2015
DOI: 10.1103/physrevd.92.095013
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Axion-Higgs interplay in the two-Higgs-doublet model

Abstract: The Zhitnitsky and Dine, Fischler and Srednicki (DFSZ) model is a natural extension of the two-Higgsdoublet model containing an additional singlet, endowed with a Peccei-Quinn symmetry, and leading to a physically acceptable axion. In this paper we reexamine this model in the light of some new developments. For generic couplings the model reproduces the minimal Standard Model showing only tiny deviations (extreme decoupling scenario) and all additional degrees of freedom (with the exception of the axion) are v… Show more

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Cited by 19 publications
(24 citation statements)
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“…leading naturally to type II two-Higgs-doublet models without FCNC [88,89]. The most general scalar potential of the model compatible with a global U (1) P Q is the following…”
Section: Axion and Neutrinosmentioning
confidence: 99%
“…leading naturally to type II two-Higgs-doublet models without FCNC [88,89]. The most general scalar potential of the model compatible with a global U (1) P Q is the following…”
Section: Axion and Neutrinosmentioning
confidence: 99%
“…In this section we shall discuss the conditions under which the scalar spectrum is phenomenologically viable and the vacuum structure of the model is stable. A necessary prerequisite to that is the analysis of the constraints on the scalar couplings coming from the measured value of the Higgs mass (125.09 ± 0.21 ± 0.11 GeV [37]) and the allowed deviations of its couplings to matter and gauge fields (for a recent study of the Higgs LHC physics and the electroweak precision observables in the DFSZ ultraweak setup see [38]). We shall give a benchmark setting of the model parameters that satisfies all the present LHC constraints with the heavier scalars possibly below the TeV scale, and thus accessible to the collider searches.…”
Section: Higgs Phenomenology and Vacuum Stabilitymentioning
confidence: 99%
“…The rotation matrix can be different form the identity. However, experimentally the parameter cos θ, appearing on the diagonal of the rotation matrix, is known [6] to be very close to one. We present a range of masses allowed by the constraints on ΔT in Fig.…”
Section: Spectrum Implicationsmentioning
confidence: 99%
“…The mass matrix can be diagonalized in the limit of large v φ , which is astrophysically constrained to be at least of order 10 7 GeV. In the paper [6] an expansion in v/v φ is carried out to the second order to get the masses of h i . It is argued that the nominal expansion in powers of v/v φ is applicable in a number of cases.…”
Section: Mass Eigenstatesmentioning
confidence: 99%
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