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Weyl invariance and the conductivity of the protoinflationary plasma

We consider a globally neutral Lorentzian plasma as a possible remnant of a preinflationary stage of expansion and pose the problem of the suitable initial conditions for the evolution of the large-scale electromagnetic inhomogeneities. During the protoinflationary regime the Weyl invariance of the...

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Autor principal: Giovannini, Massimo
Lenguaje:eng
Publicado: 2012
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.85.101301
http://cds.cern.ch/record/1424602
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author Giovannini, Massimo
author_facet Giovannini, Massimo
author_sort Giovannini, Massimo
collection CERN
description We consider a globally neutral Lorentzian plasma as a possible remnant of a preinflationary stage of expansion and pose the problem of the suitable initial conditions for the evolution of the large-scale electromagnetic inhomogeneities. During the protoinflationary regime the Weyl invariance of the Ohmic current guarantees that the comoving conductivity is approximately constant. The subsequent breaking of Weyl invariance by the masses of the charge carriers drives the conductivity to zero. The newly derived conducting initial conditions for the amplification of large-scale magnetic fields are contrasted with the conventional vacuum initial conditions. It is shown, in a specific class of examples, that when the number of inflationary efolds is close to minimal the effects of the conducting initial conditions cannot be neglected.
id cern-1424602
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2012
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spelling cern-14246022019-09-30T06:29:59Zdoi:10.1103/PhysRevD.85.101301http://cds.cern.ch/record/1424602engGiovannini, MassimoWeyl invariance and the conductivity of the protoinflationary plasmaAstrophysics and AstronomyWe consider a globally neutral Lorentzian plasma as a possible remnant of a preinflationary stage of expansion and pose the problem of the suitable initial conditions for the evolution of the large-scale electromagnetic inhomogeneities. During the protoinflationary regime the Weyl invariance of the Ohmic current guarantees that the comoving conductivity is approximately constant. The subsequent breaking of Weyl invariance by the masses of the charge carriers drives the conductivity to zero. The newly derived conducting initial conditions for the amplification of large-scale magnetic fields are contrasted with the conventional vacuum initial conditions. It is shown, in a specific class of examples, that when the number of inflationary efolds is close to minimal the effects of the conducting initial conditions cannot be neglected.arXiv:1202.3344CERN-PH-TH-2012-027oai:cds.cern.ch:14246022012-02-16
spellingShingle Astrophysics and Astronomy
Giovannini, Massimo
Weyl invariance and the conductivity of the protoinflationary plasma
title Weyl invariance and the conductivity of the protoinflationary plasma
title_full Weyl invariance and the conductivity of the protoinflationary plasma
title_fullStr Weyl invariance and the conductivity of the protoinflationary plasma
title_full_unstemmed Weyl invariance and the conductivity of the protoinflationary plasma
title_short Weyl invariance and the conductivity of the protoinflationary plasma
title_sort weyl invariance and the conductivity of the protoinflationary plasma
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1103/PhysRevD.85.101301
http://cds.cern.ch/record/1424602
work_keys_str_mv AT giovanninimassimo weylinvarianceandtheconductivityoftheprotoinflationaryplasma