GENERAL: Relic Gravity Waves Investigation by Advanced Space-Based Gravitational Waves Detector

Details GENERAL: Relic Gravity Waves Investigation by Advanced Space-Based Gravitational Waves Detector GENERAL: Relic Gravity Waves Investigation by Advanced Space-Based Gravitational Waves Detector

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010cotph..53..496l&link_type=abstract

Communications in Theoretical Physics, Volume 53, Issue 3, pp. 496-498 (2010).

Physics

2

Scientific paper

This paper focuses on the relic gravity waves produced during the transition from a radiation-dominated inflationary phase to a dust-dominated Friedman-Robertson-Walker-type expansion. We discuss how to investigate the spectral energy density by the latest space-based GWs detectors at f = 0.1 Hz (i.e. DECIGO). In the case of power-law and exponential inflation, we apply the cross-correlation method to the latest detector and get the time dependence of the very early Hubble parameter.

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