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Probing the HB/FP area for the CMSSM with Yukawa Quasi-Unification conditions

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If you have a question about this talk, please contact Damien George .

In this talk I will present a detailed analysis of the Hyperbolic Branch/Focus Point (HB/FP) area of the Constrained Minimal Supersymmetric Standard Model with Îŧ > 0 supplemented by an “asymptotic” Yukawa coupling quasi-unification condition. Imposing important constraints from the cold dark matter abundance in the universe, dark matter detection, B physics, and the mass of the lightest neutral CP-even Higgs boson, I find that the lightest neutralino can act as a cold dark matter candidate. At the same time, data from direct detection experiments play a crucial in restraining the parametric space of the model. Moreover, I will present a comparison between the neutralino-stau coannihilation area and HB/FP area regarding the predicted values of Îŧ and the mass of the lightest neutralino.

This talk is part of the HEP phenomenology joint Cavendish-DAMTP seminar series.

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