Shedding light on gravity: Black hole shadows and lensing signatures in Lorentz gauge theory

dc.contributor.authorOvgun, Ali
dc.contributor.authorFathi, Mohsen
dc.date.accessioned2026-02-06T18:40:15Z
dc.date.issued2025
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractRecent advances, including gravitational wave detections and imaging of black hole shadows, have strongly validated general relativity. Nevertheless, ongoing cosmological observations suggest potential limitations of general relativity, spurring interest in modified theories of gravity. This work investigates the Lorentz-gauge formulation of gravity-a novel framework that addresses key conceptual challenges in quantum gravity and cosmology by leveraging the recent black-hole solutions presented in [10.1103/PhysRevD.111.064008] [1]. By analyzing black hole shadow structures and gravitational lensing effects-both weak and strong deflection regimes-we highlight unique observational signatures of Lorentz gauge gravity. Our findings provide valuable tools for future observational tests, potentially distinguishing these modified gravity models from general relativity and advancing our understanding of spacetime geometry and fundamental gravitational interactions.
dc.description.sponsorshipCOST Action [CA21106, CA21136, CA22113, CA23130, CA23115]; COST (European Cooperation in Science and Technology); EMU; TUBITAK; ULAKBIM (Turkiye); SCOAP3 (Switzerland); Universidad Central de Chile [PDUCEN20240008]
dc.description.sponsorshipA.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 CA21136-Addressing observational tensions in cosmology with systematics and fundamental physics (CosmoVerse) , the COST Action CA22113-Fundamental challenges in theoretical physics (THEORY-CHALLENGES) , the COST Action CA23130-Bridging high and low energies in search of quantum gravity (BridgeQG) and the COST Action CA23115-Relativistic Quantum Information (RQI) funded by COST (European Cooperation in Science and Technology) . We also thank EMU, TUBITAK, ULAKBIM (Turkiye) and SCOAP3 (Switzerland) for their support. The work of M.F. is supported by Universidad Central de Chile through the project No. PDUCEN20240008.
dc.identifier.doi10.1016/j.nuclphysb.2025.117063
dc.identifier.issn0550-3213
dc.identifier.issn1873-1562
dc.identifier.orcid0000-0002-9889-342X
dc.identifier.orcid0000-0002-1602-0722
dc.identifier.scopus2-s2.0-105012473088
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1016/j.nuclphysb.2025.117063
dc.identifier.urihttps://hdl.handle.net/11129/13232
dc.identifier.volume1018
dc.identifier.wosWOS:001554192000001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherElsevier
dc.relation.ispartofNuclear Physics B
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectBlack holes
dc.subjectWeak deflection angle
dc.subjectBlack hole shadow
dc.subjectStrong lensing
dc.subjectLorentz gauge theory
dc.titleShedding light on gravity: Black hole shadows and lensing signatures in Lorentz gauge theory
dc.typeArticle

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