Spectra of relic gravitons and the early history of the Hubble parameter

L. P. Grishchuk and M. Solokhin
Phys. Rev. D 43, 2566 – Published 15 April 1991
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Abstract

The spectra of relic gravitational waves produced as a result of cosmological expansion of the generalized inflationary models are derived. It is shown how one can reconstruct the time dependence of the very early Hubble parameter and matter energy density from a measured frequencydependent spectrum of relic gravitational waves.

  • Received 26 November 1990

DOI:https://doi.org/10.1103/PhysRevD.43.2566

©1991 American Physical Society

Authors & Affiliations

L. P. Grishchuk

  • Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder, Colorado 80309; National Institute of Standards and Technology, Gaithersburg, Maryland 20899; and Shternberg Astronomical Institute, Moscow University, 119899 Moscow, V-234, U.S.S.R.

M. Solokhin

  • Shternberg Astronomical Institute, Moscow University, 119899 Moscow, V-234, U.S.S.R.

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Issue

Vol. 43, Iss. 8 — 15 April 1991

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