Stochastic gravitoelectromagnetic inflation

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dc.creatorAguilar, J. E. Madriz
dc.creatorBellini, Mauricio
dc.date2006-05-08
dc.date2007-05-15
dc.date.accessioned2026-07-07T10:24:18Z
dc.date.available2026-07-07T10:24:18Z
dc.descriptionGravitoelectromagnetic inflation was recently introduced to describe, in an unified manner, electromagnetic, gravitatory and inflaton fields in the early (accelerated) inflationary universe from a 5D vacuum state. In this paper, we study a stochastic treatment for the gravitoelectromagnetic components $A_B=(A_μ,ϕ)$, on cosmological scales. We focus our study on the seed magnetic fields on super Hubble scales, which could play an important role in large scale structure formation of the universe.
dc.descriptionfinal version published in Phys. Lett. B
dc.identifierhttps://arxiv.org/abs/gr-qc/0605043
dc.identifierhttp://arxiv.org/abs/gr-qc/0605043
dc.identifierPhys.Lett.B642:302-310,2006
dc.identifierdoi:10.1016/j.physletb.2006.09.050
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176138
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleStochastic gravitoelectromagnetic inflation
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