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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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_02198878_v_n_p_CiriloLombardo |
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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 |
_version_ |
1807324007057326080 |