Measurement of the Attenuation Length of a Liquid Scintillator for the Detection of Reactor Neutrinos

2017 ◽  
Vol 67 (7) ◽  
pp. 842-845
Author(s):  
Young Seo PARK ◽  
Seung Chan KIM ◽  
Kyung Kwang JOO*
2019 ◽  
Vol 30 (2) ◽  
Author(s):  
Rui Zhang ◽  
De-Wen Cao ◽  
Chang-Wei Loh ◽  
You-Hang Liu ◽  
Fang-Liang Wu ◽  
...  

2013 ◽  
Vol 37 (7) ◽  
pp. 076001 ◽  
Author(s):  
Long Gao ◽  
Bo-Xiang Yu ◽  
Ya-Yun Ding ◽  
Li Zhou ◽  
Liang-Jian Wen ◽  
...  

2020 ◽  
Vol 1643 (1) ◽  
pp. 012021
Author(s):  
Ilham El Atmani

Abstract Reactor neutrinos have played a key role in understanding neutrino physics since their discovery. The so-called reactor-anti-neutrino-anomaly RAA, a ∼6.5% deficit of the mean observed neutrino flux compared to the prediction appeared recently. This anomaly could be interpreted by the existence of a fourth, sterile, neutrino and this hypothesis is currently being tested by the very short baseline experiment STEREO. The latter is installed at very short distance (9-11m) from the compact core of the ILL research reactor in Grenoble-France and collecting data since November 2016. The ILL core is highly enriched in 235U and releases a nominal thermal power of 58.3 MW. The geometry of the STEREO detector, segmented into six identical cells filled with Gd-loaded liquid scintillator, is designed for a direct test of a new oscillation pattern in the L/E range around 1 m/MeV, relevant for the RAA. First published results of STEREO have demonstrated the mitigation of the background induced by the reactor and the cosmic-rays and a good energy response. The data taking is now in progress with very stable conditions favorable for an improved accuracy. We will present an overview of the experiment and an update of the sterile neutrino analysis. A refined prediction of the neutrino spectrum emitted by the ILL reactor is also presented.


2020 ◽  
Vol 4 (3) ◽  
pp. 312-318
Author(s):  
Xiang-Wei Yin ◽  
Tao Hu ◽  
Bo-Xiang Yu ◽  
Wei Hu ◽  
Wen-Qi Yan ◽  
...  

Author(s):  
Zhiheng Xu ◽  
Zhengrong Zhang ◽  
Kelum A. A. Gamage ◽  
Yunpeng Liu ◽  
Huangfeng Ye ◽  
...  

2021 ◽  
Vol 2021 (8) ◽  
Author(s):  
Baobiao Yue ◽  
Jiajun Liao ◽  
Jiajie Ling

Abstract Neutrino magnetic moment (νMM) is an important property of massive neutrinos. The recent anomalous excess at few keV electronic recoils observed by the XENON1T collaboration might indicate a ∼ 2.2 × 10−11μB effective neutrino magnetic moment ($$ {\mu}_{\nu}^{\mathrm{eff}} $$ μ ν eff ) from solar neutrinos. Therefore, it is essential to carry out the νMM searches at a different experiment to confirm or exclude such a hypothesis. We study the feasibility of doing νMM measurement with 4 kton fiducial mass at Jinping neutrino experiment (Jinping) using electron recoil data from both natural and artificial neutrino sources. The sensitivity of $$ {\mu}_{\nu}^{\mathrm{eff}} $$ μ ν eff can reach < 1.2 × 10−11μB at 90% C.L. with 10-year data taking of solar neutrinos. Besides the abundance of the intrinsic low energy background 14C and 85Kr in the liquid scintillator, we find the sensitivity to νMM is highly correlated with the systematic uncertainties of pp and 85Kr. Reducing systematic uncertainties (pp and 85Kr) and the intrinsic background (14C and 85Kr) can help to improve sensitivities below these levels and reach the region of astrophysical interest. With a 3 mega-Curie (MCi) artificial neutrino source 51Cr installed at Jinping neutrino detector for 55 days, it could give us a sensitivity to the electron neutrino magnetic moment ($$ {\mu}_{\nu_e} $$ μ ν e ) with < 1.1 × 10−11μB at 90% C.L. . With the combination of those two measurements, the flavor structure of the neutrino magnetic moment can be also probed at Jinping.


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