Effective-Potential Approach to Graviton Production in the Early Universe

J. B. Hartle
Phys. Rev. Lett. 39, 1373 – Published 28 November 1977
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Abstract

The production of gravitons in a homogeneous, isotropic, spatially flat universe containing radiation and a small admixture of cold baryons is studied by an effective-potential method which takes into account the back reaction of the produced gravitons on the geometry. The total probability per unit volume to produce a pair of gravitons is finite and has a very small value for a universe with parameters corresponding to my own.

  • Received 16 June 1977

DOI:https://doi.org/10.1103/PhysRevLett.39.1373

©1977 American Physical Society

Authors & Affiliations

J. B. Hartle

  • Department of Physics, University of California, Santa Barbara, California 93106

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Issue

Vol. 39, Iss. 22 — 28 November 1977

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