Noether symmetry approach in f(T, B) teleparallel gravity with a fermionic field

dc.contributor.author	Myrzakulov, Yerlan
dc.contributor.author	Bekov, Sabit
dc.contributor.author	Myrzakulov, Kairat
dc.date.accessioned	2025-01-23T06:28:15Z
dc.date.available	2025-01-23T06:28:15Z
dc.date.issued	2021
dc.identifier.issn	1742-6596
dc.identifier.other	doi:10.1088/1742-6596/2090/1/012058
dc.identifier.uri	http://rep.enu.kz/handle/enu/21043
dc.description.abstract	In 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.iso	en	ru
dc.publisher	Journal of Physics: Conference Series	ru
dc.relation.ispartofseries	2090 (2021) 012058;
dc.title	Noether symmetry approach in f(T, B) teleparallel gravity with a fermionic field	ru
dc.type	Article	ru