Comparative of light propagation in Born-Infeld, Euler-Heisenberg and ModMax nonlinear electrodynamics

Abstract We compare light propagation through an intense electromagnetic background as described by three different nonlinear electrodynamics: Born-Infeld (BI), Euler-Heisenberg (EH), and Modified Maxwell (MM). We use the concept of effective metric to determine the phase velocities of a propagating wave from the BI and EH nonlinear electrodynamics and use them to set constraints on the MM nonlinear parameter. In a second part of the paper, we consider the black hole solutions of the nonlinear electrodynamics coupled with General Relativity and determine the shadows cast by the static black holes. Confronting the observations of the shadows of M87 * and Sagittarius A * with our theoretical results allows us to set restrictions on the nonlinear parameters.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2024-11-01
DOI
https://doi.org/10.1088/1475-7516/2024/11/002
Citations
8
Primary Topic
Quantum optics and atomic interactions
Type
article
Field-Weighted Citation Impact
2.70
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article

Comparative of light propagation in Born-Infeld, Euler-Heisenberg and ModMax nonlinear electrodynamics

Ariadna Montiel, Nora Bretón, Elda Guzman‐Herrera
8 citations
Journal of Cosmology and Astroparticle Physics
Quantum optics and atomic interactions
2.70
article

Comparative of light propagation in Born-Infeld, Euler-Heisenberg and ModMax nonlinear electrodynamics

Ariadna Montiel, Nora Bretón, Elda Guzman‐Herrera
article en
8 citations

Abstract

Abstract We compare light propagation through an intense electromagnetic background as described by three different nonlinear electrodynamics: Born-Infeld (BI), Euler-Heisenberg (EH), and Modified Maxwell (MM). We use the concept of effective metric to determine the phase velocities of a propagating wave from the BI and EH nonlinear electrodynamics and use them to set constraints on the MM nonlinear parameter. In a second part of the paper, we consider the black hole solutions of the nonlinear electrodynamics coupled with General Relativity and determine the shadows cast by the static black holes. Confronting the observations of the shadows of M87 * and Sagittarius A * with our theoretical results allows us to set restrictions on the nonlinear parameters.

Journal of Cosmology and Astroparticle PhysicsVol. 2024(11)
Instituto Politécnico Nacional (MX), Universidade Federal de Itajubá (BR)
Openalex Percentile: Top 9%
Quantum optics and atomic interactions
2.70
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