Fermions in a Walecka-type cosmology

A simplified Walecka-type model is investigated in a cosmological scenario. The model includes fermionic, scalar and vector fields as sources. It is shown that their interactions, taking place in a Robertson-Walker metric, could be responsible for the transition of accelerated-decelerated periods in...

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Veröffentlicht in:Europhysics letters 2012-02, Vol.97 (4), p.P1-P1
Hauptverfasser: Ribas, M O, Zambianchi, P Jr, Devecchi, F P, Kremer, G M
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Zambianchi, P Jr
Devecchi, F P
Kremer, G M
description A simplified Walecka-type model is investigated in a cosmological scenario. The model includes fermionic, scalar and vector fields as sources. It is shown that their interactions, taking place in a Robertson-Walker metric, could be responsible for the transition of accelerated-decelerated periods in the early universe and a current accelerated regime. It is also discussed the role of the fermionic field as the promoter of the accelerated regimes in the early and the late stages of the universe.
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1286-4854
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source Institute of Physics Journals
subjects Cosmology
Fermions
Mathematical analysis
Scalars
Universe
Vectors (mathematics)
title Fermions in a Walecka-type cosmology
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