The stochastic relaxion

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.

Stellar limits on scalars from electron-nucleus bremsstrahlung

“…White-dwarf cooling then implied a bound sin θ 10 −17 [25,26], many orders of magnitude more stringent than the previous one. If true, this powerful constraint would strongly impact the parameter space of scalars mixing with the Higgs [27], such as in relaxion models [28][29][30], and suggests that white dwarfs can probe the CP-violating scalar coupling of QCD axions originating in the weak sector of the standard model [31].…”