Gravitational Waves from Gravitational Collapse
Abstract
Gravitational-wave emission from stellar collapse has been studied for nearly four decades. Current state-of-the-art numerical investigations of collapse include those that use progenitors with more realistic angular momentum profiles, properly treat microphysics issues, account for general relativity, and examine non-axisymmetric effects in three dimensions. Such simulations predict that gravitational waves from various phenomena associated with gravitational collapse could be detectable with ground-based and space-based interferometric observatories. This review covers the entire range of stellar collapse sources of gravitational waves: from the accretion-induced collapse of a white dwarf through the collapse down to neutron stars or black holes of massive stars to the collapse of supermassive stars.
- Authors:
-
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Publication Date:
- Research Org.:
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 810413
- Report Number(s):
- LA-UR-02-3583
Journal ID: ISSN 2367-3613
- Grant/Contract Number:
- W-7405-ENG-36
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Living Reviews in Relativity
- Additional Journal Information:
- Journal Volume: 6; Journal Issue: 1; Journal ID: ISSN 2367-3613
- Publisher:
- Springer Nature
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 79 ASTRONOMY AND ASTROPHYSICS; Black Hole; Neutron Star; Gravitational Wave; White Dwarf; Core Collapse
Citation Formats
Fryer, Chris L., and New, Kimberly C. B. Gravitational Waves from Gravitational Collapse. United States: N. p., 2003.
Web. doi:10.12942/lrr-2003-2.
Fryer, Chris L., & New, Kimberly C. B. Gravitational Waves from Gravitational Collapse. United States. https://doi.org/10.12942/lrr-2003-2
Fryer, Chris L., and New, Kimberly C. B. Mon .
"Gravitational Waves from Gravitational Collapse". United States. https://doi.org/10.12942/lrr-2003-2. https://www.osti.gov/servlets/purl/810413.
@article{osti_810413,
title = {Gravitational Waves from Gravitational Collapse},
author = {Fryer, Chris L. and New, Kimberly C. B.},
abstractNote = {Gravitational-wave emission from stellar collapse has been studied for nearly four decades. Current state-of-the-art numerical investigations of collapse include those that use progenitors with more realistic angular momentum profiles, properly treat microphysics issues, account for general relativity, and examine non-axisymmetric effects in three dimensions. Such simulations predict that gravitational waves from various phenomena associated with gravitational collapse could be detectable with ground-based and space-based interferometric observatories. This review covers the entire range of stellar collapse sources of gravitational waves: from the accretion-induced collapse of a white dwarf through the collapse down to neutron stars or black holes of massive stars to the collapse of supermassive stars.},
doi = {10.12942/lrr-2003-2},
journal = {Living Reviews in Relativity},
number = 1,
volume = 6,
place = {United States},
year = {2003},
month = {3}
}
Figures / Tables:

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