Gravitational Waves from Gravitational Collapse

Chris L. Fryer  
Los Alamos National Laboratory
MS D409, CCS-2
Los Alamos, New Mexico 87545, U.S.A.

and
Kimberly C. B. New  
Los Alamos National Laboratory
MS T087, X-4
Los Alamos, New Mexico 87545, U.S.A.

Major update of lrr-2003-2 (see article history and change log for details.)

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.


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