2017
DOI: 10.1007/jhep04(2017)075
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Standard coupling unification in SO(10), hybrid seesaw neutrino mass and leptogenesis, dark matter, and proton lifetime predictions

Abstract: We discuss gauge coupling unification of SU(3) C × SU(2) L × U(1) Y descending directly from non-supersymmetric SO(10) while providing solutions to the three outstanding problems of the standard model: neutrino masses, dark matter, and the baryon asymmetry of the universe. Conservation of matter parity as gauged discrete symmetry for the stability and identification of dark matter in the model calls for high-scale spontaneous symmetry breaking through 126 H Higgs representation. This naturally leads to the hyb… Show more

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Cited by 27 publications
(38 citation statements)
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“…The neutrino and charged fermion mass and mixing generation in the context of unified theories are discussed in [24,[44][45][46][47][48][49][50][51][52][53][54][55][56][57][58][59][60][61]. In [62][63][64][65][66][67][68][69][70][71][72][73][74][75][76] different cosmological aspects and dark matter scenarios are discussed. An important result of the present paper, using the goodness of fit test for unification with two-loop renormalisation group evolution equations (RGEs), is the extent to which the inclusion of threshold corrections significantly affects the proton lifetime, allowing several scenarios, which would otherwise be excluded, to survive.…”
Section: Introductionmentioning
confidence: 99%
“…The neutrino and charged fermion mass and mixing generation in the context of unified theories are discussed in [24,[44][45][46][47][48][49][50][51][52][53][54][55][56][57][58][59][60][61]. In [62][63][64][65][66][67][68][69][70][71][72][73][74][75][76] different cosmological aspects and dark matter scenarios are discussed. An important result of the present paper, using the goodness of fit test for unification with two-loop renormalisation group evolution equations (RGEs), is the extent to which the inclusion of threshold corrections significantly affects the proton lifetime, allowing several scenarios, which would otherwise be excluded, to survive.…”
Section: Introductionmentioning
confidence: 99%
“…Such a direct SO(10) breaking model is prominently well established in SUSY GUTs [74,75] and also has been applied in non-SUSY SO(10) [26,30,50,76]. In the context of protecting non-SUSY grand desert models by GUT threshold effects , particularly those due to superheavy gauge bosons, such a direct breaking model of SO (10) has been also used earlier [77,78]…”
Section: Now Rewriting the Interaction Lagrangianmentioning
confidence: 99%
“…Remnants of gauged discrete symmetries [46][47][48] such as R-parity in SUSY and matter parity in non-SUSY theories have played crucial roles in determining stability and phenomenology of dark matter [23][24][25][26][28][29][30]. In general if a higher rank gauge theory containing U (1) B−L as one of its subgroups leads to SM gauge theory SU (2) L × U (1) Y × SU (3) C ≡ G 213 , then matter parity (MP) of the SM is conserved as a gauged discrete symmetry…”
Section: Introductionmentioning
confidence: 99%
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“…All the generational mixings have been found to be much larger than the corresponding quark mixings. Theoretically [6][7][8][9][10][11][12][13] neutrino masses are predicted through various seesaw mechanisms [14][15][16][17][18][19][20][21][22][23][25][26][27][28][29][30][31][32][33][34][35][36][37][38][39][40][41][42][43]. In a minimal left-right symmetric [44][45][46][47] grand unified theory (GUT) like SO(10) [48,49] where parity (P) violation in weak interaction is explained along with fermion masses [50][51][52][53][54][55], a number of these seesa...…”
Section: Introductionmentioning
confidence: 99%