Probing neutrino flavor transition mechanism with ultrahigh energy astrophysical neutrinos

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

*Corresponding author for this work

研究成果: Article同行評審

1 引文 斯高帕斯(Scopus)

摘要

Observation of ultrahigh energy astrophysical neutrinos and identification of their flavors have been proposed for future neutrino telescopes. The flavor ratio of astrophysical neutrinos observed on the Earth depends on both the initial flavor ratio at the source and flavor transitions taking place during propagations of these neutrinos. The flavor transition mechanisms are well classified with our model-independent parametrization. We find that a new parameter R≡φe/(φμ+φτ) can probe directly the flavor transition in the framework of our model-independent parametrization, without the assumption of the νμ-ντ symmetry. A few flavor-transition models are employed to test our parametrization with this new observable. The observational constraints on flavor transition mechanisms by the new observable are discussed through our model-independent parametrization.

原文English
文章編號033002
期刊Physical Review D - Particles, Fields, Gravitation and Cosmology
89
發行號3
DOIs
出版狀態Published - 6 二月 2014

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