Gravitational Waves from Gravitational Collapse

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/8618

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DC Field	Value	Language
dc.creator	New Kimberly C.B.	-
dc.date	2003	-
dc.date.accessioned	2013-06-01T11:40:20Z	-
dc.date.available	2013-06-01T11:40:20Z	-
dc.date.issued	2013-06-01	-
dc.identifier	http://www.livingreviews.org/lrr-2003-2	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=14338351&date=2003&volume=6&issue=&spage=2	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/8618	-
dc.description	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 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.	-
dc.publisher	Albert Einstein Institut, Max-Planck Institute for Gravitati	-
dc.source	Living Reviews in Relativity	-
dc.subject	Gravitational Waves	-
dc.title	Gravitational Waves from Gravitational Collapse	-
Appears in Collections:	Physics and Astronomy

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