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Phys. Rev. D 55, 3260–3264 (1997)

Detecting relic gravitational radiation from string cosmology with LIGO

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Bruce Allen
Department of Physics, University of Wisconsin-Milwaukee, P. O. Box 413, Milwaukee, Wisconsin 53211

Ram Brustein
Department of Physics, Ben-Gurion University, Beer-Sheva 84105, Israel

Received 4 September 1996; published in the issue dated 15 March 1997

A characteristic spectrum of relic gravitational radiation is produced by a period of “stringy inflation” in the early Universe. This spectrum is unusual, because the energy density rises rapidly with frequency. We show that correlation experiments with the two gravitational-wave detectors being built for the Laser Interferometric Gravitational Wave Observatory could detect this relic radiation for certain ranges of the parameters that characterize the underlying string cosmology model.

© 1997 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.55.3260
DOI:
10.1103/PhysRevD.55.3260
PACS:
04.80.Nn, 04.30.Db, 98.80.Cq, 98.80.Es