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On the Schwinger effect during axion inflation

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arxiv 2408.16538 v2 pith:V5ZZAEPM submitted 2024-08-29 hep-ph astro-ph.COgr-qc

classification hep-phastro-ph.COgr-qc
keywords axioninflationschwingerduringfieldsresultsaccountdescription
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Pair-creation of charged particles in a strong gauge-field background - the renowned Schwinger effect - can strongly alter the efficiency of gauge-field production during axion inflation. It is therefore crucial to have a clear understanding and proper description of this phenomenon to obtain reliable predictions for the physical observables in this model. In the present work, we revisit the problem of Schwinger pair production during axion inflation in the presence of both electric and magnetic fields and improve on the state of the art in two ways: (i) taking into account that the electric- and magnetic-field three-vectors are in general not collinear, we derive the vector decomposition of the Schwinger-induced current in terms of these fields and determine the corresponding effective electric and magnetic conductivities; (ii) by identifying the physical momentum scale associated with the pair-creation process, we incorporate Schwinger damping of the gauge field in a scale-dependent fashion in the relevant equations of motion. Implementing this new description in the framework of the gradient-expansion formalism, we obtain numerical results in a benchmark scenario of axion inflation and perform a comprehensive comparison with earlier results in the literature. In some cases, the resulting energy densities of the produced gauge fields differ from the old results by more than one order of magnitude, which reflects the importance of taking the new effects into account.

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Cited by 2 Pith papers

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

  1. 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...

  2. 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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