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Chiral Anomaly, Schwinger Effect, Euler-Heisenberg Lagrangian, and application to axion inflation

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arxiv 1910.01205 v2 pith:VJ5PC6OP submitted 2019-10-02 hep-ph astro-ph.COcond-mat.mes-hallhep-th

classification hep-phastro-ph.COcond-mat.mes-hallhep-th
keywords particleproductionfieldsgaugeanomalyaxionchargedchiral
verification ladder T0 review T1 audit T2 compute T3 formal
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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.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Massless fermionic current of Schwinger pairs in 3D de Sitter spacetime

    hep-th 2026-07 reject novelty 7.0 of 10

    Massless fermions in dS_3 with a constant electric field produce a finite monotonic induced current: linear in E for weak fields, λ^{3/2} for strong fields.

  2. High-frequency gravitational waves from axion inflation in the weak-backreaction regime

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Even in the weak-backreaction regime, axion inflation produces high-frequency primordial gravitational waves many orders of magnitude above the vacuum spectrum, peaking around MHz–GHz.

  3. Conformally-flat gravitational analogues to the Schwinger effect

    hep-th 2026-02 accept novelty 6.0 of 10

    Resummed heat kernels yield exact scalar pair-creation probabilities in conformally flat spacetimes, including new curvature-induced Schwinger analogues, with the radiation-dominated rate verified independently in arb...

  4. Comparative study of the strong backreaction regime in axion inflation: the effect of the potential

    astro-ph.CO 2025-05 conditional novelty 5.0 of 10

    In lattice simulations of axion inflation, the strong-backreaction stage that lengthens inflation occurs for all seven tested potentials, but its duration varies strongly with the potential.

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