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分子量分布及短支链结构对HDPE剪切诱导结晶的影响

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上海塑料 2018年第1期46卷 53-58页

作者：高苏闽刘亚涛 HSIAO S Benjamin 邵惠丽张耀鹏东华大学纤维材料改性国家重点实验室材料科学与工程学院上海201620 南开大学新能源材料化学研究所材料科学与工程学院国家新材料研究院天津300350 石溪大学化学系美国纽约11790

高密度聚乙烯(HDPE)管道轻便、坚固、耐用,因此广泛应用于替代老化管道。应用同步辐射X射线衍射和散射技术,深入研究两种HDPE的结晶度、片层取向、长周期和取向因子。分析了聚合物分子结构对HDPE结构和性能的影响,并进行原位剪切实验以... 详细信息

高密度聚乙烯(HDPE)管道轻便、坚固、耐用,因此广泛应用于替代老化管道。应用同步辐射X射线衍射和散射技术,深入研究两种HDPE的结晶度、片层取向、长周期和取向因子。分析了聚合物分子结构对HDPE结构和性能的影响,并进行原位剪切实验以研究双峰和单峰HDPE样品的剪切诱导结晶。研究表明,所有样品都形成了离散的初级片层和次级片层,且双峰HDPE中的次级片层生长速度高于单峰HDPE。剪切易导致HDPE产生沿着剪切方向的取向,并提高其结晶度。剪切后,双峰HDPE具有比单峰HDPE样品更高的片层取向,且双峰HDPE具有相对较高的结晶度。具有短支链(SCB)的大部分中等高分子量(MMW)分子链易受剪切诱导形成结晶核。

关键词：高密度聚乙烯同步辐射技术双峰单峰

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空气灌肠MR结肠成像检测结、直肠息肉及癌

中国医学影像技术 2009年第12期25卷 2246-2249页

作者：罗明月严福华沈继章姚礼庆周康荣张国鹏卢虹冰 Jerome Z.liang 中山大学附属第六医院放射科广东广州510655 复旦大学附属中山医院放射科上海200032 复旦大学附属中山医院内镜中心上海200032 第四军医大学生物医学工程系陕西西安710032 department of Radiology State University of New York at Stomy BrookNew York 11794

目的评价空气灌肠三维Fourier变换快速扰相梯度回波（FSPGR）序列MR结肠成像检测结直肠息肉及癌的灵敏度。方法对30例因便血、大便隐血试验阳性或大便习惯改变而拟接受光学结肠镜检查者进行空气灌肠三维Fourier变换FSPGR序列MR结肠成像... 详细信息

目的评价空气灌肠三维Fourier变换快速扰相梯度回波（FSPGR）序列MR结肠成像检测结直肠息肉及癌的灵敏度。方法对30例因便血、大便隐血试验阳性或大便习惯改变而拟接受光学结肠镜检查者进行空气灌肠三维Fourier变换FSPGR序列MR结肠成像及光学结肠镜检查。以光学结肠镜及组织病理学检查为标准,按息肉及癌的大小统计分析MR结肠成像检测结直肠息肉及癌的灵敏度。结果光学结肠镜共检出76枚结直肠息肉及癌,其中1-5 mm息肉11枚、6-9 mm息肉29枚、≥10 mm息肉及癌36枚。MR结肠成像对1-5 mm息肉、6-9 mm息肉、≥10 mm息肉及癌、≥6 mm息肉及癌的检测灵敏度分别为9.09%、75.86%、100%及89.23%,总体检测灵敏度为77.63%。结论空气灌肠三维Fourier变换FSPGR序列MR结肠成像对1-5 mm结直肠息肉检测灵敏度低,但对≥6 mm息肉及癌的检测灵敏度较高,并能够检出全部≥10 mm的息肉及癌。

关键词：结肠直肠息肉肿瘤磁共振成像结肠成像

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中国极化电子离子对撞机计划

核技术 2020年第2期43卷 1-59页

作者：曹须常雷畅宁波陈旭荣陈卓俊崔钫戴凌云邓维天丁明慧龚畅桂龙成郭奉坤韩成栋何军黄虹霞黄银 Kaptari L P 李德民李衡讷李民祥李学潜梁羽铁梁作堂刘国明刘杰刘柳明刘翔罗晓峰吕准马伯强马伏马建平马余刚冒立军 Mezrag C 平加伦秦思学任航 Roberts C D 申国栋史潮宋勤涛孙昊王恩科王凡王倩王荣王睿儒王涛峰王伟王晓玉王晓云吴佳俊吴兴刚肖博文肖国青谢聚军谢亚平邢宏喜徐瑚珊许怒徐书生鄢文标闫文成闫新虎杨建成杨一玻杨智姚德良尹佩林詹文龙张建辉张金龙张鹏鸣张肇西张振宇赵红卫赵光达赵强赵宇翔赵政国郑亮周剑周详周小蓉邹冰松邹丽平中国科学院近代物理研究所兰州730000 中国科学院大学北京100049 南开大学天津300071 信阳师范学院信阳464000 湖南大学长沙410082 南京大学南京210093 华中科技大学武汉430074 European Centre for Theoretical Studies in Nuclear Physics and Related Areas(ECT*)and Fondazione Bruno Kessler Villa TambosiStrada delle Tabarelle 286I-38123 Villazzano(TN)Italy 北京大学物理学院北京100871 湖南师范大学长沙410081 中国科学院理论物理研究所中国科学院理论物理前沿重点实验室北京100190 南京师范大学南京210023 西南交通大学成都610000 Bogoliubov Laboratory of Theoretical Physics Joint Institute for Nuclear ResearchDubna 141980Russia 郑州大学物理学院郑州450001 华南师范大学量子物质研究院广东省核物质科学与技术重点实验室广州510631 兰州大学物理科学与技术学院兰州730000 山东大学粒子物理与粒子辐照教育部重点实验室青岛266237 华中师范大学夸克与轻子教育部重点实验室和粒子物理研究所武汉430079 东南大学物理学院南京211189 复旦大学现代物理研究所核物理与离子束应用教育部重点实验室上海200433 中国科学院上海应用物理研究所上海201800 IRFU CEAUniversitéParis-SaclayF-91191 Gif-sur-YvetteFrance 重庆大学物理系重庆400044 南京航空航天大学核科学与技术系南京211106 大连理工大学大连116024 北京航空航天大学物理学院北京100191 上海交通大学上海200240 兰州理工大学兰州730050 南京邮电大学南京210023 中国科学技术大学合肥230026 黄山学院黄山245021 北京师范大学高等量子研究中心北京100875 department of Physics and Astronomy Stony Brook UniversityStony BrookNY 11794USA 中山大学物理与天文学院珠海519082 武汉大学物理科学与技术学院武汉430072 中国科学院高能物理研究所中国科学院大科学装置理论中心北京100049 中国地质大学(武汉)数学与物理学院武汉430074

轻子散射实验是探索核子与原子核结构的理想工具。中国电子离子对撞机(Electron Ion Collider in China,EicC)建议书设想在已开建的强流重离子加速器装置(High Intensity heavy ion Accelerator Facility,HIAF)的基础上,升级质子束流为2... 详细信息

轻子散射实验是探索核子与原子核结构的理想工具。中国电子离子对撞机(Electron Ion Collider in China,EicC)建议书设想在已开建的强流重离子加速器装置(High Intensity heavy ion Accelerator Facility,HIAF)的基础上,升级质子束流为20 GeV的极化束流,并建造2.8~5 GeV极化电子束流,从而实现质心系能量为15~20 GeV的双极化电子-离子对撞。EicC设计的亮度为(2~4)×10^33cm^-2·s^-1,质子束流极化率达到70%,电子束流极化率达到80%。该装置除了能提供极化轻离子束流(例如:氦-3)外,也可产生非极化重离子束流(碳-12~铀-238)。EicC将聚焦核子海夸克部分子结构、原子核物质结构与性质、奇特强子态三个方面的物理研究。高亮度、高精度的对撞机有助于精确地测量核子结构函数并对核子进行三维成像,揭示强相互作用的动力学规律;原子核部分子分布包括核子短程关联以及原子核介质效应同样是该提案的重要科学目标;EicC能区接近重味夸克产生阈值,在研究重味强子谱方面拥有低背景的独特优势,有助于发现研究新的奇特强子态。质子质量起源问题也可以通过重味矢量介子的产生来研究。为了完成上述物理目标,我们将利用最先进的探测器技术建造接近全立体角覆盖的EicC对撞机谱仪。在准备EicC白皮书的过程中,我们得到世界各国专家的支持。EicC的物理与已有的实验和美国即将建设的EIC中的物理项目相互补充。EicC的建成及运行有望引领前沿的中高能核物理研究,使我国在加速器和探测器先进技术等领域实现跨越式发展,为我国核物理与强子物理以及相关科学领域提供大型综合实验平台与人才培养基地。

关键词：电子离子对撞机核子结构核子质量奇特强子态量子色动力学螺旋度横动量依赖部分子分布广义部分子分布深度虚康普顿散射深度虚介子散射能量回收型直线加速器极化度自旋旋转器三维成像

Observatory science with eXTP

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Science China(Physics,Mechanics & Astronomy) 2019年第2期62卷 97-138页

作者： Jean J.M.in 't Zand Enrico Bozzo JinLu Qu Xiang-Dong li Lorenzo Amati Yang Chen Immacolata Donnarumma Victor Doroshenko Stephen A.Drake Margarita Hernanz Peter A.Jenke Thomas J.Maccarone Simin Mahmoodifar Domitilla de Martino Alessandra De Rosa Elena M.Rossi Antonia Rowlinson Gloria Sala Giulia Stratta Thomas M.Tauris Joern Wilms XueFeng Wu Ping Zhou Iván Agudo Diego Altamirano Jean-Luc Atteia Nils A.andersson M.Cristina Baglio David R.Ballantyne Altan Baykal Ehud Behar Tomaso Belloni Sudip Bhattacharyya Stefano Bianchi Anna Bilous Pere Blay Joao Braga Sφren Brandt Edward F.Brown Niccolo Bucciantini Luciano Burderi Edward M.Cackett Riccardo Campana Sergio Campana Piergiorgio Casella Yuri Cavecchi Frank Chambers liang Chen Yu-Peng Chen Jér?me Chenevez Maria Chernyakova ChiChuan Jin Riccardo Ciolfi Elisa Costantini Andrew Cumming Antonino D'Aì Zi-Gao Dai Filippo D'Ammando Massimiliano De Pasquale Nathalie Degenaar Melania Del Santo Valerio D'Elia Tiziana Di Salvo Gerry Doyle Maurizio Falanga XiLong Fan Robert D.Ferdman Marco Feroci Federico Fraschetti Duncan K.Galloway Angelo F.Gambino Poshak Gandhi MingYu Ge Bruce Gendre Ramandeep Gill Diego G?tz Christian Gouiffès Paola Grandi Jonathan Granot Manuel Güdel Alexander Heger Craig O.Heinke Jeroen Homan Rosario Iaria Kazushi Iwasawa Luca Izzo Long Ji Peter G.Jonker Jordi José Jelle S.Kaastra Emrah Kalemci Oleg Kargaltsev Nobuyuki Kawai Laurens Keek Stefanie Komossa Ingo Kreykenbohm Lucien Kuiper Devaky Kunneriath Gang li En-Wei liang Manuel linares Francesco Longo FangJun Lu Alexander A.Lutovinov Denys Malyshev Julien Malzac Antonios Manousakis Ian McHardy Missagh Mehdipour YunPeng Men Mariano Méndez Roberto P.Mignani Romana Mikusincova M.Coleman Miller Giovanni Miniutti Christian Motch Joonas Nättilä Emanuele Nardini Torsten Neubert Paul T.O'Brien Mauro Orlandini Julian P.Osborne Luigi Pacciani Stéphane Paltani Maurizio Paolillo Iossif E.Papadakis Biswajit Paul Alberto Pellizzoni Uria Peretz Miguel A.Pérez Torres Emanuele Perinati Chanda Prescod-Weinstein Pablo Reig SRON Netherlands Institute for Space Research department of Astronomy University of Geneva Key Laboratory for Particle Astrophysics Institute of High Energy PhysicsChinese Academy of Sciences School of Astronomy and Space Science Nanjing University INAF-IASF Bologna ASI Via del Politecnico snc INAF-Istituto di Astrofisica e Planetologie Spaziali Institut für Astronomie und Astrophysik Tübingen Universit?t Tübingen NASA Goddard Space Flight Center ICREA&Institute of Space Sciences(IEEC-CSIC) Campus UABCarrer de Can Magrans CSPAR SPA University of Alabama in Huntsville department of Physics Texas Tech University INAF Osservatorio Astronomico di Capodimonte Leiden Observatory Leiden University Anton Pannekoek Institute University of Amsterdam ASTRON Netherlands Institute for Radio Astronomy Universitat Politecnica de Catalunya(UPC-IEEC) Universitádegli Studi di Urbino‘Carlo Bo’ Max-Planck-Institut für Radioastronomie Dr.Karl-Remeis-Sternwarte and Erlangen Centre for Astroparticle Physics(ECAP) Friedrich Alexander Universit?t Erlangen-Nurnberg Purple Mountain Observatory Chinese Academy of Sciences Instituto de Astrofysíca de Andalucia-CSIC department of Physics and Astronomy University of Southampton IRAP Universitéde ToulouseCNRSUPSCNES Mathematical Sciences and STAG Research Centre University of Southampton New York university Abu Dhabi Center for Relativistic Astrophysics School of PhysicsGeorgia Institute of Technology Physics department Middle East Technical University department of Physics Technion-Israel Institute of Technology INAF Osservatorio Astronomico di Brera Tata Institute of Fundamental Research Dipartimento di Matematica e Fisica Universitàdegli Studi Roma Tre Instituto de Astrofísica de Canarias Instituto Nacional de Pesquisas Espaciais-INPE National Space Institute Technical University of Denmark(DTU Space) department of Physics and Astronomy Michigan State University INAF Osservatorio Astrofisico di Arcetri Dipartimento di Fisica Universitádegli Studi di Cagliari department of Physics and A

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry(eXTP) mission for studies related to Observatory Science targets. These include flaring stars, supernova remnants, accreting white dwarfs, low and high mass X-ray binaries, radio quiet and radio loud active galactic nuclei, tidal disruption events, and gamma-ray bursts. eXTP will be excellently suited to study one common aspect of these objects: their often transient nature. Developed by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Science, the eXTP mission is expected to be launched in the mid 2020s.

关键词： space research in struments nuclear astrophysics flare stars accretion and accretion disks mass loss and stellar winds cataclysmic binaries X-ray binaries supernova remnants active galactic nuclei X-ray bursts gamma-ray bursts gravitational waves

Methods for a blind analysis of isobar data collected by the STAR collaboration

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Nuclear Science and Techniques 2021年第5期32卷 43-50页

作者： J.Adam L.Adamczyk J.R.Adams J.K.Adkins G.Agakishiev M.M.Aggarwal Z.Ahammed I.Alekseev D.M.Anderson A.Aparin E.C.Aschenauer M.U.Ashraf F.G.Atetalla A.Attri G.S.Averichev V.Bairathi K.Barish A.Behera R.Bellwied A.Bhasin J.Bielcik J.Bielcikova L.C.Bland I.G.Bordyuzhin J.D.Brandenburg A.V.Brandin J.Butterworth H.Caines M.Calderon de la Barca Sanchez D.Cebra I.Chakaberia P.Chaloupka B.K.Chan F-H.Chang Z.Chang N.Chankova-Bunzarova A.Chatterjee D.Chen J.Chen J.H.Chen X.Chen Z.Chen J.Cheng M.Cherney M.Chevalier S.Choudhury W.Christie X.Chu H.J.Crawford M.Csanad M.Daugherity T.G.Dedovich I.M.Deppner A.A.Derevschikov L.Didenko X.Dong J.L.Drachenberg J.C.Dunlop T.Edmonds N.Elsey J.Engelage G.Eppley S.Esumi O.Evdokimov A.Ewigleben O.Eyser R.Fatemi S.Fazio P.Federic J.Fedorisin C.J.Feng Y.Feng P.Filip E.Finch Y.Fisyak A.Francisco L.Fulek C.A.Gagliardi T.Galatyuk F.Geurts A.Gibson K.Gopal X.Gou D.Grosnick W.Guryn A.I.Hamad A.Hamed S.Harabasz J.W.Harris S.He W.He X.H.He Y.He S.Heppelmann S.Heppelmann N.Herrmann E.Hoffman L.Holub Y.Hong S.Horvat Y.Hu H.Z.Huang S.L.Huang T.Huang X.Huang T.J.Humanic P.Huo G.Igo D.Isenhower W.W.Jacobs C.Jena A.Jentsch Y.Ji J.Jia K.Jiang S.Jowzaee X.Ju E.G.Judd S.Kabana M.L.Kabir S.Kagamaster D.Kalinkin K.Kang D.Kapukchyan K.Kauder H.W.Ke D.Keane A.Kechechyan M.Kelsey Y.V.Khyzhniak D.P.Kikoła C.Kim B.Kimelman D.Kincses T.A.Kinghorn I.Kisel A.Kiselev M.Kocan L.Kochenda L.K.Kosarzewski L.Kramarik P.Kravtsov K.Krueger N.Kulathunga Mudiyanselage L.Kumar S.Kumar R.Kunnawalkam Elayavalli J.H.Kwasizur R.Lacey S.Lan J.M.Landgraf J.Lauret A.Lebedev R.Lednicky J.H.Lee Y.H.Leung C.li C.li W.li W.li X.li Y.li Y.liang R.licenik T.lin Y.lin M.A.lisa F.liu H.liu P.liu P.liu T.liu X.liu Y.liu Z.liu T.Ljubicic W.J.Llope R.S.Longacre N.S.Lukow S.Luo X.Luo G.L.Ma L.Ma R.Ma Y.G.Ma N.Magdy R.Majka D.Mallick S.Margetis C.Markert H.S.Matis J.A.Mazer N.G.Minaev S.Mioduszewski B.Mohanty I.Mooney Z.Moravcova D.A.Morozov M.Nagy J.D.Nam Md.Nasim K.Nayak D.Neff J.M.Nelson D.B.Nemes M.Nie G.Nigmatkulov T.Niida L.V.Nogach T.Nonak Christian university AbileneTX 796992 AGH university of Science and Technology FPACSCracow 30-059Poland Alikhanov Institute for Theoretical and Experimental Physics NRC"Kurchatov Institute" MoscowRussia 117218 Argonne National Laboratory ArgonneIL 60439 American university of Cairo New CairoNew Cairo 11835Egypt brookhaven National Laboratory UptonNY 11973 university of California BerkeleyCA 94720 university of California DavisCA 95616 university of California Los AngelesCA 90095 university of California RiversideCA 92521 Central China Normal university Wuhan 430079 university of Illinois at Chicago ChicagoIL 60607 Creighton university OmahaNE 68178 Czech Technical university in Prague FNSPEPrague 11519Czech Republic Technische Universitat Darmstadt Darmstadt 64289Germany ELTE Eotvos Lorand university Budapest 1117Hungary Frankfurt Institute for Advanced Studies FIAS Frankfurt 60438Germany Fudan university Shanghai 200433 university of Heidelberg 69120 HeidelbergGermany university of Houston HoustonTX 77204 Huzhou university Huzhou 313000 Indian Institute of Science Education and Research(IISER) Berhampur 760010India Indian Institute of Science Education and Research(IISER)Tirupati Tirupati 517507India Indian Institute Technology PatnaBihar 801106India Indiana university BloomingtonIN 47408 Institute of Modern Physics Chinese Academy of SciencesLanzhou 730000 university of Jammu Jammu 180001India Joint Institute for Nuclear Research DubnaRussia 141980 Kent State university KentOH 44242 university of Kentucky LexingtonKY 40506-0055 Lawrence Berkeley National Laboratory BerkeleyCA 94720 Lehigh university BethlehemPA 18015 Max-Planck-Institut fur Physik 80805 MunichGermany Michigan State university East LansingMI 48824 National Research Nuclear university MEPhI MoscowRussia 115409 National Institute of Science Education and Research HBNIJatni 752050India National Cheng Kung university Tainan 70101 Nuclear Physics Institute of the CAS Rez 25068Czech Republic Ohio State university

In 2018,the STAR collaboration collected data from^(96)_(44)Ru+^(96)_(44)Ru and^(96)_(40)Zr+^(96)_(40)Zr at√^(S)NN=200 Ge V to search for the presence of the chiral magnetic effect in collisions of *** isobar collision species alternated frequently between 9644 Ru+^(96)_(44)Ru and^(96)_(40)Zr+^(96)_(40)*** order to conduct blind analyses of studies related to the chiral magnetic effect in these isobar data,STAR developed a three-step blind analysis *** are initially provided a"reference sample"of data,comprised of a mix of events from the two species,the order of which respects time-dependent changes in run *** tuning analysis codes and performing time-dependent quality assurance on the reference sample,analysts are provided a species-blind sample suitable for calculating efficiencies and corrections for individual≈30-min data-taking *** this sample,species-specific information is disguised,but individual output files contain data from a single isobar *** run-by-run corrections and code alteration subsequent to these corrections are allowed at this *** these modifications,the"frozen"code is passed over the fully un-blind data,completing the blind *** a check of the feasibility of the blind analysis procedure,analysts completed a"mock data challenge,"analyzing data from Au+Au collisions at√^(S)NN=27 Ge V,collected in *** Au+Au data were prepared in the same manner intended for the isobar blind *** details of the blind analysis procedure and results from the mock data challenge are presented.

关键词： Blind analysis Chiral magnetic effect Heavy-ion collisions

Measurement of away-side broadening with self-subtraction of flow in Au+Au collisions at √sNN=200 GeV

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Chinese Physics C 2020年第10期44卷 59-67页

作者： L.Adamczyk J.R.Adams J.K.Adkins G.Agakishiev M.M.Aggarwal Z.Ahammed I.Alekseev D.M.Anderson A.Aparin E.C.Aschenauer M.U.Ashraf F.G.Atetalla A.Attri G.S.Averichev V.Bairathi K.Barish A.Behera R.Bellwied A.Bhasin J.Bielcik J.Bielcikova L.C.Bland I.G.Bordyuzhin J.D.Brandenburg A.V.Brandin J.Butterworth H.Caines M.Calderón de la Barca Sánchez D.Cebra I.Chakaberia P.Chaloupka B.K.Chan F-H.Chang Z.Chang N.Chankova-Bunzarova A.Chatterjee D.Chen J.H.Chen X.Chen Z.Chen J.Cheng M.Cherney M.Chevalier S.Choudhury W.Christie X.Chu H.J.Crawford M.Csanád M.Daugherity T.G.Dedovich I.M.Deppner A.A.Derevschikov L.Didenko X.Dong J.L.Drachenberg J.C.Dunlop T.Edmonds N.Elsey J.Engelage G.Eppley S.Esumi O.Evdokimov A.Ewigleben O.Eyser R.Fatemi S.Fazio P.Federic J.Fedorisin C.J.Feng Y.Feng P.Filip E.Finch Y.Fisyak A.Francisco L.Fulek C.A.Gagliardi T.Galatyuk F.Geurts A.Gibson K.Gopal D.Grosnick W.Guryn A.I.Hamad A.Hamed S.Harabasz J.W.Harris S.He W.He X.H.He S.Heppelmann S.Heppelmann N.Herrmann E.Hoffman L.Holub Y.Hong S.Horvat Y.Hu H.Z.Huang S.L.Huang T.Huang X.Huang T.J.Humanic P.Huo G.Igo D.Isenhower W.W.Jacobs C.Jena A.Jentsch Y.JI J.Jia K.Jiang S.Jowzaee X.Ju E.G.Judd S.Kabana M.L.Kabir S.Kagamaster D.Kalinkin K.Kang D.Kapukchyan K.Kauder H.W.Ke D.Keane A.Kechechyan M.Kelsey Y.V.Khyzhniak D.P.Kikoła C.Kim B.Kimelman D.Kincses T.A.Kinghorn I.Kisel A.Kiselev M.Kocan L.Kochenda L.K.Kosarzewski L.Kramarik P.Kravtsov K.Krueger N.Kulathunga Mudiyanselage L.Kumar S.Kumar R.Kunnawalkam Elayavalli J.H.Kwasizur R.Lacey S.Lan J.M.Landgraf J.Lauret A.Lebedev R.Lednicky J.H.Lee Y.H.Leung C.li W.li W.li X.li Y.li Y.liang R.licenik T.lin Y.lin M.A.lisa F.liu H.liu P.liu P.liu T.liu X.liu Y.liu Z.liu T.Ljubicic W.J.Llope R.S.Longacre N.S.Lukow S.Luo X.Luo G.L.Ma L.Ma R.Ma Y.G.Ma N.Magdy R.Majka D.Mallick S.Margetis C.Markert H.S.Matis J.A.Mazer N.G.Minaev S.Mioduszewski B.Mohanty I.Mooney Z.Moravcova D.A.Morozov M.Nagy J.D.Nam Nasim Md K.Nayak D.Neff J.M.Nelson D.B.Nemes M.Nie G.Nigmatkulov T.Niida L.V.Nogach T.Nonaka A.S.Nunes G.Odyniec A.Ogawa Abilene Christian university AbileneTexas 79699 AGH university of Science and Technology FPACSCracow 30-059Poland Alikhanov Institute for Theoretical and Experimental Physics NRC"Kurchatov Institute" Moscow 117218Russia Argonne National Laboratory ArgonneIllinois 60439 American university of Cairo New Cairo 11835New CairoEgypt brookhaven National Laboratory UptonNew York 11973 university of California BerkeleyCalifornia 94720 university of California DavisCalifornia 95616 university of California Los AngelesCalifornia 90095 university of California RiversideCalifornia 92521 Central China Normal university WuhanHubei 430079 university of Illinois at Chicago ChicagoIllinois 60607 Creighton university OmahaNebraska 68178 Czech Technical university in Prague FNSPEPrague 11519Czech Republic Technische Universität Darmstadt Darmstadt 64289Germany ELTE Eötvös Loránd university BudapestHungary H-1117 Frankfurt Institute for Advanced Studies FIAS Frankfurt 60438Germany Fudan university Shanghai 200433 university of Heidelberg Heidelberg 69120Germany university of Houston HoustonTexas 77204 Huzhou university HuzhouZhejiang 313000 Indian Institute of Science Education and Research(IISER) Berhampur 760010India Indian Institute of Science Education and Research(IISER)Tirupati Tirupati 517507India Indian Institute Technology PatnaBihar 801106India Indiana university BloomingtonIndiana 47408 Institute of Modern Physics Chinese Academy of SciencesLanzhouGansu 730000 university of Jammu Jammu 180001India Joint Institute for Nuclear Research Dubna 141980Russia Kent State university KentOhio 44242 university of Kentucky LexingtonKentucky 40506-0055 Lawrence Berkeley National Laboratory BerkeleyCalifornia 94720 Lehigh university BethlehemPennsylvania 18015 Max-Planck-Institut für Physik Munich 80805Germany Michigan State university East LansingMichigan 48824 National Research Nuclear university MEPhI Moscow 115409Russia National Institute of Science Education and Research HBNIJatni 752050Indi

High transverse momentum(pT)particle production is suppressed owing to the parton(jet)energy loss in the hot dense medium created in relativistic heavy-ion *** of energy at low-to-modest pT has been difficult to measure,owing to large anisotropic *** report a data-driven method for background evaluation and subtraction,exploiting the away-side pseudorapidity gaps,to measure the jetlike correlation shape in Au+Au collisions at √sNN=200 GeV in the STAR *** correlation shapes,for trigger particles pT>3GeV/c and various associated particle pT ranges within 0.5lisions.

关键词： di-hadron correlations jet heavy-ion