2016
DOI: 10.3844/pisp.2016.1.14
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Early Universe in the SU(3)<sub>L</sub>?(1)<sub>X</sub> Electroweak Models

Abstract: Abstract:We present status of the 3-3-1 models and their implications to cosmological evolution such as inflation, phase transitions and sphalerons. The models can deal not only with the issues such as neutrino physics, dark matter, etc, but they are also able to provide quite good agreement with the Standard Cosmology: The inflation happens at the GUT scale, while phase transition has two sequences corresponding two steps of symmetry breaking in the models, namely: SU(3) → SU(2) and SU(2) → U(1). Some bounds … Show more

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Cited by 4 publications
(2 citation statements)
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“…3-3-1 models are self-consistent if there exists only three generations due to the combined effect of triangle gauge anomalies cancellations and QCD asymptotic freedom [10][11][12][13][14]. Moreover, the model furnishes a suitable environment for neutrino masses through see-saw mechanisms [15][16][17][18][19][20][21][22][23][24][25][26][27][28], dark matter [29][30][31][32][33][34][35][36][37][38][39][40][41][42][43][44][45], explanation of the strong CP problem in the quark sector [46,47], first-order phase transitions [48][49][50], lepton number violation processes [51][52][53][54][55][56][57]…”
Section: Introductionmentioning
confidence: 99%
“…3-3-1 models are self-consistent if there exists only three generations due to the combined effect of triangle gauge anomalies cancellations and QCD asymptotic freedom [10][11][12][13][14]. Moreover, the model furnishes a suitable environment for neutrino masses through see-saw mechanisms [15][16][17][18][19][20][21][22][23][24][25][26][27][28], dark matter [29][30][31][32][33][34][35][36][37][38][39][40][41][42][43][44][45], explanation of the strong CP problem in the quark sector [46,47], first-order phase transitions [48][49][50], lepton number violation processes [51][52][53][54][55][56][57]…”
Section: Introductionmentioning
confidence: 99%
“…3-3-1 models stand for electroweak extensions of the SM, where left-handed fermions are arranged in the fundamental representation of SU (3) L . Such models can naturally explain the number of generations [5,6], might offer plausible dark matter candidates with gripping phenomenology [4,, explain neutrino masses through the seesaw mechanism [33,34], feature interesting connections to cosmology [35][36][37][38][39] and prospects to collider physics [40][41][42][43][44], among others [38,[45][46][47][48][49][50][51][52][53][54][55][56][57][58]. In this work we will focus our attention on the ecoomical 3-3-1 model, which has in its scalar sector two scalar triplets [59], and discuss the long standing discrepancy on the muon anomalous magnetic moment and the lepton flavor violating decay µ → eγ (see [60] for a recent review).…”
Section: Introductionmentioning
confidence: 99%