Uniqueness of the non-singular family and characterisation of cosmological models

Simple item page
dc.creatorDadhich, Naresh
dc.creatorPatel, L. K.
dc.date1994-06-21
dc.date1994-09-02
dc.date.accessioned2026-07-07T08:59:24Z
dc.date.available2026-07-07T08:59:24Z
dc.descriptionWe prove that for an orthogonal spacetime metric separable in space and time in comoving coordinates, the requirements of perfect fluid and non-singularity single out the unique family of singularity free cosmological models. Further homogeneous models could only be Bianchi I or FLRW while inhomogeneous ones can be with or without a singularity.
dc.descriptionTeX pages 13, IUCAA-14/94
dc.identifierhttps://arxiv.org/abs/gr-qc/9406034
dc.identifierhttp://arxiv.org/abs/gr-qc/9406034
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147699
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleUniqueness of the non-singular family and characterisation of cosmological models
dc.typetext

Files

Collections

arXiv