Beyond general relativity models, magnetosphere structure and dark matter stars

The magnetosphere structure of compact objects is considered in the context of a theory of gravity with dynamical torsion field beyond standard General Relativity (GR). To this end, a new spherically symmetric solution is obtained in this theoretical framework, physically representing a compact obje...

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Autores principales: Cirilo-Lombardo, D.J., Minotti, F.O.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_02198878_v_n_p_CiriloLombardo
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spelling todo:paper_02198878_v_n_p_CiriloLombardo2023-10-03T15:11:12Z Beyond general relativity models, magnetosphere structure and dark matter stars Cirilo-Lombardo, D.J. Minotti, F.O. dark matter stars magnetosphere structures Non Riemannian manifolds topology The magnetosphere structure of compact objects is considered in the context of a theory of gravity with dynamical torsion field beyond standard General Relativity (GR). To this end, a new spherically symmetric solution is obtained in this theoretical framework, physically representing a compact object of pseudoscalar fields (for example, axion field). The axially symmetric version of the Grad-Shafranov equation (GSE) is also derived in this context, and used to describe the magnetosphere dynamics of the obtained "axion star". The interplay between high-energy processes and the seed magnetic field with respect to the global structure of the magnetosphere is briefly discussed. © 2019 World Scientific Publishing Company. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_02198878_v_n_p_CiriloLombardo
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic dark matter stars
magnetosphere structures
Non Riemannian manifolds
topology
spellingShingle dark matter stars
magnetosphere structures
Non Riemannian manifolds
topology
Cirilo-Lombardo, D.J.
Minotti, F.O.
Beyond general relativity models, magnetosphere structure and dark matter stars
topic_facet dark matter stars
magnetosphere structures
Non Riemannian manifolds
topology
description The magnetosphere structure of compact objects is considered in the context of a theory of gravity with dynamical torsion field beyond standard General Relativity (GR). To this end, a new spherically symmetric solution is obtained in this theoretical framework, physically representing a compact object of pseudoscalar fields (for example, axion field). The axially symmetric version of the Grad-Shafranov equation (GSE) is also derived in this context, and used to describe the magnetosphere dynamics of the obtained "axion star". The interplay between high-energy processes and the seed magnetic field with respect to the global structure of the magnetosphere is briefly discussed. © 2019 World Scientific Publishing Company.
format JOUR
author Cirilo-Lombardo, D.J.
Minotti, F.O.
author_facet Cirilo-Lombardo, D.J.
Minotti, F.O.
author_sort Cirilo-Lombardo, D.J.
title Beyond general relativity models, magnetosphere structure and dark matter stars
title_short Beyond general relativity models, magnetosphere structure and dark matter stars
title_full Beyond general relativity models, magnetosphere structure and dark matter stars
title_fullStr Beyond general relativity models, magnetosphere structure and dark matter stars
title_full_unstemmed Beyond general relativity models, magnetosphere structure and dark matter stars
title_sort beyond general relativity models, magnetosphere structure and dark matter stars
url http://hdl.handle.net/20.500.12110/paper_02198878_v_n_p_CiriloLombardo
work_keys_str_mv AT cirilolombardodj beyondgeneralrelativitymodelsmagnetospherestructureanddarkmatterstars
AT minottifo beyondgeneralrelativitymodelsmagnetospherestructureanddarkmatterstars
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