An analytical model for the Maxwell radiation field in an axially symmetric galaxy

The Maxwell radiation field is an essential physical characteristic of a galaxy. Here, an analytical model is built to simulate that field in an axisymmetric galaxy. This analytical model is based on an explicit representation for axisymmetric source-free Maxwell fields. In a previous work, the gene...

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Main Author: Arminjon Mayeul
Format: Article
Language:English
Published: De Gruyter 2021-03-01
Series:Open Physics
Subjects:
Online Access:https://doi.org/10.1515/phys-2021-0008
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author Arminjon Mayeul
author_facet Arminjon Mayeul
author_sort Arminjon Mayeul
collection DOAJ
description The Maxwell radiation field is an essential physical characteristic of a galaxy. Here, an analytical model is built to simulate that field in an axisymmetric galaxy. This analytical model is based on an explicit representation for axisymmetric source-free Maxwell fields. In a previous work, the general applicability of this representation has been proved. The model is adjusted by fitting to it the sum of spherical radiations emitted by the composing “stars.” The huge ratio distance/wavelength needs to implement a numerical precision better than the quadruple precision. The model passes a validation test based on a spherically symmetric solution. The results for a set of “stars” representative of a disk galaxy indicate that the field is highest near the disk axis, and there the axial component of E{\bf{E}} dominates over the radial one. This work will allow us in the future to check if the interaction energy predicted by an alternative theory of gravitation might be a component of dark matter.
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spelling doaj.art-594456e14e9d4142b5560d830a006a3a2022-12-21T19:24:17ZengDe GruyterOpen Physics2391-54712021-03-01191779010.1515/phys-2021-0008An analytical model for the Maxwell radiation field in an axially symmetric galaxyArminjon Mayeul0Univ. Grenoble Alpes, CNRS, Grenoble-INP, 3SR, F-38000Grenoble, FranceThe Maxwell radiation field is an essential physical characteristic of a galaxy. Here, an analytical model is built to simulate that field in an axisymmetric galaxy. This analytical model is based on an explicit representation for axisymmetric source-free Maxwell fields. In a previous work, the general applicability of this representation has been proved. The model is adjusted by fitting to it the sum of spherical radiations emitted by the composing “stars.” The huge ratio distance/wavelength needs to implement a numerical precision better than the quadruple precision. The model passes a validation test based on a spherically symmetric solution. The results for a set of “stars” representative of a disk galaxy indicate that the field is highest near the disk axis, and there the axial component of E{\bf{E}} dominates over the radial one. This work will allow us in the future to check if the interaction energy predicted by an alternative theory of gravitation might be a component of dark matter.https://doi.org/10.1515/phys-2021-0008disk galaxymaxwell equationsaxial symmetryexact solutionsnumerical modeldark matter
spellingShingle Arminjon Mayeul
An analytical model for the Maxwell radiation field in an axially symmetric galaxy
Open Physics
disk galaxy
maxwell equations
axial symmetry
exact solutions
numerical model
dark matter
title An analytical model for the Maxwell radiation field in an axially symmetric galaxy
title_full An analytical model for the Maxwell radiation field in an axially symmetric galaxy
title_fullStr An analytical model for the Maxwell radiation field in an axially symmetric galaxy
title_full_unstemmed An analytical model for the Maxwell radiation field in an axially symmetric galaxy
title_short An analytical model for the Maxwell radiation field in an axially symmetric galaxy
title_sort analytical model for the maxwell radiation field in an axially symmetric galaxy
topic disk galaxy
maxwell equations
axial symmetry
exact solutions
numerical model
dark matter
url https://doi.org/10.1515/phys-2021-0008
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