Silk Damping in Scalar-Induced Gravitational Waves: A Novel Probe for New Physics

TL;DR

This paper explores how Silk damping affects scalar-induced gravitational waves, proposing it as a new method to detect heavy gauge bosons beyond the standard model through gravitational wave observations.

Contribution

It introduces the impact of Silk damping on SIGWs as a novel observable for probing particle interactions mediated by heavy gauge bosons beyond the standard model.

Findings

Silk damping suppresses SIGW energy-density spectrum on specific scales.

Pulsar timing arrays can detect gauge bosons with masses around 10^3-10^4 GeV.

Interferometers are sensitive to gauge bosons with masses around 10^7-10^{12} GeV.

Abstract

Silk damping is well known in the study of cosmic microwave background (CMB) and accounts for suppression of the angular power spectrum of CMB on large angular multipoles. In this Letter, we study the effect of Silk damping on the scalar-induced gravitational waves (SIGWs). Resulting from the dissipation of cosmic fluid, the Silk damping notably suppresses the energy-density spectrum of SIGWs on scales comparable to a diffusion scale at the decoupling time of feebly-interacting particles. The effect offers a novel observable for probing the underlying particle interaction, especially for those mediated by heavy gauge bosons beyond the standard model of particles. We anticipate that pulsar timing arrays are sensitive to gauge bosons with mass $\sim10^{3}-10^{4}\,\mathrm{GeV}$, while space- and ground-based interferometers to those with mass $\sim10^7-10^{12}\,\mathrm{GeV}$, leading to essential complements to on-going and future experiments of high-energy physics.