2022
DOI: 10.1103/physrevd.106.055019
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Updated constraints on the Georgi-Machacek model and its electroweak phase transition and associated gravitational waves

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Cited by 8 publications
(3 citation statements)
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“…In this paper, we discuss a model with a real and a complex isospin triplet Higgs fields as the minimal extension of the Higgs sector such that it contains new sources of CPV and keeps the electroweak rho parameter to unity at tree level, but not introducing quark FCNCs via tree-level Higgs mediations. The field content is actually the same as that of the Georgi-Machacek (GM) model [16,17] which can realize the strong firstorder electroweak phase transition [18][19][20] under the theoretical and current experimental constraints. The original GM model is, however, forbidden to have new CPV sources due to the global SU(2) L × SU(2) R symmetry in the potential, imposed to preserve the custodial SU(2) V symmetry after the spontaneous symmetry breaking.…”
Section: Jhep06(2023)069mentioning
confidence: 93%
“…In this paper, we discuss a model with a real and a complex isospin triplet Higgs fields as the minimal extension of the Higgs sector such that it contains new sources of CPV and keeps the electroweak rho parameter to unity at tree level, but not introducing quark FCNCs via tree-level Higgs mediations. The field content is actually the same as that of the Georgi-Machacek (GM) model [16,17] which can realize the strong firstorder electroweak phase transition [18][19][20] under the theoretical and current experimental constraints. The original GM model is, however, forbidden to have new CPV sources due to the global SU(2) L × SU(2) R symmetry in the potential, imposed to preserve the custodial SU(2) V symmetry after the spontaneous symmetry breaking.…”
Section: Jhep06(2023)069mentioning
confidence: 93%
“…By computing the effective scalar potential, we find the range of Higgs portal coupling where eligible first-order EWPT can happen for different types of scalar leptoquark with a mass around TeV scale. Then we apply the standard procedure [39][40][41][42][43][44][45][46][47] to calculate the gravitational wave background produced during the first-order EWPT induced by leptoquark for some benchmark cases and compare it with the detector sensitivities. We…”
Section: Introductionmentioning
confidence: 99%
“…ρ = 1 [6]. The constraints on the parameter space of the model is already well studied in the literature [7][8][9][10][11][12][13][14][15] and also a calculator is available [16] to calculate all the constraints. Various phenomenological works [17][18][19][20][21][22][23][24][25][26][27][28][29] on this model enrich the knowledge of the reader.…”
Section: Introductionmentioning
confidence: 99%