A Precise Fitting Formula for Gravitational Wave Spectra from Phase
Transitions
A Precise Fitting Formula for Gravitational Wave Spectra from Phase
Transitions
Obtaining a precise form for the predicted gravitational wave (GW) spectrum from a phase transition is a topic of great relevance for beyond Standard Model (BSM) physicists. Currently, the most sophisticated semi-analytic framework for estimating the dominant contribution to the spectrum is the sound shell model; however, full calculations within …