Abstract

Particle production in strong electromagnetic fields is a recurring theme in solid state physics, heavy ion collisions, early universe cosmology and formal quantum field theory. In this paper we discuss the Dirac equation in a background of parallel electric and magnetic fields. We review the Schwinger particle production rate, clarify the emergence of the chiral anomaly equation and compute the induced current of charged fermions. We distinguish the contributions from non-perturbative particle production, from the running of the gauge coupling constant and from non-linearities in the effective QED Lagrangian, and clarify how these contributions arise within a single framework. We apply these results to axion inflation. A Chern-Simons coupling between the pseudoscalar particle driving cosmic inflaton and an abelian gauge group induces a dual production of gauge fields and charged fermions. We show that the resulting scalar and gravitational wave power spectra strongly depend on the fermion mass.

Highlights

  • Fields [8,9,10], discussed first in [11] in the context of Weyl fermions in a crystal

  • Strong helical gauge fields appear in models of axion inflation [23,24,25], are postulated to permeate intergalactic voids [26], may play a crucial role in baryogenesis [27,28,29,30,31,32,33] and appear in some implementations of the relaxion model [34,35,36,37,38], constructed to address the hierarchy problem in the Standard Model (SM) of particle physics

  • The production and transport of charged particles in the presence of electromagnetic fields are ubiquitous in nature

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Summary

Solving the fermion equation of motion

This section is dedicated to the analysis of the Dirac equation in a background of classical (anti-)parallel electric and magnetic fields. We identify the eigenvalues (energy levels) and eigenstates (particles and anti particles), both in the absence and presence of an electric field.

Preliminaries
Landau levels
Particles and anti-particles
Particle production
Bogoliubov coefficients
Chiral anomaly and chiral asymmetry
Induced current and Euler-Heisenberg action
P m2T a2
Applications
Upper bound on gauge field production during cosmic inflation
Axion inflation
Baryogenesis from axion inflation
Conclusions
A Notation and conventions
B Solving the fermion equation of motion
C Particle production
D Weak field expansion
Full Text
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