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PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-9221
DTSTART:20250506T190000Z
DURATION:PT1H0M0S
DTSTAMP:20260413T164435Z
LAST-MODIFIED:20250501T183215Z
LOCATION:Join Zoom Meeting: https://berkeley.zoom.us/j/96596967335?pwd
 =dvtmkV9xltHbaRp3EmL2ajBpKcvjSp.1   Meeting ID: 965 9696 7335
SUMMARY:Toward understanding supranuclear-density matter with gravitat
 ional waves\, Network in Neutrinos\, Nuclear Astrophysics\, and Symmet
 ries (N3AS) Seminar\, Koutarou Kyutoku \, Chiba University
DESCRIPTION:Properties of supranuclear-density matter governed by quan
 tum chromodynamics (QCD) are yet to be understood. One of the most imp
 ortant problems is how hadronic matter transitions to quark matter as 
 the density increases. Neutron stars serve as a natural laboratory to 
 solve these problems\, and gravitational waves emitted by binary neutr
 on stars are among the promising tools. In particular\, post merger gr
 avitational waves will tell us about the densest matter in the univers
 e. In this talk\, after briefly reviewing current constraints on the e
 quation of state\, I will discuss future prospects for understanding Q
 CD phase structure mainly based on our numerical-relativity simulation
 s.<br>\n <br>\n<br>\nNOTE: All participants and hosts are now required
  to sign into a Zoom account prior to joining meetings hosted by UC Be
 rkeley.<br>\n
URL:https://www.physics.wisc.edu/events/?id=9221
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