Abstract
A solution of the Einstein field equation corresponding to a distribution of fluid with equation of stateρ = 3p but with a nonvanishing shear viscosity is presented. The solution is spherical symmetric and the flow lines are geodetic.
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Modak, B. A neutrino universe with viscosity. Pramana - J Phys 23, 809–814 (1984). https://doi.org/10.1007/BF02894772
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DOI: https://doi.org/10.1007/BF02894772