Determining the flavor ratio of astrophysical neutrinos

Guey-Lin Lin, Kwang Chang Lai, Tsung Che Liu

研究成果: Paper同行評審

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
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 200922 7月 2009

Conference

ConferenceEuropean Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009
國家/地區波蘭
城市Krakow
期間16/07/0922/07/09

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