Heavy decaying dark matter and large-scale anisotropy of high-energy cosmic rays
- 作者: Kalashev O.E.1, Kuznetsov M.Y.1
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隶属关系:
- Institute for Nuclear Research
- 期: 卷 106, 编号 2 (2017)
- 页面: 73-80
- 栏目: Astrophysics and Cosmology
- URL: https://journals.rcsi.science/0021-3640/article/view/160274
- DOI: https://doi.org/10.1134/S0021364017140016
- ID: 160274
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详细
We examine the role of the large-scale anisotropy of the high-energy cosmic ray distribution in a search for the heavy decaying dark matter (DM) signal. Using recent anisotropy measurements from the extensive air shower (EAS) observatories, we constrain the lifetime of the DM particles with masses 107 ≤ MX ≤ 1016 GeV. These constraints appear to be weaker than that obtained with the high-energy gamma-ray limits. We also estimate the desired precision level for the anisotropy measurements to discern the decaying DM signal marginally allowed by the gamma-ray limits and discuss the prospects of the DM search with the modern EAS facilities.
作者简介
O. Kalashev
Institute for Nuclear Research
Email: mkuzn@inr.ac.ru
俄罗斯联邦, Moscow, 117312
M. Kuznetsov
Institute for Nuclear Research
编辑信件的主要联系方式.
Email: mkuzn@inr.ac.ru
俄罗斯联邦, Moscow, 117312
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