Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4169
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dc.contributor.authorIyer, B.R.-
dc.date.accessioned2011-09-30T03:54:37Z-
dc.date.available2011-09-30T03:54:37Z-
dc.date.issued2011-09-
dc.identifier.citationInternational Journal of Modern Physics D, 2011, Vol.10, p2081en
dc.identifier.issn0218-2718-
dc.identifier.issn1793-6594 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/4169-
dc.descriptionRestricted Accessen
dc.description.abstractOver 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.language.isoenen
dc.publisherWorld Scientific Publishingen
dc.relation.urihttp://dx.doi.org/10.1142/S0218271811020214en
dc.relation.urihttp://adsabs.harvard.edu/abs/2011Prama..77..119Ien
dc.rights2011 World Scientific Publishing.en
dc.subjectBinary black holesen
dc.subjectgravitational wavesen
dc.subjecteffective-one-bodyen
dc.titleGravitational waveforms for binary black holesen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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