Gravitational lensing in rotating and twisting universes

dc.contributor.authorGurtug, O.
dc.contributor.authorMangut, M.
dc.contributor.authorHalilsoy, M.
dc.date.accessioned2026-02-06T18:37:17Z
dc.date.issued2021
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractGravitational lensing caused by the gravitational field of massive objects has been studied and acknowledged for a long period of time. In this paper, however, we propose a different mechanism where the bending of light stems from the non-linear interaction of gravitational, electromagnetic and axion waves that creates the high curvature zone in the space-time fabric. The striking distinction in the present study is that in contrast to the convex lensing in the gravitational field of a massive object, hyperbolic nature of the high curvature zone of the background space-time may give rise to concave lensing. Expectedly detection of this kind of lensing becomes possible through satellite detectors. (C) 2021 Elsevier B.V. All rights reserved.
dc.identifier.doi10.1016/j.astropartphys.2021.102558
dc.identifier.issn0927-6505
dc.identifier.issn1873-2852
dc.identifier.orcid0000-0001-9344-5786
dc.identifier.orcid0000-0003-3364-1923
dc.identifier.scopus2-s2.0-85099388096
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1016/j.astropartphys.2021.102558
dc.identifier.urihttps://hdl.handle.net/11129/12380
dc.identifier.volume128
dc.identifier.wosWOS:000621632600008
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherElsevier
dc.relation.ispartofAstroparticle Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectGravitational lensing
dc.titleGravitational lensing in rotating and twisting universes
dc.typeArticle

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