Calibration strategy of the JUNO experiment

被引：0

作者：

Angel Abusleme

Thomas Adam

Shakeel Ahmad

Rizwan Ahmed

Sebastiano Aiello

Muhammad Akram

Fengpeng An

Guangpeng An

Qi An

Giuseppe Andronico

Nikolay Anfimov

Vito Antonelli

Tatiana Antoshkina

Burin Asavapibhop

João Pedro Athayde Marcondes de André

Didier Auguste

Andrej Babic

Wander Baldini

Andrea Barresi

Eric Baussan

Marco Bellato

Antonio Bergnoli

Enrico Bernieri

Thilo Birkenfeld

Sylvie Blin

David Blum

Simon Blyth

Anastasia Bolshakova

Mathieu Bongrand

Clément Bordereau

Dominique Breton

Augusto Brigatti

Riccardo Brugnera

Riccardo Bruno

Antonio Budano

Mario Buscemi

Jose Busto

Ilya Butorov

Anatael Cabrera

Hao Cai

Xiao Cai

Yanke Cai

Zhiyan Cai

Antonio Cammi

Agustin Campeny

Chuanya Cao

Guofu Cao

Jun Cao

Rossella Caruso

Cédric Cerna

机构：

[1] Yerevan Physics Institute,School of Physics

[2] Université Libre de Bruxelles,College of Electronic Science and Engineering

[3] Universidade Estadual de Londrina,School of Physics and Astronomy

[4] Pontificia Universidade Catolica do Rio de Janeiro,Tsung

[5] Pontificia Universidad Católica de Chile,Dao Lee Institute

[6] Universidad Tecnica Federico Santa Maria,Institute of Hydrogeology and Environmental Geology

[7] Beijing Institute of Spacecraft Environment Engineering,School of Physics and Microelectronics

[8] Beijing Normal University,Department of Physics

[9] China Institute of Atomic Energy,III. Physikalisches Institut B

[10] Institute of High Energy Physics,Institute of Experimental Physics

[11] North China Electric Power University,Institute of Physics

[12] Peking University,Eberhard Karls Universität Tübingen

[13] Tsinghua University,Department of Physics, Faculty of Science

[14] University of Chinese Academy of Sciences,Department of Physics and Astronomy

[15] Jilin University,Department of Physics

[16] National University of Defense Technology,undefined

[17] Chongqing University,undefined

[18] Dongguan University of Technology,undefined

[19] Jinan University,undefined

[20] Sun Yat-Sen University,undefined

[21] Harbin Institute of Technology,undefined

[22] University of Science and Technology of China,undefined

[23] The Radiochemistry and Nuclear Chemistry Group in University of South China,undefined

[24] Wuyi University,undefined

[25] Shandong University,undefined

[26] Institute of Modern Physics,undefined

[27] Chinese Academy of Sciences,undefined

[28] Nanjing University,undefined

[29] Guangxi University,undefined

[30] East China University of Science and Technology,undefined

[31] Shanghai Jiao Tong University,undefined

[32] Shanghai Jiao Tong University,undefined

[33] Chinese Academy of Geological Sciences,undefined

[34] Nankai University,undefined

[35] Wuhan University,undefined

[36] Xi’an Jiaotong University,undefined

[37] Xiamen University,undefined

[38] Zhengzhou University,undefined

[39] Institute of Physics National Chiao-Tung University,undefined

[40] National United University,undefined

[41] National Taiwan University,undefined

[42] Charles University,undefined

[43] Faculty of Mathematics and Physics,undefined

[44] University of Jyvaskyla,undefined

[45] Department of Physics,undefined

[46] IJCLab,undefined

[47] Université Paris-Saclay,undefined

[48] CNRS/IN2P3,undefined

[49] Univ. Bordeaux,undefined

[50] CNRS,undefined

来源：

Journal of High Energy Physics | / 2021卷

关键词：

Neutrino Detectors and Telescopes (experiments);

D O I：

暂无

中图分类号：

学科分类号：

摘要：

We present the calibration strategy for the 20 kton liquid scintillator central detector of the Jiangmen Underground Neutrino Observatory (JUNO). By utilizing a comprehensive multiple-source and multiple-positional calibration program, in combination with a novel dual calorimetry technique exploiting two independent photosensors and readout systems, we demonstrate that the JUNO central detector can achieve a better than 1% energy linearity and a 3% effective energy resolution, required by the neutrino mass ordering determination.

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