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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. ELECTRONIC SUPPLEMENTARY MATERIAL:Supplementary material is available for this article at 10.12942/lrr-2011-1.

SUBMITTER: Fryer CL

PROVIDER: S-EPMC5255218 | biostudies-literature | 2011

REPOSITORIES: biostudies-literature

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Gravitational Waves from Gravitational Collapse.

Fryer Chris L CL New Kimberly C B KC

Living reviews in relativity 20110120 1

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 g ...[more]

PMID: 28163617

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Gravitational Waves from Gravitational Collapse.

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