Abstract

The measurements of the Higgs mass and top Yukawa coupling indicate that we live in a very special Universe, at the edge of the absolute stability of the electroweak vacuum. If fully stable, the Standard Model (SM) can be extended all the way up to the inflationary scale and the Higgs field, non-minimally coupled to gravity with strength $\xi$, can be responsible for inflation. We show that the successful Higgs inflation scenario can also take place if the SM vacuum is not absolutely stable. This conclusion is based on two effects that were overlooked previously. The first one is associated with the effective renormalization of the SM couplings at the energy scale $M_P/\xi$, where $M_P$ is the Planck scale. The second one is a symmetry restoration after inflation due to high temperature effects that leads to the (temporary) disappearance of the vacuum at Planck values of the Higgs field.

Highlights

  • One of the most interesting questions in particle physics and cosmology is the relation between the properties of elementary particles and the structure of the Universe

  • The present experimental data are perfectly consistent with the absolute stability of Standard Model within the experimental and theoretical uncertainties, one should not exclude the possibility that other experiments will be able to establish the metastability of the electroweak vacuum in the future

  • Should the Higgs inflation idea be abandoned in this case? This paper gives a negative answer to this question

Read more

Summary

INTRODUCTION

The behavior of the Higgs self-coupling λ is quite peculiar: it decreases with energy to eventually arrive at a minimum at Planck scale values and starts increasing thereafter, see Fig. 1. [6], shows the borderline between the regions of absolute stability and metastability of the SM vacuum on the plane of the Higgs boson mass and top quark Yukawa coupling in the MS scheme taken at μ 1⁄4 173.2 GeV. Sketch of the effective Higgs inflation potential for the scenario considered in this paper It contains an inflationary plateau at χ ≳ MP and two minima.

THE GENERAL FRAMEWORK
N ð2:7Þ and with them the inflationary observables ns
Sensitivity to higher-dimensional operators
Reliability of the computation of radiative corrections
Critical regime
Relation between low- and high-energy parameters
HIGH-ENERGY VERSUS LOW-ENERGY PARAMETERS OF THE STANDARD MODEL
F00F2 F4 þ
Top Yukawa coupling
HIGGS INFLATION WITH METASTABLE VACUUM
HIGH-TEMPERATURE EFFECTIVE POTENTIAL
à d3k 2jkjð2πÞ3
SM coupling SM
PREHEATING
Noncritical Higgs inflation
15 U 10 U1
Critical Higgs inflation
CONCLUSIONS
C RH ðE1Þ

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.