Geodesics structure and deflection angle of electrically charged black holes in gravity with a background Kalb-Ramond field

dc.contributor.authorAl-Badawi, Ahmad
dc.contributor.authorShaymatov, Sanjar
dc.contributor.authorSakalli, Izzet
dc.date.accessioned2026-02-06T18:51:22Z
dc.date.issued2024
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractThis article investigates the geodesic structure and deflection angle of charged black holes in the presence of a nonzero vacuum expectation value background of the Kalb-Ramond field. Topics explored include null and timelike geodesics, energy extraction by collisions, and the motion of charged particles. The photon sphere radius is calculated and plotted to examine the effects of both the black hole charge (Q) and the Lorentz-violating parameter (b) on null geodesics. The effective potential for timelike geodesics is analyzed, and second-order analytical orbits are derived. We further show that the combined effects of Lorentz-violating parameter and electric charge can mimic a Kerr black hole spin parameter up to its maximum values, i.e., a/M similar to 1\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$a/M \sim 1$$\end{document} thus suggesting that the current precision of measurements of highly spinning black hole candidates may not rule out the effect of Lorentz-violating parameter. The center of mass energy of colliding particles is also considered, demonstrating a decrease with increasing Lorentz-violating parameter. Circular orbiting particles of charged particles are discovered, with the minimum radius for a stable circular orbit decreasing as both b and Q increase. Results show that this circular orbit is particularly sensitive to changes in the Lorentz-violating parameter. Additionally, a timelike particle trajectory is demonstrated as a consequence of the combined effects of parameters b and Q. Finally, the light deflection angle is analyzed using the weak field limit approach to determine the Lorentz-breaking effect, employing the Gauss-Bonnet theorem for computation. Findings are visualized with appropriate plots and thoroughly discussed.
dc.description.sponsorshipNational Key Research and Development Program of China
dc.description.sponsorshipWe are thankful to the Editor and anonymous Referees for their constructive suggestions and comments.
dc.identifier.doi10.1140/epjc/s10052-024-13205-7
dc.identifier.issn1434-6044
dc.identifier.issn1434-6052
dc.identifier.issue8
dc.identifier.orcid0000-0001-7827-9476
dc.identifier.orcid0000-0002-5229-7657
dc.identifier.scopus2-s2.0-85201407097
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-024-13205-7
dc.identifier.urihttps://hdl.handle.net/11129/15324
dc.identifier.volume84
dc.identifier.wosWOS:001292889500003
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofEuropean Physical Journal C
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectQuasi-Normal Modes
dc.subjectGreybody Factors
dc.subjectSuzaku Observations
dc.subjectHawking Radiation
dc.subjectScalar
dc.subjectShadow
dc.subjectMass
dc.titleGeodesics structure and deflection angle of electrically charged black holes in gravity with a background Kalb-Ramond field
dc.typeArticle

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