Gravitational Waves from Gravitational Collapse

Fryer, Chris L.; New, Kimberly C.  B.

doi:10.12942/lrr-2003-2

Title: Gravitational Waves from Gravitational Collapse

Journal Article · Mon Mar 10 00:00:00 EST 2003 · Living Reviews in Relativity

DOI:https://doi.org/10.12942/lrr-2003-2· OSTI ID:810413

Fryer, Chris L. ^[1]; New, Kimberly C. B. ^[1]

Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

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.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE

Grant/Contract Number:: W-7405-ENG-36

OSTI ID:: 810413

Report Number(s):: LA-UR-02-3583

Journal Information:: Living Reviews in Relativity, Vol. 6, Issue 1; ISSN 2367-3613

Publisher:: Springer NatureCopyright Statement

Country of Publication:: United States

Language:: English

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The Rates of Hypernovae and Gamma-Ray Bursts: Implications for their Progenitors Podsiadlowski, Ph.; Mazzali, P. A.; Nomoto, K. arXiv https://doi.org/10.48550/arxiv.astro-ph/0403399	text	January 2004
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Binary Merger Progenitors for Gamma-Ray Bursts and Hypernovae Fryer, Chris L.; Heger, Alexander arXiv https://doi.org/10.48550/arxiv.astro-ph/0412024	text	January 2004
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The Spherical Accretion Shock Instability in the Linear Regime Blondin, John M.; Mezzacappa, Anthony arXiv https://doi.org/10.48550/arxiv.astro-ph/0507181	text	January 2005
Multi-Dimensional Radiation/Hydrodynamic Simulations of Protoneutron Star Convection Dessart, L.; Burrows, A.; Livne, E. arXiv https://doi.org/10.48550/arxiv.astro-ph/0510229	text	January 2005
A New Mechanism for Core-Collapse Supernova Explosions Burrows, Adam; Livne, Eli; Dessart, Luc arXiv https://doi.org/10.48550/arxiv.astro-ph/0510687	text	January 2005
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Core-Collapse Simulations of Rotating Stars Fryer, C. L.; Heger, A. arXiv https://doi.org/10.48550/arxiv.astro-ph/9907433	text	January 1999
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