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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3250

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DC Field	Value	Language
dc.contributor.author	Damour, Thibault	-
dc.contributor.author	Iyer, B.R.	-
dc.date.accessioned	2007-07-12T11:20:20Z	-
dc.date.available	2007-07-12T11:20:20Z	-
dc.date.issued	1994-05	-
dc.identifier.citation	Classical and Quantum Gravity, 1994, Vol.11, p1353-1357	en
dc.identifier.issn	0264-9381	-
dc.identifier.uri	http://hdl.handle.net/2289/3250	-
dc.description	Restricted Access.	en
dc.description.abstract	Using 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.extent	182859 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	IOP Publishing Ltd	en
dc.relation.uri	http://dx.doi.org/10.1088/0264-9381/11/5/021	en
dc.rights	1994 IOP Publishing Ltd.	en
dc.title	Generation of gravitational waves: the post-Newtonian spin octupole moment	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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