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Accurate prediction of oxygen v.cancy concentration with disordered A-site cations in high-entropy perov.kite oxides

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npj Computational Materials 2023年第1期9卷 2053-2065页

作者： Jiyun park Boyuan Xu Jie pan Dawei Zhang Stephan Lany Xingbo Liu Jian Luo Yue Qi School of Engineering Brown UniversityProvidenceRI 02912USA Department of Physics Brown UniversityProvidenceRI 02912USA Department of Chemical Engineering and Materials Science Michigan State UniversityEast LansingMI 48824USA Program of Materials Science and Engineering University of California San DiegoLa JollaCA 92093USA Materials Science Center National Renewable Energy LaboratoryGoldenCO 80401USA Department of Mechanical and Aerospace Engineering Benjamin M.Statler College of Engineering and Mineral ResourcesWest Virginia UniversityMorgantownWV 26506USA Department of NanoEngineering University of California San DiegoLa JollaCA 92093USA

Entropic stabilized ABO_(3) perov.kite oxides promise many applications,including the two-step solar thermochemical hydrogen(STCH)*** binary and quaternary A-site mixed{A}FeO_(3) as a model system,we rev.al that as more cation types,especially abov. four,are mixed on the A-site,the cell lattice becomes more cubic-like but the local Fe–O octahedrons are more *** comparing four different Density Functional Theory-informed statistical models with experiments,we show that the oxygen v.cancy formation energies(E^(f)_(v.)distribution and the v.cancy interactions must be considered to predict the oxygen non-stoichiometry(δ)*** STCH applications,the E^(f)_(v. distribution,including both the av.rage and the spread,can be optimized jointly to improv.Δδ(difference ofδbetween the two-step conditions)in some hydrogen production *** model can be used to predict the range of water splitting that can be thermodynamically improv.d by mixing cations in{A}FeO_(3) perov.kites.

关键词： perov.kite v.cancy oxides

The LEGUE high latitude bright surv.y design for the LAMOST pilot surv.y

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Research in Astronomy and Astrophysics 2012年第7期12卷 792-804页

作者： Yue-Yang Zhang Jeffrey L. Carlin fan Yang Chao Liu Li-Cai Deng Heidi Jo Newberg Hao-Tong Zhang Sebastien Lepine Yan Xu Shuang Gao Norbert Chfi' stlieb Zhan-Wen Han Jin-Liang Hou Hsu-Tai Lee Xiao-Wei Liu Kai-Ke pan Hong-Chi Wang Key Lab for Optical Astronomy National Astronomical Observatories Chinese Academy ofSciences Beijing 100012 China Graduate Univ.rsity of Chinese Academy of Sciences Beijing 100049 China Department of Astrophysics Division of Physical Sciences American Museum of NaturalHistory Central Park West at 79th Street New York NY 10024 USA Department of Physics Applied Physics and Astronomy Rensselaer Polytechnic Institute 1108th Street Troy NY 12180 USA carlij@rpi.edu Univ.rsity of Heidelberg Landesstemwarte K6nigstuhl 12 D-69117 Heidelberg Germany Yunnan Astronomical Observ.tory Chinese Academy of Sciences Kunming 65()011 China Shanghai Astronomical Observ.tory Chinese Academy of Sciences Shangthai 200030 China Institute of Astronomy and Astrophysics Academia Sinica EO. Box 23-141 Taipei 106 China Department of Astronomy & Kav.i Institute of Astronomy and Astrophysics Peking UniversityBeijing 100871 China Apache Point Observ.tory PO Box 59 Sunspot NM 88349 USA Purple Mountain Observ.tory Chinese Academy of Sciences Nanjing 210008 China

We describe the footprint and input catalog for bright nights in the LAMOST Pilot Surv.y, which began in October 2011. Targets are selected from two stripes in the north and south Galactic Cap regions, centered at δ = 29°, with 10° width in declination, cov.ring right ascensions of 135° to 290° and -30° to 30° re- spectiv.ly. We selected spectroscopic targets from a combination of the SDSS and 2MASS point source catalogs. The catalog of stars defining the field centers （as re- quired by the Shack-Hartmann wav.front sensor at the center of the LAMOST field） consists of all v.〈 8m stars from the Hipparcos catalog. We employ a statistical selection algorithm that assigns priorities to targets based on their positions in mul- tidimensional color/magnitude space. This scheme ov.remphasizes rare objects and de-emphasizes more populated regions of magnitude and color phase space, while en- suring a smooth, well-understood selection function. A demonstration of plate design is presented based on the Shack-Hartmann star catalog and an input catalog that was generated by our target selection routines.

关键词： surv.ys: LAMOST -- techniques: spectroscopic -- Galaxy: stellar con-tent

The LEGUE input catalog for dark night observ.ng in the LAMOST pilot surv.y

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Research in Astronomy and Astrophysics 2012年第7期12卷 781-791页

作者： fan Yang Jeffrey L. Carlin Chao Liu Yue-Yang Zhang Shuang Gao Yan Xu Li-Cai Deng Heidi Jo Newberg Sebastien Lepine Jin-Liang Hou Xiao-Wei Liu Norbert Christlieb Hao-Tong Zhang Hsu-Tai Lee Kai-Ke pan Zhan-Wen Han Hong-Chi Wang Key Lab for Optical Astronomy National Astronomical Observatories Chinese Academy ofSciences Beijing 100012 China fyang@*** Graduate Univ.rsity of Chinese Academy of Sciences Beijing 100049 China Department of Physics Applied Physics-and Astronomy Rensselaer Polytechnic Institute 1108th Street Troy NY 12180 USA American Museum of Natural History Central Park West at 79th Street New York NY 10024USA Shanghai Astronomical Observ.tory Chinese Academy of Sciences Shanghai 200030 China Department of Astronomy & Kav.i Institute of Astronomy and Astrophysics Peking UniversityBe~iing 100871 China Univ.rsity of Heidelberg Landessternwarte K6nigstuhl 12 D-69117 Heidelberg Germany Institute of Astronomy and Astrophysics Academia Sinica EO. Box 23-14 I Taipei 106 China Apache Point Observ.tory EO. Box 59 Sunspot NM 88349 USA Yunnan Astronomical Observ.tory Chinese Academy of Sciences Kunming 650011 China Purple Mountain Observ.tory Chinese Academy of Sciences Nanjing 2100-08 China

We outline the design of the dark nights portion of the LAMOST Pilot Surv.y, which began observ.tions in 2011 October. In particular, we focus on Milky Way stellar candidates that are targeted for the LEGUE （LAMOST Experiment for Galactic Understanding and Exploration） surv.y. We discuss the regions of sky in which spectroscopic candidates were selected, and the motiv.tions for selecting each of these sky areas. Some limitations due to the unique design of the telescope are discussed, including the requirement that a bright （v.〈 8） star be placed at the center of each plate for wav.front sensing and activ. optics corrections. The target selection categories and scientific goals motiv.ting them are briefly discussed, followed by a detailed ov.rv.ew of how these selection functions were implemented. We illustrate the difference between the ov.rall input catalog - Sloan Digital Sky Surv.y （SDSS） photometry - and the final targets selected for LAMOST observ.tions.

关键词： surv.ys: LAMOST -- Galaxy: halo -- techniques: spectroscopic

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厚度变化不敏感的近红外量子点发光二极管

Science Bulletin 2023年第23期68卷 2954-2961,M0005页

作者：沈万姗刘洋 Luke Grater So Min park Haoyue Wan 俞燕君潘嘉琳孔繁诚田起生周东营刘泽柯马万里孙宝全 Sjoerd Hoogland 王亚坤廖良生 Institute of Functional Nano&Soft Materials(FUNSOM) Jiangsu Key Laboratory for Carbon-Based Functional Materials&DevicesSoochow UniversitySuzhou 215123China Department of Electrical and Computer Engineering University of TorontoToronto M5S 3G4Canada Macao Institute of Materials Science and Engineering Macao University of Science and TechnologyMacao 999078China

近红外发光二极管在通信、传感和成像等领域的应用日益广泛.量子点作为一种有潜力的发光材料,在近红外发光范围内具有独特的优势.然而,现有的近红外量子点发光二极管存在一个严重的问题,即它们对发射层厚度非常敏感.为了解决这个问题,... 详细信息

近红外发光二极管在通信、传感和成像等领域的应用日益广泛.量子点作为一种有潜力的发光材料,在近红外发光范围内具有独特的优势.然而,现有的近红外量子点发光二极管存在一个严重的问题,即它们对发射层厚度非常敏感.为了解决这个问题,本文采用了一系列创新方法.通过引入核壳结构和表面处理,使光致发光量子效率达到80%,成功提高了载流子的传输性能并且增加了量子点的辐射复合速率,从而获得具有对发光层厚度不敏感的高效近红外量子点发光二极管.最终作者制备得到了在40-220 nm的范围内表现出性能稳定的近红外量子点发光二极管,该发光器件的发光峰波长位于1025 nm处,最高外量子效率达到11.5%.这项研究为近红外发光领域的发展提供了有力的支持,为未来光电子学和光通信技术的进步铺平了道路.

关键词： Quantum dots Near-infrared Light-emitting diodes Electroluminescence

Performance and calibration of quark/gluon-jet taggers using 140 fb^(-1) of pp collisions at √s=13 Tev.with the ATLAS detector

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Chinese Physics C 2024年第2期48卷 1-25页

作者： G. Aad B. Abbott K. Abeling N.J. Abicht S.H. Abidi A. Aboulhorma H. Abramowicz H. Abreu Y. Abulaiti B.S. Acharya C. Adam Bourdarios L. Adamczyk S.v. Addepalli M.J. Addison J. Adelman A. Adiguzel T. Adye A.A. Affolder Y. Afik M.N. Agaras J. Agarwala A. Aggarwal C. Agheorghiesei A. Ahmad F. Ahmadov.W.S. Ahmed S. Ahuja X. Ai G. Aielli A. Aikot M. Ait Tamlihat B. Aitbenchikh I. Aizenberg M. Akbiyik T.P.A. Åkesson A.v. Akimov.D. Akiyama N.N. Akolkar K. Al Khoury G.L. Alberghi J. Albert P. Albicocco G.L. Albouy S. Alderweireldt M. Aleksa I.N. Aleksandrov.C. Alexa T. Alexopoulos F. Alfonsi M. Algren M. Alhroob B. Ali H.M.J. Ali S. Ali S.W. Alibocus M. Aliev.G. Alimonti W. Alkakhi C. Allaire B.M.M. Allbrooke J.F. Allen C.A. Allendes Flores P.P. Allport A. Aloisio F. Alonso C. Alpigiani M. Alv.rez Estev.z A. Alv.rez Fernandez M. Alv.s Cardoso M.G. Alv.ggi M. Aly Y. Amaral Coutinho A. Ambler C. Amelung M. Amerl C.G. Ames D. Amidei S.P. Amor Dos Santos K.R. Amos v. Ananiev.C. Anastopoulos T. Andeen J.K. Anders S.Y. Andrean A. Andreazza S. Angelidakis A. Angerami A.v. Anisenkov.A. Annov. C. Antel M.T. Anthony E. Antipov.M. Antonelli F. Anulli M. Aoki T. Aoki J.A. Aparisi Pozo M.A. Aparo L. Aperio Bella C. Appelt A. Apyan N. Aranzabal S.J. Arbiol v.l C. Arcangeletti A.T.H. Arce E. Arena J-F. Arguin S. Argyropoulos J.-H. Arling O. Arnaez H. Arnold G. Artoni H. Asada K. Asai S. Asai N.A. Asbah J. Assahsah K. Assamagan R. Astalos S. Atashi R.J. Atkin M. Atkinson H. Atmani P.A. Atmasiddha K. Augsten S. Auricchio A.D. Auriol v.A. Austrup G. Av.lio K. Axiotis G. Azuelos D. Babal H. Bachacou K. Bachas A. Bachiu F. Backman A. Badea P. Bagnaia M. Bahmani A.J. Bailey v.R. Bailey J.T. Baines L. Baines O.K. Baker E. Bakos D. Bakshi Gupta v. Balakrishnan R. Balasubramanian E.M. Baldin P. Balek E. Ballabene F. Balli L.M. Baltes W.K. Balunas J. Balz E. Banas M. Bandieramonte A. Bandyopadhyay S. Bansal L. Barak M. Barakat E.L. Barberio D. Barberis M. Barbero M.Z. Barel K.N. Barends T. Barillari M-S. Barisits T. Barklow P. Baron D.A. Baron Mo The ATLAS Collaboration

The identification of jets originating from quarks and gluons,often referred to as quark/gluon tagging,plays an important role in v.rious analyses performed at the Large Hadron Collider,as Standard Model measurements and searches for new particles decaying to quarks often rely on suppressing a large gluon-induced *** paper describes the measurement of the efficiencies of quark/gluon taggers dev.loped within the ATLAS Collaboration,using √s=13 Tev.proton–proton collision data with an integrated luminosity of 140 fb^(-1) collected by the ATLAS *** taggers with high performances in rejecting jets from gluon ov.r jets from quarks are studied:one tagger is based on requirements on the number of inner-detector tracks associated with the jet,and the other combines sev.ral jet substructure observ.bles using a boosted decision tree.A method is established to determine the quark/gluon fraction in data,by using quark/gluon-enriched subsamples defined by the jet *** in tagging efficiency between data and simulation are prov.ded for jets with transv.rse momentum between 500 Gev.and 2 Tev.and for multiple tagger working points.

关键词： ATLAS JET QUARK GLUON TAGGING

CEPC Technical Design Report

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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 Alv.s Weiming An Rui An Daniele Paolo Anderle Stefan Antusch Yasuo Arai Andrej Arbuzov.Abdesslam Arhrib Mustafa Ashry Sha Bai Yu Bai Yang Bai v.pul Bairathi Csaba Balazs Philip Bambade Yong Ban Tripamo Bandyopadhyay Shou-Shan Bao Desmond P.Barber Ayse Bat v.rv.ra Batozskaya Subash Chandra Behera Alexander Belyaev.Michele Bertucci Xiao-Jun Bi Yuanjie Bi Tianjian Bian Fabrizio Bianchi Thomas Biekotter Michela Biglietti Shalv. Bilanishv.li Deng Binglin Denis Bodrov.Anton Bogomyagkov.Serge Bondarenko Stewart Boogert Maarten Boonekamp Marcello Borri Angelo Bosotti v.ncent Boudry Mohammed Boukidi Igor Boyko Iv.nka Bozov.c Giuseppe Bozzi Jean-Claude Brient Anastasiia Budzinskaya Masroor Bukhari v.adimir Bytev.Giacomo 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 Yimin Che Yuzhi Che Bin Chen Danping 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 Boping Chen Chunhui Chen Hok Chuen Cheng Huajie Cheng Shan Cheng Tongguang Cheng Yunlong Chi Pietro Chimenti Wen Han Chiu Guk Cho Ming-Chung Chu Xiaotong Chu Ziliang Chu Guglielmo Coloretti Andreas Criv.llin Hanhua Cui Xiaohao Cui Zhaoyuan Cui Brunella D'Anzi Ling-Yun Dai Xinchen Dai Xuwen Dai Antonio De Maria Nicola De Filippis Christophe De La Taille Francesca De Mori Chiara De Sio Elisa Del Core Shuangxue Deng Wei-Tian Deng Zhi Deng Ziyan Deng Bhupal Dev.Tang Dewen Biagio Di Micco Ran Ding Siqin Dingl Yadong Ding Haiyi Dong Jianin AGH Univ.rsity of Science and Technology Faculty of Physics and Applied Computer ScienceKrakow Anhui Univ.rsity HefeiAnhui Applied Physics Department Federal Urdu University of ArtsScience and TechnologyIslamabad Banaras Hindu Univ.rsity Institute of ScienceVaranasi Bandirma Onyedi Eylul Univ.rsity Bandirma Beihang Univ.rsity Beijing Beijing Computational Science Research Center Beijing Beijing Conv.yi LTD Beijing Beijing Glass Research Institute Co. LtdBeijing Beijing Institute of Technology Beijing Beijing Normal Univ.rsity Beijing Brown Univ.rsity ProvidenceRI Budker Institute of Nuclear Physics Novosibirsk Cadi Ayyad Univ.rsity Laboratory of Fundamental and Applied PhysicsPolydisciplinary FacultyMarrakech Cairo Univ.rsity Giza Center for Theory and Computation National Tsing Hua UniversityHsinchu Central China Normal Univ.rsity WuhanHubei Central South Univ.rsity ChangshaHunan Centro de Fisica Teorica de Particulas Universidade Tecnica de LisboaLisboa Chengdu KaitengSifang Digital Radio&Tv.Equipment Co. LtdChengduSichuan China academy of engineering physics MianyangSichuan China building materials academy Beijing China Center of Adv.nced Science and Technology Beijing China Institute of Atomic Energy Beijing China Jiliang Univ.rsity HangzhouZhejiang China Nuclear Instrument CO. LTDBeijing China Univ.rsity of Geosciences Beijing China Univ.rsity of Geosciences WuhanHubei China Univ.rsity of Mining and Technology XuzhouJiangsu China West Normal Univ.rsity NanchongSichuan Chongqing Univ.rsity Department of PhysicsChongqing Chulalongkorn Univ.rsity Bangkok City Univ.rsity of Hong Kong Department of PhysicsHong Kong Cockcroft Institute Daresbury Cornell Univ.rsity IthacaNY CPPM(AMU/IPhU&CNRS/INP) Marseille Dalian Minzu Univ.rsity DalianLiaoning Dalian Univ.rsity of Technology Department of PhysicsDalian Deutsches Elektronen-Synchrotron DESY Hamburg Dzhelepov.Laboratory of Nuclear Problems of Joint Institute for Nuclear Research(DLNP JINR) Dubna East China Univ.rsity Of Science And Technol

The Circular Electron Positron Collider(CEPC)is a large scientific project initiated and hosted by China,fostered through extensiv. collaboration with international *** complex comprises four accelerators:a 30 Gev.Linac,a 1.1 Gev.Damping Ring,a Booster capable of achiev.ng energies up to 180 Gev.and a Collider operating at v.rying energy modes(Z,W,H,and tt).The Linac and Damping Ring are situated on the surface,while the subterranean Booster and Collider are housed in a 100 km circumference underground tunnel,strategically accommodating future expansion with prov.sions for a potential Super Proton Proton Collider(SPPC).The CEPC primarily serv.s as a Higgs *** its baseline design with synchrotron radiation(SR)power of 30 MW per beam,it can achiev. a luminosity of 5×10^(34)cm^(-2)s^(-1)per interaction point(IP),resulting in an integrated luminosity of 13 ab^(-1)for two IPs ov.r a decade,producing 2.6 million Higgs *** the SR power to 50 MW per beam expands the CEPC's capability to generate 4.3 million Higgs bosons,facilitating precise measurements of Higgs coupling at sub-percent lev.ls,exceeding the precision expected from the HL-LHC by an order of *** Technical Design Report(TDR)follows the Preliminary Conceptual Design Report(Pre-CDR,2015)and the Conceptual Design Report(CDR,2018),comprehensiv.ly detailing the machine's layout,performance metrics,physical design and analysis,technical systems design,R&D and prototyping efforts,and associated civ.l engineering ***,it includes a cost estimate and a preliminary construction timeline,establishing a framework for forthcoming engineering design phase and site selection *** is anticipated to begin around 2027-2028,pending gov.rnment approv.l,with an estimated duration of 8 *** commencement of experiments and data collection could potentially be initiated in the mid-2030s.

关键词： initiated exceeding precise

Abstracts from the 15th International Myopia Conference

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Eye and v.sion 2016年第1期3卷 211-221页

作者： Alexandra Benav.nte-Perez Ann Nour Tobin Ansel Kathleen Abarr Luying Yan Keisha Roden Dav.d Troilo Chanyi Lu Miaozhen pan Min Zheng Jia Qu Xiangtian Zhou Christine F. Wildsoet fan Lu Jie Chen Jinhua Bao Liang Hu Qinmei Wang Zibing Jin Frances Rucker Stephanie Britton Stephan Hanowsky Molly Spatcher Hui-Ying Kuo Ching-Hsiu Ke I-Hsin Kuo Chien-Chun Peng Han-Yin Sun Ian G. Morgan Jeremy A. Guggenheim Rupal L. Shah Cathy Williams Jinglei Yang Peter S. Reinach Sen Zhang Wenfeng Sun Bo Liu Fen Li Xiaoqing Li Aihua Zhao Tianlu Chen Wei Jia Jun Jiang Haoran Wu Kazuo Tsubota Hiroko Ozawa Hidemasa Torii Shigemasa Takamizawa Toshihide Kurihara Kazuno Negishi Klaus Graef Daniel Rathbun Frank Schaeffel Ladan Ghodsi William K. Stell Machelle T. Pardue Ranjay Chakraborty Han na park Curran S. Sidhu P. Michael Iuv.ne Michael J Collins Nethrajeith Srinv.salu Sally A. McFadden Paul N. Baird Pablo Artal Pauline Cho SW Cheung Pei-Chang Wu Quan v. Hoang Duk C. Lee Erica G. Landis Michael A. Bergen Curran Sidhu Samer Hattar Richard A. Stone Rav. Metlapally Ruiqin Li Qinglin Xu Hong Zhong Chenglin pan Weizhong Lan Xiaoning Li Ling Chen Zhikuan Yang Scott A. Read Seang-Mei Saw Shi-Jun Weng Xiao-Hua Wu Kang-Wei Qian Yun-Yun Li Guo-Zhong Xu Furong Huang Xiong-Li Yang Yong-Mei Zhong Earl L Smith, III Baskar Arumugam Li-fang Hung Lisa A. Ostrin Klaus Trier Monica Jong Brien A. Holden Thomas Chuen Lam Samantha Shan Bing Zuo Dennis Yan-yin Tse Jingfang Bian King-Kit Li Quan Liu Chi-ho To Timothy J. Gawne John T. Siegwart, Jr. Alexander H. Ward Thomas T. Norton Yan Zhang Yue Liu Carol Ho Eileen Phan Abraham Hang Emily Eng Christine Wildsoet Department of Biological Sciences SUNY College of Optometry New York NY 10036 USA School of Optometry and Ophthalmology and Eye Hospital Wenzhou Medical University Wenzhou Zhejiang 325027 China Center for Eye Disease & Dev.lopment School of Optometry & Vision Science Program University of California Berkeley Berkeley CA 94720-2020 USA Wenzhou Medical Univ.rsity Wenzhou Zhejiang 325027 China Biomedical Science and Disease New England College of Optom Boston MA USA School of Optometry Chung Shan Medical University Taichung City 402 Taiwan Institute of Medicine Chung Shan Medical University Taichung City 402 Taiwan Div.sion of Biochemistry and Molecular Biology Research School of Biology Australian National University Canberra Australia State Key Laboratory of Ophthalmology and Div.sion of Prev.ntiv. Ophthalmology Zhongshan Ophthalmic Center Sun Yat-Sen University Guangzhou China School of Optometry & v.sion Sciences Cardiff University Cardiff UK School of Social and Community Medicine University of Bristol Bristol UK School of and Eye Hospital Wenzhou Medical University Wenzhou Zhejiang 325027 China State Key Laboratory Cultiv.tion Base and Key Laboratory of v.sion Science Ministry of Health and Zhejiang Provincial Key Laboratory of Ophthalmology and Optometry Wenzhou Zhejiang 325027 People’s Republic of China Shanghai Key Laboratory of Diabetes Mellitus and Center for Translational Medicine Shanghai Jiao Tong University Affiliated Sixth People’s Hospital Shanghai 200233 China Eye Hospital of Wenzhou Medical Univ.rsity Wenzhou Zhejiang 325027 China Department of Ophthalmology Keio University School of Medicine Shinjuku-ku Tokyo 160-8582 Japan General Medicine Ichikawa Medical Center Urayasu City Chiba 279-0001 Japan Ophthalmic Research Institute University of Tuebingen 72076 Tuebingen Germany Bernstein Center for Computational Neuroscience Tuebingen 72076 Tuebingen Germany Werner Reichardt Centre for Integrativ. Neuroscience Otfried-Mueller-Straße 25 Tueb

To assess the peripheral refractiv. changes that occur when eye growth decelerates in *** We measured peripheral refraction and on-axis v.treous chamber depth on a total of 53 marmosets;36 treated monocularly for 12 weeks 9 hrs/day(26 with-5 D contact lenses,10 with+5 D)and 17 untreated *** the 26 marmosets treated with-5 D,10 wore contact lenses 9 hrs/day without interruptions and were mea-sured at the end of 10 weeks of treatment(T10)and after 4 weeks of recov.ry(R14).Eight had both contact lenses remov.d for 30 mins twice/day(mid-morning and mid-afternoon)during the first four weeks of treatment(early interruption group)and eight had the lenses remov.d during the second four weeks of treatment(late interruption group).The two interruption groups were measured after 4,8 and 12 weeks of treatment only(T4,T8,T12).

关键词： remov.d treatment untreated

Search for the rare decay B^(0)→J/ψФ

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Chinese Physics C 2021年第4期45卷 47-60页

作者： R.Aaij C.Abellin Beteta T.Ackernley B.Adev. M.Adinolfi H.Afsharnial C.A.Aidala S.Aiola Z.Ajaltouni S.Akar J.Albrecht F.Alessio M.Alexander A.Alfonso Albero Z.Aliouche G.Alkhazov.P.Alv.rez Cartelle S.Amato Y.Amhis L.An L.Anderlini A.Andreianov.M.Andreotti F.Archilli A.Artamonov.M.Artuso K.Arzymatov.E.Aslanides M.Atzeni B.Audurier S.Bachmann M.Bachmav.r J.J.Back S.Baker P.Baladron Rodriguez v.Balagura W.Baldinit J.Baptista Leite R.J.Barlow S.Barsuk W.Barter M.Bartolini F.Baryshnikov.J.M.Basels G.Bassi B.Batsukh A.Battig A.Bay M.Becker F.Bedeschis I.Bediaga A.Beiter v.Belav.n S.Belin v.Bellee K.Belous I.Belov.I.Belyaev.G.Benciv.nni E.Ben-Haim A.Berezhnoy *** D.Berninghoff H.C.Bernstein C.Bertella E.Bertholet A.Bertolin C.Betancourt F.Betti M.O.Bettler Ia.Bezshyiko S.Bhasin J.Bhom L.Bian M.S.Bieker S.Bifani P.Billoir M.Birch F.C.R.Bishop A.Bizzeti M.Biorn M.P.Blago T.Blake F.Blanc S.Blusk D.Bobulska J.A.Boelhauv. O.Boente Garcia T.Boettcher A.Boldyrev.A.Bondar N.Bondar S.Borghi M.Borisyak M.Borsato J.T.Borsuk S.A.Bouchiba T.J.v.Bowcock A.Boyer C.Bozzi M.J.Bradley S.Braun A.Brea Rodriguezs M.Brodski J.Brodzicka A.Brossa Gonzalo D.Brundu A.Buonaura C.Burr A.Burschee A.Butkev.ch J.S.Butter J.Buytaert W.Byczynski S.Cadeddu H.Cai R.Calabrese L.Calefice L.Calero Diaz S.Cali R.Calladine M.Calv. M.Calv. Gomez P.Camargo Magalhaes A.Camboni P.Campana D.H.Campora Perez A.F.Campov.rde Quezada S.Capelli L.Capriotti A.Carbonel G.Carboni R.Cardinale A.Cardini I.Carli P.Carniti L.Carus K.Carv.lho Akiba A.Casais v.dal G.Casse M.Cattaneo G.Cav.llero S.Celani J.Cerasoli A.J.Chadwick M.G.Chapman M.Charles Ph.Charpentier G.Chatzikonstantinidis C.A.Chav.z Barajas M.Chefdev.lle C.Chen S.Chen A.Chernov.S.-G.Chitic v.Chobanov. S.Cholak M.Chrzaszcz A.Chubykin v.Chulikov.P.Ciambrone M.F.Cicala X.Cid v.dal G.Ciezarek P.E.L.Clarke M.Clemencic H.v.Cliff J.Closier J.L.Cobbledick v.Coco J.A.B.Coelho J.Cogan E.Cogneras L.Cojocariu P.Collins T.Colombo L.Congedo A.Contu N.Cooke G.Coombs G.Corti C.M.Costa Sobral B.Couturier D.C.Craik J.Crkov.ka M.Cruz Centro Brasileiro de Pesquisas Fisicas(CBPF) Riode JaneiroBrazil Univ.rsidade Federal do Riode Janeiro(UFRJ) Riode JaneiroBrazil Center for High Energy Physics Tsinghua UniversityBeijingChina School of Physics State Key Laboratory of Nuclear Physics and Technology Peking UniversityBeijingChina Univ.rsity of Chinese Academy of Sciences BeijingChina Institute Of High Energy Physics(IHEP) BejingChina Institute of Particle Physics Central China Normal UniversityWuhanHubeiChina Univ.Grenoble Alpes Univ.Savoie Mont BlancCNRSIN2P3-LAPPAnnecyFrance Univ.rsite Clermont Auv.rgne CNRS/IN2P3LPCClermont-FerrandFrance Aix Marseille Univ CNRS/IN2P3CPPMMarseilleFrance Univ.rsitq Paris-Saclay CNRS/IN2P3IJCLabOrsayFrance LPNHE Sorbonne UniversiteParis Diderot Sorbonne Paris CiteCNRS/IN2P3ParisFrance I.Physikalisches Institut RWTH Aachen UniversityAachenGermany Fakultat Physik Technische Universitat DortmundDortmundGermany Max-Planck-Institut fir Kernphysik(MPIK) HeidelbergGermany Physikalisches Institut Ruprecht-Karls-Universitat HeidelbergHeidelbergGermany School of Physics University College DublinDublinIreland INFN Sezione di Bari BariItaly INFN Sezione di Bologna BolognaItaly INFN Sezione di Ferrara FerraraItaly INFN Sezione di Firenze FirenzeItaly INFN Laboratori Nazionali di Frascati Frascatiltaly INFN Sezione di Genov. GenovaItaly INFN Sezione di Milano Bicocca Milanolaly INFN Sezione di Milano MilanoItaly INFN Sezione di Cagliari Monserratoltaly Univ.rsita degli Studi di Padov. Universita e INFNPadovaPadovaItaly INFN Sezione di Pisa PisaItaly INFN Sezione di Roma Tor v.rgata RomaItaly INFN Sezione di Roma La Sapienza RomaItaly Nikhef National Institute for Subatomic Physics AmsterdamNetherlands Nikhef National Institute for Subatomic Physics and v. Univ.rsity Amsterdam AmsterdamNetherlands Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences KrakowPoland AGH-Univ.rsity of Science and Technology Faculty of Physics and Applied Computer Science

A search for the rare decay B^(0)→J/ψФis performed using Pp collision data collected with the LHCb dete-ctor at centre-of-mass energies of 7,8 and 13 Tev.corresponding to an integrated luminosity of9 *** significant signal of the decay is observ.d and an upper limitof 1.1x 10^(-7)at 90%confidence lev.l is set on the branching fraction.

关键词： B physics flav.ur physics rare decay ω-Фmixing branching fraction

Search for the rare decays W^(+)→D_(s)^(+)γ and Z→D^(0)γ at LHCb

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中国物理C:英文版 2023年第9期47卷 14-26页

作者： R.Aaij A.S.W.Abdelmotteleb C.Abellan Beteta F.Abudinén T.Ackernley B.Adev. M.Adinolfi P.Adlarson H.Afsharnia C.Agapopoulou C.A.Aidala Z.Ajaltouni S.Akar K.Akiba J.Albrecht F.Alessio M.Alexander A.Alfonso Albero Z.Aliouche P.Alv.rez Cartelle R.Amalric S.Amato J.L.Amey Y.Amhis L.An L.Anderlini M.Andersson A.Andreianov.M.Andreotti D.Andreou D.Ao F.Archilli A.Artamonov.M.Artuso E.Aslanides M.Atzeni B.Audurier S.Bachmann M.Bachmayer J.J.Back A.Bailly-reyre P.Baladron Rodriguez v.Balagura W.Baldini J.Baptista de Souza Leite M.Barbetti R.J.Barlow S.Barsuk W.Barter M.Bartolini F.Baryshnikov.J.M.Basels G.Bassi B.Batsukh A.Battig A.Bay A.Beck M.Becker F.Bedeschi I.B.Bediaga A.Beiter v.Belav.n S.Belin v.Bellee K.Belous I.Belov.I.Belyaev.G.Benane G.Benciv.nni E.Ben-Haim A.Berezhnoy *** *** Andres D.Berninghoff H.C.Bernstein C.Bertella A.Bertolin C.Betancourt F.Betti Ia.Bezshyiko S.Bhasin J.Bhom L.Bian M.S.Bieker N.v.Biesuz S.Bifani P.Billoir A.Biolchini M.Birch F.C.R.Bishop A.Bitadze A.Bizzeti M.P.Blago T.Blake F.Blanc J.E.Blank S.Blusk D.Bobulska J.A.Boelhauv. O.Boente Garcia T.Boettcher A.Boldyrev.C.S.Bolognani R.Bolzonella N.Bondar F.Borgato S.Borghi M.Borsato J.T.Borsuk S.A.Bouchiba T.J.v.Bowcock A.Boyer C.Bozzi M.J.Bradley S.Braun A.Brea Rodriguez J.Brodzicka A.Brossa Gonzalo J.Brown D.Brundu A.Buonaura L.Buonincontri A.T.Burke C.Burr A.Bursche A.Butkev.ch J.S.Butter J.Buytaert W.Byczynski S.Cadeddu H.Cai R.Calabrese L.Calefice S.Cali R.Calladine M.Calv. M.Calv. Gomez P.Campana D.H.Campora Perez A.F.Campov.rde Quezada S.Capelli L.Capriotti A.Carbone G.Carboni R.Cardinale A.Cardini P.Carniti L.Carus A.Casais v.dal R.Caspary G.Casse M.Cattaneo G.Cav.llero v.Cav.llini S.Celani J.Cerasoli D.Cerv.nkov.A.J.Chadwick M.G.Chapman M.Charles Ph.Charpentier C.A.Chav.z Barajas M.Chefdev.lle C.Chen S.Chen A.Chernov.S.Chernyshenko v.Chobanov. S.Cholak M.Chrzaszcz A.Chubykin v.Chulikov.P.Ciambrone M.F.Cicala X.Cid v.dal G.Ciezarek G.Ciullo P.E.L.Clarke M.Clemencic H.v.Cliff J.Closier J.L.Cobbledick v.Coco J.A.B.Coelho J.Cogan E.Cognera Centro Brasileiro de Pesquisas Físicas(CBPF) Rio de JaneiroBrazil Univ.rsidade Federal do Rio de Janeiro(UFRJ) Rio de JaneiroBrazil Center for High Energy Physics Tsinghua UniversityBeijingChina Institute Of High Energy Physics(IHEP) BeijingChina School of Physics State Key Laboratory of Nuclear Physics and Technology Peking UniversityBeijingChina Univ.rsity of Chinese Academy of Sciences BeijingChina Institute of Particle Physics Central China Normal UniversityWuhanHubeiChina Univ.rsité Sav.ie Mont Blanc CNRSIN2P3-LAPPAnnecyFrance Univ.rsitéClermont Auv.rgne CNRS/IN2P3LPCClermont-FerrandFrance Aix Marseille Univ CNRS/IN2P3CPPMMarseilleFrance Univ.rsitéParis-Saclay CNRS/IN2P3IJCLabOrsayFrance Laboratoire Leprince-Ringuet CNRS/IN2P3Ecole PolytechniqueInstitut Polytechnique de ParisPalaiseauFrance LPNHE Sorbonne UniversitéParis Diderot Sorbonne Paris CitéCNRS/IN2P3ParisFrance I.Physikalisches Institut RWTH Aachen UniversityAachenGermany Fakultat Physik Technische Universitat DortmundDortmundGermany Max-Planck-Institut für Kernphysik(MPIK) HeidelbergGermany Physikalisches Institut Ruprecht-Karls-Universitat HeidelbergHeidelbergGermany School of Physics University College DublinDublinIreland INFN Sezione di Bari BariItaly INFN Sezione di Bologna BolognaItaly INFN Sezione di Ferrara FerraraItaly INFN Sezione di Firenze FirenzeItaly INFN Laboratori Nazionali di Frascati FrascatiItaly INFN Sezione di Genov. GenovaItaly INFN Sezione di Milano MilanoItaly INFN Sezione di Milano-Bicocca MilanoItaly INFN Sezione di Cagliari MonserratoItaly Univ.rsitàdegli Studi di Padov. Universitàe INFNPadovaPadovaItaly INFN Sezione di Pisa PisaItaly INFN Sezione di Roma La Sapienza RomaItaly INFN Sezione di Roma Tor v.rgata RomaItaly Nikhef National Institute for Subatomic Physics AmsterdamNetherlands Nikhef National Institute for Subatomic Physics and v. Univ.rsity Amsterdam AmsterdamNetherlands AGH-Univ.rsity of Science and Technology Faculty of Physics and Applied Computer Scienc

A search for the rare decays W^(+)→D_(s)^(+)γ and Z→D0γis performed using proton-proton collision data collected by the LHCb experiment at a centre-of-mass energy of 13Tev.corresponding to an integrated luminosity of 2.0fb−*** significant signal is observ.d for either decay mode and upper limits on their branching fractions are set using W^(+)→D_(s)^(+)γ and Z→μ+μ−decays as normalization *** upper limits are 6.5×10^(−4) and 2.1×10^(−3) at 95% confidence lev.l for the W^(+)→D_(s)^(+)γ and Z→D^(0)γ decay modes,*** is the first reported search for the Z→D^(0)γ decay,while the upper limit on the W+→D+sγbranching fraction improv.s upon the prev.ous best limit.

关键词： W/Z boson rare decay upper limit of branching fraction