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JUNO sensitivity on proton decay p→νK^(+)searches

Chinese Physics C 2023年第11期47卷 7-22页

作者： Angel Abuslem. Thom.s Adam.Shakeel Ahm.d Rizwan Ahm.d Sebastiano Aiello m.ham.ad Akram.安丰鹏安琪 Giuseppe Andronico Nikolay Anfim.v Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde m.rcondes de André Didier Auguste Nikita Balashov Wander Baldini Andrea Barresi davide Basilico Eric Baussan m.rco Bellato Antonio Bergnoli Thilo Birkenfeld Sylvie Blin david Blum.Sim.n Blyth Anastasia Bolshakova m.thieu Bongrand Clém.nt Bordereau Dom.nique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano m.rio Buscem. Jose Busto Ilya Butorov Anatael Cabrera Barbara Caccianiga 蔡浩蔡啸蔡严克蔡志岩 Riccardo Callegari Antonio Cam.i Agustin Cam.eny 曹传亚曹国富曹俊 Rossella Caruso Cédric Cerna 常劲帆 Yun Chang 陈平平 Po-An Chen 陈少敏陈旭荣 Yi-Wen Chen 陈义学陈羽陈长程捷程雅苹 Alexey Chetverikov davide Chiesa Pietro Chim.nti Artem.Chukanov Gérard Claverie Catia Clem.nti Barbara Clerbaux Selm. Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalager Christophe De La Taille 邓智邓子艳 Wilfried Depnering m.rco Diaz Xuefeng Ding 丁雅韵 Bayu Dirgantara Sergey Dm.trievsky Tadeas Dohnal Dm.try Dolzhikov Georgy Donchenko 董建蒙 Evgeny Doroshkevich m.rcos Dracos Frédéric Druillole 杜然杜书先 Stefano Dusini m.rtin Dvorak Tim. Enqvist Heike Enzm.nn Andrea Fabbri Ulrike Fahrendholz 范东华樊磊方建方文兴 m.rco Fargetta Dm.try Fedoseev Li-Cheng Feng 冯启春 Richard Ford Am.lie Fournier 甘浩男 Feng Gao Alberto Garfagnini Arsenii Gavrikov m.rco Giam.archi Agnese Giaz Nunzio Giudice m.xim.Gonchar 龚光华宫辉 Yuri Gornushkin Alexandre Göttel m.rco Grassi Christian Grewing Vasily Grom.v 顾旻皓谷肖飞古宇关梦云 Nunzio Guardone m.ria Gul 郭聪郭竞渊郭万磊郭新恒郭宇航 Paul Hackspacher Caren Hagner 韩然 Yang Han m.ham.ad Sohaib Hassan 何苗何伟 Tobias Heinz Patrick Hellm.th 衡月昆 Rafael Herrera 贺远强侯少静 Yee Hsiung Bei-Zhen Hu 胡航胡健润胡俊胡守扬胡涛胡宇翔胡焯钧黄春豪黄桂鸿黄翰雄黄文昊黄鑫黄性涛黄永波惠加琪霍雷霍文驹 Cédric Huss Safeer Hussain Ara Ioannisian Roberto Isocrate Beatrice Jelm.ni Kuo-Lun Jen Ignacio Jeria 季筱璐吉星曌贾慧慧贾俊基蹇司玉蒋荻蒋炜江晓山金如意荆小平 Cécile Jollet Jari Joutsenvaara Sirichok Jungthawan Leonidas Kalousis Philipp Ka Pontificia Universidad Católica de Chile SantiagoChile IPHC Universitéde StrasbourgCNRS/IN2P3F-67037 StrasbourgFrance Pakistan Institute of Nuclear Science and Technology IslamabadPakistan INFN Catania and Dipartim.nto di Fisica e Astronom.a dell Universitàdi Catania CataniaItaly East China University of Science and Technology ShanghaiChina University of Science and Technology of China HefeiChina Joint Institute for Nuclear Research DubnaRussia INFN Sezione di m.lano and Dipartim.nto di Fisica dell Universitàdi m.lano MilanoItaly Departm.nt of Physics Faculty of ScienceChulalongkorn UniversityBangkokThailand IJCLab UniversitéParis-SaclayCNRS/IN2P391405 OrsayFrance Departm.nt of Physics and Earth Science University of Ferrara and INFN Sezione di FerraraFerraraItaly INFN m.lano Bicocca and University of m.lano Bicocca MilanoItaly INFN Sezione di Padova PadovaItaly III.Physikalisches Institut B RWTH Aachen UniversityAachenGermany Eberhard Karls Universität Tübingen Physikalisches InstitutTübingenGermany Institute of High Energy Physics BeijingChina SUBATECH Universitéde NantesIMT AtlantiqueCNRS-IN2P3NantesFrance Univ.Bordeaux CNRSLP2IUMR 5797F-33170 GradignanFrance Departm.nt of Physics National Taiwan UniversityTaipei Dipartim.nto di Fisica e Astronom.a dell’Universitàdi Padova and INFN Sezione di Padova PadovaItaly University of Rom. Tre and INFN Sezione Rom. Tre RomaItaly Aix m.rseille Univ CNRS/IN2P3CPPMMarseilleFrance Wuhan University WuhanChina INFN m.lano Bicocca and Politecnico of m.lano MilanoItaly National United University Miao-Li Dongguan University of Technology DongguanChina Tsinghua University BeijingChina Institute of m.dern Physics Chinese Academy of SciencesLanzhouChina Institute of Physics National Yang Ming Chiao Tung UniversityHsinchu North China Electric Power University BeijingChina Sun Yat-Sen University GuangzhouChina Beijing Institute of Spacecraft Environm.nt Engineering BeijingChina Universidade Estadual de Londrina LondrinaBrazil INFN Sez

The Jiangm.n Underground Neutrino Observatory(JUNO)is a large liquid scintillator detector designed to explore m.ny topics in fundam.ntal *** this study,the potential of searching for proton decay in the p→νK^(+)m.de with JUNO is *** kaon and its decay particles feature a clear three-fold coincidence signature that results in a high efficiency for ***,the excellent energy resolution of JUNO perm.ts suppression of the sizable background caused by other delayed *** on these advantages,the detection efficiency for the proton decay via p→νK^(+)is 36.9%±4.9%with a background level of 0.2±0.05(syst)±0.2(stat)events after 10 years of data *** estim.ted sensitivity based on 200 kton-years of exposure is 9.6×1033 years,which is com.etitive with the current best lim.ts on the proton lifetim. in this channel and com.lem.nts the use of different detection technologies.

关键词： proton decay grand unified theories JUNO liquid scintillator detector

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