A class of solutions of Einstein's equations for the interior of a rigidly rotating perfect fluid

Kyriakopoulos, E

dc.contributor.author	Kyriakopoulos, E	en
dc.date.accessioned	2014-03-01T01:07:01Z
dc.date.available	2014-03-01T01:07:01Z
dc.date.issued	1988	en
dc.identifier.issn	0001-7701	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/9755
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Physics, Multidisciplinary	en
dc.subject.classification	Physics, Particles & Fields	en
dc.title	A class of solutions of Einstein's equations for the interior of a rigidly rotating perfect fluid	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF00758118	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF00758118	en
heal.language	English	en
heal.publicationDate	1988	en
heal.abstract	A general class of solutions of Einstein's equations for the interior of a rigidly rotating axisymmetric perfect fluid is presented, which depends on an arbitrary function. To get solutions explicitly one has to calculate two integrals involving the arbitrary function. The equipressure surfaces of all solutions of the class are spheres or planes. A family of solutions, which depend on four arbitrary real constants, is calculated explicitly. The solution of the family, which is obtained if we assign a specific value to one of its parameters, and which was found before, is futher generalized with the addition of one more parameter. © 1988 Plenum Publishing Corporation.	en
heal.publisher	Kluwer Academic Publishers-Plenum Publishers	en
heal.journalName	General Relativity and Gravitation	en
dc.identifier.doi	10.1007/BF00758118	en
dc.identifier.isi	ISI:A1988N552700002	en
dc.identifier.volume	20	en
dc.identifier.issue	5	en
dc.identifier.spage	427	en
dc.identifier.epage	436	en