Stochastic gravitoelectromagnetic inflation
arXiv:gr-qc/0605043 · doi:10.1016/j.physletb.2006.09.050
Abstract
Gravitoelectromagnetic 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 , 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.
final version published in Phys. Lett. B
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- Inflation from Charged Scalar and Primordial Magnetic Fields?
- Correlated curvature perturbations and magnetogenesis from the GUT gauge bosons
- Primordial large-scale electromagnetic fields from Gravitoelectromagnetic Inflation
- Coupled inflaton and electromagnetic fields from Gravitoelectromagnetic Inflation with Lorentz and Feynman gauges
- Semiclassical Gravitoelectromagnetic inflation in a Lorentz gauge: seminal inflaton fluctuations and electromagnetic fields from a 5D vacuum state
- Stochastic Inflation and Replica Field Theory
- The seed of magnetic monopoles in the early inflationary universe from a 5D vacuum state
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- Inflation from the bang of a white hole induced from a 6D vacuum state
- Mass density of the Earth from a Gravito-Electro-Magnetic 5D vacuum