Hadronically decaying heavy dark matter and high-energy neutrino limits
- Авторлар: Kuznetsov M.Y.1
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Мекемелер:
- Institute for Nuclear Research
- Шығарылым: Том 105, № 9 (2017)
- Беттер: 561-567
- Бөлім: Astrophysics and Cosmology
- URL: https://ogarev-online.ru/0021-3640/article/view/160145
- DOI: https://doi.org/10.1134/S0021364017090028
- ID: 160145
Дәйексөз келтіру
Аннотация
We consider dark matter consisting of long-living particles with masses 107 GeV ≲ M ≲1016 GeV decaying through hadronic channel as a source of high-energy neutrino. Using recent data on high-energy neutrino from IceCube and Pierre Auger experiments, we derive the upper-limits on neutrino flux from dark matter decay and constraints on dark matter parameter space. For the dark matter masses of order 108 GeV the constraints derived are slightly stronger than those obtained for the same dark matter model using the highenergy gamma-ray limits.
Авторлар туралы
M. Kuznetsov
Institute for Nuclear Research
Хат алмасуға жауапты Автор.
Email: mkuzn@inr.ac.ru
Ресей, Moscow, 117312
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