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dc.contributor.authorGÜDEKLİ, Ertan
dc.contributor.authorSong, Shi-Qin
dc.date.accessioned2023-02-21T09:57:34Z
dc.date.available2023-02-21T09:57:34Z
dc.identifier.citationSong S., GÜDEKLİ E., "Traversable wormholes in Rastall teleparallel gravity with non-commutative geometry", New Astronomy, cilt.100, 2023
dc.identifier.issn1384-1076
dc.identifier.othervv_1032021
dc.identifier.otherav_38cc7fc9-4a00-49f0-995a-e9d27c231578
dc.identifier.urihttp://hdl.handle.net/20.500.12627/187959
dc.identifier.urihttps://doi.org/10.1016/j.newast.2022.101993
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85146176341&origin=inward
dc.description.abstract© 2022The current study explores new wormhole models with the framework of Rastall teleparallel theory. For this study, we are working with non-commutative geometry with Gaussian and Lorentzian distributions. The static and spherically symmetric spacetime is taken with the anisotropic source of fluid. Further, we compare the matter density with the Gaussian and Lorentzian distributions and get two different differential equations involving shape functions. The exact solution for the wormhole shape function is calculated for both distributions. The expression for energy conditions is provided. The graphical behavior of shape functions and energy conditions is presented for Rastall teleparallel theory under the current scenario. All the inquired results with necessary findings are concluded.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.titleTraversable wormholes in Rastall teleparallel gravity with non-commutative geometry
dc.typeMakale
dc.relation.journalNew Astronomy
dc.contributor.department, ,
dc.identifier.volume100
dc.contributor.firstauthorID4244167


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