Black hole with global monopole charge in self-interacting Kalb-Ramond field

dc.contributor.authorFathi, Mohsen
dc.contributor.authorOvgun, Ali
dc.date.accessioned2026-02-06T18:51:32Z
dc.date.issued2025
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractIn this study, we explore a static, spherically symmetric black hole solution in the context of a self-interacting Kalb-Ramond field coupled with a global monopole. By incorporating the effects of Lorentz-violating term & ell;\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\ell$$\end{document} and the monopole charge eta\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\eta$$\end{document} in the KR field, we derive the modified gravitational field equations and analyze the resulting black hole spacetime. The obtained solution exhibits deviations from the Schwarzschild metric with topological defect, as it is influenced by the monopole charge and self-interaction potential. We investigate the thermodynamic properties of the black hole, including its Hawking temperature, entropy, and specific heat, revealing novel stability conditions. Additionally, we perform solar system tests such as perihelion precession, gravitational redshift, light deflection, and time delay of signals to impose constraints on the Lorentz-violating parameter and monopole charge. Our findings suggest that these parameters have to be significantly small, although there are different constraints imposed by individual tests, ranging from 10-9 <=|& ell;|<= 10-4\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$10<^>{-9}\le |\ell |\le 10<^>{-4}$$\end{document} and 10-9 <=eta <= 10-6m-1\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$10<^>{-9}\le \eta \le 10<^>{-6}\, \textrm{m}<^>{-1}$$\end{document}.
dc.description.sponsorshipUniversidad Central de Chile [PDUCEN20240008]; COST Action - COSMIC WISPers in the Dark Universe: Theory, astrophysics and experiments (CosmicWISPers) [CA21106]; COST Action - Fundamental challenges in theoretical physics (THEORY-CHALLENGES) [CA22113]; COST Action - Bridging high and low energies in search of quantum gravity (BridgeQG) [CA23130]; EMU; TUBITAK; SCOAP3
dc.description.sponsorshipM.F. is supported by Universidad Central de Chile through project No. PDUCEN20240008. A.O. would like to acknowledge the contribution of the COST Action CA21106 - COSMIC WISPers in the Dark Universe: Theory, astrophysics and experiments (CosmicWISPers), the COST Action CA22113 - Fundamental challenges in theoretical physics (THEORY-CHALLENGES) and the COST Action CA23130 - Bridging high and low energies in search of quantum gravity (BridgeQG). We also thank EMU, TUBITAK and SCOAP3 for their support.
dc.identifier.doi10.1140/epjp/s13360-025-06241-z
dc.identifier.issn2190-5444
dc.identifier.issue4
dc.identifier.orcid0000-0002-9889-342X
dc.identifier.orcid0000-0002-1602-0722
dc.identifier.scopus2-s2.0-105003006086
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjp/s13360-025-06241-z
dc.identifier.urihttps://hdl.handle.net/11129/15397
dc.identifier.volume140
dc.identifier.wosWOS:001463096400006
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer Heidelberg
dc.relation.ispartofEuropean Physical Journal Plus
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260204
dc.subjectGravitational-Field
dc.subject4Th Test
dc.subjectRelativity
dc.subjectWeyl
dc.titleBlack hole with global monopole charge in self-interacting Kalb-Ramond field
dc.typeArticle

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