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Auteurs principaux: Kim, Dong-Hoon, Kim, Chul Min, Kim, Sang Pyo
Format: Preprint
Publié: 2024
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Accès en ligne:https://arxiv.org/abs/2401.03667
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author Kim, Dong-Hoon
Kim, Chul Min
Kim, Sang Pyo
author_facet Kim, Dong-Hoon
Kim, Chul Min
Kim, Sang Pyo
contents Highly magnetized neutron stars exhibit the vacuum non-linear electrodynamics effects, which can be well described using the one-loop effective action for quantum electrodynamics. In this context, we study the propagation and polarization of pulsar radio emission, based on the post-Maxwellian Lagrangian from the Heisenberg-Euler-Schwinger action. Given the refractive index obtained from this Lagrangian, we determine the leading-order corrections to both the propagation and polarization vectors due to quantum refraction via perturbation analysis. In addition, the effects on the orthogonality between the propagation and polarization vectors and the Faraday rotation angle, all due to quantum refraction are investigated. Furthermore, from the dual refractive index and the associated polarization modes, we discuss quantum birefringence, with the optical phenomenology analogous to its classical counterpart.
format Preprint
id arxiv_https___arxiv_org_abs_2401_03667
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Quantum refraction effects in pulsar radio emission
Kim, Dong-Hoon
Kim, Chul Min
Kim, Sang Pyo
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
Highly magnetized neutron stars exhibit the vacuum non-linear electrodynamics effects, which can be well described using the one-loop effective action for quantum electrodynamics. In this context, we study the propagation and polarization of pulsar radio emission, based on the post-Maxwellian Lagrangian from the Heisenberg-Euler-Schwinger action. Given the refractive index obtained from this Lagrangian, we determine the leading-order corrections to both the propagation and polarization vectors due to quantum refraction via perturbation analysis. In addition, the effects on the orthogonality between the propagation and polarization vectors and the Faraday rotation angle, all due to quantum refraction are investigated. Furthermore, from the dual refractive index and the associated polarization modes, we discuss quantum birefringence, with the optical phenomenology analogous to its classical counterpart.
title Quantum refraction effects in pulsar radio emission
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2401.03667