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Title: Cosmological magnetic fields from inflation in extended electromagnetism

Abstract

In this work we consider an extended electromagnetic theory in which the scalar state which is usually eliminated by means of the Lorenz condition is allowed to propagate. This state has been shown to generate a small cosmological constant in the context of standard inflationary cosmology. Here we show that the usual Lorenz gauge-breaking term now plays the role of an effective electromagnetic current. Such a current is generated during inflation from quantum fluctuations and gives rise to a stochastic effective charge density distribution. Because of the high electric conductivity of the cosmic plasma after inflation, the electric charge density generates currents which give rise to both vorticity and magnetic fields on sub-Hubble scales. Present upper limits on vorticity coming from temperature anisotropies of the CMB are translated into lower limits on the present value of cosmic magnetic fields. We find that, for a nearly scale invariant vorticity spectrum, magnetic fields B{sub {lambda}>}10{sup -12} G are typically generated with coherence lengths ranging from subgalactic scales up to the present Hubble radius. Those fields could act as seeds for a galactic dynamo or even account for observations just by collapse and differential rotation of the protogalactic cloud.

Authors:
;  [1]
  1. Departamento de Fisica Teorica, Universidad Complutense de Madrid, 28040, Madrid (Spain)
Publication Date:
OSTI Identifier:
21503936
Resource Type:
Journal Article
Resource Relation:
Journal Name: Physical Review. D, Particles Fields; Journal Volume: 83; Journal Issue: 2; Other Information: DOI: 10.1103/PhysRevD.83.023514; (c) 2011 American Institute of Physics
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; ANISOTROPY; COHERENCE LENGTH; COSMOLOGICAL CONSTANT; COSMOLOGY; DENSITY; EFFECTIVE CHARGE; ELECTRIC CHARGES; ELECTRIC CONDUCTIVITY; ELECTROMAGNETISM; FLUCTUATIONS; HUBBLE EFFECT; MAGNETIC FIELDS; PLASMA; RELICT RADIATION; ROTATION; SPECTRA; STOCHASTIC PROCESSES; DIMENSIONS; ELECTRICAL PROPERTIES; ELECTROMAGNETIC RADIATION; LENGTH; MAGNETISM; MICROWAVE RADIATION; MOTION; PHYSICAL PROPERTIES; RADIATIONS; VARIATIONS

Citation Formats

Beltran Jimenez, Jose, and Maroto, Antonio L. Cosmological magnetic fields from inflation in extended electromagnetism. United States: N. p., 2011. Web. doi:10.1103/PHYSREVD.83.023514.
Beltran Jimenez, Jose, & Maroto, Antonio L. Cosmological magnetic fields from inflation in extended electromagnetism. United States. doi:10.1103/PHYSREVD.83.023514.
Beltran Jimenez, Jose, and Maroto, Antonio L. 2011. "Cosmological magnetic fields from inflation in extended electromagnetism". United States. doi:10.1103/PHYSREVD.83.023514.
@article{osti_21503936,
title = {Cosmological magnetic fields from inflation in extended electromagnetism},
author = {Beltran Jimenez, Jose and Maroto, Antonio L.},
abstractNote = {In this work we consider an extended electromagnetic theory in which the scalar state which is usually eliminated by means of the Lorenz condition is allowed to propagate. This state has been shown to generate a small cosmological constant in the context of standard inflationary cosmology. Here we show that the usual Lorenz gauge-breaking term now plays the role of an effective electromagnetic current. Such a current is generated during inflation from quantum fluctuations and gives rise to a stochastic effective charge density distribution. Because of the high electric conductivity of the cosmic plasma after inflation, the electric charge density generates currents which give rise to both vorticity and magnetic fields on sub-Hubble scales. Present upper limits on vorticity coming from temperature anisotropies of the CMB are translated into lower limits on the present value of cosmic magnetic fields. We find that, for a nearly scale invariant vorticity spectrum, magnetic fields B{sub {lambda}>}10{sup -12} G are typically generated with coherence lengths ranging from subgalactic scales up to the present Hubble radius. Those fields could act as seeds for a galactic dynamo or even account for observations just by collapse and differential rotation of the protogalactic cloud.},
doi = {10.1103/PHYSREVD.83.023514},
journal = {Physical Review. D, Particles Fields},
number = 2,
volume = 83,
place = {United States},
year = 2011,
month = 1
}
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