Cosmological magnetic fields induced by metric perturbations after inflation
We consider the amplification of electromagnetic quantum vacuum fluctuations induced by the presence of metric perturbations at the end of inflation. We obtain the amplitude of the corresponding magnetic fields on super-Hubble scales and compare it with the requirements of the galactic dynamo mechan...
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ftdatacite:10.48550/arxiv.hep-ph/0111268 2023-05-15T18:07:38+02:00 Cosmological magnetic fields induced by metric perturbations after inflation Maroto, Antonio L. 2001 https://dx.doi.org/10.48550/arxiv.hep-ph/0111268 https://arxiv.org/abs/hep-ph/0111268 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ High Energy Physics - Phenomenology hep-ph FOS Physical sciences Preprint Article article CreativeWork 2001 ftdatacite https://doi.org/10.48550/arxiv.hep-ph/0111268 2022-04-01T16:51:40Z We consider the amplification of electromagnetic quantum vacuum fluctuations induced by the presence of metric perturbations at the end of inflation. We obtain the amplitude of the corresponding magnetic fields on super-Hubble scales and compare it with the requirements of the galactic dynamo mechanism for different values of the spectral index. Finally we discuss the possible effects of the dissipation of such fields in the form of gravitational waves. : 8 pages, 1 figure. Presented at COSMO-01 conference, Rovaniemi, Finland, August 29-September 4, 2001 Report Rovaniemi DataCite Metadata Store (German National Library of Science and Technology) Hubble ENVELOPE(158.317,158.317,-80.867,-80.867) Rovaniemi ENVELOPE(26.159,26.159,66.392,66.392) |
institution |
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collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
topic |
High Energy Physics - Phenomenology hep-ph FOS Physical sciences |
spellingShingle |
High Energy Physics - Phenomenology hep-ph FOS Physical sciences Maroto, Antonio L. Cosmological magnetic fields induced by metric perturbations after inflation |
topic_facet |
High Energy Physics - Phenomenology hep-ph FOS Physical sciences |
description |
We consider the amplification of electromagnetic quantum vacuum fluctuations induced by the presence of metric perturbations at the end of inflation. We obtain the amplitude of the corresponding magnetic fields on super-Hubble scales and compare it with the requirements of the galactic dynamo mechanism for different values of the spectral index. Finally we discuss the possible effects of the dissipation of such fields in the form of gravitational waves. : 8 pages, 1 figure. Presented at COSMO-01 conference, Rovaniemi, Finland, August 29-September 4, 2001 |
format |
Report |
author |
Maroto, Antonio L. |
author_facet |
Maroto, Antonio L. |
author_sort |
Maroto, Antonio L. |
title |
Cosmological magnetic fields induced by metric perturbations after inflation |
title_short |
Cosmological magnetic fields induced by metric perturbations after inflation |
title_full |
Cosmological magnetic fields induced by metric perturbations after inflation |
title_fullStr |
Cosmological magnetic fields induced by metric perturbations after inflation |
title_full_unstemmed |
Cosmological magnetic fields induced by metric perturbations after inflation |
title_sort |
cosmological magnetic fields induced by metric perturbations after inflation |
publisher |
arXiv |
publishDate |
2001 |
url |
https://dx.doi.org/10.48550/arxiv.hep-ph/0111268 https://arxiv.org/abs/hep-ph/0111268 |
long_lat |
ENVELOPE(158.317,158.317,-80.867,-80.867) ENVELOPE(26.159,26.159,66.392,66.392) |
geographic |
Hubble Rovaniemi |
geographic_facet |
Hubble Rovaniemi |
genre |
Rovaniemi |
genre_facet |
Rovaniemi |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.hep-ph/0111268 |
_version_ |
1766179858911592448 |