A Cosmological Signature of the SM Higgs Instability: Gravitational Waves
Jos\'e Ram\'on Espinosa, Davide Racco, Antonio Riotto

TL;DR
This paper proposes that Higgs field fluctuations during inflation could produce detectable gravitational waves, offering a novel way to observe the Standard Model Higgs instability and its potential link to dark matter via primordial black holes.
Contribution
It provides a detailed characterization of gravitational waves sourced by Higgs fluctuations, linking collider physics, gravitational wave detection, and dark matter hypotheses.
Findings
Gravitational wave signals depend on Higgs and top masses.
LISA, Einstein Telescope, and Advanced LIGO could detect these signals.
The mechanism may also explain primordial black hole dark matter.
Abstract
A fundamental property of the Standard Model is that the Higgs potential becomes unstable at large values of the Higgs field. For the current central values of the Higgs and top masses, the instability scale is about GeV and therefore not accessible by colliders. We show that a possible signature of the Standard Model Higgs instability is the production of gravitational waves sourced by Higgs fluctuations generated during inflation. We fully characterise the two-point correlator of such gravitational waves by computing its amplitude, the frequency at peak, the spectral index, as well as their three-point correlators for various polarisations. We show that, depending on the Higgs and top masses, either LISA or the Einstein Telescope and Advanced-Ligo, could detect such stochastic background of gravitational waves. In this sense, collider and gravitational wave physics can…
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