time permits, we'll begin considering some applications.

Friday, April 26, 2024
11:00 AM
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384H
Leo Zepeda (Wisconsin-Madison and Google)

The advent of generative AI has turbocharged the development of a myriad of commercial applications, and it has slowly started to permeate to scientific computing. In this talk we discussed how recasting the formulation of old and new problems within a probabilistic approach opens the door to…

Friday, April 26, 2024
12:30 PM
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384I
Eric Kilgore

Student Spectral Sequences Seminar

Friday, April 26, 2024
4:00 PM
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383N
Fred Rajasekaran (Stanford)

Abstract

Monday, April 29, 2024
11:00 AM
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384H

The Riemann integral does not work well with limits, so naturally one wishes to make something better. Thus, every high school or undergraduate math student should attempt to develop a better integral before learning any measure theory. Naturally, they come up with many strange ways to do it,…

Monday, April 29, 2024
2:30 PM
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383N
Sean Cotner (Michigan)

There have been several recent approaches to defining a moduli space of L-parameters over Z[1/p], in order to obtain refined versions of the local Langlands conjecture ``at all primes away from p at once''. The components of this space are expected to be closely related to blocks in the category…

Monday, April 29, 2024
4:00 PM
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Sequoia 200
Jacob Fox (Stanford)

Various random graphs models satisfy that each edge appears independently of all other edges but those in a bounded degree graph. Examples include Erdös–Renyi random graphs, random Cayley graphs, random Latin square graphs, and random entangled graphs. We begin the systematic study of random…

Tuesday, April 30, 2024
4:00 PM
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384H
Maxime Van de Moortel (Rutgers)

Abstract: It is expected that the Klein-Gordon equation on a Schwarzschild black hole behaves very differently from the wave equation at late-time, due to the presence of stable (timelike) trapping. We present our recent work demonstrating that despite the presence of stable timelike trapping on…

Tuesday, April 30, 2024
4:00 PM
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383N
Maggie Miller (UT Austin)

Abstract

Wednesday, May 1, 2024
12:00 PM
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384H
Andrea Montanari (Stanford)

Abstract