摘要
We discuss the reconstruction of neutrino flavor ratios at astrophysical sources through the future neutrino-telescope measurements. We demonstrate that the accuracies in the measurements of R = φ ( nμ)/ (φ(ve) + f(Vτ)) and S = f(ve)/f(v τ) should both be better than 10% in order to distinguish between the pion source and the muon-damped source at the 3 σ level.
原文 | English |
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頁面 | 1-3 |
頁數 | 3 |
出版狀態 | Published - 16 7月 2009 |
事件 | European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009 - Krakow, 波蘭 持續時間: 16 7月 2009 → 22 7月 2009 |
Conference
Conference | European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009 |
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國家/地區 | 波蘭 |
城市 | Krakow |
期間 | 16/07/09 → 22/07/09 |