Prospect of a very long baseline neutrino oscillation experiment: HIPA to Beijing
Hesheng Chen, Linkai Ding, Jingtang He, Haohuai Kuang, Yusheng Lu,, Yuqian Ma, Lianyou Shan, Changquan Shen, Yifang Wang, Changgen Yang, Xinmin, Zhang, Qingqi Zhu, Chengrui Qing, Zhaohua Xiong, Jin Min Yang, Zhaoxi Zhang,, Jiaer Chen, Yanlin Ye, S.C. Lee, H.T. Wong

TL;DR
This paper evaluates the potential of a very long baseline neutrino oscillation experiment from HIPA to Beijing, identifying an optimal distance and proposing a large water Cherenkov detector for comprehensive physics measurements.
Contribution
It introduces a detailed analysis of baseline distances for neutrino experiments and proposes a large water Cherenkov detector, highlighting its multifaceted scientific capabilities.
Findings
Baseline over 2100 km is optimal for neutrino oscillation measurements.
A large water Cherenkov detector performs well in simulations.
The detector can also contribute to cosmic-ray and astrophysics research.
Abstract
We discuss the prospects of a very long baseline neutrino oscillation experiment from HIPA to Beijing. The current understanding of neutrino oscillations, both theoretically and experimentally, are summarized. The figure of merits for interested physics measurements are defined and compared at different distances: 300 km, 700 km, 2100 km and 3000 km. We conclude that a baseline more than 2100 km is optimal. A large water cerenkov calorimeter was proposed and its performance is satisfactory from a Monte Carlo simulation study. Such a large detector can do many other measurements on cosmic-rays physics and astrophysics.
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Particle physics theoretical and experimental studies
