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Non-Gaussianities from the Standard Model Higgs

We have recently proposed that the Standard Model Higgs might be responsible for generating the cosmological perturbations of the universe by acting as an isocurvature mode during a de Sitter inflationary stage. In this paper we study the level of non-Gaussianity in the cosmological perturbations wh...

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Detalles Bibliográficos
Autores principales: De Simone, Andrea, Perrier, Hideki, Riotto, Antonio
Lenguaje:eng
Publicado: 2012
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2013/01/037
http://cds.cern.ch/record/1489787
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author De Simone, Andrea
Perrier, Hideki
Riotto, Antonio
author_facet De Simone, Andrea
Perrier, Hideki
Riotto, Antonio
author_sort De Simone, Andrea
collection CERN
description We have recently proposed that the Standard Model Higgs might be responsible for generating the cosmological perturbations of the universe by acting as an isocurvature mode during a de Sitter inflationary stage. In this paper we study the level of non-Gaussianity in the cosmological perturbations which are inevitably generated due to the non-linearities of the Standard Model Higgs potential. In particular, for the current central value of the top mass, we find that a future detection of non-Gaussianity would exclude the detection of tensor modes by the PLANCK satellite.
id cern-1489787
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2012
record_format invenio
spelling cern-14897872023-10-04T08:18:43Zdoi:10.1088/1475-7516/2013/01/037http://cds.cern.ch/record/1489787engDe Simone, AndreaPerrier, HidekiRiotto, AntonioNon-Gaussianities from the Standard Model HiggsParticle Physics - PhenomenologyWe have recently proposed that the Standard Model Higgs might be responsible for generating the cosmological perturbations of the universe by acting as an isocurvature mode during a de Sitter inflationary stage. In this paper we study the level of non-Gaussianity in the cosmological perturbations which are inevitably generated due to the non-linearities of the Standard Model Higgs potential. In particular, for the current central value of the top mass, we find that a future detection of non-Gaussianity would exclude the detection of tensor modes by the PLANCK satellite.We have recently proposed that the Standard Model Higgs might be responsible for generating the cosmological perturbations of the universe by acting as an isocurvature mode during a de Sitter inflationary stage. In this paper we study the level of non-Gaussianity in the cosmological perturbations which are inevitably generated due to the non-linearities of the Standard Model Higgs potential. In particular, for the current central value of the top mass, we find that a future detection of non-Gaussianity would exclude the detection of tensor modes by the PLANCK satellite.We have recently proposed that the Standard Model Higgs might be responsible for generating the cosmological perturbations of the universe by acting as an isocurvature mode during a de Sitter inflationary stage. In this paper we study the level of non-Gaussianity in the cosmological perturbations which are inevitably generated due to the non-linearities of the Standard Model Higgs potential. In particular, for the current central value of the top mass, we find that a future detection of non-Gaussianity would exclude the detection of tensor modes by the PLANCK satellite.arXiv:1210.6618CERN-PH-TH-2012-277SISSA-29-2012-EPCERN-PH-TH-2012-277SISSA 29-2012-EPoai:cds.cern.ch:14897872012-10-25
spellingShingle Particle Physics - Phenomenology
De Simone, Andrea
Perrier, Hideki
Riotto, Antonio
Non-Gaussianities from the Standard Model Higgs
title Non-Gaussianities from the Standard Model Higgs
title_full Non-Gaussianities from the Standard Model Higgs
title_fullStr Non-Gaussianities from the Standard Model Higgs
title_full_unstemmed Non-Gaussianities from the Standard Model Higgs
title_short Non-Gaussianities from the Standard Model Higgs
title_sort non-gaussianities from the standard model higgs
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1088/1475-7516/2013/01/037
http://cds.cern.ch/record/1489787
work_keys_str_mv AT desimoneandrea nongaussianitiesfromthestandardmodelhiggs
AT perrierhideki nongaussianitiesfromthestandardmodelhiggs
AT riottoantonio nongaussianitiesfromthestandardmodelhiggs