"Gravitational Waves from Gravitational Collapse"
by
Chris L. Fryer and Kimberly C. B. New
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Abstract
1
Introduction
2
Gravitational Wave Emission
2.1
Making numerical estimates
3
Astrophysical Sources of Gravitational Wave Emission
3.1
Core-collapse supernovae
3.2
Accretion-induced collapse
3.3
Electron-capture supernovae and core-collapse supernovae below 10 – 12 solar masses: Low mass stars
3.4
Core-collapse supernovae from stars above 20 solar masses: Massive star collapse
3.5
Supermassive stars
4
Gravitational Wave Emission Mechanisms
4.1
Bounce
4.2
Convection
4.3
Bar modes
4.4
Neutrinos
4.5
r
-Modes
4.6
Fragmentation
4.7
Ringing
5
Summary
5.1
Detection of collapse GW signals
5.2
Using GWs to study core collapse
6
Acknowledgements
References
Footnotes
Updates
Figures