Shear-free perfect fluids in general relativity: IV. Petrov type III spacetimes

Carminati, John and Cyganowski, Sasha 1997, Shear-free perfect fluids in general relativity: IV. Petrov type III spacetimes, Classical and quantum gravity, vol. 14, no. 5, pp. 1167-1181, doi: 10.1088/0264-9381/14/5/020.

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Title Shear-free perfect fluids in general relativity: IV. Petrov type III spacetimes
Author(s) Carminati, John
Cyganowski, Sasha
Journal name Classical and quantum gravity
Volume number 14
Issue number 5
Start page 1167
End page 1181
Total pages 16
Publisher IOP Publishing
Place of publication Bristol, Eng.
Publication date 1997
ISSN 0264-9381
Keyword(s) Petrov type III
Einstein's field equations
Shear-free, perfect-fluid solution
Summary It 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.
Language eng
DOI 10.1088/0264-9381/14/5/020
Indigenous content off
Field of Research 02 Physical Sciences
01 Mathematical Sciences
HERDC Research category C1.1 Refereed article in a scholarly journal
Copyright notice ©1997, IOP Publishing Ltd
Persistent URL http://hdl.handle.net/10536/DRO/DU:30127934

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