Padé approximants for truncated post-Newtonian neutron star models

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1315

Full metadata record

DC Field	Value	Language
dc.contributor.author	Gupta, Anshu	-
dc.contributor.author	Gopakumar, A.	-
dc.contributor.author	Iyer, B.R.	-
dc.contributor.author	Iyer, Sai	-
dc.date.accessioned	2006-06-08T05:59:24Z	-
dc.date.available	2006-06-08T05:59:24Z	-
dc.date.issued	2000-08-15	-
dc.identifier.citation	Physical Review D, 2000, Vol.62, 044038	en
dc.identifier.issn	1550-2368 (online)	-
dc.identifier.issn	1550-7998	-
dc.identifier.uri	http://hdl.handle.net/2289/1315	-
dc.description.abstract	Padé approximants to truncated post-Newtonian neutron star models are constructed. The Padé models converge faster to the general relativistic (GR) solution than the truncated post-Newtonian ones. The evolution of initial data using the Padé 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), Padé initial data could be a better option than the straightforward truncated post-Newtonian (Taylor) initial data.	en
dc.format.extent	158005 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/PRD/v62/e044038	en
dc.rights	(2000) by the American Physical Society	en
dc.title	Padé approximants for truncated post-Newtonian neutron star models	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

Files in This Item:

File	Description	Size	Format
2000 PR-D.62.P044038.pdf	11p.	154.3 kB	Adobe PDF	View/Open