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Dirac spinors and their application to Bianchi-I space-times in 5 dimensions

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arxiv 1808.08536 v3 pith:BDUIMN74 submitted 2018-08-26 gr-qc math-phmath.MP

classification gr-qcmath-phmath.MP
keywords fieldsdimensionsdiracfivespinorapplicationbianchi-ifact
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We consider a five-dimensional Einstein--Cartan spacetime upon which Dirac spinor fields can be defined. Dirac spinor fields in five and four dimensions share many features, like the fact that both are described by four-component spinor fields, but they are also characterized by strong differences, like the fact that in five dimensions we do not have the possibility to project on left-handed and right-handed chiral parts unlike what happens in the four-dimensional instance: we conduct a polar decomposition of the spinorial fields, so to highlight all similarities and discrepancies. As an application of spinor fields in five dimensions, we study Bianchi-I spacetimes, verifying whether the Dirac fields in five dimensions can give rise to inflation or dark-energy dominated cosmological eras or not.

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