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The first observations of wide-band interferometers and the spectra of relic gravitons

By Massimo Giovannini

Abstract

Stochastic backgrounds of relic gravitons of cosmological origin extend from frequencies of the order of the aHz up to the GHz range. Since the temperature and polarization anisotropies constrain the low frequency normalization of the spectra, in the concordance paradigm the strain amplitude corresponding to the frequency window of wide-band interferometers turns out to be, approximately, nine orders of magnitude smaller than the astounding signal recently reported and attributed to a binary black hole merger. The backgrounds of relic gravitons expected from the early Universe are compared with the stochastic foregrounds stemming from the estimated multiplicity of the astrophysical sources. It is suggested that while the astrophysical foregrounds are likely to dominate between few Hz and 10 kHz, relic gravitons with frequencies exceeding 100 kHz represent a potentially uncontaminated signal for the next generation of high-frequency detectors currently under scrutiny

Topics: Physics, QC1-999
Publisher: Elsevier
Year: 2016
DOI identifier: 10.1016/j.physletb.2016.06.020
OAI identifier: oai:doaj.org/article:f3b3d080adba4122b489ba97f8a118fe
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