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dc.contributor.authorMyrzakulov, Yerlan
dc.contributor.authorBekov, Sabit
dc.contributor.authorMyrzakulov, Kairat
dc.date.accessioned2025-01-23T06:28:15Z
dc.date.available2025-01-23T06:28:15Z
dc.date.issued2021
dc.identifier.issn1742-6596
dc.identifier.otherdoi:10.1088/1742-6596/2090/1/012058
dc.identifier.urihttp://rep.enu.kz/handle/enu/21043
dc.description.abstractIn this work, we consider a homogeneous and isotropic cosmological model of the universe in f(T, B) gravity with non-minimally coupled fermionic field. In order to find the form of the coupling function F(Ψ), the potential function V (Ψ) of the fermionic field and the function f(T, B), we found through the Noether symmetry approach. The results obtain are coincide with the observational data that describe the late-time accelerated expansion of the universe.ru
dc.language.isoenru
dc.publisherJournal of Physics: Conference Seriesru
dc.relation.ispartofseries2090 (2021) 012058;
dc.titleNoether symmetry approach in f(T, B) teleparallel gravity with a fermionic fieldru
dc.typeArticleru


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Показать сокращенную информацию