Neutralino Dark Matter and Other LHC Predictions from Quasi Yukawa Unification
arXiv:1503.04196 · doi:10.1016/j.nuclphysb.2015.09.019
Abstract
We explore the dark matter and LHC implications of t-b-tau quasi Yukawa unification in the framework of supersymmetric models based on the gauge symmetry G=SU(4)_{c}\times SU(2)_{L}\times SU(2)_{R}. The deviation from exact Yukawa unification is quantified by a dimensionless parameter C (|C| <~ 0.2), such that the Yukawa couplings at M_GUT are related by y_t:y_b:y_tau=|1+C| : |1-C| : |1+3C|. In contrast to earlier studies which focused on universal gaugino masses, we consider non-universal gaugino masses at M_GUT that are compatible with the gauge symmetry G. We perform two independent scans of the fundamental parameter space, one of which employs ISAJET, while the other uses SoftSusy interfaced with SuperIso. These scans reveal qualitatively similar allowed regions in the parameter space, and yield a variety of neutralino dark matter scenarios consistent with the observations. These include stau and chargino coannihilation scenarios, the A-resonance scenario, as well as Higgsino dark matter solution which is more readily probed by direct detection searches. The gluino mass is found to be <~ 4.2 TeV, the stop mass is >~ 2 TeV, while the first two family squarks and sleptons are of order 4-5 TeV and 3 TeV respectively.
References in corpus (7)
- Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC
- Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
- Dark Matter Results from 225 Live Days of XENON100 Data
- Averages of -hadron, -hadron, and -lepton properties as of summer 2016
- SuperIso v3.0: A program for calculating flavor physics observables in 2HDM and supersymmetry
- Yukawa Unification and Neutralino Dark Matter in SU(4)_c \times SU(2)_L \times SU(2)_R
- NLSP Gluino and NLSP Stop Scenarios from b-tau Yukawa Unification
Cited by in corpus (12)
- Accelerating Cosmology and Phase Structure of F(R) Gravity with Lagrange Multiplier Constraint: Mimetic Approach
- Unimodular-Mimetic Cosmology
- Reissner-Nordström Black Holes in Mimetic Gravity
- Naturalness and Dark Matter in the BLSSM
- Muon g-2 in an Alternative Quasi-Yukawa Unification with Low Fine-Tuned Inverse SeeSaw Mechanism
- Quasi Yukawa Unification and Fine-Tuning in U(1) Extended SSM
- Yukawa Unification with Four Higgs Doublets in Supersymmetric GUT
- Masses of Third Family Vector-like Quarks and Leptons in Yukawa-Unified
- Light Higgsinos, Heavy Gluino and Quasi-Yukawa Unification: Will the LHC find the Gluino?
- Comparatively Light Extra Higgs States as Signature of SUSY GUTs with 3rd Family Yukawa Unification
- Dark Matter Spin-Spin Interaction through the Pseudo-Scalar Vacuum Field
- Cosmology in the mimetic higher-curvature gravity