Non-equilibrium dynamics of Axion-like particles: the quantum master equation

TL;DR

This paper derives a quantum master equation to describe the non-equilibrium dynamics of axion-like particles, revealing their thermalization, decoherence, and potential cosmological impacts in a unified framework.

Contribution

It introduces a comprehensive quantum master equation for ALPs coupled to a thermal bath, capturing their damped oscillations, thermalization, and entropy production at all orders in bath couplings.

Findings

ALP energy density has cold and hot components with exponential decay and thermalization.

Relaxation and thermalization occur on similar time scales, affecting cosmological evolution.

Enhanced relaxation rate due to thermal emission and absorption impacts CMB birefringence and galaxy formation.

Abstract

We study the non-equilibrium dynamics of Axion-like particles (ALP) coupled to Standard Model degrees of freedom in thermal equilibrium. The Quantum Master Equation (QME) for the (ALP) reduced density matrix is derived to leading order in the coupling of the (ALP) to the thermal bath, but to \emph{all} orders of the bath couplings to degrees of freedom within or beyond the Standard Model other than the (ALP). The (QME) describes the damped oscillation dynamics of an initial misaligned (ALP) condensate, thermalization with the bath, decoherence and entropy production within a unifying framework. The (ALP) energy density $\mathcal{E}(t)$ features two components: a ``cold'' component from the misaligned condensate and a ``hot'' component from thermalization with the bath, with $\mathcal{E}(t)= \mathcal{E}_{c}\,e^{-\gamma(T)\,t}+\mathcal{E}_{h}(1-e^{-\gamma(T)\,t})$ thus providing a ``mixed dark matter'' scenario. Relaxation of the (ALP) condensate, thermalization, decoherence and entropy production occur on similar time scales. An explicit example with (ALP)-photon coupling, valid post recombination yields a relaxation rate $\gamma(T)$ with a substantial enhancement from thermal emission and absorption. A misaligned condensate is decaying at least since recombination and on the same time scale thermalizing with the cosmic microwave background (CMB). Possible consequences for birefringence of the (CMB) and (ALP) contribution to the effective number of ultrarelativistic species and galaxy formation are discussed.