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.
