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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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SEQUENCE:1
UID:UW-Physics-Event-6601
DTSTART:20210921T190000Z
DTEND:20210921T200000Z
DTSTAMP:20260414T192154Z
LAST-MODIFIED:20210920T195337Z
LOCATION:https://berkeley.zoom.us/j/99464252867
SUMMARY:Transport in Neutron Star Mergers\, Network in Neutrinos\, Nuc
 lear Astrophysics\, and Symmetries (N3AS) Seminar\, Alexander Haber\, 
 Washington University in St. Louis
DESCRIPTION:Transport processes in hot and dense matter are an importa
 nt way to improve our understanding of fundamental interactions and mi
 ght be accessible via gravitational wave observations. In this talk I 
 will especially focus on modified and direct Urca processes in nuclear
  matter under conditions that we expect in binary neutron star mergers
 . Nuclear Urca processes have shown to be a potential significant sour
 ce of bulk viscosity under merger conditions. I will explain how a cor
 rect relativistic treatment can alter the rates and the true beta equi
 librium significantly. 
URL:https://www.physics.wisc.edu/events/?id=6601
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