Growth of Gravitational Wave Spectrum from Sound Waves in a Universe with Generic Expansion Rate

TL;DR

This paper derives a universal analytical expression for the growth of gravitational wave spectra sourced by sound waves in universes with arbitrary expansion histories, extending previous models beyond standard eras.

Contribution

It provides a general formula for gravitational wave growth factor applicable to any cosmological background with a dominant energy component.

Findings

Derived a compact analytical expression for the growth factor mma.

Reduces to known results in radiation and matter-dominated eras.

Applicable to a wide range of cosmological scenarios, not limited to phase transitions.

Abstract

We derive a compact analytical expression for the growth factor $\Upsilon$, which characterizes how the gravitational wave spectrum sourced by sound waves evolves in a universe with a generic expansion history. Assuming the dominant energy density scales as $\rho \propto a^{-3(1+w)}$, we obtain $\Upsilon =\frac{2[1-y^{3(w-1)/2}]}{3(1-w)}$, where $y = a(t)/a(t_s)$ is the ratio of the scale factor at a later time $t$ to that at $t_s$ when gravitational wave production from sound waves starts. This general result reduces to known forms in radiation-and matter-dominated eras, thereby extending previous formulas to a broader class of cosmological backgrounds. The derivation assumes only that the source is stationary, making $\Upsilon$ a universal factor that captures gravitational wave growth in various scenarios-not limited to phase transitions.