Padé approximants for gravitational waves from inspiralling compact binaries

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2772

Full metadata record

DC Field	Value	Language
dc.contributor.author	Damour, Thibault	-
dc.contributor.author	Iyer, B.R.	-
dc.contributor.author	Sathyaprakash, B.S.	-
dc.date.accessioned	2007-06-13T06:31:46Z	-
dc.date.available	2007-06-13T06:31:46Z	-
dc.date.issued	2001	-
dc.identifier.citation	Proceedings of the 10th workshop on general relativity and gravitation in Japan. Eds. M Sasaki et al. 2001, p49-59	en
dc.identifier.uri	http://hdl.handle.net/2289/2772	-
dc.description	Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)	en
dc.description.abstract	Pad\'e approximants to truncated post-Newtonian neutron star models are constructed. The Pad\'e models converge faster to the general relativistic (GR) solution than the truncated post-Newtonian ones. The evolution of initial data using the Pad\'e models approximates better the evolution of full GR initial data than the truncated Taylor models. In the absence of full GR initial data (e.g., for neutron star binaries or black hole binary systems), Pad\'e initial data could be a better option than the straightforward truncated post-Newtonian (Taylor) initial data.	en
dc.format.extent	9023292 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.relation.uri	http://arxiv.org/abs/gr-qc/0002094	en
dc.title	Padé approximants for gravitational waves from inspiralling compact binaries	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

Files in This Item:

File	Description	Size	Format
2001 GRG Proc. p49.pdf Restricted Access	Restricted Access.	8.81 MB	Adobe PDF	View/Open Request a copy