Post-Newtonian gravitational radiation reaction for two-body systems

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1286

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DC Field	Value	Language
dc.contributor.author	Iyer, B.R.	-
dc.contributor.author	Will, C.M.	-
dc.date.accessioned	2006-05-23T06:52:12Z	-
dc.date.available	2006-05-23T06:52:12Z	-
dc.date.issued	1993-01-11	-
dc.identifier.citation	Physical Review Letters, 1993, Vol.70, 113-116	en
dc.identifier.issn	0031-9007 (print)	-
dc.identifier.uri	http://hdl.handle.net/2289/1286	-
dc.description.abstract	We study gravitational radiation reaction in the equations of motion for binary systems to post-Newtonian order [O(v/c)2] beyond the quadrupole approximation. The method uses post-Newtonian expressions for energy and angular momentum flux to infinity, and an assujption of energy and angular momentum balance. The equations of motion are valid for general binary orbits. We discuss the coordinate-system dependence of the radiation-reaction formula.	en
dc.format.extent	639874 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The American Physical Society	en
dc.relation.uri	http://link.aps.org/abstract/PRL/v70/p113	en
dc.rights	(1993) by the American Physical Society	en
dc.title	Post-Newtonian gravitational radiation reaction for two-body systems	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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