分类： 物理学 >> 核物理学 提交时间： 2016-09-13
摘要： The Jiangmen Underground Neutrino Observatory (JUNO) is an experiment proposed to determine the neutrino mass hierarchy and probe the fundamental properties of neutrino oscillation. The JUNO central detector is a spherical liquid scintillator detector with 20 kton fiducial mass. It is required to achieve a 3%/E(MeV)−−−−−−−√ energy resolution with very low radioactive background, which is a big challenge to the detector design. In order to ensure the detector performance can meet the physics requirements, reliable detector simulation is necessary to provide useful information for detector design. A simulation study of natural radioactivity backgrounds in the JUNO central detector has been performed to guide the detector design and set requirements to the radiopurity of detector materials.
分类： 天文学 >> 天文学 提交时间： 2023-02-19
Ran Han
ZhiWei Li
Ruohan Gao
Yao Sun
Ya Xu
Yaping Cheng
Guangzheng Jiang
Jie Pang
Fengcheng Liu
Andong Wang
Yufei Xi
Liangjian Wen
Jun Cao
Yu-Feng Li
摘要： Geoneutrinos are a unique tool that brings to the surface information about our planet, in particular, its radiogenic power, insights formation and chemical composition. To date, only the KamLAND and Borexino experiments observed geoneutrino, with the former characterized by low concentration of heat-producing elements in the Earth in contrast to the latter that sets tight upper limits on the power of a georeactor hypothesized. With respect to the results yielded therefrom, a small discrepancy has been identified. On this account, next generation experiments like JUNO are needed if it is to provide definitive results with respect to the Earth's radiogenic power, and to fully exploit geoneutrinos to better understand deep Earth. An accurate a priori prediction of the crustal contribution plays an important role in enabling the translation of a particle physics measurement into geo-scientific questions. The existing GIGJ model of JUNO only focused on constructing a geophysical model of the local crust, without local geochemical data. Another existing JULOC includes both data, but only able to be achieved for the top layer of the upper crust, not in deep vertical. This paper reports on the development of JUNO's first 3-D integrated model, JULOC-I, which combines seismic, gravity, rock sample and thermal flow data with new building method, solved the problem in vertical depth. JULOC-I results show higher than expected geoneutrino signals are mainly attributable to higher U and Th in southern China than that found elsewhere on Earth. Moreover, the high level of accuracy of the JULOC-I model, complemented by 10 years of experimental data, indicates that JUNO has an opportunity to test different mantle models. Predictions by JULOC-I can be tested after JUNO goes online and higher accuracy local crustal model continue to play an important role to improve mantle measurements precision.
分类： 天文学 >> 天文学 提交时间： 2023-02-19
Ran Han
ZhiWei Li
Ruohan Gao
Yao Sun
Ya Xu
Yaping Cheng
Guangzheng Jiang
Jie Pang
Fengcheng Liu
Andong Wang
Yufei Xi
Liangjian Wen
Jun Cao
Yu-Feng Li
摘要： Geoneutrinos are a unique tool that brings to the surface information about our planet, in particular, its radiogenic power, insights formation and chemical composition. To date, only the KamLAND and Borexino experiments observed geoneutrino, with the former characterized by low concentration of heat-producing elements in the Earth in contrast to the latter that sets tight upper limits on the power of a georeactor hypothesized. With respect to the results yielded therefrom, a small discrepancy has been identified. On this account, next generation experiments like JUNO are needed if it is to provide definitive results with respect to the Earth's radiogenic power, and to fully exploit geoneutrinos to better understand deep Earth. An accurate a priori prediction of the crustal contribution plays an important role in enabling the translation of a particle physics measurement into geo-scientific questions. The existing GIGJ model of JUNO only focused on constructing a geophysical model of the local crust, without local geochemical data. Another existing JULOC includes both data, but only able to be achieved for the top layer of the upper crust, not in deep vertical. This paper reports on the development of JUNO's first 3-D integrated model, JULOC-I, which combines seismic, gravity, rock sample and thermal flow data with new building method, solved the problem in vertical depth. JULOC-I results show higher than expected geoneutrino signals are mainly attributable to higher U and Th in southern China than that found elsewhere on Earth. Moreover, the high level of accuracy of the JULOC-I model, complemented by 10 years of experimental data, indicates that JUNO has an opportunity to test different mantle models. Predictions by JULOC-I can be tested after JUNO goes online and higher accuracy local crustal model continue to play an important role to improve mantle measurements precision.
分类： 天文学 >> 天文学 提交时间： 2023-02-19
JUNO Collaboration
Jie Zhao
Baobiao Yue
Haoqi Lu
Yufeng Li
Jiajie Ling
Zeyuan Yu
Angel Abusleme
Thomas Adam
Shakeel Ahmad
Rizwan Ahmed
Sebastiano Aiello
Muhammad Akram
Abid Aleem
Tsagkarakis Alexandros
Fengpeng An
Qi An
Giuseppe Andronico
Nikolay Anfimov
Vito Antonelli
摘要： The physics potential of detecting $^8$B solar neutrinos is exploited at the Jiangmen Underground Neutrino Observatory (JUNO), in a model independent manner by using three distinct channels of the charged-current (CC), neutral-current (NC) and elastic scattering (ES) interactions. Due to the largest-ever mass of $^{13}$C nuclei in the liquid-scintillator detectors and the potential low background level, $^8$B solar neutrinos would be observable in the CC and NC interactions on $^{13}$C for the first time. By virtue of optimized event selections and muon veto strategies, backgrounds from the accidental coincidence, muon-induced isotopes, and external backgrounds can be greatly suppressed. Excellent signal-to-background ratios can be achieved in the CC, NC and ES channels to guarantee the $^8$B solar neutrino observation. From the sensitivity studies performed in this work, we show that one can reach the precision levels of 5%, 8% and 20% for the $^8$B neutrino flux, $\sin^2\theta_{12}$, and $\Delta m^2_{21}$, respectively, using ten years of JUNO data. It would be unique and helpful to probe the details of both solar physics and neutrino physics. In addition, when combined with SNO, the world-best precision of 3% is expected for the $^8$B neutrino flux measurement.
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