The conference will take place in Hodges Hall (Second Floor).
| Time | Event Title / Speaker / Details |
|---|---|
|
8:00 AM – 8:30 AM |
Registration and Breakfast |
|
8:30 AM – 9:15 AM |
Uniqueness and error estimates for 1D hyperbolic conservation laws
|
|
9:15 AM – 10:00 AM |
Viscous perturbations to discontinuous solutions of the compressible
Euler equation
|
|
10:00 AM – 10:20 AM |
Coffee Break |
|
10:20 AM – 11:05 AM |
Dynamics of gaseous stars
|
|
11:05 AM – 11:50 AM |
Gravity wave-borne vortices
|
|
12:00 PM – 2:00 PM |
Poster Session and Lunch |
|
2:00 PM – 2:45 PM |
Self-similar solutions to two-dimensional Riemann problems involving
transonic shocks
|
|
2:45 PM – 3:00 PM |
Coffee Break |
|
3:00 PM – 3:25 PM |
Accuracy of the finite volume approximations to nonlocal conservation
laws
On a thermodynamically consistent model for magnetoviscoelastic fluids
in 3D
|
|
3:25 PM – 3:50 PM |
Piecewise Smooth Solutions to Scalar Balance Laws with Singular Source
Terms
Exploring global solutions for the quasi-linear mKdV equations
|
|
3:50 PM – 4:15 PM |
Asymptotics of Helmholtz-Kirchhoff Point-Vortices in the Phase Space
Interface problem for the two-phase magnetohydrodynamic flows
|
|
4:15 PM – 4:40 PM |
Low Regularity Solutions for the Surface Quasi-Geostrophic Front Equation
Analysis of a multiscale interface coupling describing fluid flow between
a deformable porous media and a lumped hydraulic circuit
|
|
4:40 PM – 5:05 PM |
A Singular Family of 3D Quasi-Geostrophic Equation
Singularity for symmetric form of Ericksen-Leslie system of nematic liquid crystal flows in semi-linear case |
|
5:05 PM-5:30 PM |
On
self-similar converging shock waves |
| Time | Event Title / Speaker / Details |
|---|---|
|
8:00 AM – 8:30 AM |
Breakfast |
|
8:30 AM – 9:15 AM |
Hyperbolic and mixed-type problems in gas dynamics and geometry
|
|
9:15 AM – 10:00 AM |
Multiscale Interface Coupling of PDEs and ODEs for Tissue Perfusion
|
|
10:00 AM – 10:45 AM |
Global classical solution and singularity formation for supersonic expanding
solution for compressible Euler equations with radial symmetry
|
|
10:45 AM – 11:00 AM |
Closing |