Dark matter from unification

被引:1
|
作者
Kainulainen, Kimmo [1 ,2 ]
Tuominen, Kimmo [1 ,2 ,5 ]
Virkajarvi, Jussi [3 ,4 ]
机构
[1] Univ Jyvaskyla, Dept Phys, POB 35 YFL, FI-40014 Jyvaskyla, Finland
[2] Univ Helsinki, Helsinki Inst Phys, FI-00014 Helsinki, Finland
[3] Univ Southern Denmark, Origins CP3, DK-5230 Odense M, Denmark
[4] Univ Southern Denmark, DIAS, DK-5230 Odense M, Denmark
[5] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2013年 / 10期
基金
新加坡国家研究基金会;
关键词
dark matter theory; dark matter experiments; particle physics - cosmology connection; COSMIC ABUNDANCES; STABLE PARTICLES; GALACTIC HALO; TECHNICOLOR; MASS; HIGGS; PHENOMENOLOGY; CONSTRAINTS; SCALAR; MODEL;
D O I
10.1088/1475-7516/2013/10/036
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a minimal extension of the Standard Model (SM), which leads to unification of the SM coupling constants, breaks electroweak symmetry dynamically by a new strongly coupled sector and leads to novel dark matter candidates. In this model, the coupling constant unification requires the existence of electroweak triplet and doublet fermions singlet under QCD and new strong dynamics underlying the Higgs sector. Among these new matter fields and a new right handed neutrino, we consider the mass and mixing patterns of the neutral states. We argue for a symmetry stabilizing the lightest mass eigenstates of this sector and determine the resulting relic density. The results are constrained by available data from colliders and direct and indirect dark matter experiments. We find the model viable and outline briefly future research directions.
引用
收藏
页数:30
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