1996
DOI: 10.1016/0370-2693(96)00810-6
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Towards a viable grand unified model with M ∼ Mstring and M ∼ 1012 GeV

Abstract: We present a model based on the gauge group SU(2) L ×SU(2) R ×SU(4) C with gauge couplings that are found to be unified at a scale M G near the string unification scale. The model breaks to the minimal supersymmetric standard model at a scale M I ∼ 10 12 GeV, which is instrumental in producing a neutrino in a mass range that can serve as hot dark matter and this scale can also solve the strong CP problem via the Peccei-Quinn (PQ) mechanism with an invisible harmless axion. We show how this model can accommodat… Show more

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Cited by 9 publications
(4 citation statements)
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“…The breaking scale of the Pati-Salam gauge group is not significantly constrained by proton decay and can be as low as ∼ 10 TeV [35,36]. However, it is well known that supersymmetric Pati-Salam, broken at an intermediate scale ∼ 10 12 GeV, cannot achieve unification without additional charged fields [37]. An acceptable prediction for gauge coupling unification can be obtained however in a minimal supersymmetric Pati-Salam gauge group when PS is broken at the unification scale (for recent analyses of supersymmetric Pati-Salam, see [38] - [41]).…”
Section: Gauge Symmetry Breaking By Brane Fieldsmentioning
confidence: 99%
“…The breaking scale of the Pati-Salam gauge group is not significantly constrained by proton decay and can be as low as ∼ 10 TeV [35,36]. However, it is well known that supersymmetric Pati-Salam, broken at an intermediate scale ∼ 10 12 GeV, cannot achieve unification without additional charged fields [37]. An acceptable prediction for gauge coupling unification can be obtained however in a minimal supersymmetric Pati-Salam gauge group when PS is broken at the unification scale (for recent analyses of supersymmetric Pati-Salam, see [38] - [41]).…”
Section: Gauge Symmetry Breaking By Brane Fieldsmentioning
confidence: 99%
“…However, in such cases, one of the most attractive features like b − τ Yukawa unification for smaller values of tan β has to be sacrificed [10,11]. On the other hand, SUSY SO (10) with an intermediate gauge symmetry like SU (2) L × SU (2) R × U (1) B−L × SU (3) C (≡ G 2213 ) [12][13][14][15][16] or SU (2) L × SU (2) R × SU (4) C (≡ G 224 ) [17][18][19][20], while providing a more natural value for M N , substantially lower than the GUT scale, has the potentialities to account for the b − τ Yukawa unification at the intermediate scale M I ≃ 10 9 − 10 13 GeV. In this context it has been demonstrated that desirable values of G 2213breaking scale with M I ≃ 10 9 − 10 13 are possible provided that a number of scalar components of full SO (10) Higgs representations are light with masses near the intermediate scale [13,14].…”
Section: Introductionmentioning
confidence: 99%
“…The prospects to fill this gap by threshold corrections due to the infinite tower of massive string modes [27,28] seem rather restricted [29] as explicit calculations in superstring models show that such thresholds are very small [30]. This could be taken as an indication for the existence of intermediate scales in which extra matter states become massive and their thresholds increase the coupling unification scale up to M s [31,32,25]. One is thus motivated to incorporate this additional feature in a candidate GUT model.…”
Section: Introductionmentioning
confidence: 99%