Sparticle spectroscopy with neutralino dark matter from t-b-{tau} quasi-Yukawa unification
Journal Article
·
· Physical Review. D, Particles Fields
- Mohawk Valley Community College, 1101 Sherman Drive Utica, New York 13501 (United States)
- Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716 (United States)
We consider two classes of t-b-{tau} quasi-Yukawa unification scenarios which can arise from realistic supersymmetric SO(10) and SU(4){sub C}xSU(2){sub L}xSU(2){sub R} models. We show that these scenarios can be successfully implemented in the nonuniversal Higgs model with m{sub H{sub u}}=m{sub H{sub d}}{ne}m{sub 0} and the constrained minimal sumersymmetric model frameworks, and they yield a variety of sparticle spectra with Wilkinson Microwave Anisotropy Probe compatible neutralino dark matter. In the nonuniversal Higgs model with m{sub H{sub u}}=m{sub H{sub d}}{ne}m{sub 0}, we find bino-Higgsino dark matter as well as the stau coannihilation and A-funnel solutions. The constrained minimal sumersymmetric model case yields the stau coannihilation and A-funnel solutions. The gluino and squark masses are found to lie in the TeV range.
- OSTI ID:
- 21607948
- Journal Information:
- Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 8 Vol. 84; ISSN PRVDAQ; ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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Coannihilation scenarios and particle spectroscopy in SU(4){sub c}xSU(2){sub L}xSU(2){sub R}
Yukawa unification and neutralino dark matter in SU(4){sub c}xSU(2){sub L}xSU(2){sub R}
Journal Article
·
Sun Nov 01 00:00:00 EDT 2009
· Physical Review. D, Particles Fields
·
OSTI ID:21325501
Yukawa unification and neutralino dark matter in SU(4){sub c}xSU(2){sub L}xSU(2){sub R}
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·
Mon Jun 01 00:00:00 EDT 2009
· Physical Review. D, Particles Fields
·
OSTI ID:21300876
Related Subjects
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ANISOTROPY
ELECTROMAGNETIC RADIATION
ENERGY RANGE
HIGGS MODEL
LIE GROUPS
MASS
MATHEMATICAL MODELS
MATHEMATICAL SOLUTIONS
MATTER
MICROWAVE RADIATION
NONLUMINOUS MATTER
NUCLEAR POTENTIAL
PARTICLE MODELS
POTENTIALS
RADIATIONS
SIMULATION
SO GROUPS
SO-10 GROUPS
SPECTRA
SPECTROSCOPY
SU GROUPS
SU-2 GROUPS
SU-4 GROUPS
SUPERSYMMETRY
SYMMETRY
SYMMETRY GROUPS
TEV RANGE
YUKAWA POTENTIAL
ANISOTROPY
ELECTROMAGNETIC RADIATION
ENERGY RANGE
HIGGS MODEL
LIE GROUPS
MASS
MATHEMATICAL MODELS
MATHEMATICAL SOLUTIONS
MATTER
MICROWAVE RADIATION
NONLUMINOUS MATTER
NUCLEAR POTENTIAL
PARTICLE MODELS
POTENTIALS
RADIATIONS
SIMULATION
SO GROUPS
SO-10 GROUPS
SPECTRA
SPECTROSCOPY
SU GROUPS
SU-2 GROUPS
SU-4 GROUPS
SUPERSYMMETRY
SYMMETRY
SYMMETRY GROUPS
TEV RANGE
YUKAWA POTENTIAL