Resonant Gravitational Wave Amplification - Axion and Inflaton

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dc.creatorBassett, Bruce A.
dc.date1997-10-02
dc.date.accessioned2026-07-07T02:24:24Z
dc.date.available2026-07-07T02:24:24Z
dc.descriptionWe demonstrate the parametric amplification of the stochastic gravitational wave background during inflationary reheating and during axion/moduli oscillations. This amplification enhances the detectability of the string/inflationary gravity wave signal, leaving a finger-print on the spectrum which might be found with future gravitational wave detectors.
dc.description5 pages, 1 eps figure, World Sci style file included. Talk at the 2nd Amaldi Conference on Gravitational Waves, CERN (1997). Eds. E. Coccia et al (World Scientific, Singapore)
dc.identifierhttps://arxiv.org/abs/astro-ph/9710036
dc.identifierhttp://arxiv.org/abs/astro-ph/9710036
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11608
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleResonant Gravitational Wave Amplification - Axion and Inflaton
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