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 · 10 March 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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