| 14th International Conference on Topics in Astroparticle and Underground Physics | |
| Photonic dark matter portal revisited | |
| 物理学;天文学 | |
| Alavi, S.A.^1 ; Kazemian, F.S.^1 | |
| Department of Physics, Hakim Sabzevari University, Sabzevar, Iran^1 | |
| 关键词: Aharonov-Bohm phase; Coupling constants; Exotic atoms; Galaxy clusters; Hydrogen atoms; Standard model; Upper limits; X ray observatories; | |
| Others : https://iopscience.iop.org/article/10.1088/1742-6596/718/4/042002/pdf DOI : 10.1088/1742-6596/718/4/042002 |
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| 学科分类:天文学(综合) | |
| 来源: IOP | |
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【 摘 要 】
In our previous paper, we studied a model of dark matter (DM) in which the hidden sector interacts with standard model particles via a hidden photonic portal (HP). We investigated the effects of this new interaction on the hydrogen atom and obtained an upper bound for the coupling of the model as f ≤ 10-12. In this work, we study the effects of HP on two interesting exotic atoms namely muonium and positronium. We obtain a tighter upper limit on the coupling as f ≤ 10-13. We also calculate the change (shift) in the Aharonov-Bohm phase due to HP and find that the phase shift is negligibly small (for DM particles mass in the GeV range). Recently a 3.5 keV X-ray line signal observed in the spectrum of 73 galaxy clusters, reported by the XXM-Newton X-ray observatory. Since in HP model the DM particles can decay directly into photons, so we finally calculate the value of the coupling constant f using the condition ΔEDM= 3.5 keV.
【 预 览 】
| Files | Size | Format | View |
|---|---|---|---|
| Photonic dark matter portal revisited | 1172KB |
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