Neutrino flavor ratio on Earth and at astrophysical sources

Kwang Chang Lai; Guey Lin Lin; T. C. Liu

doi:10.1016/j.ppnp.2009.12.064

Neutrino flavor ratio on Earth and at astrophysical sources

Kwang Chang Lai, Guey Lin Lin, T. C. Liu^*

^*此作品的通信作者

研究成果: Short survey › 同行評審

摘要

We present the reconstruction of neutrino flavor ratios at astrophysical sources. For distinguishing the pion source and the muon-damped source to the 3 σ level, the neutrino flux ratios, R ≡ φ{symbol} (ν_μ) / (φ{symbol} (ν_e) + φ{symbol} (ν_τ)) and S ≡ φ{symbol} (ν_e) / (φ{symbol} (ν_τ)), need to be measured in accuracies better than 10%.

原文	English
頁（從 - 到）	420-422
頁數	3
期刊	Progress in Particle and Nuclear Physics
卷	64
發行號	2
DOIs	https://doi.org/10.1016/j.ppnp.2009.12.064
出版狀態	Published - 4月 2010

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10.1016/j.ppnp.2009.12.064

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AB - We present the reconstruction of neutrino flavor ratios at astrophysical sources. For distinguishing the pion source and the muon-damped source to the 3 σ level, the neutrino flux ratios, R ≡ φ{symbol} (νμ) / (φ{symbol} (νe) + φ{symbol} (ντ)) and S ≡ φ{symbol} (νe) / (φ{symbol} (ντ)), need to be measured in accuracies better than 10%.

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JO - Progress in Particle and Nuclear Physics

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Neutrino flavor ratio on Earth and at astrophysical sources

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