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Spin dynamics in general relativity
Affiliation:1. Department of Physics, University of Oslo, PB 1048 Blindern, N-0316 Oslo, Norway;2. Taras Shevchenko National University of Kyiv, UA-01033 Kyiv, Ukraine;3. Skobeltzyn Institute for Nuclear Physics, Moscow State University, RU-119899 Moscow, Russia
Abstract:The energy-momentum tensor of a fluid composed of spinning particles is presented in a form that is structurally similar to that of a fluid with the energy flux qa with respect to the fluid velocity ua, isotropic pressure p and the trace-free anisotropic pressure πab. The effect of spin in the evolution of a shear free cosmological model with irrotational geodesic flow is considered.
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