Neutrinos from Colliding Wind Binaries: Future Prospects for PINGU and ORCA
Massive stars play an important role in explaining the cosmic ray spectrum below the knee, possibly even up to the ankle, i.e. up to energies of 1e15 eV or 1e18.5 eV, respectively. In particular, Supernova Remnants are discussed as one of the main candidates to explain the cosmic ray spectrum. Even...
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Format: | Report |
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arXiv
2014
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Online Access: | https://dx.doi.org/10.48550/arxiv.1405.0471 https://arxiv.org/abs/1405.0471 |