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Shear-free perfect fluids in general relativity: IV. Petrov type III spacetimes
Version 2 2024-06-18, 06:19
Version 1 2019-07-22, 09:28
journal contribution
posted on 2024-06-18, 06:19 authored by J Carminati, S CyganowskiIt is shown that for any Petrov type III, shear-free, perfect-fluid solution of Einstein's field equations, in which the perfect fluid satisfies a barotropic equation of state p = p(w) such that w + p ≢ 0, the fluid volume expansion is zero. In addition, the fluid must necessarily be rotating.
History
Journal
Classical and quantum gravityVolume
14Pagination
1167-1181Location
Bristol, Eng.Publisher DOI
ISSN
0264-9381Language
engPublication classification
C1.1 Refereed article in a scholarly journalCopyright notice
1997, IOP Publishing LtdIssue
5Publisher
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