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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...
Autores principales: | De Simone, Andrea, Perrier, Hideki, Riotto, Antonio |
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Lenguaje: | eng |
Publicado: |
2012
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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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