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Dirac field as a source of the inflation in \(2 + 1\) dimensional teleparallel gravity - MaRDI portal

Dirac field as a source of the inflation in \(2 + 1\) dimensional teleparallel gravity (Q2364263)

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Dirac field as a source of the inflation in \(2 + 1\) dimensional teleparallel gravity
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    Dirac field as a source of the inflation in \(2 + 1\) dimensional teleparallel gravity (English)
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    18 July 2017
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    Summary: In this paper, we study early-time inflation and late-time acceleration of the universe by nonminimally coupling the Dirac field with torsion in the spatially flat Friedman-Robertson-Walker (FRW) cosmological model background. The results obtained by the Noether symmetry approach with and without a gauge term are compared. Additionally, we compare these results with that of the \(3 + 1\) dimensional teleparallel gravity under Noether symmetry approach. And we see that the study explains early-time inflation and late-time acceleration of the universe.
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