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Generation of gravitational waves: the post-Newtonian spin octupole moment

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dc.contributor.authorDamour, Thibault
dc.contributor.authorIyer, B R
dc.date.accessioned2007-07-12T11:20:20Z
dc.date.available2007-07-12T11:20:20Z
dc.date.issued1994-05
dc.descriptionRestricted Access.en
dc.description.abstractUsing the gravitational wave generation formalism developed by Blanchet, Damour and Iyer, this paper computes the post-Newtonian-accurate spin octupole moment. The result is checked by explicitly verifying the transformation of the radiative spin octupole moment under shifts of the spatial origin.en
dc.format.extent182859 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationClassical and Quantum Gravity, 1994, Vol.11, p1353-1357en
dc.identifier.issn0264-9381
dc.identifier.urihttp://hdl.handle.net/2289/3250
dc.language.isoenen
dc.publisherIOP Publishing Ltden
dc.relation.urihttp://dx.doi.org/10.1088/0264-9381/11/5/021en
dc.rights1994 IOP Publishing Ltd.en
dc.titleGeneration of gravitational waves: the post-Newtonian spin octupole momenten
dc.typeArticleen

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