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Non-minimal Coupling of the Higgs Boson to Curvature in an Inflationary Universe

In the absence of new physics around [Formula: see text] GeV, the electroweak vacuum is at best metastable. This represents a major challenge for high scale inflationary models as, during the early rapid expansion of the universe, it seems difficult to understand how the Higgs vacuum would not decay...

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Detalles Bibliográficos
Autores principales: Calmet, Xavier, Kuntz, Iberê, Moss, Ian G.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer US 2017
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6956876/
https://www.ncbi.nlm.nih.gov/pubmed/31997830
http://dx.doi.org/10.1007/s10701-017-0131-2
Descripción
Sumario:In the absence of new physics around [Formula: see text] GeV, the electroweak vacuum is at best metastable. This represents a major challenge for high scale inflationary models as, during the early rapid expansion of the universe, it seems difficult to understand how the Higgs vacuum would not decay to the true lower vacuum of the theory with catastrophic consequences if inflation took place at a scale above [Formula: see text] GeV. In this paper we show that the non-minimal coupling of the Higgs boson to curvature could solve this problem by generating a direct coupling of the Higgs boson to the inflationary potential thereby stabilizing the electroweak vacuum. For specific values of the Higgs field initial condition and of its non-minimal coupling, inflation can drive the Higgs field to the electroweak vacuum quickly during inflation.