2021
DOI: 10.1007/jhep04(2021)218
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t − b − τ Yukawa unification in non-holomorphic MSSM

Abstract: We show that in the CMSSM with the non-holomorphic soft SUSY breaking terms, the Yukawa coupling unification of the third family fermions at the GUT scale, called t − b − τ Yukawa unification (YU), is possible under the recent collider and Dark Matter results. The YU parameter can also be found Rtbτ≈ 1, called perfect unification. We find that the squark masses exceed 3 TeV while the stau can be considerably lighter. In the case of YU, the tan β is in the interval [46,55]. We obtain bino-like dark matter (DM) … Show more

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Cited by 4 publications
(4 citation statements)
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“…In a hidden sector based supergravity type of model these interactions are typically suppressed by the scale of mediation [74]. Similar to the past analyses [66][67][68][69][70][71][72][73][80][81][82][83], in this work, without imposing any model-dependent restrictions, we treat such soft breaking at par with all the standard MSSM soft interactions 3 .…”
Section: 2mentioning
confidence: 88%
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“…In a hidden sector based supergravity type of model these interactions are typically suppressed by the scale of mediation [74]. Similar to the past analyses [66][67][68][69][70][71][72][73][80][81][82][83], in this work, without imposing any model-dependent restrictions, we treat such soft breaking at par with all the standard MSSM soft interactions 3 .…”
Section: 2mentioning
confidence: 88%
“…In contrast to the above analyses that had to manage the flavor issues carefully and are strongly constrained by µ → eγ or may have to live with light SUSY spectra or very large tan β, we focus on including nonstandard soft terms. Non-holomorphic trilinear terms may be augmented with MSSM leading to the so-called Non-holomorphic Supersymmetric Standard Model (NHSSM) [66][67][68][69][70][71][72][73][74]. The above terms are soft and may be included in a SUSY model if there is no gauge singlet.…”
Section: 2mentioning
confidence: 99%
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“…Analyses of Refs. [39][40][41][42][43][44][45][46][47][48] used renormalization group evolutions within a Constrained MSSM (CMSSM [9]) like setup. Here the NH parameters were considered to be of unknown origin and were at par with other CMSSM mass and trilinear parameters.…”
Section: Non-holomorphic Soft Termsmentioning
confidence: 99%