Supernova neutrino detection on earth

Supernova neutrino detection on earth

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摘要 In this paper, we first discuss the detection of supernova neutrinos on earth. Then we propose a possible method to acquire information about θ13 smaller than 1.5° by detecting the ratio of the event numbers of different flavor supernova neutrinos. Such an sensitivity cannot yet be achieved by the Daya Bay reactor neutrino experiment. In this paper, we first discuss the detection of supernova neutrinos on earth. Then we propose a possible method to acquire information about θ13 smaller than 1.5° by detecting the ratio of the event numbers of different flavor supernova neutrinos. Such an sensitivity cannot yet be achieved by the Daya Bay reactor neutrino experiment.

作者郭新恒黄明阳杨炳麟

机构地区 College of Nuclear Science and Technology Department of Physics and Astronomy Institute of Theoretical Physics

出处《Chinese Physics C》 SCIE CAS CSCD 2010年第2期257-261,共5页 中国物理C（英文版）

基金 Supported by National Natural Science Foundation of China (10535050,10675022) Key Project of Chinese Ministry of Education (106024) Special Grants from Beijing Normal University

关键词 SUPERNOVA NEUTRINO collective effects MSW effects earth matter effects Daya Bay supernova, neutrino, collective effects, MSW effects, earth matter effects, Daya Bay

分类号 O572.321 [理学—粒子物理与原子核物理]

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参考文献37

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Chinese Physics C

2010年第2期

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Supernova neutrino detection on earth

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