A non-diagonal singularity-free model in torsion gravity

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dc.contributor.authorKorunur, Murat
dc.date.accessioned2024-04-24T17:20:20Z
dc.date.available2024-04-24T17:20:20Z
dc.date.issued2012
dc.departmentDicle Üniversitesien_US
dc.description.abstractIn the context of torsion (teleparallel) gravity, we focus on discussing the spin effects of Dirac particles associated with the non-diagonal singularity-free model (Mars space-time). We see that the vector part depends on the radial r and z directions and the axial-vector will be along the radial direction, that is, it will be symmetric about radial direction. Furthermore, the t = 0 case of the Mars metric is considered, thence it is seen that the axial-vector vanishes.en_US
dc.identifier.doi10.2478/s11534-012-0083-2
dc.identifier.endpage849en_US
dc.identifier.issn1895-1082
dc.identifier.issn1644-3608
dc.identifier.issue4en_US
dc.identifier.scopus2-s2.0-84864104030
dc.identifier.scopusqualityN/A
dc.identifier.startpage846en_US
dc.identifier.urihttps://doi.org/10.2478/s11534-012-0083-2
dc.identifier.urihttps://hdl.handle.net/11468/18946
dc.identifier.volume10en_US
dc.identifier.wosWOS:000306484600011
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoenen_US
dc.publisherDe Gruyter Poland Sp Zooen_US
dc.relation.ispartofCentral European Journal of Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectMars Space-Timeen_US
dc.subjectTeleparallel Gravityen_US
dc.subjectAxial Vectoren_US
dc.subjectTorsionen_US
dc.titleA non-diagonal singularity-free model in torsion gravityen_US
dc.titleA non-diagonal singularity-free model in torsion gravity
dc.typeArticleen_US

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