Explore the constraints on nuclear matter equation of state derived from gravitational wave observations in this 35-minute conference talk by Wolfgang Kastaun at the International Centre for Theoretical Sciences. Delve into topics including inspiral parameter space, measurable EOS aspects for GW170817, model-agnostic studies, universal relations, and EOS model selection. Examine the implications of remnant type, kilonova modeling, short gamma-ray burst models, and numerical simulations. Learn about emerging avenues for research such as post-merger signals and searches for p-g mode effects. Gain insights into the future challenges and opportunities in gravitational wave astronomy as discussed in this panel from the "Future of Gravitational-Wave Astronomy" meeting.
Nuclear Matter EOS Constraints from Gravitational Waves by Wolfgang Kastaun
International Centre for Theoretical Sciences via YouTube
Overview
Syllabus
Nuclear matter EOS constraints from GW
Outline
Inspiral Parameter Space
Impact of Parameters
Measurable EOS Aspects For GW170817 Maximum NS mass _ 1.36Mo
Model-Agnostic Study
Universal Relations Studies
Parametrization
Evidence for Tidal Effects?
EOS Model Selection Study
Implication of Remnant Type
Implication of Remnant Type Recent analysis [Shibata et al, Phys. Rev. 100 2019] Less assumptions
Kilonova
Mass ejection
Kilonova Modeling
Constraints from Kilonova
Short Gamma Ray Burst Models
Numerical Simulations
Other Avenues
Post-Merger Signal
Searching p-g effects
Appendix
Q&A
Taught by
International Centre for Theoretical Sciences
