Interior axisymmetric stationary perfect fluid solution of Einstein's equations

Kyriakopoulos, E

dc.contributor.author	Kyriakopoulos, E	en
dc.date.accessioned	2014-03-01T01:08:54Z
dc.date.available	2014-03-01T01:08:54Z
dc.date.issued	1992	en
dc.identifier.issn	0264-9381	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/10720
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Physics, Multidisciplinary	en
dc.subject.classification	Physics, Particles & Fields	en
dc.title	Interior axisymmetric stationary perfect fluid solution of Einstein's equations	en
heal.type	journalArticle	en
heal.identifier.primary	10.1088/0264-9381/9/1/019	en
heal.identifier.secondary	019	en
heal.identifier.secondary	http://dx.doi.org/10.1088/0264-9381/9/1/019	en
heal.language	English	en
heal.publicationDate	1992	en
heal.abstract	A solution of Einstein's equations for the interior of a rigidly rotating axisymmetric perfect fluid is presented, with an equation of state mu + 3p = 0. The equipressure surfaces are closed. The solution has a static limit. The metric functions of the line element of the solution, in the usual coordinates, are expressed in terms of the Weierstrass elliptic function.	en
heal.publisher	IOP PUBLISHING LTD	en
heal.journalName	Classical and Quantum Gravity	en
dc.identifier.doi	10.1088/0264-9381/9/1/019	en
dc.identifier.isi	ISI:A1992GZ75200019	en
dc.identifier.volume	9	en
dc.identifier.issue	1	en
dc.identifier.spage	217	en
dc.identifier.epage	223	en