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Title: 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:
 [1];  [1]
  1. 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}
}

Journal Article:
Free Publicly Available Full Text
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Figure 1 Figure 1: Diagram of the convective engine for supernova explosions.

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