2020
DOI: 10.3390/physics2030028
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The Higgs Field and Early Universe Cosmology: A (Brief) Review

Abstract: We review and discuss recent work exploring the implications of the Higgs field for early universe cosmology, and vice versa. Depending on the model under consideration, the Higgs may be one of a few scalar fields determining the evolution and fate of the Universe, or the Higgs field may be connected to a rich sector of scalar moduli with complicated dynamics. In particular, we look at the potential consequences of the Higgs field for inflation and its predictions, for the (meta)stability of the Standard Model… Show more

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Cited by 14 publications
(10 citation statements)
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References 174 publications
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“…If the mass of the left-handed tauon neutrino is estimated at ∼0.1 eV [99], and the Dirac mass of tauon leptons and quarks is estimated at ∼10 GeV [96], then the see-saw mechanism would predict the mass of the right-handed tauon neutrino to be ∼10 12 GeV. This is consistent with the 10 12 GeV energy scale of Pati-Salam symmetry breaking found in section 7, equation (86).…”
Section: Neutrino Massessupporting
confidence: 78%
“…If the mass of the left-handed tauon neutrino is estimated at ∼0.1 eV [99], and the Dirac mass of tauon leptons and quarks is estimated at ∼10 GeV [96], then the see-saw mechanism would predict the mass of the right-handed tauon neutrino to be ∼10 12 GeV. This is consistent with the 10 12 GeV energy scale of Pati-Salam symmetry breaking found in section 7, equation (86).…”
Section: Neutrino Massessupporting
confidence: 78%
“…(2.105 ± 0.030) × 10 −9 at 68%CL. By imposing this constraint, we see that B varies from 7.7 × 10 14 to 1.2 × 10 15 for N e = 50, and from 1.2 × 10 15 to 1.9 × 10 15 for N e = 60, when ξ decreases from 1000 to 10. We can conclude from figure 2 that the smaller values of ξ requires larger values of B to produce the same amplitude of scalar perturbations.…”
Section: Non-canonical Higgs Inflationmentioning
confidence: 99%
“…One of the best suited model of inflation from Planck-2018 observations [8] is Higgs inflation [10][11][12][13][14][15], where the Higgs field of the standard model of particle physics is nonminimally coupled to gravity to achieve inflation. The quartic potential for the minimally coupled Higgs field does not fit well with CMB observations, however, the Higgs field coupled with gravity leads to a model that agrees very well with the current observations [10,16].…”
Section: Introductionmentioning
confidence: 99%
“…Higgs Field is a field of energy that exists everywhere in the entire universe [34], [35]. The particle known as Higgs boson attracts other particles towards itself to gain mass [36]- [38].…”
Section: B Higgs Fieldmentioning
confidence: 99%
“…The theory of particle was first introduced by PW Higgs in 1964, describing the existence of a particle having a mass of 125 GeV (giga-electron volt) [40]. On 4th of July, 2012, by collaboration of Compact Muon Solenoid and Atlas, the Higgs Boson was first discovered using the LHC tunnel [34], [37].…”
Section: B Higgs Fieldmentioning
confidence: 99%