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Dietary Coleus amboinicus Lour. decreases ruminal methanogenesis and biohydrogenation, and improves meat quality and fatty acid composition in longissimus thoracis muscle of lambs.

畜牧与生物技术杂志(英文版) 2023年第1期

作者： Haihao Huang Dorota Lechniak malgorzata Szumacher-Strabel Amlan Kumar Patra Martyna Koz?owska Pawel Kolodziejski Min Gao Sylwester ?lusarczyk Daniel Petri? Adam Cieslak

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欧洲儿科胃肠病学、肝病学和营养协会儿童及青少年炎症性肠病诊断的改良波尔图标准(2014年版)

畜牧与生物技术杂志(英文版) 2022年第3期

作者： Yulianri Rizki Yanza malgorzata Szumacher-Strabel Dorota Lechniak Sylwester ?lusarczyk Pawel Kolodziejski Amlan Kumar Patra Zora Váradyová Dariusz Lisiak Mina Vazirigohar Adam Cieslak

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中华儿科杂志 2016年第10期54卷 728-732页

作者： Arie Levine Sibylle Koletzko Dan Turner Johanna C.Escher Salvatore Cucchiara Lissy de Ridder Kaija-Leena Kolho Gabor Veres Richard K.Russell Anders Paerregaard Stephan Buderus Mary-Louise C.Greer Jorge A.Dias Gigi Veereman-Wauters Paolo Lionetti malgorzata Sladek Javier Martin de Carpi Annamaria Staiano Frank M.Ruemmele David C.Wilson 罗优优陈洁 Pediatric Gastroenterology and Nutrition Unit Wolfson Medical CenterSackler School of MedicineTel-Aviv University the Dr von Hauner Children's Hospital Ludwig Maximilians University the Pediatric Gastroenterology Unit Shaare Zedek Medical CenterThe Hebrew University of Jerusalem the Pediatric Gastroenterology Department of PediatricsErasmus MC-Sophia Children's Hospital 5. the Pediatric Gastroenterology and Liver UnitSapienza University of Rome 6. the Children's HospitalUniversity of Helsinki 7. the Semmelweis University 8. the Department of Paediatric Gastroenterology and NutritionYorkhill Children's Hospital 9. the Department of PaediatricsHvidovre University Hospital 10. the St.Marien-HospitalDepartment of Pediatrics 11. the Department of Diagnostic ImagingThe Hospital for Sick Childrenthe Department of Medical ImagingUniversity of Toronto 12. the Hospital S.Joao 13. the-Pediatric Gastroenterology and Nutrition 14. the Departement NeurofarbaUniversity of FlorenceMeyer Children Hospital 15. the Department of PediatricsGastroenterology and NutritionJagiellonian University Medical College 16. the Department of Pediatric GastroenterologyHepatology and NutritionHospital Sant Joan de De'u 17. the Department of Translational Medical SciencesSection of PediatricsUniversit

炎症性肠病(IBD)包括克罗恩病(CD)、溃疡性结肠炎(UC)和未分型IBD(IBDU)。IBD的确切诊断需综合病史、体检、实验室检查、内镜以及影像学的检查,并严格排除肠道感染、过敏性疾病或原发性免疫缺陷病(PID)。近年对儿童期起病的IBD(PIBD)的... 详细信息

炎症性肠病(IBD)包括克罗恩病(CD)、溃疡性结肠炎(UC)和未分型IBD(IBDU)。IBD的确切诊断需综合病史、体检、实验室检查、内镜以及影像学的检查,并严格排除肠道感染、过敏性疾病或原发性免疫缺陷病(PID)。近年对儿童期起病的IBD(PIBD)的研究高度提示3种PIBD的亚型均存在不典型的表型。本标准对2005年波尔图标准进行改良,利用循证方法,整合最新证据,包括诊断方法、以巴黎分型为基础的PIBD亚型的定义以及诊断误区,为新一代的PIBD提供优质的个体化管理以及可靠的诊断、评估和预后。

关键词：体检实验室检查内镜

Reduced cardiac output is associated with decreased mitochondrial efficiency in the non-ischemic ventricular wall of the acute myocardial-infarcted dog

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Cell Research 2006年第03期16卷 297-305页

作者： Zakaria A Almsherqi malgorzata B Slocinska Yuru Deng Department of Physiology,National University of Singapore,Block MD9,2 Medical Drive,Singapore 117597,Singapore Craig S McLachlan Peter Mossop Department of Medical Imaging,St Vincents Hospital,Melbourne,Fitzroy VIC 3065,Australia Francis E Sluse Rachel Navet Laboratory of Bioenergetics,Institute of Chemistry B6,University of Liége,Start Tilman,B-4000 Liége,Belgium Nikolai Kocherginsky Iouri Kostetski Biophysics Laboratory,Division of Bioengineering,National University of Singapore,Singapore 117576,Singapore Dong-Yun Shi Shan-Lin Liu Department of Biochemistry,Shanghai Medical College of Fudan University,Free Radical Regulation Research Center of Fudan University,Shanghai 200032,China DepartmentofPhysiology NationalUniversityofSingaporeBlockMD92MedicalDriveSingapore117597Singapore DepartmentofMedicallmaging StVincentsHospitalMelbourneFitzroyVIC3065Australia

Cardiogenic shock is the leading cause of death among patients hospitalized with acute myocardial infarction (MI).Understanding the mechanisms for acute pump failure is therefore *** aim of this study is to examine in anacute MI dog model whether mitochondrial bio-energetic function within non-ischemic wall regions are associated withpump *** MI was produced in dogs via ligation of left anterior descending (LAD) coronary artery,thatresulted in an infract size of about 30% of the left ventricular *** of hemodynamic status,mitochondrialfunction,free radical production and mitochondrial uncoupling protein 3 (UCP3) expression were determined over 24h *** measurements revealed a>50% reduction in cardiac output at 24 h post infarction when com-pared to *** samples were obtained from the posterior non-ischemic wall during acute ***/Oratios for isolated mitochondria from non-ischemic myocardium at 6 h and 24 h were decreased when compared to theADP/O ratios within the same samples with and without palmitic acid (PA).GTP inhibition of (PA)-stimulated state 4respiration in isolated mitochondria from the non-ischemic wall increased by 7% and 33% at 6 h and 24 h post-infarctionrespectively when compared to sham and pre-infarction *** would suggest that the mitochondria are uncoupledand this is supported by an associated increase in UCP3 expression observed on western blots from these same *** samples from the coronary sinus measured by electron paramagnetic resonance (EPR) methods showedan increase in reactive oxygen species (ROS) over baseline at 6 h and 24 h *** conclusion,mitochondrialbio-energetic ADP/O ratios as a result of acute infarction are abnormal within the non-ischemic *** ap-pear to be energetically uncoupled and this is associated with declining pump *** radical production may beassociated with the induction of uncoupling prot

关键词： mitochondria uncoupling proteins bioenergetics infarction cardiogenic shock non-ischemic ventricle

Accretion in strong field gravity with eXTP

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Science China(Physics,Mechanics & Astronomy) 2019年第2期62卷 45-73页

作者： Alessandra De Rosa Phil Uttley LiJun Gou Yuan Liu Cosimo Bambi Didier Barret Tomaso Belloni Emanuele Berti Stefano Bianchi Ilaria Caiazzo Piergiorgio Casella Marco Feroci Valeria Ferrari Leonardo Gualtieri Jeremy Heyl Adam Ingram Vladimir Karas FangJun Lu Bin Luo Giorgio Matt Sara Motta Joseph Neilsen Paolo Pani Andrea Santangelo XinWen Shu JunFeng Wang Jian-Min Wang YongQuan Xue YuPeng Xu WeiMin Yuan YeFei Yuan Shuang-Nan Zhang Shu Zhang Ivan Agudo Lorenzo Amati Nils Andersson Cristina Baglio Pavel Bakala Altan Baykal Sudip Bhattacharyya Ignazio Bombaci NiccolóBucciantini Fiamma Capitanio Riccardo Ciolfi Wei K.Cui Filippo D'Ammando Thomas Dauser Melania Del Santo Barbara De Marco Tiziana Di Salvo Chris Done Michal Dovciak Andrew C.Fabian Maurizio Falanga Angelo Francesco Gambino Bruce Gendre Victoria Grinberg Alexander Heger Jeroen Homan Rosario Iaria JiaChen Jiang ChiChuan Jin Elmar Koerding Manu Linares Zhu Liu Thomas J.Maccarone Julien Malzac Antonios Manousakis Frédéric Marin Andea Marinucci Missagh Mehdipour Mariano Méndez Simone Migliari Cole Miller Giovanni Miniutti Emanuele Nardini Paul T.O'Brien Julian P.Osborne Pierre Olivier Petrucci Andrea Possenti Alessandro Riggio Jerome Rodriguez Andrea Sanna LiJing Shao Malgosia sobolewska Eva Sramkova Abigail L.Stevens Holger Stiele Giulia Stratta Zdenek Stuchlik Jiri Svoboda Fabrizio Tamburini Thomas M.Tauris Francesco Tombesi Gabriel Torok Martin Urbanec Frederic Vincent QingWen Wu Feng Yuan Jean J.M.in't Zand Andrzej A.Zdziarski XinLin Zhou INAF-Istituto di Astrofisica e Planetologie Spaziali Via Fosso del Cavaliere Anton Pannekoek Institute for Astronomy University of Amsterdam National Astronomical Observatories Chinese Academy of Science Institute of High Energy Physics Chinese Academy of Science Center for Field Theory and Particle Physics and Department of Physics Fudan University IRAP Universitéde ToulouseCNRSUPSCNES INAF-Osservatorio Astronomico di Brera Department of Physics and Astronomy The University of MississippiUniversity Dipartimento di Matematica e Fisica Universitàdegli studi Roma Tre University of British Columbia INAF-Osservatorio Astronomico di Roma INFN-Roma 2 c/o Dipartimento di Fisica II Universit?di Roma"Tor Vergata" Dipartimento di Fisica Universitàdegli Studi di Roma"La Sapienza"&Sezione INFN Roma1 Department of Physics University of OxfordClarendon Laboratory Astronomical Institute Academy of Sciences School of Astronomy and Space Science Nanjing University MIT Kavli Institute for Astrophysics and Space Research Institut für Astronomie und Astrophysik Eberhard Karls Universität Department of Physics Anhui Normal University Department of Astronomy and Institute of Theoretical Physics and Astrophysics Xiamen University CAS Key Laboratory for Research in Galaxies and Cosmology Department of AstronomyUniversity of Science and Technology of China Instituto de Astrofísica de Andalucia(CSIC) Glorieta de la Astronomía s/n INAF-Istituto di Astrofisica Spaziale e Fisica cosmica di Bologna Mathematical Sciences and STAG Research Centre University of Southampton New York University Abu Dhabi Institute of Physics and Research Centre for Computational Physics and Data Processing Faculty of Philosophy&ScienceSilesian University in OpavaíBezru?ovo nám. Department of Physics Middle East Technical University Department of Astronomy and Astrophysics Tata Institute of Fundamental Research Dipartimento di Fisica Universit?di Pisa&INFN INAF-Osservatorio Astrofisico di Arcetri INAF-Osservatorio Astronomico di Padova INFN-TIFPA Trento Ins

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry(eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced "spectral-timing-polarimetry" techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process.

关键词： X-ray black holes physics accretion

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转基因食物：不确定性，信任与责任

洛阳师范学院学报 2017年第7期36卷 9-15,18页

作者：鲁西亚·马蒂内利玛戈扎塔·卡巴兹文森佐·帕沃尼别应龙(译) 李宏伟(校) 意大利特兰托市缪斯-特伦托科学博物馆波兰厄索夫大学基础科学与应用生物技术研究所西班牙马德里公共产品与政策研究所重庆科技学院人事处重庆401331 华中师范大学马克思主义学院湖北武汉430079

那些正式通过的与转基因食物有关的规定,被期待能够给予那些一直认为被批准售卖的产品是安全的消费者以安全保障。大多数科学家一致认同转基因农作物的安全性。然而,对健康风险作出的相互矛盾的报道,与出现在科学文献中的那些转基因农... 详细信息

那些正式通过的与转基因食物有关的规定,被期待能够给予那些一直认为被批准售卖的产品是安全的消费者以安全保障。大多数科学家一致认同转基因农作物的安全性。然而,对健康风险作出的相互矛盾的报道,与出现在科学文献中的那些转基因农作物联系在了一起。这样一来,人们都赞同这样一种结论,即风险评估也具有科学不确定性,并且,这种科学不确定性需要的不仅仅是科学知识。要建立并解决科学内在的不确定性与来自普通消费者所要求的安全感之间的争论,科学共同体连同业界、政策制定者一起,应该创建一个开放的、具有自我反思性的、兼顾了多个学科背景的技术评估程序,并且,这个技术评估是,经由不同社会参与者们所构成的社会知识再综合形成的科学知识而做出的技术评估。尤其是参与其中的科学共同体,还应该坦承转基因农作物的一些不确定性和风险性的存在,并保证有关转基因农作物的研究不受那些大公司地位的左右。从某种程度上来说,一些研究机构所委任完成的科学知识的增长应该促使把这些研究机构本身当作一个新的讨论事情的聚集点,并使民众能获得有建立民主管理的可能性的必要工具,使他们能够通过生物学创新,在现在和未来两者间作出选择,并能够成为知识社会中的积极参与者。

关键词：转基因食物公众参与风险评估安全性科学不确定性社会信任与社会责任

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森林郑州中心

城市环境设计 2023年第2期 206-209页

作者：张堇盈王典唐晓棠宋和贞 Andrew Irvin 贾城杨秉鑫杨佩琛 malgorzata Mutkowska Bernardo Taliani 李秋橙 Larade Pedro 陈相宇马瑞君陈洋扬苏禹竹张妍顾嘉诚 Erin Chen Lisa Chen 杨新越谢博宇周原仰郑丽丽辛海鸥洪明月

中原地区是华夏文明的摇篮。6世纪末,位于此地的郑州古城逐渐成为重要城市之一。如今的郑州快速崛起,成为河南省的政治与经济中心,不懈地试图在未来图景中重塑昔日形象。由如恩设计的郑州中心大楼位于城市一处待开发区域。在这座城市中...

中原地区是华夏文明的摇篮。6世纪末,位于此地的郑州古城逐渐成为重要城市之一。如今的郑州快速崛起,成为河南省的政治与经济中心,不懈地试图在未来图景中重塑昔日形象。由如恩设计的郑州中心大楼位于城市一处待开发区域。在这座城市中,文化遗产与现代化发展之间充斥着各样的矛盾。郑州的历史古迹,如城墙和要塞塔楼,其建造形式和材料与这片土地密切相关。而如今的郑州规划了新的城市中心,并用大片的玻璃塔楼群向天空示意,

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Identification of new genetic risk factors for prostate cancer

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Asian Journal of Andrology 2009年第1期11卷 49-55页

作者： Michelle Guy Zsofia Kote-Jarai Graham G. Giles Ali Amin Al Olama Sarah K. Jugurnauth Shani Mulholland Daniel A. Leongamomlert Stephen M. Edwards Jonathan Morrison Helen I. Field Melissa C. Southey Gianluca Severi Jenny L. Donovan Freddie C. Hamdy David R Dearnaley Kenneth R. Muir Charmaine Smith Melisa Bagnato Audrey T. Ardern-Jones Amanda L. Hall Lynne T. O＇Brien Beatrice N. Gehr-Swain Rosemary A. Wilkinson Angela Cox Sarah Lewis Paul M. Brown Sameer G. Jhavar malgorzata Tymrakiewicz Artitaya Lophatananon Sarah L. Bryant The UK Genetic Prostate Cancer Study Collaborators British Association of Urological Surgeons＇ Section of Oncology and The UK ProtecT Study Collaborators Alan Horwich Robert A. Huddart Vincent S. Khoo Christopher C. Parker Christopher J. Woodhouse Alan Thompson Tim Christmas Chris Ogden Cyril Fisher Charles Jameson Colin S. Cooper Dallas R. English John L. Hopper David E. Neal Douglas E Easton Rosalind A. Eeles Section of Cancer Genetics The Institute of Cancer Research Sutton Surrey SM2 5NG UK Cancer Epidemiology Centre The Cancer Council Victoria Carlton VIC 3053 Australia Centre for Molecular Environmental Genetic and Analytic Epidemiology The University of Melbourne Carlton VIC 3053 Australia Cancer Research UK Genetic Epidemiology Unit University of Cambridge Strangeways Laboratory Worts Causeway Cambridge CB1 8RN UK Department of Oncology University of Cambridge Strangeways Laboratory Worts Causeway Cambridge CB1 8RN UK Genetic Epidemiology Laboratory Department of Pathology The University of Melbourne Parkville VIC 3052 Australia Department of Social Medicine University of Bristol Bristol BS8 2PR UK Academic Urology Unit University of Sheffield Sheffield SIO 2JF UK The Royal Marsden NHS Foundation Trust Sutton Surrey SM2 5PT and London SW3 6JJ UK University of Nottingham Medical School Queens Medical Centre Nottingham NG7 2UH UK Institute for Cancer Studies University of Sheffield Sheffield SIO 2RX UK Surgical Oncology （Uro-Oncology S4） Departments of Oncology and Surgery University of Cambridge Addenbrooke＇s Hospital Cambridge CB2 2QQ UK A full list of authors is provided in the Supplementary Note online Ka Shing Centre Cambridge CB2 ORE UK Cancer Research UK Cambridge Research Institute Li Ka Shing Centre Cambridge CB2 ORE UK.

There is evidence that a substantial part of genetic predisposition to prostate cancer （PCa） may be due to lower penetrance genes which are found by genome-wide association studies. We have recently conducted such a study and seven new regions of the genome linked to PCa risk have been identified. Three of these loci contain candidate susceptibility genes： MSMB, LMTK2 and KLK2/3. The MSMB and KLK2/3 genes may be useful for PCa screening, and the LMTK2 gene might provide a potential therapeutic target. Together with results from other groups, there are now 23 germline genetic variants which have been reported. These results have the potential to be developed into a genetic test. However, we consider that marketing of tests to the public is premature, as PCa risk can not be evaluated fully at this stage and the appropriate screening protocols need to be developed. Follow-up validation studies, as well as studies to explore the psychological implications of genetic profile testing, will be vital prior to roll out into healthcare.

关键词： prostate cancer genetics susceptibility loci SNPs relative risks

The enhanced X-ray Timing and Polarimetry mission—eXTP

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Science China(Physics,Mechanics & Astronomy) 2019年第2期62卷 3-27页

作者： ShuangNan Zhang Andrea Santangelo Marco Feroci YuPeng Xu FangJun Lu Yong Chen Hua Feng Shu Zhang Sφren Brandt Margarita Hernanz Luca Baldini Enrico Bozzo Riccardo Campana Alessandra De Rosa YongWei Dong Yuri Evangelista Vladimir Karas Norbert Meidinger Aline Meuris Kirpal Nandra Teng Pan Giovanni Pareschi Piotr Orleanski QiuShi Huang Stephane Schanne Giorgia Sironi Daniele Spiga Jiri Svoboda Gianpiero Tagliaferri Christoph Tenzer Andrea Vacchi Silvia Zane Dave Walton ZhanShan Wang Berend Winter Xin Wu Jean J.M.in't Zand Mahdi Ahangarianabhari Giovanni Ambrosi Filippo Ambrosino Marco Barbera Stefano Basso Jörg Bayer Ronaldo Bellazzini Pierluigi Bellutti Bruna Bertucci Giuseppe Bertuccio Giacomo Borghi XueLei Cao Franck Cadoux Francesco Ceraudo TianXiang Chen Yu Peng Chen Jerome Chevenez Marta Civitani Wei Cui WeiWei Cui Thomas Dauser Ettore Del Monte Sergio Di Cosimo Sebastian Diebold Victor Doroshenko Michal Dovciak YuanYuan Du Lorenzo Ducci QingMei Fan Yannick Favre Fabio Fuschino JoséLuis Ga'lvez Min Gao MingYu Ge Olivier Gevin Marco Grassi QuanYing Gu YuDong Gu DaWei Han Bin Hong Wei Hu Long Ji ShuMei Jia WeiChun Jiang Thomas Kennedy Ingo Kreykenbohm Irfan Kuvvetli Claudio Labanti Luca Latronico Gang Li MaoShun Li Xian Li Wei Li ZhengWei Li Olivier Limousin HongWei Liu XiaoJing Liu Bo Lu Tao Luo Daniele Macera Piero Malcovati Adrian Martindale malgorzata Michalska Bin Meng Massimo Minuti Alfredo Morbidini Fabio Muleri Stephane Paltani Emanuele Perinati Antonino Picciotto Claudio Piemonte JinLu Qu Alexandre Rachevski Irina Rashevskaya Jerome Rodriguez Thomas Schanz ZhengXiang Shen LiZhi Sheng JiangBo Song LiMing Song Carmelo Sgro Liang Sun Ying Tan Phil Uttley Bo Wang DianLong Wang GuoFeng Wang Juan Wang LangPing Wang YuSa Wang Anna L.Watts XiangYang Wen Jörn Wilms ShaoLin Xiong JiaWei Yang Sheng Yang YanJi Yang Nian Yu WenDa Zhang Gianluigi Zampa Nicola Zampa Andrzej A.Zdziarski AiMei Zhang ChengMo Zhang Fan Zhang Long Zhang Tong Zhang Yi Zhang XiaoLi Zhang ZiLiang Zhang BaoSheng Zhao ShiJie Zheng Yu Peng Zhou Key Laboratory for Particle Astrophysics Institute of High Energy PhysicsChinese Academy of Sciences Institut für Astronomie und Astrophysik Eberhard Karls Universität INAF-Istituto di Astrofisica e Planetologia Spaziali INFN-Roma Tor Vergata Via della Ricerca Scientifica 1 Department of Engineering Physics and Center for Astrophysics Tsinghua University DTU Building 327DK-2800 Kongens Institute of Space Sciences 08193 Cerdanyola del Valles Institut d’Estudis Espacials de Catalunya Sezione di Pisa Istituto Nazionale di Fisica NucleareLargo Bruno Pontecorvo3 Department of Astronomy University of Genevachemin d’Ecogia 16 Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna Istituto Nazionale di Astofisica Astronomical Institute Czech Academy of Sciences Max Planck Institute for Extraterrestrial Physics Giessenbachstr.1 CEA Paris-Saclay/IRFU Beijing Institute of Spacecraft System Engineering CAST Osservatorio Astronomico di Brera Istituto Nazionale di Astofisica Space Research Center Polish Academy of Sciences Key Laboratory of Advanced Material Microstructure of Education Ministry of China Institute of Precision Optical EngineeringSchool of Physics Science and EngineeringTongji University Department of Physics and Center for Astrophysics Tsinghua University Universita’degli Studi di Udine Via delle Scienze 206 Mullard Space Science Laboratory University College London Department of Nuclear and Particle Physics University of Geneva SRON Netherlands Institute for Space Research Politecnico di Milano Sezione di Perugia Istituto Nazionale di Fisica Nucleare Dipartimento di Fisica e Chimica Fondazione Bruno Kessler Dr.Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics Universität Erlangen-Nürnberg University of Pavia Department of ElectronicsInformation and Biomedical Engineering and INFN Pavia Sezione di Torino Istituto Nazionale di Fisica NucleareVia Pietro Giuria1 Department of Physics and Astronomy University of Leicester Sezione di Trieste Istituto Nazionale di Fisica Nucleare

In this paper we present the enhanced X-ray Timing and Polarimetry mission—eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave *** paper provides a detailed description of:(1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload;(2) the elements and functions of the mission, from the spacecraft to the ground segment.

关键词： X-ray instrumentation X-ray polarimetry X-ray timing space mission:eXTP

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 Fengpeng An Qi An Giuseppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Auguste Weidong Bai Nikita Balashov Wander Baldini Andrea Barresi Davide Basilico Eric Baussan Marco Bellato Antonio Bergnoli Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Jose Busto Ilya Butorov Anatael Cabrera Barbara Caccianiga Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Riccardo Callegari Antonio Cammi Agustin Campeny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Chi Chan Jinfan Chang Yun Chang Guoming Chen Pingping Chen Po-An Chen Shaomin Chen Xurong Chen Yixue Chen Yu Chen Zhiyuan Chen Zikang Chen Jie Cheng Yaping Cheng Yu Chin Cheng Alexey Chetverikov Davide Chiesa Pietro Chimenti Artem Chukanov Gérard Claverie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalager Christophe De La Taille Zhi Deng Ziyan Deng Wilfried Depnering Marco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov Georgy Donchenko Jianmeng Dong Evgeny Doroshkevich Marcos Dracos Frédéric Druillole Ran Du Shuxian Du Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea Fabbri Donghua Fan Lei Fan Jian Fang Wenxing Fang Marco Fargetta Dmitry Fedoseev Zhengyong Fei Li-Cheng Feng Qichun Feng Richard Ford Amélie Fournier Haonan Gan Feng Gao Alberto Garfagnini Arsenii Gavrikov Marco Giammarchi Nunzio Giudice Maxim Gonchar Guanghua Gong Hui Gong Yuri Gornushkin Alexandre Göttel Marco Grassi Vasily Gromov Minghao Gu Xiaofei Gu Yu Gu Mengyun Guan Yuduo Guan Nunzio Guardone Cong Guo Jingyuan Guo Wanlei Guo Xinheng Guo Yuhang Guo Paul Hackspacher Caren Hagner Ran Han Yang Han Miao He Wei He Tobias Heinz Patrick Hellmuth Yuekun Heng Rafael Herrera YuenKeung Ho Yerevan Physics Institute YerevanArmenia UniversiéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontificia Universidade Catolica do Rio de Janeiro Rio de JaneiroBrazil Pontificia Universidad Católica de Chile SantiagoChile Universidad Tecnica Federico Santa Maria ValparaisoChile Beijing Institute of Spacecraft Environment Engineering BeijingChina Beijing Normal University BeijingChina China Institute of Atomic 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 Academy 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 Radiochemistry and Nuclear Chemistry Group in University of South China HengyangChina Wuyi University JiangmenChina Shandong University JinanChinaand Key Laboratory of Particle Physics and Particle Irradiation of Ministry of EducationShandong UniversityQingdaoChina Institute of Modern Physics Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East China University 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 Environmental Geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina Wuhan University WuhanChina Xi'an Jiaotong University Xi'anChina Xiamen University XiamenChina School of Physics and Microelectronics Zhengzhou UniversityZhengzhou

JUNO is a multi-purpose neutrino observatory under construction in the south of *** publication presents new sensitivity 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 *** sensitivities are obtained using the best knowledge available to date on the location and overburden 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 improvement over existing constraints for these three parameters.

关键词： neutrino oscillation reactor antineutrino precision measurement JUNO