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The pregalactic cosmic gravitational wave backgroundAn outline is given that estimates the expected gravitational wave background, based on plausible pregalactic sources. Some cosmologically significant limits can be put on incoherent gravitational wave background arising from pregalactic cosmic evolution. The spectral region of cosmically generated and cosmically limited radiation is, at long periods, P greater than 1 year, in contrast to more recent cosmological sources, which have P approx. 10 to 10(exp -3).
Document ID
19900010629
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Matzner, Richard A. (Texas Univ. Austin, TX, United States)
Date Acquired
September 6, 2013
Publication Date
August 1, 1989
Publication Information
Publication: NASA, Relativistic Gravitational Experiments in Space
Subject Category
Astrophysics
Accession Number
90N19945
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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