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arXiv · 2302.05032

Simulation study on the optical processes at deep-sea neutrino telescope sites

Fan Hu·Zhenyu Wei·Wei Tian·Ziping Ye·Fuyudi Zhang·Zhengyang Sun·Wei Zhi·Qichao Chang·Qiao Xue·Zhuo Li·Donglian Xu
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Abstract

The performance of a large-scale water Cherenkov neutrino telescope relies heavily on the transparency of the surrounding water, quantified by its level of light absorption and scattering. A pathfinder experiment was carried out to measure the optical properties of deep seawater in South China Sea with light-emitting diodes (LEDs) as light sources, photon multiplier tubes (PMTs) and cameras as photon sensors. Here, we present an optical simulation program employing the Geant4 toolkit to understand the absorption and scattering processes in the deep seawater, which helps to extract the underlying optical properties from the experimental data. The simulation results are compared with the experimental data and show good agreements. We also verify the analysis methods that utilize various observables of the PMTs and the cameras with this simulation program, which can be easily adapted by other neutrino telescope pathfinder experiments and future large-scale detectors.

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Fan Hu, Zhenyu Wei, Wei Tian, Ziping Ye, Fuyudi Zhang, Zhengyang Sun, Wei Zhi, Qichao Chang, Qiao Xue, Zhuo Li, Donglian Xu. 2023-02-10. Simulation study on the optical processes at deep-sea neutrino telescope sites. https://doi.org/10.1016/j.nima.2023.168367

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