The photon time delay in magnetized vacuum magnetosphere

We study the transverse propagation of photons in a magnetized vacuum considering radiative corrections in the one-loop approximation. The dispersion equation is modified due to the magnetized photon self-energy in the transparency region (\(0

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Veröffentlicht in:arXiv.org 2019-12
Hauptverfasser: Romero Jorge, A W, E Rodríguez Querts, H Pérez Rojas, A Pérez Martínez, L Cruz Rodríguez, G Piccinelli Bocchi, Rueda, J A
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E Rodríguez Querts
H Pérez Rojas
A Pérez Martínez
L Cruz Rodríguez
G Piccinelli Bocchi
Rueda, J A
description We study the transverse propagation of photons in a magnetized vacuum considering radiative corrections in the one-loop approximation. The dispersion equation is modified due to the magnetized photon self-energy in the transparency region (\(0
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The dispersion equation is modified due to the magnetized photon self-energy in the transparency region (\(0&lt;\omega&lt;2m_e\)). The aim of our study is to explore propagation of photons in a neutron star magnetosphere (described by magnetized vacuum). The solution of the dispersion equation is obtained in terms of analytic functions. The larger the magnetic field, the lower the phase velocity and the more the dispersion curve deviates from the light-cone. For fixed values of the frequency, we study the dependence of photon time delay with the magnetic field strength, as well as with distance. For the latter, we adopt a magnetic dipole configuration and obtain that -- contrary to the expectation, according to the traditional time delay of photons in the interstellar medium -- photons of higher energy experience a longer time delay. 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subjects Analytic functions
Dispersion curve analysis
Field strength
Magnetic dipoles
Magnetic fields
Magnetospheres
Mathematical analysis
Neutron stars
Phase velocity
Photons
Physics - High Energy Astrophysical Phenomena
Physics - High Energy Physics - Phenomenology
Propagation
Time dependence
Time lag
title The photon time delay in magnetized vacuum magnetosphere
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