Self-gravitating fluids in cylindrically-symmetric non-static space-time

Details Self-gravitating fluids in cylindrically-symmetric non-static space-time Self-gravitating fluids in cylindrically-symmetric non-static space-time

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.116..389n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 116, no. 2, Nov. 1985, p. 389-394.

Mathematics

Einstein Equations, Gravitation Theory, Ideal Fluids, Space-Time Functions, Field Theory (Physics), Transformations (Mathematics)

Scientific paper

In this paper we have obtained a cylindrically symmetric non-static
model of the perfect fluid distribution, satisfying one of the Petrov
type D conditions. This turned out to be a FRW model

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