High frequency sources of gravitational waves
Kostas D. Kokkotas
TL;DR
This paper reviews potential high frequency gravitational wave sources like collapses and instabilities, emphasizing how their signals can reveal details about stellar evolution and the physics of compact objects.
Contribution
It provides a comprehensive overview of high frequency gravitational wave sources and discusses how their signals can inform us about stellar collapse and neutron star physics.
Findings
Gravitational collapse and instabilities are key high frequency sources.
Gravitational wave signals can reveal details of stellar evolution.
Signals provide insights into the equations of state of compact objects.
Abstract
Sources of high frequency gravitational waves are reviewed. Gravitational collapse, rotational instabilities and oscillations of the remnant compact objects are potentially important sources of gravitational waves. Significant and unique information for the various stages of the collapse, the evolution of protoneutron stars and the details of the equations of state of such objects can be drawn from careful study of the gravitational wave signal.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.