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PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-8049
DTSTART:20221206T200000Z
DURATION:PT1H0M0S
DTSTAMP:20260414T122623Z
LAST-MODIFIED:20221130T142742Z
LOCATION:Join Zoom Meeting https://berkeley.zoom.us/j/91230714547  Mee
 ting ID: 912 3071 4547
SUMMARY:Gravitational-wave signatures of dense matter in neutron star 
 binary inspirals  \, Network in Neutrinos\, Nuclear Astrophysics\, and
  Symmetries (N3AS) Seminar\, Tanja Hinderer \, Institute for Theoretic
 al Physics\, Utrecht University
DESCRIPTION:The gravitational waves from merging binary systems carry 
 unique information about the internal structure of neutron stars. Extr
 acting and interpreting this information requires accurate models base
 d on a detailed understanding of the interplay of matter with nonlinea
 r gravity. I will outline recent progress on going beyond the dominant
  tidal deformability effects and discuss examples of the impact of inc
 orporating more realistic physics. I will conclude with an outlook ont
 o the remaining challenges and prospects for the coming years\, as gra
 vitational-wave science continues to move towards an era of precision 
 physics.<br>\n <br>\n
URL:https://www.physics.wisc.edu/events/?id=8049
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