Larry L Smalley and J P Krisch 1994 Class. Quantum Grav. 11 2375 doi:10.1088/0264-9381/11/9/017
Larry L Smalley
and J P Krisch![]()
We consider self-consistent spinning fluid cosmologies in both general relativity in Riemannian spacetimes and Einstein-Cartan theory in Riemann-Cartan spacetimes. First we extend slightly the cosmological calculation of Martin et al for general relativistic self-consistent spinning fluids. The existence of spin-squared terms in the field equations in the Einstein-Cartan theory shows, however, that an expanded class of meaningful cosmologies is possible. Under certain assumptions on the arbitrariness of the cosmological shear and expansion the results for the ad hoc Weyssenhoff spin fluid in a spherically symmetric spacetime can be reproduced.
04.40.Nr Einstein-Maxwell spacetimes, spacetimes with fluids, radiation or classical fields
Issue 9 (September 1994)
Received 6 June 1994
Larry L Smalley and J P Krisch 1994 Class. Quantum Grav. 11 2375
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