Hidden photon dark matter in the light of XENON1T and stellar cooling

被引:41
作者
Alonso-Alvarez, Gonzalo [1 ]
Ertas, Fatih [2 ]
Jaeckel, Joerg [1 ]
Kahlhoefer, Felix [2 ]
Thormaehlen, Lennert J. [1 ]
机构
[1] Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany
[2] Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol TTK, D-52056 Aachen, Germany
关键词
cosmology of theories beyond the SM; dark matter theory; dark matter experiments; CONSTRAINTS; BOUNDS; PARTICLES; AXIONS; SECTOR; U(1)S;
D O I
10.1088/1475-7516/2020/11/029
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The low-energy electronic recoil spectrum in XENON1T provides an intriguing hint for potential new physics. At the same time, observations of horizontal branch stars favor the existence of a small amount of extra cooling compared to the one expected from the Standard Model particle content. In this note, we argue that a hidden photon with a mass of similar to 2.5 keV and a kinetic mixing of similar to 10(-15) allows for a good fit to both of these excesses. In this scenario, the signal detected in XENON1T is due to the absorption of hidden photon dark matter particles, whereas the anomalous cooling of horizontal branch stars arises from resonant production of hidden photons in the stellar interior.
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页数:13
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