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VERSION:2.0
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PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-6462
DTSTART:20210615T190000Z
DTEND:20210615T200000Z
DTSTAMP:20260414T221018Z
LAST-MODIFIED:20210611T132623Z
LOCATION:Zoom https://berkeley.zoom.us/j/91922781599
SUMMARY:Signature of a quark-hadron phase transition from g-mode oscil
 lations in neutron stars\, Network in Neutrinos\, Nuclear Astrophysics
 \, and Symmetries (N3AS) Seminar\, Prashanth Jaikumar\, California Sta
 te University Long Beach
DESCRIPTION:Neutron stars contain matter at extremely high density and
  gravitational waves from neutron stars can help us discover new forms
  of matter. I will present my recent work on computing the adiabatic s
 ound speed in neutron stars and its application to g-mode oscillations
  as a promising signature of a mixed phase. I will also discuss estima
 tes of g-mode damping in neutron/quark matter.<br>
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URL:https://www.physics.wisc.edu/events/?id=6462
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