Einstein's Field Equations for the Interior of a Uniformly Rotating Stationary Axisymmetric Perfect Fluid

Kyriakopoulos, E

dc.contributor.author	Kyriakopoulos, E	en
dc.date.accessioned	2014-03-01T01:50:44Z
dc.date.available	2014-03-01T01:50:44Z
dc.date.issued	2001	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/26094
dc.relation.uri	http://arxiv.org/abs/gr-qc/0102005	en
dc.subject	Energy Density	en
dc.subject	Partial Differential Equation	en
dc.subject	Second Order	en
dc.title	Einstein's Field Equations for the Interior of a Uniformly Rotating Stationary Axisymmetric Perfect Fluid	en
heal.type	journalArticle	en
heal.publicationDate	2001	en
heal.abstract	We reduce Einstein's field equations for the interior of a uniformlyrotating, axisymmetric perfect fluid to a system of six second order partialdifferential equations for the pressure p the energy density $\mu$ and fourdependent variables.Four of these equations do not depend on p and $\mu$and the other two determine p and $\mu$.	en