2013
DOI: 10.1007/jhep10(2013)226
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Supersymmetric SU(5) grand unification for a post Higgs boson era

Abstract: We investigate models of supersymmetric grand unification based on the gauge group SU (5). We consider models with non-universal gaugino masses and confront them with low energy constraints, including the Higgs boson mass and the Dark Matter relic density. We also discuss fine-tuning and show the effect of not including the µ-parameter into fine tuning determinations. With this relaxation, we find viable scenarios with low fine tuning and study some model choices for gaugino mass ratios. We demonstrate that so… Show more

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Cited by 8 publications
(16 citation statements)
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“…Thus, a detailed analysis of the Renormalization Group (RG) is required in order to evolve the couplings of the theory from the high scale down to the low scale. Some recent phenomenological work in light of the recently discovered Higgs boson and dark matter can be found in [33][34][35][36][37].…”
Section: Introductionmentioning
confidence: 99%
“…Thus, a detailed analysis of the Renormalization Group (RG) is required in order to evolve the couplings of the theory from the high scale down to the low scale. Some recent phenomenological work in light of the recently discovered Higgs boson and dark matter can be found in [33][34][35][36][37].…”
Section: Introductionmentioning
confidence: 99%
“…Using the electroweak scale outputs of SOFTSUSY as inputs for micrOMEGAS, we generate predictions for the remaining experimental observables, such as the dark matter relic density, and derive a probability P tot for each scenario (again using the procedure described in [9]). We require P tot > 10 −3 , reducing the number of viable scenarios to 2151, corresponding to 0.2% of the initial attempts, of which 458 (0.05% of the initial attempts) have the preferred relic density.…”
Section: Universal Gaugino Massesmentioning
confidence: 99%
“…In a recent publication [9], we investigated supersymmetric Grand Unified Theories (GUTs) with an SU(5) gauge group. We considered models with both universal and nonuniversal gaugino masses and confronted our spectra with low energy constraints from the newly discovered Higgs boson [1][2][3][4] and the dark matter (DM) relic density [10,11].…”
Section: Introductionmentioning
confidence: 99%
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