Gravitational Waves from Gravitational Collapse

Abstract

Gravitational wave emission from the gravitational collapse of massive stars has been studied for more than three decades. Current state of the art numerical investigations of collapse include those that use progenitors with 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 advanced ground--based and future space--based interferometric observatories.

68 pages including 13 figures; revised version accepted for publication in Living Reviews in Relativity (http://www.livingreviews.org)

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• Non-linear axisymmetric pulsations of rotating relativistic stars in the conformal flatness approximation
• "Mariage des Maillages": A new numerical approach for 3D relativistic core collapse simulations
• All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run
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• Neutrinos from Supernovae as a Trigger for Gravitational Wave Search
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• Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves
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