Gravitational Wave Echo of Relaxion Trapping
Abhishek Banerjee, Eric Madge, Gilad Perez, Wolfram Ratzinger and, Pedro Schwaller

TL;DR
This paper explores a novel mechanism where dark photon-induced gravitational waves are generated during relaxion trapping, providing potential observational signatures and dark matter constraints in the context of solving the hierarchy problem.
Contribution
It introduces a new gravitational wave production mechanism involving dark photon tachyonic instability during relaxion trapping, with implications for dark matter and experimental detection.
Findings
Calculated gravitational wave spectrum from dark photon tachyonic instability.
Identified parameter space where gravitational waves are detectable.
Discussed constraints on relaxion dark matter from gravitational wave observations.
Abstract
To solve the hierarchy problem, the relaxion must remain trapped in the correct minimum, even if the electroweak symmetry is restored after reheating. In this scenario, the relaxion starts rolling again until the backreaction potential, with its set of local minima, reappears. Depending on the time of barrier reappearance, Hubble friction alone may be insufficient to retrap the relaxion in a large portion of the parameter space. Thus, an additional source of friction is required, which might be provided by coupling to a dark photon.The dark photon experiences a tachyonic instability as the relaxion rolls, which slows down the relaxion by backreacting to its motion, and efficiently creates anisotropies in the dark photon energy-momentum tensor, sourcing gravitational waves. We calculate the spectrum of the resulting gravitational wave background from this new mechanism, and evaluate its…
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