Running Inflation in the Standard Model
Andrea De Simone, Mark P. Hertzberg, Frank Wilczek
TL;DR
The paper tests whether the Standard Model Higgs field, non-minimally coupled to gravity, can drive inflation when quantum corrections are included via renormalization group methods. They derive the RG-improved effective action, showing that the running of the effective Planck mass and SM couplings affects inflationary observables, notably producing a Higgs-mass–dependent spectral index n_s. Their results yield n_s around 0.968 for typical parameters, with a sharp increase toward ~0.98 as the Higgs mass approaches vacuum instability, and predict small tensor-to-scalar ratio r ~ 0.003. The work connects high-energy SM parameters to Planck-scale cosmology, offering testable predictions for PLANCK and LHC and discussing EFT validity and possible generalizations.
Abstract
An interacting scalar field with largish coupling to curvature can support a distinctive inflationary universe scenario. Previously this has been discussed for the Standard Model Higgs field, treated classically or in a leading log approximation. Here we investigate the quantum theory using renormalization group methods. In this model the running of both the effective Planck mass and the couplings is important. The cosmological predictions are consistent with existing WMAP5 data, with 0.967 < n_s < 0.98 (for N_e = 60) and negligible gravity waves. We find a relationship between the spectral index and the Higgs mass that is sharply varying for m_h ~ 120-135 GeV (depending on the top mass); in the future, that relationship could be tested against data from PLANCK and LHC. We also comment briefly on how similar dynamics might arise in more general settings, and discuss our assumptions from the effective field theory point of view.
