The Stochastic Relaxion

TL;DR

This paper analyzes the stochastic dynamics of the relaxion field during inflation, revealing how large fluctuations influence its trapping and potential to solve the hierarchy problem, and exploring new parameter space regimes.

Contribution

It introduces a new stopping condition for the relaxion considering transitions between minima and examines the impact of large fluctuations on relaxion trapping and phenomenology.

Findings

Large Hubble parameter prevents relaxion trapping at the first minimum.

Relaxion fluctuations can open new phenomenological opportunities.

The stochastic approach restores relaxion viability against finite-density threats.

Abstract

We revisit the original proposal of cosmological relaxation of the electroweak scale by Graham, Kaplan and Rajendran in which the Higgs mass is scanned during inflation by an axion field, the relaxion. We investigate the regime where the relaxion is subject to large fluctuations during inflation. The stochastic dynamics of the relaxion is described by means of the Fokker-Planck formalism. We derive a new stopping condition for the relaxion taking into account transitions between the neighboring local minima of its potential. Relaxion fluctuations have important consequences even in the "classical-beats-quantum" regime. We determine that for a large Hubble parameter during inflation, the random walk prevents the relaxion from getting trapped at the first minimum. The relaxion stops much further away, where the potential is less shallow. Interestingly, this essentially jeopardises the "runaway relaxion" threat from finite-density effects, restoring most of the relaxion parameter space. We also explore the "quantum-beats-classical" regime, opening large new regions of parameter space. We investigate the consequences for both the QCD and the non-QCD relaxion. The misalignment of the relaxion due to fluctuations around its local minimum opens new phenomenological opportunities.