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Spin-density and Vorticity Contribution to the Cosmological Background

Relativistic non-Abelian spinning fluids can be formulated in group theory language, where the corresponding Mathisson-Papapetrou equation for spinning fluids can be obtained in terms of a specific de Sitter group contraction. This framework is very suitable for studying the effects of a spinning fluid of matter with vorticity and a spin density in a cosmological background.

preprint2014arXivOpen access
Dario Capasso
gr-qchep-th
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Dario Capasso

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