scholarly journals Yukawa unification and neutralino dark matter inSU(4)c×SU(2)L×SU(2)R

2009 ◽  
Vol 79 (11) ◽  
Author(s):  
Ilia Gogoladze ◽  
Rizwan Khalid ◽  
Qaisar Shafi
Keyword(s):  
Dark Matter ◽  
Yukawa Unification

scholarly journals Upper bound on hot dark matter density from SO(10) Yukawa unification

1994 ◽  
Vol 335 (3-4) ◽  
pp. 345-354 ◽  
Author(s):  
Andrea Brignole ◽  
Hitoshi Murayama ◽  
Riccardo Rattazzi
Keyword(s):  
Dark Matter ◽  
Upper Bound ◽  
Matter Density ◽  
Dark Matter Density ◽  
Yukawa Unification

scholarly journals Supersymmetric cold dark matter with Yukawa unification

2000 ◽  
Vol 61 (12) ◽  
Author(s):  
M. E. Gómez ◽  
G. Lazarides ◽  
C. Pallis
Keyword(s):  
Dark Matter ◽  
Cold Dark Matter ◽  
Yukawa Unification

scholarly journals Supersymmetric dark matter and Yukawa unification

2002 ◽  
Vol 66 (3) ◽  
Author(s):  
Utpal Chattopadhyay ◽  
Achille Corsetti ◽  
Pran Nath
Keyword(s):  
Dark Matter ◽  
Yukawa Unification

scholarly journals WMAP dark matter constraints and Yukawa unification in supergravity models withCPphases

2005 ◽  
Vol 72 (9) ◽  
Author(s):  
Mario E. Gómez ◽  
Tarek Ibrahim ◽  
Pran Nath ◽  
Solveig Skadhauge
Keyword(s):  
Dark Matter ◽  
Supergravity Models ◽  
Yukawa Unification

scholarly journals t − b − τ Yukawa unification in non-holomorphic MSSM

2021 ◽  
Vol 2021 (4) ◽  
Author(s):  
Yaşar Hiçyılmaz
Keyword(s):  
Dark Matter ◽  
Yukawa Coupling ◽  
Direct Detection ◽  
Detection Limits ◽  
Susy Breaking ◽  
The Third ◽  
Gut Scale ◽  
Yukawa Unification ◽  
Relic Abundance

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) of mass in the range of 0.6 TeV ≲ $$ {m}_{\upchi_1^0} $$ m χ 1 0 ≲ 1.3 TeV where the recent Dark Matter direct detection limits are also satisfied. We also identify A-resonance solutions which reduce the relic abundance of LSP neutralino down to the ranges compatible with the current Planck measurements.

scholarly journals Dark Matter and Yukawa Unification with Massive Neutrinos

2009 ◽  
Author(s):  
M. E. Gómez ◽  
S. Lola ◽  
P. Naranjo ◽  
J. Rodríguez-Quintero ◽  
Shaaban Khalil
Keyword(s):  
Dark Matter ◽  
Massive Neutrinos ◽  
Yukawa Unification

scholarly journals Neutralino dark matter and other LHC predictions from quasi Yukawa unification

2015 ◽  
Vol 900 ◽  
pp. 400-411 ◽  
Author(s):  
Qaisar Shafi ◽  
Şükrü Hanif Tanyıldızı ◽  
Cem Salih Ün
Keyword(s):  
Dark Matter ◽  
Yukawa Unification

scholarly journals WMAP dark matter constraints onb−τ Yukawa unification with massive neutrinos

2009 ◽  
Vol 2009 (04) ◽  
pp. 043-043 ◽  
Author(s):  
M.E Gomez ◽  
S Lola ◽  
P Naranjo ◽  
J Rodriguez-Quintero
Keyword(s):  
Dark Matter ◽  
Massive Neutrinos ◽  
Yukawa Unification
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