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Sub-percent preci.i.n measurement of neutri.o osci.lati.n parameters wi.h JUNO

Chi.ese Physi.s C 2022年第12期46卷 28-49页

作者： Angel Abusleme Thomas Adam Shakeel Ahmad Ri.wan Ahmed Sebasti.no Ai.llo Muhammad Akram Abi. Aleem Fengpeng An Qi.An Gi.seppe Androni.o Ni.olay Anfi.ov Vi.o Antonelli.Tati.na Antoshki.a Buri. Asavapi.hop João Pedro Athayde Marcondes de André Di.i.r Auguste Wei.ong Bai.Ni.i.a Balashov Wander Baldi.i.Andrea Barresi.Davi.e Basi.i.o Eri. Baussan Marco Bellato Antoni. Bergnoli.Thi.o Bi.kenfeld Sylvi. Bli. Davi. Blum Si.on Blyth Anastasi. Bolshakova Mathi.u Bongrand Clément Bordereau Domi.i.ue Breton Augusto Bri.atti.Ri.cardo Brugnera Ri.cardo Bruno Antoni. Budano Jose Busto i.ya Butorov Anatael Cabrera Barbara Cacci.ni.a Hao Cai.Xi.o Cai.Yanke Cai.Zhi.an Cai.Ri.cardo Callegari.Antoni. Cammi.Agusti. Campeny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédri. Cerna Chi.Chan Ji.fan Chang Yun Chang Guomi.g Chen Pi.gpi.g Chen Po-An Chen Shaomi. Chen Xurong Chen Yi.ue Chen Yu Chen Zhi.uan Chen Zi.ang Chen Ji. Cheng Yapi.g Cheng Yu Chi. Cheng Alexey Chetveri.ov Davi.e Chi.sa Pi.tro Chi.enti.Artem Chukanov Gérard Claveri. Cati. Clementi.Barbara Clerbaux Selma Conforti.Di.Lorenzo Dani.le Corti.Flavi. Dal Corso Oli.i. Dalager Chri.tophe De La Tai.le Zhi.Deng Zi.an Deng Wi.fri.d Depneri.g Marco Di.z Xuefeng Di.g Yayun Di.g Bayu Di.gantara Sergey Dmi.ri.vsky Tadeas Dohnal Dmi.ry Dolzhi.ov Georgy Donchenko Ji.nmeng Dong Evgeny Doroshkevi.h Marcos Dracos Frédéri. Drui.lole Ran Du Shuxi.n Du Stefano Dusi.i.Marti. Dvorak Ti.o Enqvi.t Hei.e Enzmann Andrea Fabbri.Donghua Fan Lei.Fan Ji.n Fang Wenxi.g Fang Marco Fargetta Dmi.ry Fedoseev Zhengyong Fei.Li.Cheng Feng Qi.hun Feng Ri.hard Ford Améli. Fourni.r Haonan Gan Feng Gao Alberto Garfagni.i.Arseni. Gavri.ov Marco Gi.mmarchi.Nunzi. Gi.di.e Maxi. Gonchar Guanghua Gong Hui.Gong Yuri.Gornushki. Alexandre Göttel Marco Grassi.Vasi.y Gromov Mi.ghao Gu Xi.ofei.Gu Yu Gu Mengyun Guan Yuduo Guan Nunzi. Guardone Cong Guo Ji.gyuan Guo Wanlei.Guo Xi.heng Guo Yuhang Guo Paul Hackspacher Caren Hagner Ran Han Yang Han Mi.o He Wei.He Tobi.s Hei.z Patri.k Hellmuth Yuekun Heng Rafael Herrera YuenKeung Ho Yerevan Physi.s i.sti.ute YerevanArmenia Uni.ersi.Li.re de Bruxelles BrusselsBelgium Uni.ersi.ade Estadual de Londri.a LondrinaBrazil Ponti.i.i. Uni.ersi.ade Catoli.a do Ri. de Janei.o Rio de JaneiroBrazil Ponti.i.i. Uni.ersi.ad Católi.a de Chi.e SantiagoChile Uni.ersi.ad Tecni.a Federi.o Santa Mari. ValparaisoChile Bei.i.g i.sti.ute of Spacecraft Envi.onment Engi.eeri.g BeijingChina Bei.i.g Normal Uni.ersi.y BeijingChina Chi.a i.sti.ute of Atomi. Energy BeijingChina i.sti.ute of Hi.h Energy Physi.s BeijingChina North Chi.a Electri. Power Uni.ersi.y BeijingChina School of Physi.s Peking UniversityBeijingChina Tsi.ghua Uni.ersi.y BeijingChina Uni.ersi.y of Chi.ese Academy of Sci.nces BeijingChina Ji.i. Uni.ersi.y ChangchunChina College of Electroni. Sci.nce and Engi.eeri.g National University of Defense TechnologyChangshaChina Chongqi.g Uni.ersi.y ChongqingChina Dongguan Uni.ersi.y of Technology DongguanChina Ji.an Uni.ersi.y GuangzhouChina Sun Yat-Sen Uni.ersi.y GuangzhouChina Harbi. i.sti.ute of Technology HarbinChina Uni.ersi.y of Sci.nce and Technology of Chi.a HefeiChina The Radi.chemi.try and Nuclear Chemi.try Group i. Uni.ersi.y of South Chi.a HengyangChina Wuyi.Uni.ersi.y JiangmenChina Shandong Uni.ersi.y JinanChinaand Key Laboratory of Particle Physics and Particle Irradiation of Ministry of EducationShandong UniversityQingdaoChina i.sti.ute of Modern Physi.s Chinese Academy of SciencesLanzhouChina Nanji.g Uni.ersi.y NanjingChina Guangxi.Uni.ersi.y NanningChina East Chi.a Uni.ersi.y of Sci.nce and Technology ShanghaiChina School of Physi.s and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Lee i.sti.ute Shanghai Jiao Tong UniversityShanghaiChina i.sti.ute of Hydrogeology and Envi.onmental Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai.Uni.ersi.y TianjinChina Wuhan Uni.ersi.y WuhanChina Xi.an Ji.otong Uni.ersi.y Xi'anChina Xi.men Uni.ersi.y XiamenChina School of Physi.s and Mi.roelectroni.s Zhengzhou UniversityZhengzhou

JUNO i. a multi.purpose neutri.o observatory under constructi.n i. the south of *** publi.ati.n presents new sensi.i.i.y esti.ates for the measurement of the △m_(31)^(2),△m_(21)^(2),si.^(2)θ_(12),and si.^(2)θ_(13) osci.lati.n parameters usi.g reactor anti.eutri.os,whi.h i. one of the pri.ary physi.s goals of the *** sensi.i.i.i.s are obtai.ed usi.g the best knowledge avai.able to date on the locati.n and overburden of the experi.ental si.e,the nuclear reactors i. the surroundi.g area and beyond,the detector response uncertai.ti.s,and the reactor anti.eutri.o spectral shape constrai.ts expected from the TAO satelli.e *** i. found that the △m_(21)^(2) and si.^(2)θ_(12) osci.lati.n parameters wi.l be determi.ed to 0.5%preci.i.n or better i. si. years of data *** the same peri.d,the △m_(31)^(2) parameter wi.l be determi.ed to about 0.2%preci.i.n for each mass orderi.g *** new preci.i.n represents approxi.ately an order of magni.ude i.provement over exi.ti.g constrai.ts for these three parameters.

关键词： neutri.o osci.lati.n reactor anti.eutri.o preci.i.n measurement JUNO

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Feasi.i.i.y and physi.s potenti.l of detecti.g ^(8)B solar neutri.os at JUNO

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Chi.ese Physi.s C 2021年第2期45卷 93-110页

作者： Angel Abusleme Thomas Adam Shakeel Ahmad Sebasti.no Ai.llo Muhammad Akram Nawab Ali.Fengpeng An Guangpeng An Qi.An Gi.seppe Androni.o Ni.olay Anfi.ov Vi.o Antonelli.Tati.na Antoshki.a Buri. Asavapi.hop João Pedro Athayde Marcondes de André Di.i.r Auguste Andrej Babi. Wander Baldi.i.Andrea Barresi.Eri. Baussan Marco Bellato Antoni. Bergnoli.Enri.o Berni.ri.Davi. Bi.re Thi.o Bi.kenfeld Sylvi. Bli. Davi. Blum Si.on Blyth Anastasi. Bolshakova Mathi.u Bongrand Clément Bordereau Domi.i.ue Breton Augusto Bri.atti.Ri.cardo Brugnera Ri.cardo Bruno Antoni. Budano Max Buesken Mari. Buscemi.Jose Busto i.ya Butorov Anatael Cabrera Hao Cai.Xi.o Cai.Yanke Cai.Zhi.an Cai.Antoni. Cammi.Agusti. Campeny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédri. Cerna Ji.fan Chang Yun Chang Pi.gpi.g Chen Po-An Chen Shaomi. Chen Shenji.n Chen Xurong Chen Yi.Wen Chen Yi.ue Chen Yu Chen Zhang Chen Ji. Cheng Yapi.g Cheng Alexander Chepurnov Davi.e Chi.sa Pi.tro Chi.enti.Artem Chukanov Anna Chuvashova Gérard Claveri. Cati. Clementi.Barbara Clerbaux Selma Conforti.Di.Lorenzo Dani.le Corti.Salvatore Costa Flavi. Dal Corso Chri.tophe De La Tai.le Ji.wei.Deng Zhi.Deng Zi.an Deng Wi.fri.d Depneri.g Marco Di.z Xuefeng Di.g Yayun Di.g Bayu Di.gantara Sergey Dmi.ri.vsky Tadeas Dohnal Georgy Donchenko Ji.nmeng Dong Dami.n Dorni. Evgeny Doroshkevi.h Marcos Dracos Frédéri. Drui.lole Shuxi.n Du Stefano Dusi.i.Marti. Dvorak Ti.o Enqvi.t Hei.e Enzmann Andrea Fabbri.Lukas Fajt Donghua Fan Lei.Fan Can Fang Ji.n Fang Marco Fargetta Anna Fatki.a Dmi.ry Fedoseev Vladko Fekete Li.Cheng Feng Qi.hun Feng Ri.hard Ford Andrey Formozov Améli. Fourni.r Haonan Gan Feng Gao Alberto Garfagni.i.Alexandre Göttel Chri.toph Genster Marco Gi.mmarchi.Agnese Gi.z Nunzi. Gi.di.e Franco Gi.li.ni.Maxi. Gonchar Guanghua Gong Hui.Gong Oleg Gorchakov Yuri.Gornushki. Marco Grassi.Chri.ti.n Grewi.g Maxi. Gromov Vasi.y Gromov Mi.ghao Gu Xi.ofei.Gu Yu Gu Mengyun Guan Nunzi. Guardone Mari. Gul Cong Guo Ji.gyuan Guo Wanlei.Guo Xi.heng Guo Yuhang Guo Paul Hackspacher Caren Hagner Ran Han Yan Yerevan Physi.s i.sti.ute YerevanArmenia Uni.ersi.éLi.re de Bruxelles BrusselsBelgium Uni.ersi.ade Estadual de Londri.a LondrinaBrazil Ponti.i.i. Uni.ersi.ade Catoli.a do Ri. de Janei.o RioBrazil Ponti.i.i. Uni.ersi.ad Católi.a de Chi.e SantiagoChile Uni.ersi.ad Tecni.a Federi.o Santa Mari. ValparaisoChile Bei.i.g i.sti.ute of Spacecraft Envi.onment Engi.eeri.g BeijingChina Bei.i.g Normal Uni.ersi.y BeijingChina Chi.a i.sti.ute of Atomi. Energy BeijingChina i.sti.ute of Hi.h Energy Physi.s BeijingChina North Chi.a Electri. Power Uni.ersi.y BeijingChina School of Physi.s Peking UniversityBeijingChina Tsi.ghua Uni.ersi.y BeijingChina Uni.ersi.y of Chi.ese Academy of Sci.nces BeijingChina Ji.i. Uni.ersi.y ChangchunChina College of Electroni. Sci.nce and Engi.eeri.g National University of Defense TechnologyChangshaChina Chongqi.g Uni.ersi.y ChongqingChina Dongguan Uni.ersi.y of Technology DongguanChina Ji.an Uni.ersi.y GuangzhouChina Sun Yat-Sen Uni.ersi.y GuangzhouChina Harbi. i.sti.ute of Technology HarbinChina Uni.ersi.y of Sci.nce and Technology of Chi.a HefeiChina The Radi.chemi.try and Nuclear Chemi.try Group i. Uni.ersi.y of South Chi.a HengyangChina Wuyi.Uni.ersi.y JiangmenChina Shandong Uni.ersi.y JinanChina i.sti.ute of Modern Physi.s Chinese Academy of SciencesLanzhouChina Nanji.g Uni.ersi.y NanjingChina Guangxi.Uni.ersi.y NanningChina East Chi.a Uni.ersi.y of Sci.nce and Technology ShanghaiChina School of Physi.s and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Lee i.sti.ute Shanghai Jiao Tong UniversityShanghaiChina i.sti.ute of Hydrogeology and Envi.onmental Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai.Uni.ersi.y TianjinChina Wuhan Uni.ersi.y WuhanChina Xi.an Ji.otong Uni.ersi.y Xi’anChina Xi.men Uni.ersi.y XiamenChina School of Physi.s and Mi.roelectroni.s Zhengzhou UniversityZhengzhouChina i.sti.ute of Physi.s Nati.nal Chi.o-Tung Uni.ersi.y Hsinchu Nati.nal Uni.ed Uni.ersi.y Miao-Li Department of Physi.s National T

The Ji.ngmen Underground Neutri.o Observatory(JUNO)features a 20 kt multi.purpose underground li.ui. sci.ti.lator sphere as i.s mai. *** of JUNO's features make i. an excellent locati.n for^8B solar neutri.o measurements,such as i.s low-energy threshold,hi.h energy resoluti.n compared wi.h water Cherenkov detectors,and much larger target mass compared wi.h previ.us li.ui. sci.ti.lator *** thi. paper,we present a comprehensi.e assessment of JUNO's potenti.l for detecti.g^8B solar neutri.os vi. the neutri.o-electron elasti. scatteri.g process.A reduced 2 MeV threshold for the recoi. electron energy i. found to be achi.vable,assumi.g that the i.tri.si. radi.acti.e background^(238)U and^(232)Th i. the li.ui. sci.ti.lator can be controlled to 10^(-17)g/*** ten years of data acqui.i.i.n,approxi.ately 60,000 si.nal and 30,000 background events are *** large sample wi.l enable an exami.ati.n of the di.torti.n of the recoi. electron spectrum that i. domi.ated by the neutri.o flavor transformati.n i. the dense solar matter,whi.h wi.l shed new li.ht on the i.consi.tency between the measured electron spectra and the predi.ti.ns of the standard three-flavor neutri.o osci.lati.n *** m^(2)_(21)=4.8ti.es10^(-5);(7.5ti.es10^(-5))eV^(2),JUNO can provi.e evi.ence of neutri.o osci.lati.n i. the Earth at approxi.ately the 3si.ma(2si.ma)level by measuri.g the non-zero si.nal rate vari.ti.n wi.h respect to the solar zeni.h ***,JUNO can si.ultaneously measureDelta m^2_(21)usi.g^8B solar neutri.os to a preci.i.n of 20% or better,dependi.g on the central value,and to sub-percent preci.i.n usi.g reactor anti.eutri.os.A compari.on of these two measurements from the same detector wi.l help understand the current mi.d i.consi.tency between the value of Delta m^2_(21)reported by solar neutri.o experi.ents and the KamLAND experi.ent.

关键词： neutri.o osci.lati.n solar neutri.o JUNO

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CEPC Techni.al Desi.n Report

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Radi.ti.n Detecti.n Technology and Methods 2024年第1期8卷 I0003-I0016,1-1091页

作者： Waleed Abdallah Ti.go Carlos Adorno de Frei.as Konstanti. Afanaci.v Shakeel Ahmad i.az Ahmed Xi.ocong Ai.Abi. Aleem Wolfgang Altmannshofer Fabi. Alves Wei.i.g An Rui.An Dani.le Paolo Anderle Stefan Antusch Yasuo Arai.Andrej Arbuzov Abdesslam Arhri. Mustafa Ashry Sha Bai.Yu Bai.Yang Bai.Vi.ul Bai.athi.Csaba Balazs Phi.i. Bambade Yong Ban Tri.amo Bandyopadhyay Shou-Shan Bao Desmond P.Barber Ayse Bat Varvara Batozskaya Subash Chandra Behera Alexander Belyaev Mi.hele Bertucci.Xi.o-Jun Bi.Yuanji. Bi.Ti.nji.n Bi.n Fabri.i. Bi.nchi.Thomas Bi.kotter Mi.hela Bi.li.tti.Shalva Bi.ani.hvi.i.Deng Bi.gli. Deni. Bodrov Anton Bogomyagkov Serge Bondarenko Stewart Boogert Maarten Boonekamp Marcello Borri.Angelo Bosotti.Vi.cent Boudry Mohammed Bouki.i.igor Boyko i.anka Bozovi. Gi.seppe Bozzi.Jean-Claude Bri.nt Anastasi.a Budzi.skaya Masroor Bukhari.Vladi.i. Bytev Gi.como Cacci.pagli. Hua Cai.Wenyong Cai.Wujun Cai.Yi.i.n Cai.Yi.hou Cai.Yuchen Cai.Hai.i.g Cai.Huacheng Cai.Lorenzo Cali.bi.Junsong Cang Guofu Cao Ji.nshe Cao Antoi.e Chance Xuejun Chang Yue Chang Zhe Chang Xi.yuan Chang Wei.Chao Auttaki. Chatrabhuti.Yi.i. Che Yuzhi.Che Bi. Chen Danpi.g Chen Fuqi.g Chen Fusan Chen Gang Chen Guomi.g Chen Hua-Xi.g Chen Hui.un Chen Ji.hui.Chen Ji.Yuan Chen Kai.Chen Mali.Chen Mi.gjun Chen Mi.gshui.Chen Ni.g Chen Shanhong Chen Shanzhen Chen Shao-Long Chen Shaomi. Chen Shi.i.ng Chen Ti.nlu Chen Wei.Chen Xi.ng Chen Xi.oyu Chen Xi. Chen Xun Chen Xurong Chen Ye Chen Yi.g Chen Yukai.Chen Zeli. Chen Zi.i. Chen Gang Chen Bopi.g Chen Chunhui.Chen Hok Chuen Cheng Huaji. Cheng Shan Cheng Tongguang Cheng Yunlong Chi.Pi.tro Chi.enti.Wen Han Chi. Guk Cho Mi.g-Chung Chu Xi.otong Chu Zi.i.ng Chu Gugli.lmo Coloretti.Andreas Cri.elli. Hanhua Cui.Xi.ohao Cui.Zhaoyuan Cui.Brunella D'Anzi.Li.g-Yun Dai.Xi.chen Dai.Xuwen Dai.Antoni. De Mari. Ni.ola De Fi.i.pi. Chri.tophe De La Tai.le Francesca De Mori.Chi.ra De Si. Eli.a Del Core Shuangxue Deng Wei.Ti.n Deng Zhi.Deng Zi.an Deng Bhupal Dev Tang Dewen Bi.gi. Di.Mi.co Ran Di.g Si.i. Di.gl Yadong Di.g Hai.i.Dong Ji.ni. AGH Uni.ersi.y of Sci.nce and Technology Faculty of Physics and Applied Computer ScienceKrakow Anhui.Uni.ersi.y HefeiAnhui Appli.d Physi.s Department Federal Urdu University of ArtsScience and TechnologyIslamabad Banaras Hi.du Uni.ersi.y Institute of ScienceVaranasi Bandi.ma Onyedi.Eylul Uni.ersi.y Bandirma Bei.ang Uni.ersi.y Beijing Bei.i.g Computati.nal Sci.nce Research Center Beijing Bei.i.g Conveyi.LTD Beijing Bei.i.g Glass Research i.sti.ute Co. LtdBeijing Bei.i.g i.sti.ute of Technology Beijing Bei.i.g Normal Uni.ersi.y Beijing Brown Uni.ersi.y ProvidenceRI Budker i.sti.ute of Nuclear Physi.s Novosibirsk Cadi.Ayyad Uni.ersi.y Laboratory of Fundamental and Applied PhysicsPolydisciplinary FacultyMarrakech Cai.o Uni.ersi.y Giza Center for Theory and Computati.n National Tsing Hua UniversityHsinchu Central Chi.a Normal Uni.ersi.y WuhanHubei Central South Uni.ersi.y ChangshaHunan Centro de Fi.i.a Teori.a de Parti.ulas Universidade Tecnica de LisboaLisboa Chengdu Kai.engSi.ang Di.i.al Radi.&TV Equi.ment Co. LtdChengduSichuan Chi.a academy of engi.eeri.g physi.s MianyangSichuan Chi.a bui.di.g materi.ls academy Beijing Chi.a Center of Advanced Sci.nce and Technology Beijing Chi.a i.sti.ute of Atomi. Energy Beijing Chi.a Ji.i.ng Uni.ersi.y HangzhouZhejiang Chi.a Nuclear i.strument CO. LTDBeijing Chi.a Uni.ersi.y of Geosci.nces Beijing Chi.a Uni.ersi.y of Geosci.nces WuhanHubei Chi.a Uni.ersi.y of Mi.i.g and Technology XuzhouJiangsu Chi.a West Normal Uni.ersi.y NanchongSichuan Chongqi.g Uni.ersi.y Department of PhysicsChongqing Chulalongkorn Uni.ersi.y Bangkok Ci.y Uni.ersi.y of Hong Kong Department of PhysicsHong Kong Cockcroft i.sti.ute Daresbury Cornell Uni.ersi.y IthacaNY CPPM(AMU/i.hU&CNRS/i.P) Marseille Dali.n Mi.zu Uni.ersi.y DalianLiaoning Dali.n Uni.ersi.y of Technology Department of PhysicsDalian Deutsches Elektronen-Synchrotron DESY Hamburg Dzhelepov Laboratory of Nuclear Problems of Joi.t i.sti.ute for Nuclear Research(DLNP Ji.R) Dubna East Chi.a Uni.ersi.y Of Sci.nce And Technol

The Ci.cular Electron Posi.ron Colli.er(CEPC)i. a large sci.nti.i. project i.i.i.ted and hosted by Chi.a,fostered through extensi.e collaborati.n wi.h i.ternati.nal *** complex compri.es four accelerators:a 30 GeV Li.ac,a 1.1 GeV Dampi.g Ri.g,a Booster capable of achi.vi.g energi.s up to 180 GeV,and a Colli.er operati.g at varyi.g energy modes(Z,W,H,and tt).The Li.ac and Dampi.g Ri.g are si.uated on the surface,whi.e the subterranean Booster and Colli.er are housed i. a 100 km ci.cumference underground tunnel,strategi.ally accommodati.g future expansi.n wi.h provi.i.ns for a potenti.l Super Proton Proton Colli.er(SPPC).The CEPC pri.ari.y serves as a Hi.gs *** i.s baseli.e desi.n wi.h synchrotron radi.ti.n(SR)power of 30 MW per beam,i. can achi.ve a lumi.osi.y of 5×10^(34)cm^(-2)s^(-1)per i.teracti.n poi.t(i.),resulti.g i. an i.tegrated lumi.osi.y of 13 ab^(-1)for two i.s over a decade,produci.g 2.6 mi.li.n Hi.gs *** the SR power to 50 MW per beam expands the CEPC's capabi.i.y to generate 4.3 mi.li.n Hi.gs bosons,faci.i.ati.g preci.e measurements of Hi.gs coupli.g at sub-percent levels,exceedi.g the preci.i.n expected from the HL-LHC by an order of *** Techni.al Desi.n Report(TDR)follows the Preli.i.ary Conceptual Desi.n Report(Pre-CDR,2015)and the Conceptual Desi.n Report(CDR,2018),comprehensi.ely detai.i.g the machi.e's layout,performance metri.s,physi.al desi.n and analysi.,techni.al systems desi.n,R&D and prototypi.g efforts,and associ.ted ci.i. engi.eeri.g ***,i. i.cludes a cost esti.ate and a preli.i.ary constructi.n ti.eli.e,establi.hi.g a framework for forthcomi.g engi.eeri.g desi.n phase and si.e selecti.n *** i. anti.i.ated to begi. around 2027-2028,pendi.g government approval,wi.h an esti.ated durati.n of 8 *** commencement of experi.ents and data collecti.n could potenti.lly be i.i.i.ted i. the mi.-2030s.

关键词： i.i.i.ted exceedi.g preci.e

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JUNO sensi.i.i.y on proton decay p→νK^(+)searches

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Chi.ese Physi.s C 2023年第11期47卷 7-22页

作者： Angel Abusleme Thomas Adam Shakeel Ahmad Ri.wan Ahmed Sebasti.no Ai.llo Muhammad Akram 安丰鹏安琪 Gi.seppe Androni.o Ni.olay Anfi.ov Vi.o Antonelli.Tati.na Antoshki.a Buri. Asavapi.hop João Pedro Athayde Marcondes de André Di.i.r Auguste Ni.i.a Balashov Wander Baldi.i.Andrea Barresi.Davi.e Basi.i.o Eri. Baussan Marco Bellato Antoni. Bergnoli.Thi.o Bi.kenfeld Sylvi. Bli. Davi. Blum Si.on Blyth Anastasi. Bolshakova Mathi.u Bongrand Clément Bordereau Domi.i.ue Breton Augusto Bri.atti.Ri.cardo Brugnera Ri.cardo Bruno Antoni. Budano Mari. Buscemi.Jose Busto i.ya Butorov Anatael Cabrera Barbara Cacci.ni.a 蔡浩蔡啸蔡严克蔡志岩 Ri.cardo Callegari.Antoni. Cammi.Agusti. Campeny 曹传亚曹国富曹俊 Rossella Caruso Cédri. 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 Chetveri.ov Davi.e Chi.sa Pi.tro Chi.enti.Artem Chukanov Gérard Claveri. Cati. Clementi.Barbara Clerbaux Selma Conforti.Di.Lorenzo Dani.le Corti.Flavi. Dal Corso Oli.i. Dalager Chri.tophe De La Tai.le 邓智邓子艳 Wi.fri.d Depneri.g Marco Di.z Xuefeng Di.g 丁雅韵 Bayu Di.gantara Sergey Dmi.ri.vsky Tadeas Dohnal Dmi.ry Dolzhi.ov Georgy Donchenko 董建蒙 Evgeny Doroshkevi.h Marcos Dracos Frédéri. Drui.lole 杜然杜书先 Stefano Dusi.i.Marti. Dvorak Ti.o Enqvi.t Hei.e Enzmann Andrea Fabbri.Ulri.e Fahrendholz 范东华樊磊方建方文兴 Marco Fargetta Dmi.ry Fedoseev Li.Cheng Feng 冯启春 Ri.hard Ford Améli. Fourni.r 甘浩男 Feng Gao Alberto Garfagni.i.Arseni. Gavri.ov Marco Gi.mmarchi.Agnese Gi.z Nunzi. Gi.di.e Maxi. Gonchar 龚光华宫辉 Yuri.Gornushki. Alexandre Göttel Marco Grassi.Chri.ti.n Grewi.g Vasi.y Gromov 顾旻皓谷肖飞古宇关梦云 Nunzi. Guardone Mari. Gul 郭聪郭竞渊郭万磊郭新恒郭宇航 Paul Hackspacher Caren Hagner 韩然 Yang Han Muhammad Sohai. Hassan 何苗何伟 Tobi.s Hei.z Patri.k Hellmuth 衡月昆 Rafael Herrera 贺远强侯少静 Yee Hsi.ng 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 Cédri. Huss Safeer Hussai. Ara i.anni.i.n Roberto i.ocrate Beatri.e Jelmi.i.Kuo-Lun Jen i.naci. Jeri. 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 Céci.e Jollet Jari.Joutsenvaara Si.i.hok Jungthawan Leoni.as Kalousi. Phi.i.p Ka Ponti.i.i. Uni.ersi.ad Católi.a de Chi.e SantiagoChile i.HC Universitéde StrasbourgCNRS/IN2P3F-67037 StrasbourgFrance Paki.tan i.sti.ute of Nuclear Sci.nce and Technology IslamabadPakistan i.FN Catani. and Di.arti.ento di.Fi.i.a e Astronomi. dell Uni.ersi.àdi.Catani. CataniaItaly East Chi.a Uni.ersi.y of Sci.nce and Technology ShanghaiChina Uni.ersi.y of Sci.nce and Technology of Chi.a HefeiChina Joi.t i.sti.ute for Nuclear Research DubnaRussia i.FN Sezi.ne di.Mi.ano and Di.arti.ento di.Fi.i.a dell Uni.ersi.àdi.Mi.ano MilanoItaly Department of Physi.s Faculty of ScienceChulalongkorn UniversityBangkokThailand i.CLab UniversitéParis-SaclayCNRS/IN2P391405 OrsayFrance Department of Physi.s and Earth Sci.nce University of Ferrara and INFN Sezione di FerraraFerraraItaly i.FN Mi.ano Bi.occa and Uni.ersi.y of Mi.ano Bi.occa MilanoItaly i.FN Sezi.ne di.Padova PadovaItaly i.i.Physi.ali.ches i.sti.ut B RWTH Aachen UniversityAachenGermany Eberhard Karls Uni.ersi.ät Tübi.gen Physikalisches InstitutTübingenGermany i.sti.ute of Hi.h Energy Physi.s BeijingChina SUBATECH Universitéde NantesIMT AtlantiqueCNRS-IN2P3NantesFrance Uni..Bordeaux CNRSLP2IUMR 5797F-33170 GradignanFrance Department of Physi.s National Taiwan UniversityTaipei Di.arti.ento di.Fi.i.a e Astronomi. dell’Uni.ersi.àdi.Padova and i.FN Sezi.ne di.Padova PadovaItaly Uni.ersi.y of Roma Tre and i.FN Sezi.ne Roma Tre RomaItaly Ai. Marsei.le Uni. CNRS/IN2P3CPPMMarseilleFrance Wuhan Uni.ersi.y WuhanChina i.FN Mi.ano Bi.occa and Poli.ecni.o of Mi.ano MilanoItaly Nati.nal Uni.ed Uni.ersi.y Miao-Li Dongguan Uni.ersi.y of Technology DongguanChina Tsi.ghua Uni.ersi.y BeijingChina i.sti.ute of Modern Physi.s Chinese Academy of SciencesLanzhouChina i.sti.ute of Physi.s National Yang Ming Chiao Tung UniversityHsinchu North Chi.a Electri. Power Uni.ersi.y BeijingChina Sun Yat-Sen Uni.ersi.y GuangzhouChina Bei.i.g i.sti.ute of Spacecraft Envi.onment Engi.eeri.g BeijingChina Uni.ersi.ade Estadual de Londri.a LondrinaBrazil i.FN Sez

The Ji.ngmen Underground Neutri.o Observatory(JUNO)i. a large li.ui. sci.ti.lator detector desi.ned to explore many topi.s i. fundamental *** thi. study,the potenti.l of searchi.g for proton decay i. the p→νK^(+)mode wi.h JUNO i. *** kaon and i.s decay parti.les feature a clear three-fold coi.ci.ence si.nature that results i. a hi.h effi.i.ncy for ***,the excellent energy resoluti.n of JUNO permi.s suppressi.n of the si.able background caused by other delayed *** on these advantages,the detecti.n effi.i.ncy for the proton decay vi. p→νK^(+)i. 36.9%±4.9%wi.h a background level of 0.2±0.05(syst)±0.2(stat)events after 10 years of data *** esti.ated sensi.i.i.y based on 200 kton-years of exposure i. 9.6×1033 years,whi.h i. competi.i.e wi.h the current best li.i.s on the proton li.eti.e i. thi. channel and complements the use of di.ferent detecti.n technologi.s.

关键词： proton decay grand uni.i.d theori.s JUNO li.ui. sci.ti.lator detector

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