Non-singular cosmology in five dimensions with or without heat flux

Details Non-singular cosmology in five dimensions with or without heat flux Non-singular cosmology in five dimensions with or without heat flux

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cqgra..13..153b&link_type=abstract

Classical and Quantum Gravity, Volume 13, Issue 1, pp. 153-160 (1996).

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Exact singularity-free Senovilla-type solutions are obtained in five-dimensional spacetime for a fluid with or without heat flow. The energy density and the pressure of the fluid satisfy a barotropic equation of state and remain finite throughout the evolution in each case. It is possible to find exact solutions in both the cases - one with the anisotropic pressure 0264-9381/13/1/014/img1 and the other with isotropic pressure where 0264-9381/13/1/014/img2. The latter includes, in a special case, one of the vacuum solutions obtained earlier.

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