Actions for The direct detection of boosted dark matter at high energies and PeV events at IceCube [electronic resource].
The direct detection of boosted dark matter at high energies and PeV events at IceCube [electronic resource].
- Published
- Washington, D.C. : United States. Dept. of Energy. High Energy Physics Division, 2015.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy - Physical Description
- 14 pages : digital, PDF file
- Additional Creators
- Fermi National Accelerator Laboratory, United States. Department of Energy. High Energy Physics Division, and United States. Department of Energy. Office of Scientific and Technical Information
Access Online
- Restrictions on Access
- Free-to-read Unrestricted online access
- Summary
- We study the possibility of detecting dark matter directly via a small but energetic component that is allowed within present-day constraints. Drawing closely upon the fact that neutral current neutrino nucleon interactions are indistinguishable from DM-nucleon interactions at low energies, we extend this feature to high energies for a small, non-thermal but highly energetic population of DM particle χ, created via the decay of a significantly more massive and long-lived non-thermal relic Φ, which forms the bulk of DM. If χ interacts with nucleons, its cross-section, like the neutrino-nucleus coherent cross-section, can rise sharply with energy leading to deep inelastic scattering, similar to neutral current neutrino-nucleon interactions at high energies. Thus, its direct detection may be possible via cascades in very large neutrino detectors. As a specific example, we apply this notion to the recently reported three ultra-high energy PeV cascade events clustered around 1 – 2 PeV at IceCube (IC). We discuss the features which may help discriminate this scenario from one in which only astrophysical neutrinos constitute the event sample in detectors like IC.
- Report Numbers
- E 1.99:1214549
- Subject(s)
- Other Subject(s)
- Note
- Published through SciTech Connect.
03/13/2015.
Journal of Cosmology and Astroparticle Physics 2015 03 ISSN 1475-7516 AM
Bhattacharya, A. [Univ. of Arizona, Tucson, AZ (United States)]; R. Gandhi; Gupta, A. [Harish-Chandra Research Institute, Jhunsi, Allahabad (India)]. - Funding Information
- FG02-04ER41298
FG02-13ER41976
View MARC record | catkey: 23496244