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

Abstract

We derive a compact analytical expression for the growth factor ${\rm Y}$, 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 ${\rm Y}=\frac{2[1-y^{3(w-1)/2}]}{3(1-w)}$, 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 ${\rm Y}$ a universal factor that captures gravitational wave growth in various scenarios-not limited to phase transitions.

7 pages, 3 figures (PRD Letter Accepted Version)