Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry

被引:34
作者
Alves, Alexandre [1 ]
Camargo, Daniel A. [2 ]
Dias, Alex G. [2 ]
Longas, Robinson [3 ]
Nishi, Celso C. [4 ]
Queiroz, Farinaldo S. [5 ]
机构
[1] Univ Fed Sao Paulo, Dept Ciencias Exatas & Terra, BR-09972270 Diadema, SP, Brazil
[2] Univ Fed ABC, Ctr Ciencias Nat & Humanas, BR-09210580 Santo Andre, SP, Brazil
[3] Univ Antioquia, Inst Fis, Calle 70 52-21, Medellin, Colombia
[4] Univ Fed ABC, Ctr Matemat Comp & Cognicao Nat, BR-09210580 Santo Andre, SP, Brazil
[5] Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2016年 / 10期
基金
巴西圣保罗研究基金会;
关键词
Beyond Standard Model; Cosmology of Theories beyond the SM; Discrete Symmetries; SINGLET; AXION; LHC; ANNIHILATION; CONSTRAINTS; INVARIANCE; PROGRAM; WIMP; MASS;
D O I
10.1007/JHEP10(2016)015
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Weakly Interacting Massive Particles (WIMPs) and axions are arguably the most compelling dark matter candidates in the literature. Could they coexist as dark matter particles? More importantly, can they be incorporated in a well motivated framework in agreement with experimental data? In this work, we show that this two component dark matter can be realized in the Inert Doublet Model in an elegant and natural manner by virtue of the spontaneous breaking of a Peccei-Quinn U(1)(PQ) symmetry into a residual Z(2) symmetry. The WIMP stability is guaranteed by the Z(2) symmetry and a new dark matter component, the axion, arises. There are two interesting outcomes: (i) vector-like quarks needed to implement the Peccei-Quinn symmetry in the model may act as a portal between the dark sector and the SM fields with a supersymmetry-type phenomenology at colliders; (ii) two-component Inert Doublet Model re-opens the phenomenologically interesting 100{500 GeV mass region. We show that the model can successfully realize a two component dark matter framework and at the same time avoid low and high energy physics constraints such as monojet and dijet plus missing energy, as well as indirect and direct dark matter detection bounds.
引用
收藏
页数:29
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