Boosted dark matter from a phantom fluid

被引:3
|
作者
Cline, James M. [1 ]
Puel, Matteo [1 ]
Toma, Takashi [2 ,3 ]
机构
[1] McGill Univ, Dept Phys, 3600 Univ St, Montreal, PQ H3A 2T8, Canada
[2] Kanazawa Univ, Inst Liberal Arts & Sci, Kanazawa, Ishikawa 9201192, Japan
[3] Kanazawa Univ, Inst Theoret Phys, Kanazawa, Ishikawa 9201192, Japan
基金
加拿大自然科学与工程研究理事会;
关键词
D O I
10.1016/j.physletb.2023.138377
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is known that theories of phantom dark energy, considered as quantu m fields, predict a continuous production of positive-plus negative-energy particles, from spontaneous decay of the vacuum. We show that this can be a new source of boosted dark matter or radiation, with consequences for direct detection. We set constraints on such models using data from the XENONnT experiment, and we show that recent excess events reported by the DAMIC experiment can be consistently described as coming from dark radiation, produced by vacuu m decay, interacting with electrons.
引用
收藏
页数:4
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