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Dev.lopment of X-band accelerating structures for high gradients

Chinese Physics C 2012年第7期36卷 639-647页

作者： S. Bini v. chimenti A. Marcelli L. Palumbo B. Spataro v. A. Dolgashev.S. Tantawi A. D. Yeremian Y. Higashi M. G. Grimaldi L. Romano F. Ruffino R. Parodi INFN-LNF Via E. Fermi 40 00044 Frascati (RM) Italy Univ.rsity of Rome Sapienza Dipartimento di EnergeticaVia A. Scarpa 14 00185 Rome Italy SLAC National Accelerator Laboratory 2575 Sand Hill Road Menlo Park CA 94025 USA KEK 1-1 Oho Tsukuba Ibaraki 305 Japan Univ.rsity of Catania Dipartimento di Fisica e Astronomia & MATIS-IMM-CNRVia S. Sofia 64 95123 Catania Italy INFN-Genov. Via Dodecaneso 33 16146 Genova Italy

Short copper standing wav. （SW） structures operating at an X-band frequency hav. been recently designed and manufactured at the Laboratori Nazionali di Frascati of the Istituto Nazionale di Fisica Nucleare （INFN） using the v.cuum brazing technique. High power tests of the structures hav. been performed at the SLAC National Accelerator Laboratory. In this manuscript we report the results of these tests and the activ.ty in progress to enhance the high gradient performance of the next generation of structures, particularly the technological characterization of high performance coatings obtained v.a molybdenum sputtering.

关键词： high-gradients soft X-ray FEL RF cav.ties for particle accelerators RF sputtering

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Sub-percent precision measurement of neutrino oscillation parameters with JUNO

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Chinese Physics C 2022年第12期46卷 28-49页

作者： Angel Abusleme Thomas Adam Shakeel Ahmad Rizwan Ahmed Sebastiano Aiello Muhammad Akram Abid Aleem 安丰鹏安琪 Giuseppe Andronico Nikolay Anfimov.v.to Antonelli Tatiana Antoshkina Burin Asav.pibhop João Pedro Athayde Marcondes de André Didier Auguste 白伟东 Nikita Balashov.Wander Baldini Andrea Barresi Dav.de Basilico Eric Baussan Marco Bellato Antonio Bergnoli Thilo Birkenfeld Sylv.e Blin Dav.d Blum Simon Blyth Anastasia Bolshakov. Mathieu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Jose Busto Ilya Butorov.Anatael Cabrera Barbara Caccianiga 蔡浩蔡啸蔡严克蔡志岩 Riccardo Callegari Antonio Cammi Agustin Campeny 曹传亚曹国富曹俊 Rossella Caruso Cédric Cerna Chi Chan 常劲帆 Yun Chang 陈国明陈平平 Po-An Chen 陈少敏 Xurong Chen 陈义学陈羽陈志源陈梓康程捷程雅苹 Yu Chin Cheng Alexey Chetv.rikov.Dav.de Chiesa Pietro chimenti Artem Chukanov.Gérard Clav.rie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Flav.o Dal Corso Oliv.a Dalager Christophe De La Taille 邓智邓子艳 Wilfried Depnering Marco Diaz Xuefeng Ding 丁雅韵 Bayu Dirgantara Sergey Dmitriev.ky Tadeas Dohnal Dmitry Dolzhikov.Georgy Donchenko 董建蒙 Ev.eny Doroshkev.ch Marcos Dracos Frédéric Druillole 杜然杜书先 Stefano Dusini Martin Dv.rak Timo Enqv.st Heike Enzmann Andrea Fabbri Donghua Fan 樊磊方建方文兴 Marco Fargetta Dmitry Fedoseev.费政勇 Li-Cheng Feng 冯启春 Richard Ford Amélie Fournier 甘浩男高峰 Alberto Garfagnini Arsenii Gav.ikov.Marco Giammarchi Nunzio Giudice Maxim Gonchar 龚光华宫辉 Yuri Gornushkin Alexandre Göttel Marco Grassi v.sily Gromov.顾旻皓谷肖飞古宇关梦云管宇铎 Nunzio Guardone 郭聪郭竞渊郭万磊 Xinheng Guo 郭宇航 Paul Hackspacher Caren Hagner 韩然 Yang Han 何苗 Wei He Tobias Heinz Patrick Hellmuth 衡月昆 Rafael Herrera 贺远强侯少静 Yee Hsiung Bei-Zhen Hu 胡航 Jianrun Hu 胡俊胡守扬胡涛胡宇翔胡焯钧黄桂鸿黄翰雄黄凯旋黄文昊 Xin Huang 黄性涛黄永波惠加琪霍雷霍文驹 Cédric Huss Safeer Hussain Ara Ioannisian Roberto Isocrate Beatrice Jelmini Ignacio Jeria 季筱璐贾慧慧贾俊基蹇司玉蒋荻蒋炜江晓山荆小平 Cécile Jollet Jari Joutsenv.ara Leonidas Kalousis Philipp Kampmann 康丽 Rebin Karaparambil Narine Kazarian Amina Khatun Yerev.n Physics Institute YerevanArmenia Univ.rsiéLibre de Bruxelles BrusselsBelgium Univ.rsidade Estadual de Londrina LondrinaBrazil Pontificia Univ.rsidade Catolica do Rio de Janeiro Rio de JaneiroBrazil Pontificia Univ.rsidad Católica de Chile SantiagoChile Univ.rsidad Tecnica Federico Santa Maria ValparaisoChile Beijing Institute of Spacecraft Env.ronment Engineering BeijingChina Beijing Normal Univ.rsity BeijingChina China Institute of Atomic Energy BeijingChina Institute of High Energy Physics BeijingChina North China Electric Power Univ.rsity BeijingChina School of Physics Peking UniversityBeijingChina Tsinghua Univ.rsity BeijingChina Univ.rsity of Chinese Academy of Sciences BeijingChina Jilin Univ.rsity ChangchunChina College of Electronic Science and Engineering National University of Defense TechnologyChangshaChina Chongqing Univ.rsity ChongqingChina Dongguan Univ.rsity of Technology DongguanChina Jinan Univ.rsity GuangzhouChina Sun Yat-Sen Univ.rsity GuangzhouChina Harbin Institute of Technology HarbinChina Univ.rsity of Science and Technology of China HefeiChina The Radiochemistry and Nuclear Chemistry Group in Univ.rsity of South China HengyangChina Wuyi Univ.rsity JiangmenChina Shandong Univ.rsity JinanChinaand Key Laboratory of Particle Physics and Particle Irradiation of Ministry of EducationShandong UniversityQingdaoChina Institute of Modern Physics Chinese Academy of SciencesLanzhouChina Nanjing Univ.rsity NanjingChina Guangxi Univ.rsity NanningChina East China Univ.rsity of Science and Technology ShanghaiChina School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of Hydrogeology and Env.ronmental Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai Univ.rsity TianjinChina Wuhan Univ.rsity WuhanChina Xi'an Jiaotong Univ.rsity Xi'anChina Xiamen Univ.rsity XiamenChina School of Physics and Microelectronics Zhengzhou UniversityZhengzhou

JUNO is a multi-purpose neutrino observ.tory under construction in the south of *** publication presents new sensitiv.ty estimates for the measurement of the △m_(31)^(2),△m_(21)^(2),sin^(2)θ_(12),and sin^(2)θ_(13) oscillation parameters using reactor antineutrinos,which is one of the primary physics goals of the *** sensitiv.ties are obtained using the best knowledge av.ilable to date on the location and ov.rburden of the experimental site,the nuclear reactors in the surrounding area and beyond,the detector response uncertainties,and the reactor antineutrino spectral shape constraints expected from the TAO satellite *** is found that the △m_(21)^(2) and sin^(2)θ_(12) oscillation parameters will be determined to 0.5%precision or better in six years of data *** the same period,the △m_(31)^(2) parameter will be determined to about 0.2%precision for each mass ordering *** new precision represents approximately an order of magnitude improv.ment ov.r existing constraints for these three parameters.

关键词： neutrino oscillation reactor antineutrino precision measurement JUNO

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JUNO sensitiv.ty on proton decay p→νK^(+)searches

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Chinese Physics C 2023年第11期47卷 7-22页

作者： Angel Abusleme Thomas Adam Shakeel Ahmad Rizwan Ahmed Sebastiano Aiello Muhammad Akram 安丰鹏安琪 Giuseppe Andronico Nikolay Anfimov.v.to Antonelli Tatiana Antoshkina Burin Asav.pibhop João Pedro Athayde Marcondes de André Didier Auguste Nikita Balashov.Wander Baldini Andrea Barresi Dav.de Basilico Eric Baussan Marco Bellato Antonio Bergnoli Thilo Birkenfeld Sylv.e Blin Dav.d Blum Simon Blyth Anastasia Bolshakov. Mathieu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Mario Buscemi Jose Busto Ilya Butorov.Anatael Cabrera Barbara Caccianiga 蔡浩蔡啸蔡严克蔡志岩 Riccardo Callegari Antonio Cammi Agustin Campeny 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 Chetv.rikov.Dav.de Chiesa Pietro chimenti Artem Chukanov.Gérard Clav.rie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Flav.o Dal Corso Oliv.a Dalager Christophe De La Taille 邓智邓子艳 Wilfried Depnering Marco Diaz Xuefeng Ding 丁雅韵 Bayu Dirgantara Sergey Dmitriev.ky Tadeas Dohnal Dmitry Dolzhikov.Georgy Donchenko 董建蒙 Ev.eny Doroshkev.ch Marcos Dracos Frédéric Druillole 杜然杜书先 Stefano Dusini Martin Dv.rak Timo Enqv.st Heike Enzmann Andrea Fabbri Ulrike Fahrendholz 范东华樊磊方建方文兴 Marco Fargetta Dmitry Fedoseev.Li-Cheng Feng 冯启春 Richard Ford Amélie Fournier 甘浩男 Feng Gao Alberto Garfagnini Arsenii Gav.ikov.Marco Giammarchi Agnese Giaz Nunzio Giudice Maxim Gonchar 龚光华宫辉 Yuri Gornushkin Alexandre Göttel Marco Grassi Christian Grewing v.sily Gromov.顾旻皓谷肖飞古宇关梦云 Nunzio Guardone Maria Gul 郭聪郭竞渊郭万磊郭新恒郭宇航 Paul Hackspacher Caren Hagner 韩然 Yang Han Muhammad Sohaib Hassan 何苗何伟 Tobias Heinz Patrick Hellmuth 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 Jelmini 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 Joutsenv.ara Sirichok Jungthawan Leonidas Kalousis Philipp Ka Pontificia Univ.rsidad Católica de Chile SantiagoChile IPHC Universitéde StrasbourgCNRS/IN2P3F-67037 StrasbourgFrance Pakistan Institute of Nuclear Science and Technology IslamabadPakistan INFN Catania and Dipartimento di Fisica e Astronomia dell Univ.rsitàdi Catania CataniaItaly East China Univ.rsity of Science and Technology ShanghaiChina Univ.rsity of Science and Technology of China HefeiChina Joint Institute for Nuclear Research DubnaRussia INFN Sezione di Milano and Dipartimento di Fisica dell Univ.rsitàdi Milano MilanoItaly Department of Physics Faculty of ScienceChulalongkorn UniversityBangkokThailand IJCLab UniversitéParis-SaclayCNRS/IN2P391405 OrsayFrance Department of Physics and Earth Science University of Ferrara and INFN Sezione di FerraraFerraraItaly INFN Milano Bicocca and Univ.rsity of Milano Bicocca MilanoItaly INFN Sezione di Padov. PadovaItaly III.Physikalisches Institut B RWTH Aachen UniversityAachenGermany Eberhard Karls Univ.rsität Tübingen Physikalisches InstitutTübingenGermany Institute of High Energy Physics BeijingChina SUBATECH Universitéde NantesIMT AtlantiqueCNRS-IN2P3NantesFrance Univ.Bordeaux CNRSLP2IUMR 5797F-33170 GradignanFrance Department of Physics National Taiwan UniversityTaipei Dipartimento di Fisica e Astronomia dell’Univ.rsitàdi Padov. and INFN Sezione di Padov. PadovaItaly Univ.rsity of Roma Tre and INFN Sezione Roma Tre RomaItaly Aix Marseille Univ CNRS/IN2P3CPPMMarseilleFrance Wuhan Univ.rsity WuhanChina INFN Milano Bicocca and Politecnico of Milano MilanoItaly National United Univ.rsity Miao-Li Dongguan Univ.rsity of Technology DongguanChina Tsinghua Univ.rsity BeijingChina Institute of Modern Physics Chinese Academy of SciencesLanzhouChina Institute of Physics National Yang Ming Chiao Tung UniversityHsinchu North China Electric Power Univ.rsity BeijingChina Sun Yat-Sen Univ.rsity GuangzhouChina Beijing Institute of Spacecraft Env.ronment Engineering BeijingChina Univ.rsidade Estadual de Londrina LondrinaBrazil INFN Sez

The Jiangmen Underground Neutrino Observ.tory(JUNO)is a large liquid scintillator detector designed to explore many topics in fundamental *** this study,the potential of searching for proton decay in the p→νK^(+)mode 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 permits suppression of the sizable background caused by other delayed *** on these adv.ntages,the detection efficiency for the proton decay v.a p→νK^(+)is 36.9%±4.9%with a background lev.l of 0.2±0.05(syst)±0.2(stat)ev.nts after 10 years of data *** estimated sensitiv.ty based on 200 kton-years of exposure is 9.6×1033 years,which is competitiv. with the current best limits on the proton lifetime in this channel and complements the use of different detection technologies.

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

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