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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creator | Romero Jorge, A W 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 |
doi_str_mv | 10.48550/arxiv.1912.02904 |
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The dispersion equation is modified due to the magnetized photon self-energy in the transparency region (\(0<\omega<2m_e\)). 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. A discussion of potential causes of this behaviour is presented.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1912.02904</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>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</subject><ispartof>arXiv.org, 2019-12</ispartof><rights>2019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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A discussion of potential causes of this behaviour is presented.</description><subject>Analytic functions</subject><subject>Dispersion curve analysis</subject><subject>Field strength</subject><subject>Magnetic dipoles</subject><subject>Magnetic fields</subject><subject>Magnetospheres</subject><subject>Mathematical analysis</subject><subject>Neutron stars</subject><subject>Phase velocity</subject><subject>Photons</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - High Energy Physics - Phenomenology</subject><subject>Propagation</subject><subject>Time dependence</subject><subject>Time lag</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotj0tLw0AUhQdBsNT-AFcOuE6cufPozFKKj0LBTfbhJrkxKc3DSVKsv97YdnXgcDh8H2MPUsTaGSOeMfzUx1h6CbEAL_QNW4BSMnIa4I6thmEvhAC7BmPUgrmkIt5X3di1fKwb4gUd8MTrljf41dJY_1LBj5hPU3NtuqGvKNA9uy3xMNDqmkuWvL0mm49o9_m-3bzsIjTgI8BMegAUSK7UwhlbZrbwpbXGailNkUsBTjuX5UTgySOVM2huEKRUUqkle7zcnrXSPtQNhlP6r5ee9ebF02XRh-57omFM990U2pkpBQVKrJXSXv0B1CBRig</recordid><startdate>20191210</startdate><enddate>20191210</enddate><creator>Romero Jorge, A W</creator><creator>E Rodríguez Querts</creator><creator>H Pérez Rojas</creator><creator>A Pérez Martínez</creator><creator>L Cruz Rodríguez</creator><creator>G Piccinelli Bocchi</creator><creator>Rueda, J A</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20191210</creationdate><title>The photon time delay in magnetized vacuum magnetosphere</title><author>Romero Jorge, A W ; 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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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