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Magnetogenesis, variation of gauge couplings and inflation
The interplay among the possible variation of gauge coupling and the inflationary dynamics is investigated in a simplified toy model. Depending upon various parameters (scalar mass, curvature scale at the end of inflation and at the onset of the radiation epoch), the two-point function of the magnet...
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Lenguaje: | eng |
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2002
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Acceso en línea: | http://cds.cern.ch/record/597285 |
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author | Giovannini, Massimo |
author_facet | Giovannini, Massimo |
author_sort | Giovannini, Massimo |
collection | CERN |
description | The interplay among the possible variation of gauge coupling and the inflationary dynamics is investigated in a simplified toy model. Depending upon various parameters (scalar mass, curvature scale at the end of inflation and at the onset of the radiation epoch), the two-point function of the magnetic inhomogeneities grows during the de Sitter stage of expansion and, consequently, large scale magnetic fields are generated. The requirements coming from inflationary magnetogenesis are examined together with the theoretical constraints stemming from the explicit model of the evolution of the gauge coupling. |
id | cern-597285 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2002 |
record_format | invenio |
spelling | cern-5972852023-03-20T10:06:01Zhttp://cds.cern.ch/record/597285engGiovannini, MassimoMagnetogenesis, variation of gauge couplings and inflationAstrophysics and AstronomyThe interplay among the possible variation of gauge coupling and the inflationary dynamics is investigated in a simplified toy model. Depending upon various parameters (scalar mass, curvature scale at the end of inflation and at the onset of the radiation epoch), the two-point function of the magnetic inhomogeneities grows during the de Sitter stage of expansion and, consequently, large scale magnetic fields are generated. The requirements coming from inflationary magnetogenesis are examined together with the theoretical constraints stemming from the explicit model of the evolution of the gauge coupling.The interplay among the possible variation of gauge coupling and the inflationary dynamics is investigated in a simplified toy model. Depending upon various parameters (scalar mass, curvature scale at the end of inflation and at the onset of the radiation epoch), the two-point function of the magnetic inhomogeneities grows during the de Sitter stage of expansion and, consequently, large scale magnetic fields are generated. The requirements coming from inflationary magnetogenesis are examined together with the theoretical constraints stemming from the explicit model of the evolution of the gauge coupling.astro-ph/0212346CERN-TH-2002-371CERN-TH-2002-371oai:cds.cern.ch:5972852002-12-16 |
spellingShingle | Astrophysics and Astronomy Giovannini, Massimo Magnetogenesis, variation of gauge couplings and inflation |
title | Magnetogenesis, variation of gauge couplings and inflation |
title_full | Magnetogenesis, variation of gauge couplings and inflation |
title_fullStr | Magnetogenesis, variation of gauge couplings and inflation |
title_full_unstemmed | Magnetogenesis, variation of gauge couplings and inflation |
title_short | Magnetogenesis, variation of gauge couplings and inflation |
title_sort | magnetogenesis, variation of gauge couplings and inflation |
topic | Astrophysics and Astronomy |
url | http://cds.cern.ch/record/597285 |
work_keys_str_mv | AT giovanninimassimo magnetogenesisvariationofgaugecouplingsandinflation |