Slowly rotating cosmological perfect fluids in Brans-Dicke theory

Details Slowly rotating cosmological perfect fluids in Brans-Dicke theory Slowly rotating cosmological perfect fluids in Brans-Dicke theory

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.185..181s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 185, no. 2, Nov. 1991, p. 181-187.

Astronomy and Astrophysics

Astrophysics

Cosmology, Ideal Fluids, Rotating Fluids, Angular Velocity, Physical Properties, Space-Time Functions

Scientific paper

The Brans-Dicke field equations for a perfect fluid distribution
representing slowly rotating fluid spheres are investigated. Exact
solutions are obtained for differential rotation and perfect dragging by
imposing some physical restrictions on the matter rotation omega(r, t).
The physical properties are discussed for k = +/-1.

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