Existence and causality of cosmological models with spinning fluids and torsion

Physics

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Scientific paper

Cosmological models with time dependent scale factors for Lewis type cylindrically symmetric geometries and Ray-Smalley rotating spin fluids cannot be expanding in Einstein Cartan theory. However, these fluids can generate anisotropic and inhomogeneous stationary stably causal rotating spacetimes with strong (and weak) spin-vorticity coupling and reasonable physical properties.

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