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Classical and quantum initial conditions for Higgs inflation

2015/06/30 by Alberto Salvio, Anupam Mazumdar · 149 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Einstein #Higgs boson #Higgs field #Homogeneity (statistics) #Inflation (cosmology) #Mathematical physics #Mathematics #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum #Quantum gravity #Quantum mechanics #Renormalization #Theoretical physics #astro-ph.CO #gr-qc #hep-ph #hep-th

paper · pdf · doi:10.1016/j.physletb.2015.09.020

published in Physics Letters B 750, 194-200 (Elsevier BV) · 8 pages, 2 figures; v2: some wording changed and references added

arxiv created 2015/07/02 · openalex publication_date 2015/09/12 · arxiv updated 2016/02/16 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We investigate whether Higgs inflation can occur in the Standard Model starting from natural initial conditions or not. The Higgs has a non-minimal coupling to the Ricci scalar. We confine our attention to the regime where quantum Einstein gravity effects are small in order to have results that are independent of the ultraviolet completion of gravity. At the classical level we find no tuning is required to have successful Higgs inflation, provided the initial homogeneity condition is satisfied. On the other hand, at the quantum level we obtain that the renormalization for large non-minimal coupling requires an additional degree of freedom, unless a tuning of the initial values of the running parameters is made. In order to see that this effect may change the predictions we finally include such degree of freedom in the field content and show that Starobinsky's R2 inflation dominates over Higgs inflation.

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