Resonant Gravitational Wave Amplification - Axion and Inflaton
Abstract
Description
We 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.
5 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)
5 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)