Seminars and Colloquia by Series

On the Stabilizing Effect of Fluid Expansion for Relativistic Gaseous Stars

Series
PDE Seminar
Time
Tuesday, February 10, 2026 - 15:30 for 1 hour (actually 50 minutes)
Location
Skiles 254
Speaker
Zhongtian HuPrinceton University

It is well-known that a spacetime which expands sufficiently fast can stabilize the fluid for relativistic/Einstein-fluid systems. One may wonder whether the expansion of the fluid, instead of the background spacetime geometry, is also able to achieve a similar stabilizing effect. As an attempt to address this question, we consider the free boundary relativistic Euler equations in Minkowski background M1+3 equipped with a physical vacuum boundary, which models the motion of relativistic gas. For the class of isentropic, barotropic, and polytropic gas, we construct an open class of initial data which launch future-global solutions. Such solutions are spherically symmetric, have small initial density, and expand asymptotically linearly in time. In particular, the asymptotic rate of expansion is allowed to be arbitrarily close to the speed of light. Therefore, our main result is far from a perturbation of existing results concerning the classical Euler counterparts. This is joint work with Marcelo Disconzi and Chenyun Luo.

The Guderley Problem: Existence of Self-Similar Converging and Diverging Shocks

Series
PDE Seminar
Time
Tuesday, February 3, 2026 - 15:30 for 1 hour (actually 50 minutes)
Location
Skiles 254
Speaker
Jiaqi LiuUniversity of Southern California

The Guderley problem describes the behavior of a strong self-similar shock wave propagating radially in an ideal gas. A spherical shock converges radially inwards to the spatial origin, strengthening as it collapses. At the collapse point, the shock's strength becomes infinite, leading to the formation of a new outgoing shock wave of finite strength, which then propagates outwards to infinity. 

In this talk, I will present recent work on the rigorous construction of the self-similar converging and diverging shock solutions for $\gamma \in (1,3]$. These solutions are analytic away from the shock interfaces and the blow-up point. The proof relies on continuity arguments, nonlinear invariances, and barrier functions.

Mass inflation for spherically symmetric charged black holes

Series
PDE Seminar
Time
Tuesday, January 20, 2026 - 15:30 for 1 hour (actually 50 minutes)
Location
Skiles 254
Speaker
Onyx Gautam Princeton University

The Reissner–Nordström spacetime models a spherically symmetric and time-independent charged black hole in general relativity. The Cauchy horizon in the interior of such a black hole is subject to an infinite blueshift instability. In 1989, Poisson and Israel discovered a nonlinear manifestation of this instability in the spherically symmetric setting called "mass inflation," where the Hawking mass becomes identically infinite at the Cauchy horizon. 

We complete the first proof of mass inflation for a wave-type matter model, namely the spherically symmetric Einstein–Maxwell–scalar field system. This result follows from a large-data decay result for the scalar field in the black hole exterior combined with works of Dafermos, Luk–Oh, and Luk–Oh–Shlapentokh-Rothman.

Analytical Approach To Continuous-Time Causal Optimal Transport

Series
PDE Seminar
Time
Tuesday, December 2, 2025 - 15:30 for 1 hour (actually 50 minutes)
Location
Skiles 154
Speaker
Ibrahim EkrenUniversity of Michigan

We study causal optimal transport problems with Markovian cost and prescribed Markovian marginal laws. We show that the associated value function solves a fully nonlinear parabolic PDE, for which we establish a comparison principle and, consequently, uniqueness of its viscosity solution. This PDE characterization allows us to identify the value with that of a constrained version of the control problem for the Kushner–Stratonovich equation. We also obtain a third equivalent optimal control formulation with a state constraint, which leads to implementable numerical schemes for causal optimal transport. This is joint ongoing work with Julio Backhoff, Erhan Bayraktar, and Antonios Zitridis.

Asymptotic stability of solitary waves for the 1D focusing cubic Schrödinger equation

Series
PDE Seminar
Time
Tuesday, November 18, 2025 - 15:30 for 1 hour (actually 50 minutes)
Location
Online: https://gatech.zoom.us/j/95574359880?pwd=cGpCa3J1MFRkY0RUeU1xVFJRV0x3dz09
Speaker
Yongming LiTexas A&M University

 In this talk we present a perturbative proof of the asymptotic stability of the solitary wave solutions for the 1D focusing cubic Schrödinger equation under small perturbations in weighted Sobolev spaces. The strategy of our proof is based on the space-time resonances approach based on the distorted Fourier transform and modulation techniques to capture the asymptotic behavior of the solution. A major difficulty throughout the nonlinear analysis is the slow local decay of the radiation term caused by the threshold resonances in the spectrum of the linearized operator around the solitary wave. The presence of favorable null structures in the quadratic terms mitigates this problem through the use of normal form transformations. 

Separation rates for non-unique Navier-Stokes flows

Series
PDE Seminar
Time
Tuesday, November 11, 2025 - 15:30 for 1 hour (actually 50 minutes)
Location
Skiles 154
Speaker
Zachary BradshawUniversity of Arkansas

 

Fluid models are used to make predictions about critical real-world systems arising in diverse fields including but not limited to meteorology, climate science, mechanical engineering, and geophysics. Simulations based on fluid models can, for example, be used to make predictions about the strength of a tornado or the stresses on an aircraft wing passing through turbulent air. The possibility that a mathematical model does not capture the full range of possible real-world scenarios is concerning if the predictions do not account for extreme events. It has been confirmed by computer assisted proof that the 3D Navier-Stokes equations possess non-unique solutions. The existence of such solutions can, in principle, pose a challenge to forecasters. This talk explores mathematical work aiming to quantify the rate at which non-unique solutions can separate.

Second-order PDEs on Wasserstein Space

Series
PDE Seminar
Time
Tuesday, November 4, 2025 - 15:30 for 1 hour (actually 50 minutes)
Location
Skiles 154
Speaker
Xin ZhangNew York University

Mean-field control with common noise and filtering problems naturally lead to second-order PDEs on Wasserstein space. In this talk, we analyze a class of such equations in which the second-order operator is finite-dimensional in nature. We establish comparison principles and apply them to obtain particle convergence rates in mean-field control. The talk is based on joint work with Erhan Bayraktar, Ibrahim Ekren, and Xihao He.

Extreme internal waves

Series
PDE Seminar
Time
Tuesday, October 28, 2025 - 15:30 for 1 hour (actually 50 minutes)
Location
Skiles 154
Speaker
Samuel Walsh University of Missouri
Internal waves are traveling waves that propagate along the interface dividing two immiscible fluids. In this talk, we discuss recent progress on rigorously constructing two related species of extreme internal waves: overturning bores and gravity currents. “Extreme" refers to the fact that there is a stagnation point on the interface, which allows for the boundary to be non-smooth. 

Hydrodynamic bores are front-type traveling wave solutions to the two-layer free boundary Euler equations in two dimensions. We  prove that there exists a family of bores that starts at trivial laminar flow where the interface is flat and continues until the interface develops a vertical tangent. This type of behavior was first observed over 45 years ago in computations of internal gravity waves and gravity water waves with vorticity via numerical continuation. Despite considerable progress over the past decade in constructing global families of water waves that potentially overturn, a rigorous proof that overturning definitively occurs has been stubbornly elusive.  

Gravity currents arise when a heavier fluid intrudes into a region of lighter fluid. Typical examples are muddy water flowing into a cleaner body of water and haboobs (dust storms). We give the first rigorous proof of a conjecture of von Kármán on the structure of gravity currents near the rigid boundary. 

This is joint work with Ming Chen (Pittsburgh) and Miles Wheeler (Bath)

Space-time nonlocal integrable systems

Series
PDE Seminar
Time
Tuesday, October 21, 2025 - 15:30 for 1 hour (actually 50 minutes)
Location
Skiles 154
Speaker
Ziad MusslimaniFlorida State University

In this talk we will review past and recent results pertaining to the emerging field of integrable space-time nonlocal nonlinear evolution equations. In particular, we will discuss blow-up in finite time of soliton solutions as well as the physical derivations of many integrable nonlocal systems.

Universality in the small-dispersion limit of the Benjamin-Ono equation

Series
PDE Seminar
Time
Tuesday, October 14, 2025 - 15:30 for 1 hour (actually 50 minutes)
Location
Skiles 154
Speaker
Peter MillerUniversity of Michigan

This talk concerns the Benjamin-Ono (BO) equation of internal wave theory, and properties of the solution of the Cauchy initial-value problem in the situation that the initial data is fixed but the coefficient of the nonlocal dispersive term in the equation is allowed to tend to zero (i.e., the zero-dispersion limit). It is well-known that existence of a limit requires the weak topology because high-frequency oscillations appear even though they are not present in the initial data.  Physically, this phenomenon corresponds to the generation of a dispersive shock wave. In the setting of the Korteweg-de Vries (KdV) equation, it has been shown that dispersive shock waves exhibit a universal form independent of initial data near the two edges of the dispersive shock wave, and also near the gradient catastrophe point for the inviscid Burgers equation from which the shock wave forms. In this talk, we will present corresponding universality results for the BO equation. These have quite a different character than in the KdV case; while for KdV one has universal wave profiles expressed in terms of solutions of Painlevé-type equations, for BO one instead has expressions in terms of classical Airy functions and Pearcey integrals. These results are proved for general rational initial data using a new approach based on an explicit formula for the solution of the Cauchy problem for BO. This is joint work with Elliot Blackstone and Matthew Mitchell, based on other work with Blackstone, Louise Gassot, and Patrick Gérard.

Pages