Gravitational waveforms for binary black holes

dc.contributor.author	Iyer, B R
dc.date.accessioned	2011-09-30T03:54:37Z
dc.date.available	2011-09-30T03:54:37Z
dc.date.issued	2011-09
dc.description	Restricted Access	en
dc.description.abstract	Over the last decade gravitational waveforms of binary black holes have been investigated using a variety of approaches like the Multipolar post-Minkowskian formalism, Numerical Relativity and the Effective-One-Body method. We review these complementary approaches and summarize the current status of these investigations of relevance to construct the best templates for the next generation Advanced gravitational wave detectors.	en
dc.identifier.citation	International Journal of Modern Physics D, 2011, Vol.10, p2081	en
dc.identifier.issn	0218-2718
dc.identifier.issn	1793-6594 (online)
dc.identifier.uri	http://hdl.handle.net/2289/4169
dc.language.iso	en	en
dc.publisher	World Scientific Publishing	en
dc.relation.uri	http://dx.doi.org/10.1142/S0218271811020214	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2011Prama..77..119I	en
dc.rights	2011 World Scientific Publishing.	en
dc.subject	Binary black holes	en
dc.subject	gravitational waves	en
dc.subject	effective-one-body	en
dc.title	Gravitational waveforms for binary black holes	en
dc.type	Article	en

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