Teleparallel energy-momentum distribution of various black hole and wormhole metrics

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dc.authoridAygün, Sezgin / 0000-0002-2969-4195
dc.authoridBaysal, Hüsnü / 0000-0002-5709-6301
dc.authoridAktaş, Can / 0000-0002-0603-7862
dc.authoridYılmaz, İhsan / 0000-0001-7684-9690
dc.authoridTarhan, İsmail / 0000-0001-6156-0827
dc.contributor.authorAygün, Sezgin
dc.contributor.authorBaysal, Hüsnü
dc.contributor.authorAktaş, Can
dc.contributor.authorYılmaz, İhsan
dc.contributor.authorSahoo, P. K.
dc.contributor.authorTarhan, İsmail
dc.date.accessioned2025-01-27T20:12:29Z
dc.date.available2025-01-27T20:12:29Z
dc.date.issued2018
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractUsing the Einstein, Bergmann-Thomson (BT) and Landau-Lifshitz (LL) energy and momentum formulations in teleparallel gravity (TG), we obtain the total energy and momentum distributions for phantom black hole metric. We get different energy distributions similar to the earlier study and the momentum distributions vanish for phantom black hole metric in TG. These momentum solutions agree with the study of Sahoo et al. in general relativity. However, using Einstein, Bergmann-Thomson and Landau-Lifshitz energy and momentum complexes, we investigate regular black hole, asymptotically flat wormhole, anti-de Sitter wormhole and Ellis wormhole solutions in TG. We obtain i) same BT and LL energy density solutions for regular black hole metric, (ii) same and zero energy distribution for asymptotically flat wormhole, (iii) proportion with Einstein and BT energy density solutions for anti-de Sitter wormhole, (iv) same and negative Einstein and BT energy density solutions for Ellis wormhole in TG.
dc.description.sponsorshipCanakkale Onsekiz Mart University, The Scientific Research Coordination Unit [FBA-2018-1437]
dc.description.sponsorshipThis work was supported by Canakkale Onsekiz Mart University, The Scientific Research Coordination Unit, Project number: FBA-2018-1437. The authors also thank the reviewers and the editor for the valuable suggestions, which improved the presentation of the present results.
dc.identifier.doi10.1142/S0217751X18501841
dc.identifier.issn0217-751X
dc.identifier.issn1793-656X
dc.identifier.issue30
dc.identifier.scopus2-s2.0-85056544107
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1142/S0217751X18501841
dc.identifier.urihttps://hdl.handle.net/20.500.12428/20956
dc.identifier.volume33
dc.identifier.wosWOS:000450007500009
dc.identifier.wosqualityQ4
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.ispartofInternational Journal of Modern Physics A
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectPhantom black hole
dc.subjectenergy-momentum complexes
dc.subjectteleparallel gravity
dc.subjectregular black hole
dc.subjectEllis wormhole
dc.titleTeleparallel energy-momentum distribution of various black hole and wormhole metrics
dc.typeArticle

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