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Network in Neutrinos, Nuclear Astrophysics, and Symmetries (N3AS) Seminar
Signature of a quark-hadron phase transition from g-mode oscillations in neutron stars
Date: Tuesday, June 15th
Time: 2:00 pm - 3:00 pm
Place: Zoom
Speaker: Prashanth Jaikumar, California State University Long Beach
Abstract: 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 sound speed in neutron stars and its application to g-mode oscillations as a promising signature of a mixed phase. I will also discuss estimates of g-mode damping in neutron/quark matter.
Host: Baha Balantekin
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