Neutralino dark matter and other LHC predictions from quasi Yukawa unification

We explore the dark matter and LHC implications of t−b−τ quasi Yukawa unification in the framework of supersymmetric models based on the gauge symmetry G=SU(4)c×SU(2)L×SU(2)R. The deviation from exact Yukawa unification is quantified by a dimensionless parameter C (|C|≲0.2), such that the Yukawa cou...

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Main Authors: Qaisar Shafi, Şükrü Hanif Tanyıldızı, Cem Salih Ün
Format: Article
Language:English
Published: Elsevier 2015-11-01
Series:Nuclear Physics B
Online Access:http://www.sciencedirect.com/science/article/pii/S0550321315003387
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author Qaisar Shafi
Şükrü Hanif Tanyıldızı
Cem Salih Ün
author_facet Qaisar Shafi
Şükrü Hanif Tanyıldızı
Cem Salih Ün
author_sort Qaisar Shafi
collection DOAJ
description We explore the dark matter and LHC implications of t−b−τ quasi Yukawa unification in the framework of supersymmetric models based on the gauge symmetry G=SU(4)c×SU(2)L×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 MGUT are related by yt:yb:yτ=|1+C|:|1−C|:|1+3C|. In contrast to earlier studies which focused on universal gaugino masses, we consider non-universal gaugino masses at MGUT that are compatible with the gauge symmetry G. Our results reveal 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 solutions which are more readily probed by direct detection searches. The gluino mass is found to be ≲4 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.
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spelling doaj.art-8934bc208fa24eb29d488fb4c095b5db2022-12-21T18:10:48ZengElsevierNuclear Physics B0550-32131873-15622015-11-01900C40041110.1016/j.nuclphysb.2015.09.019Neutralino dark matter and other LHC predictions from quasi Yukawa unificationQaisar Shafi0Şükrü Hanif Tanyıldızı1Cem Salih Ün2Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, USABogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, 141980 Dubna, Moscow Region, RussiaDepartment of Physics, Uludağ University, Bursa TR16059, TurkeyWe explore the dark matter and LHC implications of t−b−τ quasi Yukawa unification in the framework of supersymmetric models based on the gauge symmetry G=SU(4)c×SU(2)L×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 MGUT are related by yt:yb:yτ=|1+C|:|1−C|:|1+3C|. In contrast to earlier studies which focused on universal gaugino masses, we consider non-universal gaugino masses at MGUT that are compatible with the gauge symmetry G. Our results reveal 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 solutions which are more readily probed by direct detection searches. The gluino mass is found to be ≲4 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.http://www.sciencedirect.com/science/article/pii/S0550321315003387
spellingShingle Qaisar Shafi
Şükrü Hanif Tanyıldızı
Cem Salih Ün
Neutralino dark matter and other LHC predictions from quasi Yukawa unification
Nuclear Physics B
title Neutralino dark matter and other LHC predictions from quasi Yukawa unification
title_full Neutralino dark matter and other LHC predictions from quasi Yukawa unification
title_fullStr Neutralino dark matter and other LHC predictions from quasi Yukawa unification
title_full_unstemmed Neutralino dark matter and other LHC predictions from quasi Yukawa unification
title_short Neutralino dark matter and other LHC predictions from quasi Yukawa unification
title_sort neutralino dark matter and other lhc predictions from quasi yukawa unification
url http://www.sciencedirect.com/science/article/pii/S0550321315003387
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AT sukruhaniftanyıldızı neutralinodarkmatterandotherlhcpredictionsfromquasiyukawaunification
AT cemsalihun neutralinodarkmatterandotherlhcpredictionsfromquasiyukawaunification