6533b85afe1ef96bd12b8dd3
RESEARCH PRODUCT
A model for dark matter, naturalness and a complete gauge unification
Jussi VirkajärviJussi VirkajärviKimmo TuominenKimmo TuominenKimmo KainulainenKimmo Kainulainensubject
Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesTechnicolorParameter space01 natural sciences7. Clean energyStandard ModelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsCoupling constantPhysicsdark matter theory010308 nuclear & particles physicsdark matter experimentsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsCoupling (probability)High Energy Physics - Phenomenologyparticle physics - cosmology connectionHigh Energy Physics::ExperimentDiscrete symmetryAstrophysics - Cosmology and Nongalactic Astrophysicsdescription
We consider dark matter in a minimal extension of the Standard Model (SM) which breaks electroweak symmetry dynamically and leads to a complete unification of the SM and technicolor coupling constants. The unification scale is determined to be $M_{\rm U} \approx 2.2 \times 10^{15}$ GeV and the unified coupling $\alpha_{\rm U} \approx 0.0304$. Moreover, unification strongly suggest that the technicolor sector of the model must become strong at the scale of ${\cal O}$(TeV). The model also contains a tightly constrained sector of mixing neutral fields stabilized by a discrete symmetry. We find the lightest of these states can be DM with a mass in the range $m_{\rm DM} \approx 30-800$ GeV. We find a large set of parameters that satisfy all available constraints from colliders and from dark matter search experiments. However, most of the available parameter space is within the reach of the next generation of DM search experiments. The model is also sensitive to a modest improvement in the measurement of the precision electroweak parameters.
year | journal | country | edition | language |
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2015-07-21 | Journal of Cosmology and Astroparticle Physics |