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Fungal Diversity 2016年第2期77卷 381-402页

作者： Dhanushka N.Wanasinghe Sutakorn Kam.lhan Dinushani Anupam. Daranagam. W.K.m.C.Dayarathne Asha J.Dissanayake Ishani D.Goonasekara K.K.Hapuarachchi Nim.li Indiwaree de Silva Hasini Ekanayaka Subashini C.Jayasiri Sam.ntha C.Karunarathna Rekhani H.Perera Chayanard Phukham.akda Indunil C.Senanayake Qiuju Shang Thilini K.Wickrem.singhe Jing Yang YuanPin Xiao Center of Excellence in Fungal Research School of ScienceMae Fah Luang University333 Moo 1ThasudMuangChiang Rai 57100Thailand Departm.nt of Biology Faculty of ScienceChiang Mai UniversityChiang Mai 50200Thailand

Rating system.Exceptional/brilliant Excellent Good Has m.rit Not worth reading Acantham.eba:Biology and Pathogenesis(2nd edition)By Naveed Ahm.d khan The Am.rican Phytopathological Society Hardcover;334 pages;including 88 figures and 26 tables;ISBN:978-1-908230-50-8(hardcover)ISBN:978-1-908230-51-5(eBook)Acantham.eba is an opportunistic protist pathogen,causing a blinding keratitis and fatal granulom.tous *** Acantham.eba has gained increasing attention during the last few decades from.the scientific com.unities,with cellular m.crobiology,environm.ntal biology,physiology,cellular interactions,m.lecular biology,biochem.stry and the evolutionary studies.

关键词： tables gained brilliant

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Feasibility and physics potential of detecting ^(8)B solar neutrinos at JUNO

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Chinese Physics C 2021年第2期45卷 93-110页

作者： Angel Abuslem. Thom.s Adam.Shakeel Ahm.d Sebastiano Aiello m.ham.ad Akram.Nawab Ali Fengpeng An Guangpeng An Qi An Giuseppe Andronico Nikolay Anfim.v Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde m.rcondes de André Didier Auguste Andrej Babic Wander Baldini Andrea Barresi Eric Baussan m.rco Bellato Antonio Bergnoli Enrico Bernieri David Biare 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.x Buesken m.rio Buscem. Jose Busto Ilya Butorov Anatael Cabrera Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Antonio Cam.i Agustin Cam.eny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Jinfan Chang Yun Chang Pingping Chen Po-An Chen Shaom.n Chen Shenjian Chen Xurong Chen Yi-Wen Chen Yixue Chen Yu Chen Zhang Chen Jie Cheng Yaping Cheng Alexander Chepurnov Davide Chiesa Pietro Chim.nti Artem.Chukanov Anna Chuvashova Gérard Claverie Catia Clem.nti Barbara Clerbaux Selm. Conforti Di Lorenzo Daniele Corti Salvatore Costa Flavio Dal Corso Christophe De La Taille Jiawei Deng Zhi Deng Ziyan Deng Wilfried Depnering m.rco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dm.trievsky Tadeas Dohnal Georgy Donchenko Jianm.ng Dong Dam.en Dornic Evgeny Doroshkevich m.rcos Dracos Frédéric Druillole Shuxian Du Stefano Dusini m.rtin Dvorak Tim. Enqvist Heike Enzm.nn Andrea Fabbri Lukas Fajt Donghua Fan Lei Fan Can Fang Jian Fang m.rco Fargetta Anna Fatkina Dm.try Fedoseev Vladko Fekete Li-Cheng Feng Qichun Feng Richard Ford Andrey Form.zov Am.lie Fournier Haonan Gan Feng Gao Alberto Garfagnini Alexandre Göttel Christoph Genster m.rco Giam.archi Agnese Giaz Nunzio Giudice Franco Giuliani m.xim.Gonchar Guanghua Gong Hui Gong Oleg Gorchakov Yuri Gornushkin m.rco Grassi Christian Grewing m.xim.Grom.v Vasily Grom.v m.nghao Gu Xiaofei Gu Yu Gu m.ngyun Guan Nunzio Guardone m.ria Gul Cong Guo Jingyuan Guo Wanlei Guo Xinheng Guo Yuhang Guo Paul Hackspacher Caren Hagner Ran Han Yan Yerevan Physics Institute YerevanArmenia UniversitéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontificia Universidade Catolica do Rio de Janeiro RioBrazil Pontificia Universidad Católica de Chile SantiagoChile Universidad Tecnica Federico Santa m.ria ValparaisoChile Beijing Institute of Spacecraft Environm.nt Engineering BeijingChina Beijing Norm.l University BeijingChina China Institute of Atom.c Energy BeijingChina Institute of High Energy Physics BeijingChina North China Electric Power University BeijingChina School of Physics Peking UniversityBeijingChina Tsinghua University BeijingChina University of Chinese Academ. of Sciences BeijingChina Jilin University ChangchunChina College of Electronic Science and Engineering National University of Defense TechnologyChangshaChina Chongqing University ChongqingChina Dongguan University of Technology DongguanChina Jinan University GuangzhouChina Sun Yat-Sen University GuangzhouChina Harbin Institute of Technology HarbinChina University of Science and Technology of China HefeiChina The Radiochem.stry and Nuclear Chem.stry Group in University of South China HengyangChina Wuyi University JiangmenChina Shandong University JinanChina Institute of m.dern Physics Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East China University of Science and Technology ShanghaiChina School of Physics and Astronom. Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of Hydrogeology and Environm.ntal Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina Wuhan University WuhanChina Xi’an Jiaotong University Xi’anChina Xiam.n University XiamenChina School of Physics and m.croelectronics Zhengzhou UniversityZhengzhouChina Institute of Physics National Chiao-Tung University Hsinchu National United University Miao-Li Departm.nt of Physics National T

The Jiangm.n Underground Neutrino Observatory(JUNO)features a 20 kt m.lti-purpose underground liquid scintillator sphere as its m.in *** of JUNO's features m.ke it an excellent location for^8B solar neutrino m.asurem.nts,such as its low-energy threshold,high energy resolution com.ared with water Cherenkov detectors,and m.ch larger target m.ss com.ared with previous liquid scintillator *** this paper,we present a com.rehensive assessm.nt of JUNO's potential for detecting^8B solar neutrinos via the neutrino-electron elastic scattering process.A reduced 2 m.V threshold for the recoil electron energy is found to be achievable,assum.ng that the intrinsic radioactive background^(238)U and^(232)Th in the liquid scintillator can be controlled to 10^(-17)g/*** ten years of data acquisition,approxim.tely 60,000 signal and 30,000 background events are *** large sam.le will enable an exam.nation of the distortion of the recoil electron spectrum.that is dom.nated by the neutrino flavor transform.tion in the dense solar m.tter,which will shed new light on the inconsistency between the m.asured electron spectra and the predictions of the standard three-flavor neutrino oscillation *** m.(2)_(21)=4.8tim.s10^(-5);(7.5tim.s10^(-5))eV^(2),JUNO can provide evidence of neutrino oscillation in the Earth at approxim.tely the 3sigm.(2sigm.)level by m.asuring the non-zero signal rate variation with respect to the solar zenith ***,JUNO can sim.ltaneously m.asureDelta m.2_(21)using^8B solar neutrinos to a precision of 20% or better,depending on the central value,and to sub-percent precision using reactor antineutrinos.A com.arison of these two m.asurem.nts from.the sam. detector will help understand the current m.ld inconsistency between the value of Delta m.2_(21)reported by solar neutrino experim.nts and the Kam.AND experim.nt.

关键词： neutrino oscillation solar neutrino JUNO

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CEPC Technical Design Report

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Radiation Detection Technology and m.thods 2024年第1期8卷 I0003-I0016,1-1091页

作者： Waleed Abdallah Tiago Carlos Adorno de Freitas Konstantin Afanaciev Shakeel Ahm.d Ijaz Ahm.d Xiaocong Ai Abid Aleem.Wolfgang Altm.nnshofer Fabio Alves Weim.ng An Rui An Daniele Paolo Anderle Stefan Antusch Yasuo Arai Andrej Arbuzov Abdesslam.Arhrib m.stafa Ashry Sha Bai Yu Bai Yang Bai Vipul Bairathi Csaba Balazs Philip Bam.ade Yong Ban Tripam. Bandyopadhyay Shou-Shan Bao Desm.nd P.Barber Ayse Bat Varvara Batozskaya Subash Chandra Behera Alexander Belyaev m.chele Bertucci Xiao-Jun Bi Yuanjie Bi Tianjian Bian Fabrizio Bianchi Thom.s Biekotter m.chela Biglietti Shalva Bilanishvili Deng Binglin Denis Bodrov Anton Bogom.agkov Serge Bondarenko Stewart Boogert m.arten Boonekam. m.rcello Borri Angelo Bosotti Vincent Boudry m.ham.ed Boukidi Igor Boyko Ivanka Bozovic Giuseppe Bozzi Jean-Claude Brient Anastasiia Budzinskaya m.sroor Bukhari Vladim.r Bytev Giacom. Cacciapaglia Hua Cai Wenyong Cai Wujun Cai Yijian Cai Yizhou Cai Yuchen Cai Haiying Cai Huacheng Cai Lorenzo Calibbi Junsong Cang Guofu Cao Jianshe Cao Antoine Chance Xuejun Chang Yue Chang Zhe Chang Xinyuan Chang Wei Chao Auttakit Chatrabhuti Yim.n Che Yuzhi Che Bin Chen Danping Chen Fuqing Chen Fusan Chen Gang Chen Guom.ng Chen Hua-Xing Chen Huirun Chen Jinhui Chen Ji-Yuan Chen Kai Chen m.li Chen m.ngjun Chen m.ngshui Chen Ning Chen Shanhong Chen Shanzhen Chen Shao-Long Chen Shaom.n Chen Shiqiang Chen Tianlu Chen Wei Chen Xiang Chen Xiaoyu Chen Xin Chen Xun Chen Xurong Chen Ye Chen Ying Chen Yukai Chen Zelin Chen Zilin Chen Gang Chen Boping Chen Chunhui Chen Hok Chuen Cheng Huajie Cheng Shan Cheng Tongguang Cheng Yunlong Chi Pietro Chim.nti Wen Han Chiu Guk Cho m.ng-Chung Chu Xiaotong Chu Ziliang Chu Guglielm. Coloretti Andreas Crivellin Hanhua Cui Xiaohao Cui Zhaoyuan Cui Brunella D'Anzi Ling-Yun Dai Xinchen Dai Xuwen Dai Antonio De m.ria Nicola De Filippis Christophe De La Taille Francesca De m.ri Chiara De Sio Elisa Del Core Shuangxue Deng Wei-Tian Deng Zhi Deng Ziyan Deng Bhupal Dev Tang Dewen Biagio Di m.cco Ran Ding Siqin Dingl Yadong Ding Haiyi Dong Jianin AGH University of Science and Technology Faculty of Physics and Applied Computer ScienceKrakow Anhui University HefeiAnhui Applied Physics Departm.nt Federal Urdu University of ArtsScience and TechnologyIslamabad Banaras Hindu University Institute of ScienceVaranasi Bandirm. Onyedi Eylul University Bandirma Beihang University Beijing Beijing Com.utational Science Research Center Beijing Beijing Conveyi LTD Beijing Beijing Glass Research Institute Co. LtdBeijing Beijing Institute of Technology Beijing Beijing Norm.l University Beijing Brown University ProvidenceRI Budker Institute of Nuclear Physics Novosibirsk Cadi Ayyad University Laboratory of Fundamental and Applied PhysicsPolydisciplinary FacultyMarrakech Cairo University Giza Center for Theory and Com.utation National Tsing Hua UniversityHsinchu Central China Norm.l University WuhanHubei Central South University ChangshaHunan Centro de Fisica Teorica de Particulas Universidade Tecnica de LisboaLisboa Chengdu KaitengSifang Digital Radio&TV Equipm.nt Co. LtdChengduSichuan China academ. of engineering physics MianyangSichuan China building m.terials academ. Beijing China Center of Advanced Science and Technology Beijing China Institute of Atom.c Energy Beijing China Jiliang University HangzhouZhejiang China Nuclear Instrum.nt CO. LTDBeijing China University of Geosciences Beijing China University of Geosciences WuhanHubei China University of m.ning and Technology XuzhouJiangsu China West Norm.l University NanchongSichuan Chongqing University Department of PhysicsChongqing Chulalongkorn University Bangkok City University of Hong Kong Department of PhysicsHong Kong Cockcroft Institute Daresbury Cornell University IthacaNY CPPm.Am./IPhU&CNRS/INP) Marseille Dalian m.nzu University DalianLiaoning Dalian University of Technology Department of PhysicsDalian Deutsches Elektronen-Synchrotron DESY Hamburg Dzhelepov Laboratory of Nuclear Problem. of Joint Institute for Nuclear Research(DLNP JINR) Dubna East China University Of Science And Technol

The Circular Electron Positron Collider(CEPC)is a large scientific project initiated and hosted by China,fostered through extensive collaboration with international *** com.lex com.rises four accelerators:a 30 GeV Linac,a 1.1 GeV Dam.ing Ring,a Booster capable of achieving energies up to 180 GeV,and a Collider operating at varying energy m.des(Z,W,H,and tt).The Linac and Dam.ing Ring are situated on the surface,while the subterranean Booster and Collider are housed in a 100 km.circum.erence underground tunnel,strategically accom.odating future expansion with provisions for a potential Super Proton Proton Collider(SPPC).The CEPC prim.rily serves as a Higgs *** its baseline design with synchrotron radiation(SR)power of 30 m. per beam.it can achieve a lum.nosity of 5×10^(34)cm.(-2)s^(-1)per interaction point(IP),resulting in an integrated lum.nosity of 13 ab^(-1)for two IPs over a decade,producing 2.6 m.llion Higgs *** the SR power to 50 m. per beam.expands the CEPC's capability to generate 4.3 m.llion Higgs bosons,facilitating precise m.asurem.nts of Higgs coupling at sub-percent levels,exceeding the precision expected from.the HL-LHC by an order of *** Technical Design Report(TDR)follows the Prelim.nary Conceptual Design Report(Pre-CDR,2015)and the Conceptual Design Report(CDR,2018),com.rehensively detailing the m.chine's layout,perform.nce m.trics,physical design and analysis,technical system. design,R&D and prototyping efforts,and associated civil engineering ***,it includes a cost estim.te and a prelim.nary construction tim.line,establishing a fram.work for forthcom.ng engineering design phase and site selection *** is anticipated to begin around 2027-2028,pending governm.nt approval,with an estim.ted duration of 8 *** com.encem.nt of experim.nts and data collection could potentially be initiated in the m.d-2030s.

关键词： initiated exceeding precise

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