Abstract
Rotating cosmological models under the influence of both shear and bulk viscosity, together with scalar field and heat flow, are studied. Exact solutions of the field equations are obtained. The solutions have nonzero expansion, shear, and rotation. The properties of the solutions are studied and the temperature distribution is also given explicitly.
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Patel, L.K., Koppar, S.S. Rotating viscous-fluid cosmologies with scalar field and heat flux. Lett Math Phys 18, 347–353 (1989). https://doi.org/10.1007/BF00405266
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DOI: https://doi.org/10.1007/BF00405266