Browsing by Author "Mustafayev, Azar"

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    Gauge mediation models with adjoint messengers
    (Amer Physical Soc, 2016-10-24) Gogoladze, Ilia; Mustafayev, Azar; Shafi, Qaisar; Ün, Cem Salih; Uludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Bölümü.; 0000-0002-0595-8803; N-3421-2014; 7004752140; 55325758100
    We present a class of models in the framework of gauge mediation supersymmetry breaking where the messenger fields transform in the adjoint representation of the standard model gauge symmetry. To avoid unacceptably light right-handed sleptons in the spectrum we introduce a nonzero U(1)(B-L) D-term. This leads to an additional contribution to the soft supersymmetry breaking mass terms which makes the right-handed slepton masses compatible with the current experimental bounds. We show that in this framework the observed 125 GeV Higgs boson mass can be accommodated with the sleptons accessible at the LHC, while the squarks and gluinos lie in the multi-TeV range. We also discuss the issue of the fine-tuning and show that the desired relic dark matter abundance can also be accommodated.
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    Yukawa unification and sparticle spectroscopy in gauge mediation models
    (Amer Physical, 2015-05-18) Gogoladze, Ilia; Mustafayev, Azar; Shafi, Qaisar; Un, Cem Salih; Uludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Bölümü.; 0000-0002-0595-8803; N-3421-2014; 55325758100
    We explore the implications of the t-b-tau (and b-tau) Yukawa coupling unification condition on the fundamental parameter space and sparticle spectroscopy in the minimal gauge mediated supersymmetry breaking model. We find that this scenario prefers values of the CP-odd Higgs mass m(A) greater than or similar to 1 TeV, with all colored sparticle masses above 3 TeV. These predictions will be hard to test at LHC13 but they may be testable at the high-energy LHC (HE-LHC) 33 TeV or a 100 TeV collider. Both the t-b-tau and the b-tau Yukawa coupling unification prefer a relatively light gravitino with mass less than or similar to 30 eV, which makes it a candidate hot dark matter particle. However, it cannot account for more than 15% of the observed dark matter density.