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

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

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cqgra..14.1167c&link_type=abstract

Classical and Quantum Gravity, Volume 14, Issue 5, pp. 1167-1181 (1997).

Physics

8

Scientific paper

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 0264-9381/14/5/020/img1 such
that 0264-9381/14/5/020/img2, the fluid volume expansion is zero. In
addition, the fluid must necessarily be rotating.

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