UHE neutrinos with E410 17 eV are produced by ultra-high energy cosmic rays (UHECR) interacting with CMB photons (cosmogenic neutrinos) and by top-down sources, such as topological defects (TDs) and superheavy dark matter (SHDM). Cosmogenic neutrinos are reliably predicted and their fluxes can be nu
β¦ LIBER β¦
Neutrino magnetic moment: a window to new physics
β Scribed by A. Studenikin
- Publisher
- Elsevier Science
- Year
- 2009
- Tongue
- English
- Weight
- 164 KB
- Volume
- 188
- Category
- Article
- ISSN
- 0920-5632
No coin nor oath required. For personal study only.
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