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No-hair conjectures, primordial shear and protoinflationary initial conditions

Anisotropic inflationary background geometries are analyzed in the context of an extended gauge action where the electric and magnetic susceptibilities are not bound to coincide and depend on the inflaton field. After deriving various classes of solutions with electric and magnetic hairs, we discuss...

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Autor principal: Giovannini, Massimo
Lenguaje:eng
Publicado: 2013
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.89.063512
http://cds.cern.ch/record/1637584
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author Giovannini, Massimo
author_facet Giovannini, Massimo
author_sort Giovannini, Massimo
collection CERN
description Anisotropic inflationary background geometries are analyzed in the context of an extended gauge action where the electric and magnetic susceptibilities are not bound to coincide and depend on the inflaton field. After deriving various classes of solutions with electric and magnetic hairs, we discuss the problem of the initial boundary conditions of the shear parameter and consider a globally neutral plasma as a possible relic of a preinflationary stage of expansion. While electric hairs are washed out by the finite value of the protoinflationary conductivity, magnetic hairs can persist and introduce a tiny amount of shear causing a different inflationary rate of expansion along orthogonal spatial directions. The plasma interactions are a necessary criterion to discriminate between physical and unphysical initial conditions but they are not strictly sufficient to warrant the stability of a given magnetic solution.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2013
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spelling cern-16375842021-06-15T02:01:05Zdoi:10.1103/PhysRevD.89.063512http://cds.cern.ch/record/1637584engGiovannini, MassimoNo-hair conjectures, primordial shear and protoinflationary initial conditionsParticle Physics - TheoryAnisotropic inflationary background geometries are analyzed in the context of an extended gauge action where the electric and magnetic susceptibilities are not bound to coincide and depend on the inflaton field. After deriving various classes of solutions with electric and magnetic hairs, we discuss the problem of the initial boundary conditions of the shear parameter and consider a globally neutral plasma as a possible relic of a preinflationary stage of expansion. While electric hairs are washed out by the finite value of the protoinflationary conductivity, magnetic hairs can persist and introduce a tiny amount of shear causing a different inflationary rate of expansion along orthogonal spatial directions. The plasma interactions are a necessary criterion to discriminate between physical and unphysical initial conditions but they are not strictly sufficient to warrant the stability of a given magnetic solution.Anisotropic inflationary background geometries are analyzed in the context of an extended gauge action where the electric and magnetic susceptibilities are not bound to coincide and depend on the inflaton field. After deriving various classes of solutions with electric and magnetic hairs, we discuss the problem of the initial boundary conditions of the shear parameter and consider a globally neutral plasma as a possible relic of a preinflationary stage of expansion. While electric hairs are washed out by the finite value of the protoinflationary conductivity, magnetic hairs can persist and introduce a tiny amount of shear causing a different inflationary rate of expansion along orthogonal spatial directions. The plasma interactions are a necessary criterion to discriminate between physical and unphysical initial conditions but they are not strictly sufficient to warrant the stability of a given magnetic solution.Anisotropic inflationary background geometries are analyzed in the context of an extended gauge action where the electric and magnetic susceptibilities are not bound to coincide and depend on the inflaton field. After deriving various classes of solutions with electric and magnetic hairs, we discuss the problem of the initial boundary conditions of the shear parameter and consider a globally neutral plasma as a possible relic of a preinflationary stage of expansion. While electric hairs are washed out by the finite value of the protoinflationary conductivity, magnetic hairs can persist and introduce a tiny amount of shear causing a different inflationary rate of expansion along orthogonal spatial directions. The plasma interactions are a necessary criterion to discriminate between physical and unphysical initial conditions but they are not strictly sufficient to warrant the stability of a given magnetic solution.CERN-PH-TH-2013-300arXiv:1312.4832CERN-PH-TH-2013-300oai:cds.cern.ch:16375842013-12-17
spellingShingle Particle Physics - Theory
Giovannini, Massimo
No-hair conjectures, primordial shear and protoinflationary initial conditions
title No-hair conjectures, primordial shear and protoinflationary initial conditions
title_full No-hair conjectures, primordial shear and protoinflationary initial conditions
title_fullStr No-hair conjectures, primordial shear and protoinflationary initial conditions
title_full_unstemmed No-hair conjectures, primordial shear and protoinflationary initial conditions
title_short No-hair conjectures, primordial shear and protoinflationary initial conditions
title_sort no-hair conjectures, primordial shear and protoinflationary initial conditions
topic Particle Physics - Theory
url https://dx.doi.org/10.1103/PhysRevD.89.063512
http://cds.cern.ch/record/1637584
work_keys_str_mv AT giovanninimassimo nohairconjecturesprimordialshearandprotoinflationaryinitialconditions