2019
DOI: 10.1007/jhep12(2019)137
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Vacuum stability and symmetry breaking in left-right symmetric model

Abstract: We derive analytic conditions for the vacuum stability of the left-right symmetric model by using the concepts of copositivity and gauge orbit spaces. We also derive the necessary and sufficient conditions for successful symmetry breaking and the existence of a correct vacuum. We then compare results obtained from the derived conditions with those from numerical minimization of the scalar potential. Finally, we discuss the renormalization group analysis of the scalar quartic couplings through an example study … Show more

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Cited by 29 publications
(27 citation statements)
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“…After the spontaneous symmetry breaking, all the scalar fields have to form some specific structure in the phase space such that we reside in the correct vacuum, i.e. the vacuum with the lowest VEV in the potential [104,157].…”
Section: )mentioning
confidence: 99%
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“…After the spontaneous symmetry breaking, all the scalar fields have to form some specific structure in the phase space such that we reside in the correct vacuum, i.e. the vacuum with the lowest VEV in the potential [104,157].…”
Section: )mentioning
confidence: 99%
“…The sufficient but not necessary conditions for vacuum stability and correct vacuum in the LRSM are worked out in [104] and listed below (simple analytic formula can only be obtained in the condition α 2 = 0): where the condition structure "p ⇐ q" means p needs to be checked if and only if the condition q is true. In this paper, we have chosen λ 2,3,4 = 0, which corresponds to the case of η = σ = 0.…”
Section: B Conditions For Vacuum Stability and Correct Vacuummentioning
confidence: 99%
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“…In the minimal LRSM, the Higgs potential for Φ and ∆ L,R and the symmetry breaking have been investigated in detail [23][24][25][26][27][28][29][30][31][32]. We extend the Higgs potential by adding φ X as follows:…”
Section: Minimally Extended Lrsm With Majorana Fermion Dmmentioning
confidence: 99%
“…The issue of vacuum stability in presence of additional scalars has been extensively studied in the literature. An incomplete list of models include SM-singlet scalar models [19][20][21][22][23][24][25], Two-Higgs doublet models (2HDM) [26][27][28][29][30][31], type-II seesaw models with SU(2) L -triplet scalars [32][33][34][35][36][37][38], U(1) extensions [39][40][41][42][43][44][45], left-right symmetric models [46][47][48], universal seesaw models [49,50], Zee-Babu model [51,52], models with Majorons [53,54], axions [22,55], moduli [56,57], scalar leptoquarks [58] or higher color-multiplet scalars [59,60], as well as various supersymmetric models [61][62][63][64]…”
Section: Introductionmentioning
confidence: 99%