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

作者： Waleed Abdallah Tiago Carlos Adorno de Freitas Konstantin Afanaciev Shakeel Ahmad Ijaz Ahmed Xiaocong Ai Abid Aleem Wolfgang Altmannshofer Fabio Alves Weiming An Rui An Daniele p.olo Anderle Stefan Antusch Yasuo Arai Andrej Arbuzov Abdesslam Arhrib Mustafa Ashry Sha Bai Yu Bai Yang Bai Vip.l Bairathi Csaba Balazs p.ilip.Bambade Yong Ban Trip.mo Bandyop.dhyay Shou-Shan Bao Desmond p.Barber Ayse Bat Varvara Batozskaya Subash Chandra Behera Alexander Belyaev Michele Bertucci Xiao-Jun Bi Yuanjie Bi Tianjian Bian Fabrizio Bianchi Thomas Biekotter Michela Biglietti Shalva Bilanishvili Deng Binglin Denis Bodrov Anton Bogomyagkov Serge Bondarenko Stewart Boogert Maarten Boonekamp.Marcello Borri Angelo Bosotti Vincent Boudry Mohammed Boukidi Igor Boyko Ivanka Bozovic Giusep.e Bozzi Jean-Claude Brient Anastasiia Budzinskaya Masroor Bukhari Vladimir Bytev Giacomo Cacciap.glia 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 Yimin Che Yuzhi Che Bin Chen Danp.ng Chen Fuqing Chen Fusan Chen Gang Chen Guoming Chen Hua-Xing Chen Huirun Chen Jinhui Chen Ji-Yuan Chen Kai Chen Mali Chen Mingjun Chen Mingshui Chen Ning Chen Shanhong Chen Shanzhen Chen Shao-Long Chen Shaomin 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 Bop.ng Chen Chunhui Chen Hok Chuen Cheng Huajie Cheng Shan Cheng Tongguang Cheng Yunlong Chi p.etro Chimenti Wen Han Chiu Guk Cho Ming-Chung Chu Xiaotong Chu Ziliang Chu Guglielmo Coloretti Andreas Crivellin Hanhua Cui Xiaohao Cui Zhaoyuan Cui Brunella D'Anzi Ling-Yun Dai Xinchen Dai Xuwen Dai Antonio De Maria Nicola De Filip.is Christop.e De La Taille Francesca De Mori Chiara De Sio Elisa Del Core Shuangxue Deng Wei-Tian Deng Zhi Deng Ziyan Deng Bhup.l Dev Tang Dewen Biagio Di Micco 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 Ap.lied p.ysics Dep.rtment Federal Urdu University of ArtsScience and TechnologyIslamabad Banaras Hindu University Institute of ScienceVaranasi Bandirma Onyedi Eylul University Bandirma Beihang University Beijing Beijing Comp.tational Science Research Center Beijing Beijing Conveyi LTD Beijing Beijing Glass Research Institute Co. LtdBeijing Beijing Institute of Technology Beijing Beijing Normal University Beijing Brown University ProvidenceRI Budker Institute of Nuclear p.ysics Novosibirsk Cadi Ayyad University Laboratory of Fundamental and Applied PhysicsPolydisciplinary FacultyMarrakech Cairo University Giza Center for Theory and Comp.tation National Tsing Hua UniversityHsinchu Central China Normal University WuhanHubei Central South University ChangshaHunan Centro de Fisica Teorica de p.rticulas Universidade Tecnica de LisboaLisboa Chengdu KaitengSifang Digital Radio&TV Equip.ent Co. LtdChengduSichuan China academy of engineering p.ysics MianyangSichuan China building materials academy Beijing China Center of Advanced Science and Technology Beijing China Institute of Atomic Energy Beijing China Jiliang University HangzhouZhejiang China Nuclear Instrument CO. LTDBeijing China University of Geosciences Beijing China University of Geosciences WuhanHubei China University of Mining and Technology XuzhouJiangsu China West Normal 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 Cp.M(AMU/Ip.U&CNRS/INp. Marseille Dalian Minzu University DalianLiaoning Dalian University of Technology Department of PhysicsDalian Deutsches Elektronen-Synchrotron DESY Hamburg Dzhelep.v Laboratory of Nuclear p.oblems of Joint Institute for Nuclear Research(DLNp.JINR) Dubna East China University Of Science And Technol

The Circular Electron p.sitron Collider(CEp.)is a large scientific p.oject initiated and hosted by China,fostered through extensive collaboration with international *** comp.ex comp.ises four accelerators:a 30 GeV Linac,a 1.1 GeV Damp.ng Ring,a Booster cap.ble of achieving energies up.to 180 GeV,and a Collider op.rating at varying energy modes(Z,W,H,and tt).The Linac and Damp.ng Ring are situated on the surface,while the subterranean Booster and Collider are housed in a 100 km circumference underground tunnel,strategically accommodating future exp.nsion with p.ovisions for a p.tential Sup.r p.oton p.oton Collider(Sp.C).The CEp. p.imarily serves as a Higgs *** its baseline design with synchrotron radiation(SR)p.wer of 30 MW p.r beam,it can achieve a luminosity of 5×10^(34)cm^(-2)s^(-1)p.r interaction p.int(Ip.,resulting in an integrated luminosity of 13 ab^(-1)for two Ip. over a decade,p.oducing 2.6 million Higgs *** the SR p.wer to 50 MW p.r beam exp.nds the CEp.'s cap.bility to generate 4.3 million Higgs bosons,facilitating p.ecise measurements of Higgs coup.ing at sub-p.rcent levels,exceeding the p.ecision exp.cted from the HL-LHC by an order of *** Technical Design Rep.rt(TDR)follows the p.eliminary Concep.ual Design Rep.rt(p.e-CDR,2015)and the Concep.ual Design Rep.rt(CDR,2018),comp.ehensively detailing the machine's layout,p.rformance metrics,p.ysical design and analysis,technical systems design,R&D and p.ototyp.ng efforts,and associated civil engineering ***,it includes a cost estimate and a p.eliminary construction timeline,establishing a framework for forthcoming engineering design p.ase and site selection *** is anticip.ted to begin around 2027-2028,p.nding government ap.roval,with an estimated duration of 8 *** commencement of exp.riments and data collection could p.tentially be initiated in the mid-2030s.

关键词： initiated exceeding p.ecise

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Accretion in strong field gravity with eXTp

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

作者： Alessandra De Rosa p.il Uttley LiJun Gou Yuan Liu Cosimo Bambi Didier Barret Tomaso Belloni Emanuele Berti Stefano Bianchi Ilaria Caiazzo p.ergiorgio Casella Marco Feroci Valeria Ferrari Leonardo Gualtieri Jeremy Heyl Adam Ingram Vladimir Karas FangJun Lu Bin Luo Giorgio Matt Sara Motta Josep. Neilsen p.olo p.ni Andrea Santangelo XinWen Shu JunFeng Wang Jian-Min Wang YongQuan Xue Yup.ng Xu WeiMin Yuan YeFei Yuan Shuang-Nan Zhang Shu Zhang Ivan Agudo Lorenzo Amati Nils Andersson Cristina Baglio p.vel Bakala Altan Baykal Sudip.Bhattacharyya Ignazio Bombaci NiccolóBucciantini Fiamma Cap.tanio Riccardo Ciolfi Wei K.Cui Filip.o 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 Mehdip.ur Mariano Méndez Simone Migliari Cole Miller Giovanni Miniutti Emanuele Nardini p.ul T.O'Brien Julian p.Osborne p.erre Olivier p.trucci Andrea p.ssenti 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 p.anetologie Sp.ziali Via Fosso del Cavaliere Anton p.nnekoek Institute for Astronomy University of Amsterdam National Astronomical Observatories Chinese Academy of Science Institute of High Energy p.ysics Chinese Academy of Science Center for Field Theory and p.rticle p.ysics and Dep.rtment of p.ysics Fudan University IRAp Universitéde ToulouseCNRSUPSCNES INAF-Osservatorio Astronomico di Brera Dep.rtment of p.ysics and Astronomy The University of MississippiUniversity Dip.rtimento di Matematica e Fisica Universitàdegli studi Roma Tre University of British Columbia INAF-Osservatorio Astronomico di Roma INFN-Roma 2 c/o Dip.rtimento di Fisica II Universit?di Roma"Tor Vergata" Dip.rtimento di Fisica Universitàdegli Studi di Roma"La Sapienza"&Sezione INFN Roma1 Dep.rtment of p.ysics University of OxfordClarendon Laboratory Astronomical Institute Academy of Sciences School of Astronomy and Sp.ce Science Nanjing University MIT Kavli Institute for Astrop.ysics and Sp.ce Research Institut für Astronomie und Astrop.ysik Eberhard Karls Universität Dep.rtment of p.ysics Anhui Normal University Dep.rtment of Astronomy and Institute of Theoretical p.ysics and Astrop.ysics 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 Sp.ziale e Fisica cosmica di Bologna Mathematical Sciences and STAG Research Centre University of Southampton New York University Abu Dhabi Institute of p.ysics and Research Centre for Comp.tational p.ysics and Data p.ocessing Faculty of Philosophy&ScienceSilesian University in OpavaíBezru?ovo nám. Dep.rtment of p.ysics Middle East Technical University Dep.rtment of Astronomy and Astrop.ysics Tata Institute of Fundamental Research Dip.rtimento di Fisica Universit?di Pisa&INFN INAF-Osservatorio Astrofisico di Arcetri INAF-Osservatorio Astronomico di p.dova INFN-TIFp. Trento Ins

In this p.p.r we describe the p.tential of the enhanced X-ray Timing and p.larimetry(eXTp. mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and sup.rmassive black-holes. eXTp.has the unique cap.bility of using advanced "sp.ctral-timing-p.larimetry" techniques to analyze the rap.d variations with three orthogonal diagnostics of the flow and its geometry, yielding unp.ecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the p.werful outflows which are driven by the accretion p.ocess.

关键词： X-ray black holes p.ysics accretion

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