Primordial Dark Energy from a Condensate of Spinors in a 5D Vacuum

We explore the possibility that the expansion of the universe can be driven by a condensate of spinors which are free of interactions in a 5D relativistic vacuum defined in an extended de Sitter spacetime which is Riemann flat. The extra coordinate is considered as noncompact. After making a static...

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Main Authors: Pablo Alejandro Sánchez, Mauricio Bellini
Format: Article
Language:English
Published: Wiley 2013-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2013/789476
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author Pablo Alejandro Sánchez
Mauricio Bellini
author_facet Pablo Alejandro Sánchez
Mauricio Bellini
author_sort Pablo Alejandro Sánchez
collection DOAJ
description We explore the possibility that the expansion of the universe can be driven by a condensate of spinors which are free of interactions in a 5D relativistic vacuum defined in an extended de Sitter spacetime which is Riemann flat. The extra coordinate is considered as noncompact. After making a static foliation on the extra coordinate, we obtain an effective 4D (inflationary) de Sitter expansion which describes an inflationary universe. We found that the condensate of spinors studied here could be an interesting candidate to explain the presence of dark energy in the early universe. The dark energy density which we are talking about is poured into smaller subhorizon scales with the evolution of the inflationary expansion.
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spelling doaj-art-ef779c844a78452cad9050044f6989e52025-02-03T05:58:20ZengWileyAdvances in High Energy Physics1687-73571687-73652013-01-01201310.1155/2013/789476789476Primordial Dark Energy from a Condensate of Spinors in a 5D VacuumPablo Alejandro Sánchez0Mauricio Bellini1Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad Nacional de Mar del Plata, Funes 3350, 7600 Mar del Plata, ArgentinaDepartamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad Nacional de Mar del Plata, Funes 3350, 7600 Mar del Plata, ArgentinaWe explore the possibility that the expansion of the universe can be driven by a condensate of spinors which are free of interactions in a 5D relativistic vacuum defined in an extended de Sitter spacetime which is Riemann flat. The extra coordinate is considered as noncompact. After making a static foliation on the extra coordinate, we obtain an effective 4D (inflationary) de Sitter expansion which describes an inflationary universe. We found that the condensate of spinors studied here could be an interesting candidate to explain the presence of dark energy in the early universe. The dark energy density which we are talking about is poured into smaller subhorizon scales with the evolution of the inflationary expansion.http://dx.doi.org/10.1155/2013/789476
spellingShingle Pablo Alejandro Sánchez
Mauricio Bellini
Primordial Dark Energy from a Condensate of Spinors in a 5D Vacuum
Advances in High Energy Physics
title Primordial Dark Energy from a Condensate of Spinors in a 5D Vacuum
title_full Primordial Dark Energy from a Condensate of Spinors in a 5D Vacuum
title_fullStr Primordial Dark Energy from a Condensate of Spinors in a 5D Vacuum
title_full_unstemmed Primordial Dark Energy from a Condensate of Spinors in a 5D Vacuum
title_short Primordial Dark Energy from a Condensate of Spinors in a 5D Vacuum
title_sort primordial dark energy from a condensate of spinors in a 5d vacuum
url http://dx.doi.org/10.1155/2013/789476
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