An algebraically general, stationary, axisymmetric, perfect fluid solution of Einstein's equations

Bonanos, S; Kyriakopoulos, E

dc.contributor.author	Bonanos, S	en
dc.contributor.author	Kyriakopoulos, E	en
dc.date.accessioned	2014-03-01T01:09:42Z
dc.date.available	2014-03-01T01:09:42Z
dc.date.issued	1994	en
dc.identifier.issn	0264-9381	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/11149
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Physics, Multidisciplinary	en
dc.subject.classification	Physics, Particles & Fields	en
dc.subject.other	RELATIVITY	en
dc.subject.other	METRICS	en
dc.title	An algebraically general, stationary, axisymmetric, perfect fluid solution of Einstein's equations	en
heal.type	journalArticle	en
heal.identifier.primary	10.1088/0264-9381/11/2/001	en
heal.identifier.secondary	001	en
heal.identifier.secondary	http://dx.doi.org/10.1088/0264-9381/11/2/001	en
heal.language	English	en
heal.publicationDate	1994	en
heal.abstract	A three-parameter solution of Einstein's equations for the interior of a uniformly rotating, stationary, axisymmetric perfect fluid is presented. The solution is analytically simple, behaves properly on the axis, and has finite non-rotating and vacuum limits. It is algebraically general and has no higher symmetry. The equation of state is mu + 3p = 0, and the fluid's vorticity and acceleration vectors are parallel.	en
heal.publisher	IOP PUBLISHING LTD	en
heal.journalName	Classical and Quantum Gravity	en
dc.identifier.doi	10.1088/0264-9381/11/2/001	en
dc.identifier.isi	ISI:A1994NA11200001	en
dc.identifier.volume	11	en
dc.identifier.issue	2	en
dc.identifier.spage	L23	en
dc.identifier.epage	L28	en