The Bubble Wall Velocity in Local Thermal Equilibrium and Energy Budget with Full Effective Potential
Zongguo Si, Hongxin Wang, Lei Wang, Yang Xiao, Yang Zhang

TL;DR
This paper develops a framework using the full one-loop finite-temperature effective potential to accurately compute bubble wall velocities and kinetic energy fractions in cosmological phase transitions, significantly impacting gravitational wave predictions.
Contribution
It introduces a comprehensive method to calculate bubble wall velocity and energy budget using the full effective potential within LTE, improving upon the simplified bag model approach.
Findings
Deflagration is the dominant fluid motion mode.
Significant differences in gravitational wave spectra between full potential and bag model.
The bag model often approximates the full equation of state well.
Abstract
We develop a framework based on the full one-loop finite-temperature effective potential model, within which the bubble wall velocity is calculated using the local thermal equilibrium (LTE) approximation, and the kinetic energy fraction is computed directly. In cosmological phase transitions, these quantities play a critical role in determining the resulting gravitational wave signals. Using the xSM as a benchmark model, we compute the peak gravitational wave spectra under different methods for determining the wall velocity and the kinetic energy fraction , and compare these results to those obtained using the commonly employed bag model. Within the scanned parameter space, we find: (1) Deflagration is the most prevalent mode of fluid motion.(2) Gravitational wave spectra based on the full effective potential with LTE-derived wall velocity and integrated can differ…
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