检索结果-南通市图书馆

frontiers of physics 2024年第1期19卷 1-154页

作者： M.Achasov x.C.Ai l.P.An R.Aliberti q.An x.z.bai Y.bai O.bakina A.barnyakov V.blinov V.bobrovnikov D.bodrov A.bogomyagkov A.bondar I.boyko z.h.bu f.M.Cai h.Cai J.J.Cao q.h.Cao x.Cao z.Cao q.Chang K.T.Chao D.Y.chen h.chen h.x.chen J.f.chen K.chen l.l.chen P.chen S.l.chen S.M.chen S.chen S.P.chen W.chen x.chen x.f.chen x.R.chen Y.chen Y.q.chen h.Y.cheng J.cheng S.cheng T.G.cheng J.P.Dai l.Y.Dai x.C.Dai D.Dedovich A.Denig I.Denisenko J.M.Dias D.z.Ding l.Y.Dong W.h.Dong V.Druzhinin D.S.Du Y.J.Du z.G.Du l.M.Duan D.Epifanov Y.l.fan S.S.fang z.J.fang G.fedotovich C.q.feng x.feng Y.T.feng J.l.fu J.Gao Y.N.Gao P.S.Ge C.q.Geng l.S.Geng A.Gilman l.Gong T.Gong b.Gou W.Gradl J.l.Gu A.Guevara l.C.Gui A.q.Guo f.K.Guo J.C.Guo J.Guo Y.P.Guo z.h.Guo A.Guskov K.l.han l.han M.han x.q.hao J.b.he S.q.he x.G.he Y.l.he z.b.he z.x.heng b.l.hou T.J.hou Y.R.hou C.Y.hu h.M.hu K.hu R.J.hu W.h.hu x.h.hu Y.C.hu J.hua G.S.huang J.S.huang M.huang q.Y.huang W.q.huang x.T.huang x.J.huang Y.b.huang Y.S.huang N.hüsken V.Ivanov q.P.Ji J.J.Jia S.Jia z.K.Jia h.b.Jiang J.Jiang S.z.Jiang J.b.Jiao z.Jiao h.J.Jing x.l.Kang x.S.Kang b.C.Ke M.Kenzie A.Khoukaz I.Koop E.Kravchenko A.Kuzmin Y.lei E.levichev C.h.li C.li D.Y.li f.li G.li G.li h.b.li h.li h.N.li h.J.li h.l.li J.M.li J.li l.li l.li l.Y.li N.li P.R.li R.h.li S.li T.li W.J.li x.li x.h.li x.q.li x.h.li Y.li Y.Y.li z.J.li h.liang J.h.liang Y.T.liang G.R.liao l.z.liao Y.liao C.x.lin D.x.lin x.S.lin b.J.liu C.W.liu D.liu f.liu G.M.liu h.b.liu J.liu J.J.liu J.b.liu K.liu K.Y.liu K.liu l.liu q.liu S.b.liu T.liu x.liu Y.W.liu Y.liu Y.l.liu z.q.liu z.Y.liu z.W.liu I.logashenko Y.long C.G.lu J.x.lu N.lu q.f.lü Y.lu Y.lu z.lu P.lukin f.J.luo T.luo x.f.luo Y.h.luo h.J.lyu x.R.lyu J.P.Ma P.Ma Y.Ma Y.M.Ma f.Maas S.Malde D.Matvienko z.x.Meng R.Mitchell A.Nefediev Y.Nefedov S.l.Olsen q.Ouyang P.Pakhlov G.Pakhlova x.Pan Y.Pan E.Passemar Y.P.Pei h.P.Peng l.Peng x.Y.Peng x.J.Peng K.Peters S.Pivovarov E.Pyata b.b.qi Y.q.qi W.b.qian Y.qian C.f.qiao J.J.qin J.J.qin l.q.qin x.S.qin T.l.qiu J.Rademacker C.f.Redmer h.Y.Sang Anhui university Hefei 230039China beihang university Beijing 100191China budker Institute of Nuclear Physics Novosibirsk 630090Russia CAS key laboratory of Theoretical Physics Institute of Theoretical PhysicsChinese Academy of SciencesBeijing 100190China Cavendish laboratory University of CambridgeJJ Thomson AveCambridge CB30HEUnited Kingdom Central china Normal university Wuhan 430079China Central South university Changsha 410083China china university of Geosciences Wuhan 430074China china university of Mining and Technology Xuzhou 221116China École Polytechnique fédérale de lausanne(EPfl) LausanneSwitzerland fudan university Shanghai 200433China Goethe university frankfurt D-60325 Frankfurt am MainGermany Guangxi Normal university Guilin 541004China Guangxi Uninversity Nanning 530004China hangzhou Institute for Advanced Study UCASHangzhou 310024China hebei Normal university Shijiazhuang 050024China hebei university Baoding 071002China hefei university of Technology Hefei 230601China helmholtz Institute Mainz Staudinger Weg 18D-55099 MainzGermany henan Normal university Xinxiang 453007China henan university Kaifeng 475004China high Energy Physics Center Chung-Ang UniversitySeoul 06974Korea higher School of Economy 11 Pokrovsky bulvar Moscow 109028Russia huangshan university Huangshan 245000China hubei university of Automotive Technology Shiyan 442002China hunan Normal university Changsha 410081China hunan university of Science and Technology Xiangtan 411201China hunan university Changsha 410082China Indiana university BloomingtonIndiana 47405USA Inner Mongolia university Hohhot 010021China Institute of Advanced Science facilities Shenzhen 518107China Institute of high Energy Physics Chinese Academy of SciencesBeijing 100049China Institute of Modern Physics Chinese Academy of SciencesLanzhou 730000China Institute of Physics Academia SinicaTaipeiTaiwan 11529China Institute of Theoretical Physics Chinese Academy of SciencesBeijing 100190China Jilin university Changch

The superτ-charm facility(STCf)is an electron–positron collider proposed by the Chinese particle physics *** is designed to operate in a center-of-mass energy range from 2 to 7 GeV with a peak luminosity of 0.5×10^(35) cm^(–2)·s^(–1) or *** STCf will produce a data sample about a factor of 100 larger than that of the presentτ-charm factory—the bEPCII,providing a unique platform for exploring the asymmetry of matter-antimatter(charge-parity violation),in-depth studies of the internal structure of hadrons and the nature of non-perturbative strong interactions,as well as searching for exotic hadrons and physics beyond the Standard *** STCf project in china is under development with an extensive R&D *** document presents the physics opportunities at the STCf,describes conceptual designs of the STCf detector system,and discusses future plans for detector R&D and physics case studies.

关键词： electron–positron collider tau-charm region high luminosity STCf detector conceptual design

Amplitude analysis of the decays D^(0)→π^(+)π^(−)π^(+)π^(−)and D^(0)→π^(+)π^(−)π^(0)π^(0)

在线全文

维普期刊数据库

学校读者我要写书评

暂无评论

Chinese Physics C 2024年第8期48卷 6-33页

作者： M.Ablikim M.N.Achasov P.Adlarson O.Afedulidis x.C.Ai R.Aliberti A.Amoroso q.An Y.bai O.bakina I.balossino Y.ban h.-R.bao V.batozskaya K.begzsuren N.berger M.berlowski M.bertani D.bettoni f.bianchi E.bianco A.bortone I.boyko R.A.briere A.brueggemann h.Cai x.Cai A.Calcaterra G.f.Cao N.Cao S.A.Cetin J.f.Chang W.l.Chang G.R.Che G.Chelkov C.chen C.h.chen Chao chen G.chen h.S.chen M.l.chen S.J.chen S.l.chen S.M.chen T.chen x.R.chen x.T.chen Y.b.chen Y.q.chen z.J.chen z.Y.chen S.K.Choi x.Chu G.Cibinetto f.Cossio J.J.Cui h.l.Dai J.P.Dai A.Dbeyssi R.E.de boer D.Dedovich C.q.Deng z.Y.Deng A.Denig I.Denysenko M.Destefanis f.De Mori b.fang S.S.fang W.x.fang Y.fang Y.q.fang R.farinelli l.fava f.feldbauer G.felici C.q.feng J.h.feng Y.T.feng K.fischer M.fritsch C.D.fu J.l.fu Y.W.fu h.Gao Y.N.Gao Yang Gao S.Garbolino I.Garzia P.T.Ge z.W.Ge C.Geng E.M.Gersabeck b.Ding x.x.Ding Y.Ding Y.Ding J.Dong l.Y.Dong M.Y.Dong x.Dong M.C.Du S.x.Du z.h.Duan P.Egorov Y.h.fan J.fang JA.Gilman K.Goetzen l.Gong W.x.Gong W.Gradl S.Gramigna M.Greco M.h.Gu Y.T.Gu C.Y.Guan z.l.Guan A.q.Guo l.b.Guo M.J.Guo R.P.Guo Y.P.Guo A.Guskov J.Gutierrez K.l.han T.T.han x.q.hao f.A.harris K.K.he K.l.he f.h.heinsius C.h.heinz Y.K.heng C.herold T.holtmann P.C.hong G.Y.hou x.T.hou Y.R.hou z.l.hou b.Y.hu h.M.hu J.f.hu T.hu Y.hu G.S.huang K.x.huang l.q.huang x.T.huang Y.P.huang T.hussain f.h\"olzken N.h\"usken N.in der Wiesche M.Irshad J.Jackson S.Janchiv J.h.Jeong q.Ji q.P.Ji W.Ji x.b.Ji x.l.Ji Y.Y.Ji x.q.Jia z.K.Jia D.Jiang h.b.Jiang P.C.Jiang S.S.Jiang T.J.Jiang x.S.Jiang Y.Jiang J.b.Jiao J.K.Jiao z.Jiao S.Jin Y.Jin M.q.Jing x.M.Jing T.Johansson S.Kabana N.Kalantar-Nayestanaki x.l.Kang x.S.Kang M.Kavatsyuk b.C.Ke V.Khachatryan A.Khoukaz R.Kiuchi O.b.Kolcu b.Kopf M.Kuessner x.Kui A.Kupsc W.K\"uhn J.J.lane P.larin l.lavezzi T.T.lei z.h.lei h.leithoff M.lellmann T.lenz C.li C.li C.h.li cheng li D.M.li f.li G.li h.li h.b.li h.J.li h.N.li hui li J.R.li J.S.li K.li l.J.li l.K.li lei li M.h.li P.R.li q.M.li q.x.li R.li S.x.li T.li W.D.li W.G.li x.li x.h.li x.l.li x.Y.li Y Institute of high Energy Physics Chinese Academy of SciencesBeijing 100049China beihang university Beijing 100191China bochum Ruhr-university D-44780 BochumGermany budker Institute of Nuclear Physics Sb RAS(bINP) Novosibirsk 630090Russia Carnegie Mellon university PittsburghPennsylvania 15213USA Central china Normal university Wuhan 430079China Central South university Changsha 410083China china Center of Advanced Science and Technology Beijing 100190China china university of Geosciences Wuhan 430074China Chung-Ang university Seoul06974Republic of Korea COMSATS university Islamabad Lahore CampusDefence RoadOff Raiwind Road54000 LahorePakistan fudan university Shanghai 200433China GSI helmholtzcentre for heavy Ion Research Gmbh D-64291 DarmstadtGermany Guangxi Normal university Guilin 541004China Guangxi university Nanning 530004China hangzhou Normal university Hangzhou 310036China hebei university Baoding 071002China helmholtz Institute Mainz Staudinger Weg 18D-55099 MainzGermany henan Normal university Xinxiang 453007China henan university Kaifeng 475004China henan university of Science and Technology Luoyang 471003China henan university of Technology Zhengzhou 450001China huangshan college Huangshan 245000China hunan Normal university Changsha 410081China hunan university Changsha 410082China Indian Institute of Technology Madras Chennai 600036India Indiana university BloomingtonIndiana 47405USA INfN laboratori Nazionali di frascati INFN Laboratori Nazionali di FrascatiI-00044FrascatiItaly INfN laboratori Nazionali di frascati INFN Sezione di PerugiaI-06100PerugiaItaly INfN laboratori Nazionali di frascati University of PerugiaI-06100PerugiaItaly INfN Sezione di ferrara INFN Sezione di FerraraI-44122FerraraItaly INfN Sezione di ferrara University of FerraraI-44122FerraraItaly Inner Mongolia university Hohhot 010021China Institute of Modern Physics Lanzhou 730000China Institute of Physics and Technology Peace Avenue 54BUlaanbaatar 13330Mongolia Instituto de A

Using e^(+)e^(−)annihilation data corresponding to an integrated luminosity of 2.93 fb^(−1)taken at the center-of-mass energy√s=3.773 GeV with the bESIII detector,a joint amplitude analysis is performed on the decays D^(0)→π^(+)π^(−)π^(+)π^(−)and D^(0)→π^(+)π^(−)π^(0)π^(0)(non-η).The fit fractions of individual components are obtained,and large interferences among the dominant components of the decays D^(0)→a_(1)(1260)π,D^(0)→π(1300)π,D^(0)→ρ(770)ρ(770),and D^(0)→2(ππ)_(S)are observed in both *** the obtained amplitude model,the CP-even fractions of D^(0)→π^(+)π^(−)π^(+)π^(−)and D^(0)→π^(+)π^(−)π^(0)π^(0)(non-η)are determined to be(75.2±1.1_(stat).±1.5_(syst.))%and(68.9±1.5_(stat).±2.4_(syst.))%,*** branching fractions of D^(0)→π^(+)π^(−)π^(+)π^(−)and D^(0)→π^(+)π^(−)π^(0)π^(0)(non-η)are measured to be(0.688±0.010_(stat.)±0.010_(syst.))%and(0.951±0.025_(stat.)±0.021_(syst.))%,*** amplitude analysis provides an important model for the binning strategy in measuring the strong phase parameters of D^(0)→4πwhen used to determine the CKM angleγ(ϕ_(3))via the b^(−)→DK^(−)decay.

关键词： bESIII D^(0)meson decays amplitude analysis CP-even fraction

由超拍电子伏特加速器产生的超高能伽马射线气泡

在线全文

维普期刊数据库

学校读者我要写书评

暂无评论

Science bulletin 2024年第4期69卷 449-457页

作者： lhAASO Collaboration zhen Cao Chuandong Gao Cong li Ruo-Yu liu Ruizhi Yang 不详 key laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China university of Chinese Academy of Sciences Beijing 100049China TIANfU Cosmic Ray Research Center ChengduChina Institute of frontier and Interdisciplinary Science Shandong UniversityQingdao 266237China School of Astronomy and Space Science Nanjing UniversityNanjing 210023China university of Science and Technology of china Hefei 230026China

We report the detection of aγ-ray bubble spanning at least 100deg2 in ultra-high energy(UhE)up to a few PeV in the direction of the star-forming region Cygnus x,implying the presence super PeVatron(s)accelerating protons to at least 10 PeV.A log-parabola form with the photon indexΓ(E)=(2.71±0.02)+(0.11±0.02)×log10(E/10 TeV)is found fitting the gamma-ray energy spectrum of the bubble *** sources,“hot spots”correlated with very massive molecular clouds,and a quasi-spherical amorphousγ-ray emitter with a sharp central brightening are observed in the *** the core of~0.5°,spatially associating with a region containing massive Ob association(Cygnus Ob2)and a microquasar(Cygnus x-3),as well as previously reported multi-TeV sources,an enhanced concentration of UhEγ-rays is observed with 2 photons at energies above 1 *** general feature of the bubble,the morphology,and the energy spectrum,are reasonably reproduced by the assumption of a particle accelerator in the core,continuously injecting protons into the ambient medium.

关键词： Cosmic rays γ-rays Interstellar medium Star cluster

Optimization of performance of the KM2A full array using the Crab Nebula

在线全文

维普期刊数据库

学校读者我要写书评

暂无评论

Chinese Physics C 2024年第6期48卷 169-178页

作者：曹臻 f.Aharonian 安琪阿西克古白云翔包逸炜 D.bastieri 毕效军毕玉江蔡金庭曹晴曹文羽曹喆常进常劲帆陈尚明陈恩生陈亮陈林陈龙陈明君陈玛丽陈起辉陈素弘陈天禄陈阳程宁程耀东崔明阳崔树旺崔晓红崔昱东戴本忠代洪亮戴子高单增罗布 D.della Volpe 董绪强段凯凯樊军辉范一中方军方堃冯存峰封莉冯少辉丰晓婷冯有亮 S.Gabici 高博高川东高林青高启高卫高伟康葛茂茂耿利斯 G.Giacinti 龚光华苟全补顾旻皓郭福来郭晓磊郭义庆郭莹莹韩毅昂何会海贺昊宁何佳银何新波何钰 M.heller 贺远强侯博文侯超侯贤胡红波胡铨胡世聪黄代绘黄天奇黄文俊黄性涛黄晓渊黄勇黄志成季筱璐贾焕玉贾康江琨姜晓巍姜泽军金敏康明铭柯通 D.Kuleshov.K.Kurinov 李兵兵李澄李骢李丹李飞李海波李会财李华阳李军李剑李捷李凯李文龙李文莲李秀荣李昕李一卓李哲黎卓梁恩维梁云峰林苏杰刘冰刘成刘栋刘虎刘海东刘佳刘江来刘金艳刘茂元柳若愚刘四明刘伟刘怡刘以农鲁睿罗晴吕洪魁马伯强马玲玲马欣华毛基荣闵振 W.Mitthumsiri 穆慧君南云程 A.Neronov 区子维庞彬宇 P.Pattarakijwanich 裴致远齐孟尧祁业情乔冰强秦家军 D.Ruffolo A.Sáiz D.Semikoz 邵澄宇邵琅 O.Shchegolev 盛祥东舒富文宋慧超 Yu.V.Stenkin V.Stepanov 苏扬孙秦宁孙晓娜孙志斌谭柏轩唐庆文唐泽波田文武王超王昌贝王广威王洪光王惠惠王建成汪凯王利苹王玲玉王培汉王冉王为王祥高王祥玉王阳王玉东王岩谨王忠海王仲翔王振王铮韦大明魏俊杰魏永健文韬吴超勇吴含荣武莎吴雪峰吴雨生席邵强夏捷夏君集项光漫肖迪泫肖刚辛广广辛玉良邢祎熊峥徐东莲徐仁峰徐仁新徐伟立薛良闫大海颜景志颜田杨朝文杨帆杨冯帆杨何文杨佳盈杨莉莉杨明洁杨睿智杨深邦姚玉华姚志国叶一锰尹丽巧尹娜游晓浩游智勇于艳红袁强岳华曾厚敦曾婷轩曾玮查敏张彬彬张丰张海明张恒英张建立张丽霞张力张鹏飞张佩佩张瑞张少博张少如张寿山张潇张笑鹏张云峰张毅张勇赵兵赵静赵雷赵立志赵世平郑福周斌周浩周佳能周猛周平周荣周勋秀祝成光祝凤荣朱辉朱科军左雄 lhAASO Collaboration key laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China university of Chinese Academy of Sciences Beijing 100049China Tianfu Cosmic Ray Research Center Chengdu 610000China Dublin Institute for Advanced Studies 31 Fitzwilliam Place2 DublinIreland Max-Planck-Institut for Nuclear Physics P.O.Box 10398069029 HeidelbergGermany state key laboratory of Particle Detection and Electronics China university of Science and Technology of china Hefei 230026China School of physical Science and Technology&School of Information Science and Technology Southwest Jiaotong UniversityChengdu 610031China School of Astronomy and Space Science Nanjing UniversityNanjing 210023China Center for Astrophysics Guangzhou UniversityGuangzhou 510006China hebei Normal university Shijiazhuang 050024China key laboratory of Dark Matter and Space Astronomy&key laboratory of Radio Astronomy Purple Mountain ObservatoryChinese Academy of SciencesNanjing 210023China Tsung-Dao lee Institute&School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghai 200240China key laboratory for Research in Galaxies and Cosmology Shanghai Astronomical ObservatoryChinese Academy of SciencesShanghai 200030China key laboratory of Cosmic Rays(Tibet university) Ministry of EducationLhasa 850000TibetChina National Astronomical Observatories Chinese Academy of SciencesBeijing 100101China School of Physics and Astronomy(zhuhai)&School of Physics(Guangzhou)&Sino-french Institute of Nuclear engineering and Technology(zhuhai) Sun Yat-sen UniversityZhuhai 519000&Guangzhou 510275China School of Physics and Astronomy Yunnan UniversityKunming 650091China Département de Physique Nucléaire et Corpusculaire Facultéde SciencesUniversitéde Genève24 Quai Ernest Ansermet1211 GenevaSwitzerland Institute of frontier and Interdisciplinary Science Shandong UniversityQingdao 266237China APC Universit'e Paris Cit'eCNRS/IN2P3CEA/IRFUObservat

The full array of the large high Altitude Air Shower Observatory(lhAASO)has been in operation since July *** its kilometer-square array(KM2A),we optimized the selection criteria for very high and ultrahigh energyγ-rays using data collected from August 2021 to August 2022,resulting in an improvement in significance of the detection in the Crab Nebula of approximately 15%,compared with that of previous *** the implementation of these new selection criteria,the angular resolution was also significantly improved by approximately 10%at tens of *** aspects of the full KM2A array performance,such as the pointing error,were also calibrated using the Crab *** resulting energy spectrum of the Crab Nebula in the energy range of 10-1000 TeV are well fitted by a log-parabola model,which is consistent with the previous results from lhAASO and other experiments.

关键词： γ-ray Crab Nebula significance

Ground-state mass of ^(22)Al and test of state-of-the-art ab initio calculations

在线全文

维普期刊数据库

学校读者我要写书评

暂无评论

Chinese Physics C 2024年第3期48卷 72-78页

作者：孙铭泽于越王新鹏王猛李健国张玉虎 K.blaum 陈祖毅陈瑞九邓涵宇付超义葛文文黄文嘉焦红扬李红蕙李宏福罗胤芳廖挺 YuAlitvinov 司敏帅鹏史金阳王茜邢元明徐星徐瑚珊许甫荣袁琪 T.Yamaguchi 颜鑫亮杨建成原有进周小红周旭张敏曾奇 CAS key laboratory of high Precision Nuclear Spectroscopy Institute of Modern PhysicsChinese Academy of SciencesLanzhou 730000China School of Nuclear Science and Technology University of Chinese Academy of SciencesBeijing 100049China Max-Planck-Institut für Kernphysik Saupfercheckweg 169117 HeidelbergGermany GSI helmholtzzentrum für Schwerionenforschung Planckstraße 164291 DarmstadtGermany Advanced Energy Science and Technology Guangdong laboratory Huizhou516007China state key laboratory of Nuclear Physics and Technology School of PhysicsPeking UniversityBeijing 100871China department of Physics Saitama UniversitySaitama 338-8570Japan School of Nuclear Science and engineering East China University of TechnologyNanchang 330013China

The ground-state mass excess of the T_(z)=−2 drip-line nucleus ^(22)Al is measured for the first time as 18103(10)keV using the newly-developed bρ-defined isochronous mass spectrometry method at the cooler storage ring in *** new mass excess value allowed us to determine the excitation energies of the two low-lying 1+states in ^(22)Al with significantly reduced uncertainties of 51 *** compared to the analogue states in its mirror nucleus ^(22)f,the mirror energy differences of the two 1^(+)states in the ^(22)Al-^(22)f mirror pair are determined to be−625(51)keV and−330(51)*** excitation energies and mirror energy differences are used to test the state-of-the-art ab initio valence-space in-medium similarity renormalization group calculations with four sets of interactions derived from the chiral effective field *** mechanism leading to the large mirror energy differences is investigated and attributed to the occupation of theπs_(1/2) orbital.

关键词： nuclear mass bρ-defined IMS mirror energy difference ab initio VS-IMSRG calculations chiral interactions

SRY-box transcription factor 9 triggers YAP nuclear entry via direct interaction in tumors

维普期刊数据库

同方期刊数据库评论

在线全文

学校读者我要写书评

暂无评论

Signal Transduction and Targeted Therapy 2024年第5期9卷 2285-2297页

作者： hui qian chen-hong Ding fang liu Shi-Jie chen chen-Kai huang Meng-Chao xiao xia-lu hong Ming-chen Wang fang-zhi Yan Kai Ding Ya-lu Cui bai-Nan zheng Jin Ding cheng luo xin zhang Wei-fen xie department of Gastroenterology Changzheng HospitalNaval Medical UniversityShanghaiChina department of Gastroenterology Shanghai East HospitalSchool of MedicineTongji UniversityShanghaiChina Drug Discovery and Design Center CAS Key Laboratory of Receptor ResearchState Key Laboratory of Drug ResearchShanghai Institute of Materia MedicaChinese Academy of SciencesShanghaiChina department of Gastroenterology First Affiliated Hospital of Nanchang UniversityNanchangChina Clinical Cancer Institute Center for Translational MedicineNaval Medical UniversityShanghaiChina

The translocation of YAP from the cytoplasm to the nucleus is critical for its activation and plays a key role in tumor ***,the precise molecular mechanisms governing the nuclear import of YAP are not fully *** this study,we have uncovered a crucial role of SOx9 in the activation of ***9 promotes the nuclear translocation of YAP by direct ***,we have identified that the binding between Asp-125 of SOx9 and Arg-124 of YAP is essential for SOx9-YAP interaction and subsequent nuclear entry of ***,we have discovered a novel asymmetrical dimethylation of YAP at Arg-124(YAP-R124me2a)catalyzed by ***-R124me2a enhances the interaction between YAP and SOx9 and is associated with poor prognosis in multiple ***,we disrupted the interaction between SOx9 and YAP using a competitive peptide,S-A1,which mimics anα-helix of SOx9 containing Asp-125.S-A1 significantly inhibits YAP nuclear translocation and effectively suppresses tumor *** study provides the first evidence of SOx9 as a pivotal regulator driving YAP nuclear translocation and presents a potential therapeutic strategy for YAP-driven human cancers by targeting SOx9-YAP interaction.

关键词： interaction interaction precise

Anisotropy of the Wear behavior for Carbon Nanotube-Reinforced 6061Al Composites

在线全文

维普期刊数据库

学校读者我要写书评

暂无评论

Acta Metallurgica Sinica(English letters) 2023年第5期36卷 814-826页

作者： x.N.li J.f.zhang W.h.xue K.Ma P.Y.li z.Y.liu b.l.xiao D.R.ni q.z.Wang D.Wang z.Y.Ma School of Materials Science and engineering University of Science and Technology of ChinaShenyang110016China Shi-Changxu Innovation Center for Advanced Materials Institute of Metal ResearchChinese Academy of SciencesShenyang110016China

Carbon nanotube(CNT)-reinforced 6061Al(CNT/6061Al)composites with directionally aligned CNT were fabricated,and their wear behavior was *** results indicate that the wear properties of CNT/6061Al composites exhibited a significant anisotropy.A certain CNT concentrations(1 wt%and 2 wt%)could effectively improve the wear resistance of CNT/6061Al composites along the CNT circumferential and CNT radial directions for the load transfer,grain refinement and self-lubrication effect of *** brass{011}and{112}textures inhibited the load transfer effect of CNT along the CNT radial direction,resulting in a better wear resistance along CNT circumferential direction than CNT radial *** the CNT axial direction,the weak deformability of composites caused by the intensifyingfiber texture was the main reasons for the poor wear resistance of CNT/6061Al composites with increasing CNT concentration.

关键词： Carbon nanotube Metal matrix composite Wear Anisotropy

Corrosion and cavitation erosion resistance enhancement of cast ni–Al bronze by laser surface melting

在线全文

维普期刊数据库

学校读者我要写书评

暂无评论

Journal of Iron and Steel Research International 2022年第2期29卷 359-369页

作者： q.N.Song Y.Tong h.l.li h.N.zhang N.xu G.Y.zhang Y.f.bao W.liu z.G.liu Y.x.qiao engineering Research Center of Dredging Technology of Ministry of Education Hohai UniversityChangzhou213022JiangsuChina college of Mechanical and Electrical engineering Hohai UniversityChangzhou213022JiangsuChina college of Materials Science and engineering Jiangsu University of Science and TechnologyZhenjiang212003JiangsuChina

laser surface melting (lSM) was applied on a cast ni–Al bronze (NAb), which was a crucial material for marine ship propellers. A 720 μm-thick lSM layer with fine equiaxed and dendritic microstructures was obtained. After immersion for 30 days, the corrosion rate of cast NAb was reduced by 25% after lSM. Preferential corrosion occurred and deep corrosion pits appeared at α + κIII microstructure for the cast NAb. lSM NAb underwent general corrosion, and a much more protective film formed on the surface because of the homogenized microstructure. The mass loss of the cast NAb was approximately 2.1 times larger than that of lSM NAb after cavitation erosion (CE) in 3.5 wt.% NaCl solution for 5 h. for the two materials, the mechanical impact effect was dominantly responsible for CE damage. Therefore, the improved hardness and homogenized microstructure contributed to the improved CE resistance of lSM NAb. CE destructed the film, shifted the open circuit potential toward a more negative value, and raised the current density by an order of magnitude. Corrosion at the cast eutectoid microstructure and the dendrites of lSM NAb facilitates the degradation under the cavitation attack. CE-corrosion synergy was largely caused by corrosion-enhanced-CE.

关键词： laser surface melting ni-Al bronze Microstructure Corrosion Cavitation erosion Synergy

Geometrical reconstruction of fluorescence events observed by the lhAASO experiment

在线全文

维普期刊数据库

学校读者我要写书评

暂无评论

Chinese Physics C 2021年第4期45卷 416-425页

作者： f.Aharonian q.An Axikegu l.x.bai Y.x.bai Y.W.bao D.bastieri x.J.bi Y.J.bi h.Cai J.T.Cai z.Cao z.Cao J.Chang J.f.Chang x.C.Chang b.M.chen J.chen l.chen l.chen l.chen M.J.chen M.l.chen q.h.chen S.h.chen S.z.chen T.l.chen x.l.chen Y.chen N.cheng Y.D.cheng S.W.Cui x.h.Cui Y.D.Cui b.z.Dai h.l.Dai z.G.Dai Danzengluobu D.della Volpe b.DEtorre Piazzoli x.J.Dong J.h.fan Y.z.fan z.x.fan J.fang J.fang C.f.feng l.feng S.h.feng Y.l.feng b.Gao C.D.Gao q.Gao W.Gao M.M.Ge l.S.Geng G.h.Gong q.b.Gou M.h.Gu J.G.Guo x.l.Guo Y.q.Guo Y.Y.Guo Y.A.han h.h.he h.N.he J.C.he S.l.he x.b.he Y.he M.heller Y.K.hor C.hou x.hou h.b.hu S.hu S.C.hu x.J.hu D.h.huang q.l.huang W.h.huang x.T.huang z.C.huang f.Ji x.l.Ji h.Y.Jia K.Jiang z.J.Jiang C.Jin D.Kuleshov K.levochkin b.b.li C.li C.li f.li h.b.li h.C.li h.Y.li J.li K.li W.l.li x.li x.li x.R.li Y.li Y.z.li z.li z.li E.W.liang Y.f.liang S.J.lin b.liu C.liu D.liu h.liu h.D.liu J.liu J.l.liu J.l.liu J.S.liu J.Y.liu M.Y.liu R.Y.liu S.M.liu W.liu Y.N.liu z.x.liu W.J.long R.lu h.K.lv b.q.Ma l.l.Ma x.h.Ma J.R.Mao A.Masood W.Mitthumsiri T.Montaruli Y.C.Nan b.Y..Pang P.Pattarakijwanich z.Y.Pei M.Y.qi D.Ruffolo V.Rulev A.Saiz l.Shao O.Shchegolev x.D.Sheng J.R.Shi h.C.Song Yu.V.Stenkin V.Stepanov q.N.Sun x.N.Sun z.b.Sun P.h.T.Tam z.b.Tang W.W.Tian b.D.Wang C.Wang h.Wang h.G.Wang J.C.Wang J.S.Wang l.P.Wang l.Y.Wang R.N.Wang W.Wang W.Wang x.G.Wang x.J.Wang x.Y.Wang Y.D.Wang Y.J.Wang Y.P.Wang z.Wang z.Wang z.h.Wang z.x.Wang D.M.Wei J.J.Wei Y.J.Wei T.Wen C.Y.Wu h.R.Wu S.Wu W.x.Wu x.f.Wu S.q.xi J.xia J.J.xia G.M.xiang G.xiao h.b.xiao G.G.xin Y.l.xin Y.xing D.l.xu R.x.xu l.xue D.h.Yan C.W.Yang f.f.Yang J.Y.Yang l.l.Yang M.J.Yang R.z.Yang S.b.Yang Y.h.Yao z.G.Yao Y.M.Ye l.q.Yin N.Yin x.h.You z.Y.You Y.h.Yu q.Yuan h.D.zeng T.x.zeng W.zeng z.K.zeng M.zha x.x.zhai b.b.zhang h.M.zhang h.Y.zhang J.l.zhang J.W.zhang l.zhang l.zhang l.x.zhang P.f.zhang P.f.zhang R.zhang S.R.zhang S.S.zhang x.zhang x.P.zhang Y.zhang Y.zhang Y.f.zhang Y.l.zhang b.zhao J.zhao l.zhao l.z.zhao S.P.zhao f.zheng Y.zheng b.zhou h.zhou J.N.zhou P key laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China university of Chinese Academy of Sciences Beijing 100049China TIANfU Cosmic Ray Research Center ChengduSichuanChina state key laboratory of Paricle Detection and Electronics China university of Science and Technology of china HefeiAnhui 230026China department of engineering Physics Tsinghua UniversityBeijing 100084China National Astronomical Observatories Chinese Academy of SciencesBeijing 100101China National Space Science Center Chinese Academy of SciencesBeijing 100190China School of Physics Peking UniversityBeijing 100871China Center for Astrophysics Guangzhou UniversityGuangzhouGuangdong 510006China School of Physics and Astronomy&School of Physics(Guangzhou) Sun Yat-sen UniversityZhuhaiGuangdong 519000China School of physical Science and Technology Guangxi UniversityNanningGuangxi 530004China hebei Normal university ShijiazhuangHebei 050024China School of Physics and Microelectronics Zhengzhou UniversityZhengzhouHenan 450001China School of Astronomy and Space Science Nanjing UniversityNanjingJiangsu 210023China key laboratory of Dark Matter and Space Astronomy Purple Mountain ObservatoryChinese Academy of SciencesNanjingJiangsu 210023China Institute of frontier and Interdisciplinary Science Shandong UniversityQingdaoShandong 266237China key laboratory for Research in Galaxies and Cosmology Shanghai Astronomical ObservatoryChinese Academy of SciencesShanghai 200030China Tsung-Dao lee Institute&School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghai 200240China School of physical Science and Technology Southwest Jiaotong UniversityChengduSichuan 610031China college of Physics Sichuan UniversityChengduSichuan 610065China key laboratory of Cosmic Rays(Tibet university) Ministry of EducationLhasaTibet 850000China School of physics and technology Wuhan UniversityWuhanHubei 430072Ch

The lhAASO-WfCTA experiment,which aims to observe cosmic rays in the sub-EeV range using the fluorescence technique,uses a new generation of high-performance *** ensure that the experiment has ex-cellent detection capability associated with the measurement of the energy spectrum,the primary composition of cosmic rays,and so on,an accurate geometrical reconstruction of air-shower events is *** paper de-scribes the development and testing of geometrical reconstruction for stereo viewed events using the WfCTA(Wide field of view Cherenkov/fluorescence Telescope Array)*** approaches,which take full advantage ofthe WfCTA *** *** is the stereo-angular method,which uses the pointing of triggered SiPMs in the shower trajectory,and the other is the stereo-timing method,which uses the triggering time of the fired *** results show that both methods have good geometrical resolution:the resolution of the stereo-timing method is slightly better than the stereo-angular method because the resolution of the latter is slightly limited by the shower track length.

关键词： cosmic ray fluorescence telescope stereo observation geometrical reconstruction