Fall 2022 Colloquium Schedule

Wednesday, August 31, 2022

Raffi Budakian, University of Waterloo

Nuclear Magnetic Resonance Diffraction

 

Wednesday, September 7, 2022

Hui Li, Los Alamos National Laboratory

Binary Stellar Mass Black Holes in AGN Disks as Possible LIGO Sources

 

Wednesday, September22, 2022

Shri Kulkarni, Caltach

The far ultra-violet background

 

Wednesday, October 5, 2022

Hans Rinderknecht, UR Laboratory for Laser Energetics

Relativistically Transparent Magnetic Filaments: short-pulse laser experiments for ultra strong-field physics

 

Wednesday, October 12, 2022

Gerald Dunne, University of Connecticut

Decoding the Path Integral: Resurgence and Extreme Physics

 

Monday, October 17, 2022

Tessa Fisher, Arizona State University

Atmospheric Chemical Reaction Network Topology as a Tool For Understanding

Exoplanet Atmospheres

 

Wednesday, October 19, 2022

Hannes Bernien, University of Chicago

Building quantum processors and quantum networks atom-by-atom

 

Thursday, October 20, 2022

Gerd Leuchs, MPI for Light ?????????

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Monday, October 31, 2022

Ryan MacDonald, University of Michigan

Exoplanet Atmospheric Retrieval in the Era of JWST

 

 

Wednesday, November 9, 2022

Yannick Meurice, University of Iowa

Quantum simulation of scalar electrodynamics with Rydberg atoms

 

Wednesday, November 16, 2022

Alec Kirkley, University of Hong Kong

Complex network inference: Efficient algorithms and insights for urban spatial segregation

 

Monday, November 28, 2022

Abel Mendez, University of Puerto Rico at Arecibo

Habitability models applied to planets and exoplanets

 

Wednesday, November 30, 2022

Suxing Hu, UR Laboratory for Laser Energetics

Understanding High-Energy-Density Physics Through ab initio Calculations

 

Wednesday, December 7, 2022

Dan Watson, University of Rochester Physics Department

Protostars, birthplaces, and their interactions

Wednesday, December 14, 2022

Carolyn Kuranz, University of Michigan

Creating Astrophysically Relevant Systems in the Laboratory in the Highly-Radiative,

High-Energy-Density Regime