Effective action and cosmological evolution of scale factors in higher-dimensional curved spacetime

M. Yoshimura
Phys. Rev. D 30, 344 – Published 15 July 1984
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Abstract

The quantum effective action is computed at finite temperatures in a Robertson-Walker type of metric suggested in Kaluza-Klein theories. The most interesting result is that above a critical temperature the effective gravitational constant becomes negative if the extra dimension is large enough. This provides a mechanism for the bounce from a contracting phase and may explain how the extra space has decoupled from the general expansion. The bounce mechanism also leads to a picture of the recycling universe, in which entropy produced after many cycles of expansion and contraction may solve the horizon and the flatness problem of the standard cosmology.

  • Received 30 January 1984

DOI:https://doi.org/10.1103/PhysRevD.30.344

©1984 American Physical Society

Authors & Affiliations

M. Yoshimura

  • National Laboratory for High Energy Physics (KEK), Tsukuba, Ibaraki 305 Japan

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Issue

Vol. 30, Iss. 2 — 15 July 1984

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