Moduli portal dark matter

被引:42
作者
Chowdhury, Debtosh [1 ,2 ]
Dudas, Emilian [1 ]
Dutra, Maira [2 ,3 ]
Mambrini, Yann [2 ]
机构
[1] Univ Paris Saclay, Ctr Phys Theor, CNRS, Ecok Polytech, F-91128 Palaiseau, France
[2] Univ Paris Sud, Univ Paris Saclay, CNRS, Lab Phys Theor,UMR8627, F-91405 Orsay, France
[3] Carleton Univ, Ottawa Carleton Inst Phys, 1125 Colonel By Dr, Ottawa, ON K1S 5B6, Canada
基金
欧盟地平线“2020”;
关键词
COSMOLOGICAL IMPLICATIONS; MASS HIERARCHIES; DILATON; FORCES; HIGGS;
D O I
10.1103/PhysRevD.99.095028
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that moduli fields as mediators between the Standard Model and the dark sector can naturally lead to the observed relic abundance. Indeed, even if moduli are very massive, the nature of their couplings with matter and gauge fields allows to produce a sufficiently large amount of dark matter in the early Universe through the freeze-in mechanism. Moreover, the complex nature of the moduli fields whose real and imaginary parts couple differently to the thermal bath gives an interesting and unusual phenomenology compared to other freeze-in models of that type.
引用
收藏
页数:11
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