Supernova Neutrinos Detection On Earth
Xin-Heng Guo, Ming-Yang Huang, and Bing-Lin Young

TL;DR
This paper discusses methods for detecting supernova neutrinos on Earth and proposes a new approach to measure small mixing angles like θ13, surpassing current experimental sensitivities.
Contribution
It introduces a novel detection method for supernova neutrinos to infer very small neutrino mixing angles, improving upon existing experimental capabilities.
Findings
Proposes a method to detect supernova neutrinos on Earth.
Suggests a way to measure θ13 smaller than 1.5°.
Highlights potential sensitivity improvements over Daya Bay.
Abstract
In this paper, we first discuss the detection of supernova neutrino on Earth. Then we propose a possible method to acquire information about smaller than 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.
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