Cylindrically symmetric viscous universes.

Details Cylindrically symmetric viscous universes. Cylindrically symmetric viscous universes.

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jmp....34.1927p&link_type=abstract

Journal of Mathematical Physics, Vol. 34, No. 5, p. 1927 - 1936

Mathematics

Mathematical Physics

5

Scientific paper

The cylindrically symmetric cosmological models with viscous fluid having the Kasnerian time evolution are considered herein. It turns out that the "no-matter" limit of geodetic viscous universes, which can as well be looked upon as string-dust universes, is the nonflat empty Kasner space-time. It is proposed that the universe may be born with the Kasner geometry at t = 0 with matter in the form of viscous fluid, then it may follow the path: geodetic to nongeodetic and finally to the radiation phase when viscosity is fully worn out. Solutions to describe each phase separately are given.

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