Stability of the Friedmann Universe in the Poincaré Gauge Theory. II

Details Stability of the Friedmann Universe in the Poincaré Gauge Theory. II Stability of the Friedmann Universe in the Poincaré Gauge Theory. II

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pthph..89..371o&link_type=abstract

Progress of Theoretical Physics, Vol. 89, No. 2, pp. 371-388.

Physics

Scientific paper

In the Poincaré Gauge Theory, solutions of the Friedmann universe stable against quantum corrections due to vacuum polarization are obtained under linear approximation for the cases k = 0, +/-1 of the radiation dominant universe (RDU), the matter dominant universe (MDU) and the de Sitter universe (dSU). These solutions are small oscillations around the standard Big Bang solution of General Relativity and exist for each era of RDU, MDU and dSU, respectively, if we choose the parameters of the Poincaré Gauge Theory and the total entropy of the universe properly.

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