Gravitational lensing, wave propagation, and GUP-modified Hawking radiation in charged Bopp-Podolsky BTZ black holes with disclinations

dc.contributor.authorAhmed, Faizuddin
dc.contributor.authorAl-Badawi, Ahmad
dc.contributor.authorBouzenada, Abdelmalek
dc.contributor.authorSucu, Erdem
dc.contributor.authorSakalli, Izzet
dc.date.accessioned2026-02-06T18:51:45Z
dc.date.issued2025
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractblackWe investigate the gravitational and electromagnetic dynamics of charged BTZ-like black holes featuring disclination defects within the framework of Bopp-Podolsky electrodynamics [R. V. Maluf, J. E. G. Silva, C. A. S. Almeida and G. J. Olmo, Eur. Phys. J. C 85(5) (2025) 594]. Our analysis encompasses photon geodesics, scalar field propagation, and quantum gravitational corrections to thermal radiation. We derive the effective potential governing null geodesic motion and analyze how the black hole mass M, electric charge Q, cosmological constant Lambda, BP coupling parameter b(2), and disclination parameter beta influence photon trajectories and circular orbits. The critical impact parameter and photon sphere radius are computed, revealing distinctive signatures in gravitational lensing and shadow formation. For scalar perturbations, we solve the Klein-Gordon equation using coordinate transformations to obtain a Schrodinger-like wave equation with an effective potential encoding both electromagnetic corrections and topological defect contributions. Applying the Generalized Uncertainty Principle, we derive quantum-corrected Hawking temperatures that exhibit systematic suppression compared to classical predictions, suggesting potential black hole remnant formation. The GUP corrections scale quadratically with particle energy, providing natural ultraviolet regularization. Additionally, we compute Keplerian frequencies for circular orbits, demonstrating how nonlinear electrodynamics and cosmic string-like defects create observable modifications to orbital dynamics. Our results establish charged BTZ-like geometries as valuable laboratories for testing modified gravity theories, nonlinear electromagnetic effects, and quantum gravitational phenomena in lower-dimensional spacetimes, with potential implications for precision timing observations and gravitational wave astronomy.
dc.identifier.doi10.1142/S0219887826500891
dc.identifier.issn0219-8878
dc.identifier.issn1793-6977
dc.identifier.orcid0000-0002-3127-3453
dc.identifier.orcid0000-0001-7827-9476
dc.identifier.orcid0000-0002-3363-980X
dc.identifier.orcid0009-0000-3619-1492
dc.identifier.orcid0000-0003-2196-9622
dc.identifier.scopus2-s2.0-105024083370
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1142/S0219887826500891
dc.identifier.urihttps://hdl.handle.net/11129/15501
dc.identifier.wosWOS:001632119100001
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.ispartofInternational Journal of Geometric Methods in Modern Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260204
dc.subjectBTZ-like black hole
dc.subjectdisclination defects
dc.subjectgeodesic motion
dc.subjectgeneralized uncertainty principle (GUP)
dc.subjectscalar field dynamics
dc.subjectKeplerian frequencies
dc.titleGravitational lensing, wave propagation, and GUP-modified Hawking radiation in charged Bopp-Podolsky BTZ black holes with disclinations
dc.typeArticle

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