Gravitational waves from first-order phase transitions: Towards model separation by bubble nucleation rate
arXiv:1708.01253 · doi:10.1088/1475-7516/2017/11/050
Abstract
We study gravitational-wave production from bubble collisions in a cosmic first-order phase transition, focusing on the possibility of model separation by the bubble nucleation rate dependence of the resulting gravitational-wave spectrum. By using the method of relating the spectrum with the two-point correlator of the energy-momentum tensor , we first write down analytic expressions for the spectrum with a Gaussian correction to the commonly used nucleation rate, , under the thin-wall and envelope approximations. Then we quantitatively investigate how the spectrum changes with the size of the Gaussian correction. It is found that the spectral shape shows deviation from case for some physically motivated scenarios. We also briefly discuss detector sensitivities required to distinguish different spectral shapes.
36 pages, 13 figures, 1 figure from arXiv:1605.01403
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