Euler-Heisenberg actions for gauge-axial background vectors: Hessian diagonalization, sector classification, and applications
hep-th, astro-ph.CO, cond-mat.other, gr-qc, hep-ph
Submitted: 2025-11-03
Updated: 2026-08-25
Comments: 33 pages, 2 figures, based on the author's M.Sc. Dissertation available at https://repositorio.ufjf.br/jspui/handle/ufjf/19665?mode=full
Journal ref: Eur. Phys. J. C 86, 995 (2026)
DOI: 10.1140/epjc/s10052-026-16218-6
License: http://creativecommons.org/licenses/by/4.0/
The gist: We derive the closed-form one-loop Euler-Heisenberg effective actions for Dirac fermions coupled simultaneously to classical electromagnetic vector and massive pseudo-vector backgrounds within a
Terminology
Abstract
We derive the closed-form one-loop Euler-Heisenberg effective actions for Dirac fermions coupled simultaneously to classical electromagnetic vector and massive pseudo-vector backgrounds within a controlled quasi-static approximation. Through complete diagonalization of the functional Hessian, we systematically delineate the parameter space into distinct sectors characterized by stability properties and spectral structure. We identify subspaces that encompass and extend results from previous studies into a broader class, admitting propagating axial fields as physically viable regimes; strikingly, we note sectors presenting chirality-asymmetric instability. This addresses long-standing questions regarding the well-defined nature, diagonalizability, and stability of these models. From the effective actions, we derive novel nonperturbative pair-production rates for simultaneously propagating electromagnetic and axial vector backgrounds; remarkably, we find pronounced vacuum stabilization compared to previous results. Furthermore, we derive the non-perturbative contributions to the chiral current divergence, which enables dynamical chiral symmetry breaking and show that the electromagnetic coupling induces instanton-like configurations for the axial field, even when it is not a fundamental gauge field. As a proof-of-concept, we analyze a cosmological toy model of baryogenesis driven by an axial vector, providing numerical estimates that support the viability of this hypothesis. Additionally, we outline qualitative predictions for Weyl/Dirac semi-metals and briefly discuss potential applications in related phenomena, such as Quark-Gluon plasma, Electroweak scenarios and the Strong-CP problem.
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