Probing Beyond Standard Model via Hawking Radiated Gravitational Waves

TL;DR

This paper introduces a new method to explore beyond standard model particles by analyzing gravitational waves emitted from Hawking radiation of primordial black holes, potentially revealing BSM physics through GW spectra.

Contribution

It presents a comprehensive calculation of GW spectra from evaporating black holes including greybody factors, enabling BSM particle detection via gravitational wave observations.

Findings

GW spectra encode information about BSM particles.

Primordial black hole GWs are redshifted into observable frequencies.

Method offers a new avenue for probing BSM physics in the early universe.

Abstract

We propose a novel technique to probe the beyond standard model (BSM) of particle physics. The mass spectrum of unknown BSM particles can be scanned by observing gravitational waves (GWs) emitted by Hawking radiation of black holes. This is because information on the radiation of the BSM particles is imprinted in the spectrum of the GWs. We fully calculate the GW spectrum from evaporating black holes taking into account the greybody factor. As an observationally interesting application, we consider primordial black holes which evaporate in the very early universe. In that case, since the frequencies of GWs are substantially redshifted, the GWs emitted with the BSM energy scales become accessible by observations.