Gravitational Waves and Cosmological Observables from First-Order Phase Transitions: Thermal Corrections at Low Temperature

TL;DR

This paper investigates how low-temperature thermal corrections to the effective potential influence first-order phase transitions in the early universe, affecting gravitational wave signals and cosmological observables.

Contribution

It introduces a simplified model with a single parameter to capture complex thermal corrections and analyzes their effects on phase transition dynamics and observable signals.

Findings

Thermal corrections can significantly shift phase transition parameters.

A single parameter effectively models complex thermal effects.

Impacts on gravitational wave signals are quantitatively assessed.

Abstract

We consider the impact on cosmological first-order phase transitions (FOPTs) of low-temperature thermal corrections to the effective potential. These are corrections from degrees of freedom whose field-dependent masses in the true vacuum are much larger than the nucleation temperature, though in the false vacuum the field-dependent masses may be much smaller than the nucleation temperature. Although the general form of these corrections to the thermal effective potential can be quite complicated, we argue that the net effect of all such corrections can be well-modeled with a single new parameter. We determine the shift in the parameters of the FOPT in terms of this new parameter, and the impact on gravitational wave signals and cosmological observables.