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The evolutionary history of 2,658 cancers (vol 578, pg 122, 2020)

NATURE 2023年第7948期614卷 E42-E42页

作者： Gerstung, Moritz Jolly, Clemency Leshchiner, Ignaty Dentro, Stefan C. Gonzalez, Santiago Rosebrock, Daniel Mitchell, Thomas J. Rubanova, Yulia Anur, Pavana Yu, Kaixian Tarabichi, Maxime Deshwar, Amit Wintersinger, Jeff Kleinheinz, Kortine Vazquez-Garcia, Ignacio Haase, Kerstin Jerman, Lara Sengupta, Subhajit Macintyre, Geoff Malikic, Salem Donmez, Nilgun Livitz, Dimitri G. Cmero, Marek Demeulemeester, Jonas Schumacher, Steven Fan, Yu Yao, Xiaotong Lee, Juhee Schlesner, Matthias Boutros, Paul C. Bowtell, David D. Zhu, Hongtu Getz, Gad Imielinski, Marcin Beroukhim, Rameen Sahinalp, S. Cenk Ji, Yuan Peifer, Martin Markowetz, Florian Mustonen, Ville Yuan, Ke Wang, Wenyi Morris, Quaid D. Spellman, Paul T. Wedge, David C. Van Loo, Peter European Molecular Biology Laboratory European Bioinformatics Institute (EMBL-EBI) Cambridge UK European Molecular Biology Laboratory Genome Biology Unit Heidelberg Germany Wellcome Sanger Institute Cambridge UK Genome Biology Unit European Molecular Biology Laboratory (EMBL) Heidelberg Germany University of Ljubljana Ljubljana Slovenia The Francis Crick Institute London UK Big Data Institute University of Oxford Oxford UK Wellcome Sanger Institute Wellcome Genome Campus Hinxton UK Big Data Institute Li Ka Shing Centre University of Oxford Oxford UK University of Cambridge Cambridge UK Cambridge University Hospitals NHS Foundation Trust Cambridge UK Department of Applied Mathematics and Theoretical Physics Centre for Mathematical Sciences University of Cambridge Cambridge UK Department of Epidemiology and Biostatistics Memorial Sloan Kettering Cancer Center New York NY USA Department of Statistics Columbia University New York NY USA Department of Haematology University of Cambridge Cambridge UK University of Leuven Leuven Belgium Broad Institute of MIT and Harvard Cambridge MA USA Center for Cancer Research Massachusetts General Hospital Charlestown MA USA Department of Pathology Massachusetts General Hospital Boston MA USA Harvard Medical School Boston MA USA Center for Cancer Research Massachusetts General Hospital Boston MA USA Dana-Farber Cancer Institute Boston MA USA Department of Medical Oncology Dana-Farber Cancer Institute Boston MA USA Department of Cancer Biology Dana-Farber Cancer Institute Boston MA USA Oxford NIHR Biomedical Research Centre Oxford UK Oxford NIHR Biomedical Research Centre University of Oxford Oxford UK University of Toronto Toronto Ontario Canada Vector Institute Toronto Ontario Canada Vector Institute Toronto ON Canada Department of Computer Science University of Toronto Toronto ON Canada Ontario Institute for Cancer Research Toronto Ontario Canada University of California Los Angeles

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Periodic fast radio bursts from luminous X-ray binaries

arXiv

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arXiv 2021年

作者： Sridhar, Navin Metzger, Brian D. Beniamini, Paz Margalit, Ben Renzo, Mathieu Sironi, Lorenzo Kovlakas, Konstantinos Department of Astronomy Columbia University New YorkNY10027 United States Columbia Astrophysics Laboratory Columbia University New YorkNY10027 United States Center for Computational Astrophysics Flatiron Institute 162 W. 5th Avenue New YorkNY10011 United States Division of Physics Mathematics and Astronomy California Institute of Technology PasadenaCA91125 United States The Open University of Israel P.O. Box 808 Ra'anana43537 Israel Astronomy Department Theoretical Astrophysics Center University of California Berkeley BerkeleyCA94720 United States Geneva Observatory University of Geneva Chemin des Maillettes 51 Versoix1290 Switzerland Physics Department University of Crete HeraklionGR 71003 Greece Institute of Astrophysics Foundation for Research and Technology-Hellas HeraklionGR 71110 Greece

The discovery of periodicity in the arrival times of the fast radio bursts (FRBs) poses a challenge to the oft-studied magnetar scenarios. However, models that postulate that FRBs result from magnetized shocks or magnetic reconnection in a relativistic outflow are not specific to magnetar engines;instead, they require only the impulsive injection of relativistic energy into a dense magnetized medium. Motivated thus, we outline a new scenario in which FRBs are powered by short-lived relativistic outflows ("flares") from accreting black holes or neutron stars, which propagate into the cavity of the pre-existing ("quiescent") jet. In order to reproduce FRB luminosities and rates, we are driven to consider binaries of stellar-mass compact objects undergoing super-Eddington mass-transfer, similar to ultraluminous X-ray (ULX) sources. Indeed, the host galaxies of FRBs, and their spatial offsets within their hosts, show broad similarities with ULXs. Periodicity on timescales of days to years could be attributed to precession (e.g., Lens-Thirring) of the polar accretion funnel, along which the FRB emission is geometrically and relativistically beamed, which sweeps across the observer line of sight. Accounting for the most luminous FRBs via accretion power may require a population of binaries undergoing brief-lived phases of unstable (dynamical-timescale) mass-transfer. This will lead to secular evolution in the properties of some repeating FRBs on timescales of months to years, followed by a transient optical/IR counterpart akin to a luminous red nova, or a more luminous accretion-powered optical/X-ray transient. We encourage targeted FRB searches of known ULX sources. Copyright © 2021, The Authors. All rights reserved.

关键词： Stars

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DP-GEN: A concurrent learning platform for the generation of reliable deep learning based potential energy models

arXiv

引用

arXiv 2019年

作者： Wang, Haidi Chen, Weijie Zeng, Jinzhe Zhang, Linfeng Wang, Han Zhang, Yuzhi Weinan, E. Yuanpei College of Peking University Beijing100871 China School of Electronic Science and Applied Physics Hefei University of Technology Hefei230601 China Academy for Advanced Interdisciplinary Studies Peking University Beijing100871 China School of Chemistry and Molecular Engineering East China Normal University Shanghai200062 China Program in Applied and Computational Mathematics Princeton University PrincetonNJ United States Laboratory of Computational Physics Institute of Applied Physics and Computational Mathematics Huayuan Road 6 Beijing100088 China Beijing Institute of Big Data Research Beijing100871 China Program in Applied and Computational Mathematics Princeton University PrincetonNJ United States Beijing Institute of Big Data Research Beijing100871 China

In recent years, promising deep learning based interatomic potential energy surface (PES) models have been proposed that can potentially allow us to perform molecular dynamics simulations for large scale systems with quantum accuracy. However, making these models truly reliable and practically useful is still a very non-trivial task. A key component in this task is the generation of datasets used in model training. In this paper, we introduce the Deep Potential GENerator (DP-GEN), an open-source software platform that implements the recently proposed"on-the-fly" learning procedure [Phys. Rev. Materials 3, 023804] and is capable of generating uniformly accurate deep learning based PES models in a way that minimizes human intervention and the computational cost for data generation and model training. DP-GEN automatically and iteratively performs three steps: exploration, labeling, and training. It supports various popular packages for these three steps: LAMMPS for exploration, Quantum Espresso, VASP, CP2K, etc. for labeling, and DeePMD-kit for training. It also allows automatic job submission and result collection on different types of machines, such as high performance clusters and cloud machines, and is adaptive to different job management tools, including Slurm, PBS, and LSF. As a concrete example, we illustrate the details of the process for generating a general-purpose PES model for Cu using DP-GEN. Copyright © 2019, The Authors. All rights reserved.

关键词： Potential energy

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Genomic basis for RNA alterations in cancer (vol 578, pg 129, 2020)

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NATURE 2023年第7948期614卷 E37-E37页

作者： Calabrese, Claudia Davidson, Natalie R. Demircioglu, Deniz Fonseca, Nuno A. He, Yao Lehmann, Kjong-Van Liu, Fenglin Shiraishi, Yuichi Soulette, Cameron M. Urban, Lara Greger, Liliana Li, Siliang Liu, Dongbing Perry, Marc D. Xiang, Qian Zhang, Fan Zhang, Junjun Bailey, Peter Erkek, Serap Hoadley, Katherine A. Hou, Yong Huska, Matthew R. Kilpinen, Helena Korbel, Jan O. Marin, Maximillian G. Markowski, Julia Nandi, Tannistha Pan-Hammarstrom, Qiang Pedamallu, Chandra Sekhar Siebert, Reiner Stark, Stefan G. Su, Hong Tan, Patrick Waszak, Sebastian M. Yung, Christina Zhu, Shida Awadalla, Philip Creighton, Chad J. Meyerson, Matthew Ouellette, B. F. Francis Wu, Kui Yang, Huanming Brazma, Alvis Brooks, Angela N. Goke, Jonathan Ratsch, Gunnar Schwarz, Roland F. Stegle, Oliver Zhang, Zemin European Molecular Biology Laboratory European Bioinformatics Institute Hinxton UK European Molecular Biology Laboratory European Bioinformatics Institute (EMBL-EBI) Cambridge UK Genome Biology Unit European Molecular Biology Laboratory (EMBL) Heidelberg Germany CIBIO/InBIO - Research Center in Biodiversity and Genetic Resources Universidade do Porto Vairão Portugal Berlin Institute for Medical Systems Biology Max Delbruck Center for Molecular Medicine Berlin Germany German Cancer Consortium (DKTK) partner site Berlin Germany German Cancer Research Center (DKFZ) Heidelberg Germany Berlin Institute for Medical Systems Biology Max Delbrück Center for Molecular Medicine Berlin Germany German Cancer Consortium (DKTK) Partner site Berlin Berlin Germany European Molecular Biology Laboratory Genome Biology Unit Heidelberg Germany Division of Computational Genomics and Systems Genetics German Cancer Research Center (DKFZ) Heidelberg Germany ETH Zurich Zurich Switzerland Memorial Sloan Kettering Cancer Center New York NY USA Weill Cornell Medical College New York NY USA SIB Swiss Institute of Bioinformatics Lausanne Switzerland University Hospital Zurich Zurich Switzerland Computational Biology Center Memorial Sloan Kettering Cancer Center New York NY USA Department of Biology ETH Zurich Zürich Switzerland Department of Computer Science ETH Zurich Zurich Switzerland Korea University Seoul South Korea Computational and Systems Biology Program Memorial Sloan Kettering Cancer Center New York NY USA Department of Physiology and Biophysics Weill Cornell Medicine New York NY USA Institute for Computational Biomedicine Weill Cornell Medicine New York NY USA Controlled Department and Institution New York NY USA Englander Institute for Precision Medicine Weill Cornell Medicine New York NY USA National University of Singapore Singapore Singapore Genome Institute of Singapore Singapore Singapore Computational and Systems Biology Genome Institute of Singap

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Corrigendum to “Pure TeO 2 glass: Influence of synthesis conditions on linear and non-linear optical, magneto-optical and structural properties,” [J. Alloys Compd., 997 (2024) 174788]

引用

Journal of Alloys and Compounds 2024年 1004卷

作者： J. Hrabovsky N.S. Tagiara J. Mistrik L. Strizik P. Rysanek V. Kopecky J. Kozlik J. Orava S. Wang T. Ishibashi E.I. Kamitsos M. Veis Institute of Physics Faculty of Mathematics and Physics Charles University Ke Karlovu 5 Prague 2 121 16 Czech Republic National Hellenic Research Foundation Theoretical and Physical Chemistry Institute 48 Vassileos Constantinou Ave. Athens 116 35 Greece University of Pardubice Faculty of Chemical Technology Center of Materials and Nanotechnologies nam. Cs. Legii 565 Pardubice 530 02 Czech Republic University of Pardubice Faculty of Chemical Technology Institute of Applied Physics and Mathematics Pardubice Czech Republic Department of General and Inorganic Chemistry Faculty of Chemical Technology University of Pardubice Studentska 573 Pardubice 532 10 Czech Republic Faculty of Science Jan Evangelista Purkyne University in Usti nad Labem Pasteurova 3632/15 Usti nad Labem 400 96 Czech Republic Charles University Faculty of Mathematics and Physics Depart. of Physics of Materials Ke Karlovu 5 Prague 121 16 Czech Republic Faculty of Environment Jan Evangelista Purkyne University in Usti nad Labem Pasteurova 3632/15 Usti nad Labem 400 96 Czech Republic Nagaoka University of Technology Department of Materials Science and Bioengineering Kamitomioka 1603-1 Nagaoka 940-2188 Japan

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Transition from the mean-field to the bosonic Laughlin state in a rotating Bose-Einstein condensate

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Physical Review A 2019年第2期100卷 023606-023606页

作者： G. Vasilakis A. Roussou J. Smyrnakis M. Magiropoulos W. von Klitzing G. M. Kavoulakis Hellenic Mediterranean University School of Engineering P.O. Box 1939 GR-71004 Heraklion Greece Department of Mathematics and Applied Mathematics University of Crete GR-71004 Heraklion Greece Institute of Electronic Structure and Laser (IESL) Foundation for Research and Technology (FORTH) N. Plastira 100 Vassilika Vouton 70013 Heraklion Crete Greece

We consider a weakly interacting Bose-Einstein condensate that rotates in either a harmonic, or a weakly anharmonic trapping potential. Performing numerical calculations, we investigate the behavior of the gas in these two cases as the angular momentum, or equivalently as the rotational frequency of the trap increases. While in the case of a purely harmonic potential the gas makes a transition from the mean-field regime to the correlated Laughlin regime, in the case of anharmonic confinement the mean-field approximation remains always valid. We compare our derived results in these two cases, using both the mean-field approximation, as well as the diagonalization of the many-body Hamiltonian considering a small atom number.

关键词： Vortices in superfluids

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The observational uncertainty of coronal hole boundaries in automated detection schemes

arXiv

引用

arXiv 2021年

作者： Reiss, Martin A. Muglach, Karin Möstl, Christian Arge, Charles N. Bailey, Rachel Delouille, Véronique Garton, Tadhg M. Hamada, Amr Hofmeister, Stefan Illarionov, Egor Jarolim, Robert Kirk, Michael S.F. Kosovichev, Alexander Krista, Larisza Lee, Sangwoo Lowder, Chris MacNeice, Peter J. Veronig, Astrid Space Research Institute Austrian Academy of Sciences Graz Austria Heliophysics Science Division NASA Goddard Space Flight Center GreenbeltMD20771 United States Catholic University of America WashingtonDC20064 United States Conrad Observatory Zentralanstalt für Meteorologie und Geodynamik Vienna Austria Royal Observatory of Belgium Brussels Belgium University of Southampton Southampton United Kingdom Space Physics and Astronomy Research Unit Space Climate Group University of Oulu Oulu Finland University of Graz Institute of Physics Graz Austria Columbia Astrophysics Laboratory Columbia University New YorkNY10027 United States Moscow State University Moscow119991 Russia Moscow Center of Fundamental and Applied Mathematics Moscow119234 Russia ASTRA llc LouisvilleCO80027 United States Center for Computational Heliophysics New Jersey Institute of Technology NewarkNJ07102 United States Department of Physics New Jersey Institute of Technology NewarkNJ07102 United States NASA Ames Research Center Moffett FieldCA94035 United States Cooperative Institute for Research in Environmental Sciences University of Colorado BoulderCO80309 United States National Centers for Environmental Information National Oceanic and Atmospheric Administration BoulderCO80305 United States Korean Space Weather Center Jeju Korea Republic of Southwest Research Institute BoulderCO United States Kanzelhöhe Observatory for Solar and Environmental Research University of Graz Graz Austria

Coronal holes are the observational manifestation of the solar magnetic field open to the heliosphere and are of pivotal importance for our understanding of the origin and acceleration of the solar wind. Observations from space missions such as the Solar Dynamics Observatory now allow us to study coronal holes in unprecedented detail. Instrumental effects and other factors, however, pose a challenge to automatically detect coronal holes in solar imagery. The science community addresses these challenges with different detection schemes. Until now, little attention has been paid to assessing the disagreement between these schemes. In this COSPAR ISWAT initiative, we present a comparison of nine automated detection schemes widely-applied in solar and space science. We study, specifically, a prevailing coronal hole observed by the Atmospheric Imaging Assembly instrument on 2018 May 30. Our results indicate that the choice of detection scheme has a significant effect on the location of the coronal hole boundary. Physical properties in coronal holes such as the area, mean intensity, and mean magnetic field strength vary by a factor of up to 4.5 between the maximum and minimum values. We conclude that our findings are relevant for coronal hole research from the past decade, and are therefore of interest to the solar and space research community. © 2021, CC BY.

关键词： Space research

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Phylogenomics,divergence times and notes of orders in Basidiomycota

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Fungal Diversity 2024年第3期126卷 127-406页

作者： Mao-Qiang He Bin Cao Fei Liu Teun Boekhout Teodor T.Denchev Nathan Schoutteten Cvetomir M.Denchev Martin Kemler Sergio P.Gorjón Dominik Begerow Ricardo Valenzuela Naveed Davoodian Tuula Niskanen Alfredo Vizzini Scott A.Redhead Virginia Ramírez-Cruz Viktor Papp Vasiliy A.Dudka Arun Kumar Dutta Ricardo García-Sandoval Xin-Zhan Liu Teeratas Kijpornyongpan Anton Savchenko Leho Tedersoo Bart Theelen Larissa Trierveiler-Pereira Fang Wu Juan Carlos Zamora Xiang-Yu Zeng Li-Wei Zhou Shi-Liang Liu Masoomeh Ghobad-Nejhad Admir J.Giachini Guo-Jie Li Makoto Kakishima Ibai Olariaga Danny Haelewaters Bobby Sulistyo Junta Sugiyama Sten Svantesson Andrey Yurkov Pablo Alvarado Vladimír Antonín AndréFelipe da Silva Irina Druzhinina Tatiana B.Gibertoni Laura Guzmán-Dávalos Alfredo Justo Samantha C.Karunarathna Mahesh C.A.Galappaththi Merje Toome-Heller Tsuyoshi Hosoya Kare Liimatainen Rodrigo Márquez Armin Mešić Jean-Marc Moncalvo LászlóG.Nagy Torda Varga Takamichi Orihara Tania Raymundo Isabel Salcedo Alexandre G.S.Silva-Filho Zdenko Tkalčec Felipe Wartchow Chang-Lin Zhao Tolgor Bau Milay Cabarroi-Hernández Alonso Cortés-Pérez Cony Decock Ruben De Lange Michael Weiss Nelson Menolli Jr. R.Henrik Nilsson Yu-Guang Fan Annemieke Verbeken Yusufjon Gafforov Angelina Meiras-Ottoni Renato L.Mendes-Alvarenga Nian-Kai Zeng Qi Wu Kevin D.Hyde Paul M.Kirk Rui-Lin Zhao State Key Laboratory of Mycology Institute of MicrobiologyChinese Academy of SciencesBeijing 100101People’s Republic of China The Yeasts Foundation Amsterdamthe Netherlands Institute of Biodiversity and Ecosystem Research Bulgarian Academy of Sciences2 Gagarin St.1113 SofiaBulgaria IUCN SSC Rusts and Smuts Specialist Group SofiaBulgaria Research Group Mycology Department of BiologyGhent UniversityK.L.Ledeganckstraat 359000 GhentBelgium Institute of Plant Science and Microbiology Organismic Botany and MycologyUniversität HamburgOhnhorststr.1822609 HamburgGermany Department of Botany and Plant Physiology Plant DNA-BiobankUniversity of SalamancaC/Licenciado Méndez Nieto s/n37007 SalamancaSpain Departamento de Botánica Instituto Politécnico NacionalEscuela Nacional de Ciencias BiológicasPlan de Ayala y Carpio s/nSanto TomásDel.Miguel HidalgoCP 11340 MexicoMexico Royal Botanic Gardens Victoria MelbourneVIC 3004Australia Fungal Diversity and Systematics Team Royal Botanic GardensKewSurrey TW93ABUK Botany Unit Finnish Museum of Natural HistoryUniversity of HelsinkiP.O.Box 700014 HelsinkiFinland Department of Life Sciences and Systems Biology University of TorinoViale P.A.Mattioli 2510125 TurinItaly Institute for Sustainable Plant Protection(IPSP-SS Turin) C.N.R.Viale P.A.Mattioli2510125 TurinItaly National Mycological Herbarium/DAOM Ottawa Research and Development CentreScience and Technology BranchAgriculture and Agri-Food Canada960 Carling Ave.William Saunders Building(Bldg.49)OttawaON K1A0C6Canada University of Guadalajara Apdo.postal 1-13945147 ZapopanJaliscoMexico Department of Botany Hungarian University of Agriculture and Life Sciences1518 BudapestHungary Komarov Botanical Institute of the Russian Academy of Sciences Prof.Popov Str.2St PetersburgRussia 197376 Yugra State University Chekhova str.16Khanty-MansiyskKhanty-Mansi Autonomous Okrug-YugraRussia 628012 Molecular&Applied Mycology Laboratory Department of BotanyGauhati UniversityGopinath Bordoloi

Basidiomycota is one of the major phyla in the fungal tree of *** outline of Basidiomycota provides essential taxonomic information for researchers and workers in *** this study,we present a time-framed phylogenomic tree with 487 species of Basidiomycota from 127 families,47 orders,14 classes and four subphyla;we update the outline of Basidiomycota based on the phylogenomic relationships and the taxonomic studies since 2019;and we provide notes for each order and discuss the history,defining characteristics,evolution,justification of orders,problems,significance,and *** phylogenomic analysis suggests that the subphyla diverged in a time range of 443-490 Myr(million years),classes in a time range of 312-412 Myr,and orders in a time range of 102-361 *** diverged in a time range of 50-289 Myr,76-224 Myr,and 62-156 Myr in Agaricomycotina,Pucciniomycotina,and Ustilaginomycotina,*** on the phylogenomic relationships and divergence times,we propose a new suborder Mycenineae in Agaricales to accommodate *** the current outline of Basidiomycota,there are four subphyla,20 classes,77 orders,297 families,and 2134 genera *** building a robust taxonomy of Basidiomycota in the genomic era,the generation of molecular phylogenetic data has become relatively *** phenotypical characters,especially those that can be applied for identification and classification,however,has become increasingly challenging.

关键词： Classification Fungi Molecular clock Systematics Taxonomy

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Underlying Topological Dirac Nodal Line Mechanism of the Anomalously Large Electron-Phonon Coupling Strength on a Be (0001) Surface

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Physical Review Letters 2019年第13期123卷 136802-136802页

作者： Ronghan Li Jiangxu Li Lei Wang Jiaxi Liu Hui Ma Hai-Feng Song Dianzhong Li Yiyi Li Xing-Qiu Chen Shenyang National Laboratory for Materials Science Institute of Metal Research Chinese Academy of Science 110016 Shenyang Liaoning People’s Republic of China School of Materials Science and Engineering University of Science and Technology of China Heifei 230026 People’s Republic of China Institute of Applied Physics and Computational Mathematics Beijing 100094 People’s Republic of China

Beryllium has recently been discovered to harbor a Dirac nodal line (DNL) in its bulk phase and the DNL-induced nontrivial surface states (DNSSs) on its (0001) surface, rationalizing several already-existing historic puzzles [Phys. Rev. Lett. 117, 096401 (2016)]. However, to date the underlying mechanism as to why its (0001) surface exhibits an anomalously large electron-phonon coupling effect (λe−phs≈1.0) remains unresolved. Here, by means of first-principles calculations, we show that the coupling of the DNSSs with the phononic states mainly contributes to its novel surface e-ph enhancement. Besides the fact that the experimentally observed λe−phs and the main Eliashberg coupling function (ECF) peaks are reproduced well in our current calculations, we decompose the ECF α2F(k,q;v) and the e-ph coupling strength λ(k,q;v) as a function of each electron momentum (k), each phonon momentum (q), and each phonon mode (v), evidencing the robust connection between the DNSSs and both α2F(k,q;v) and λ(k,q;v). The results reveal the strong e-ph coupling between the DNSSs and the phonon modes, which contributes over 80% of the λe−phs coefficient on the Be (0001) surface. It highlights that the anomalously large e-ph coefficient on the Be (0001) surface can be attributed to the presence of its DNL-induced DNSSs, clarifying the long-debated mechanism.

关键词： Electron-phonon coupling Topological phases of matter

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Search for the radiative penguin decays B0→KS0KS0γ in the Belle experiment

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Physical Review D 2022年第1期106卷 012006-012006页

作者： H. B. Jeon K. H. Kang H. Park I. Adachi H. Aihara S. Al Said D. M. Asner H. Atmacan T. Aushev R. Ayad V. Babu S. Bahinipati P. Behera K. Belous J. Bennett F. Bernlochner M. Bessner V. Bhardwaj B. Bhuyan T. Bilka A. Bobrov D. Bodrov J. Borah A. Bozek M. Bračko P. Branchini T. E. Browder A. Budano M. Campajola D. Červenkov M.-C. Chang P. Chang A. Chen B. G. Cheon K. Chilikin H. E. Cho K. Cho S.-J. Cho S.-K. Choi Y. Choi S. Choudhury D. Cinabro S. Cunliffe S. Das N. Dash G. De Pietro R. Dhamija F. Di Capua J. Dingfelder Z. Doležal T. V. Dong D. Epifanov T. Ferber D. Ferlewicz B. G. Fulsom R. Garg V. Gaur N. Gabyshev A. Giri P. Goldenzweig B. Golob E. Graziani T. Gu K. Gudkova C. Hadjivasiliou T. Hara K. Hayasaka H. Hayashii M. T. Hedges T. Higuchi W.-S. Hou C.-L. Hsu K. Inami G. Inguglia A. Ishikawa R. Itoh M. Iwasaki Y. Iwasaki W. W. Jacobs E.-J. Jang S. Jia Y. Jin K. K. Joo J. Kahn H. Kakuno A. B. Kaliyar T. Kawasaki C. Kiesling C. H. Kim D. Y. Kim K.-H. Kim K. T. Kim Y.-K. Kim K. Kinoshita P. Kodyš T. Konno A. Korobov S. Korpar E. Kovalenko P. Križan R. Kroeger P. Krokovny T. Kuhr M. Kumar K. Kumara A. Kuzmin Y.-J. Kwon Y.-T. Lai K. Lalwani T. Lam J. S. Lange M. Laurenza S. C. Lee C. H. Li J. Li Y. Li Y. B. Li L. Li Gioi J. Libby K. Lieret D. Liventsev A. Martini M. Masuda T. Matsuda D. Matvienko S. K. Maurya M. Merola F. Metzner K. Miyabayashi R. Mizuk G. B. Mohanty M. Nakao D. Narwal Z. Natkaniec A. Natochii L. Nayak M. Nayak N. K. Nisar S. Nishida K. Ogawa S. Ogawa H. Ono Y. Onuki P. Oskin P. Pakhlov G. Pakhlova T. Pang S. Pardi S.-H. Park A. Passeri S. Patra S. Paul T. K. Pedlar R. Pestotnik L. E. Piilonen T. Podobnik V. Popov E. Prencipe M. T. Prim M. V. Purohit M. Röhrken A. Rostomyan N. Rout G. Russo D. Sahoo S. Sandilya A. Sangal L. Santelj T. Sanuki V. Savinov G. Schnell C. Schwanda Y. Seino K. Senyo M. E. Sevior M. Shapkin C. Sharma V. Shebalin C. P. Shen J.-G. Shiu J. B. Singh A. Sokolov E. Solovieva M. Starič Z. S. Stottler J. F. Strube M. Sumihama T. Sumiyoshi M. Takizawa U. Tamponi K. Tanida F. Tenc Kyungpook National University Daegu 41566 Kavli Institute for the Physics and Mathematics of the Universe (WPI) University of Tokyo Kashiwa 277-8583 High Energy Accelerator Research Organization (KEK) Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies) Hayama 240-0193 Department of Physics University of Tokyo Tokyo 113-0033 Department of Physics Faculty of Science University of Tabuk Tabuk 71451 Department of Physics Faculty of Science King Abdulaziz University Jeddah 21589 Brookhaven National Laboratory Upton New York 11973 University of Cincinnati Cincinnati Ohio 45221 National Research University Higher School of Economics Moscow 101000 Deutsches Elektronen–Synchrotron 22607 Hamburg Indian Institute of Technology Bhubaneswar Satya Nagar 751007 Indian Institute of Technology Madras Chennai 600036 Institute for High Energy Physics Protvino 142281 University of Mississippi University Mississippi 38677 University of Bonn 53115 Bonn University of Hawaii Honolulu Hawaii 96822 Indian Institute of Science Education and Research Mohali SAS Nagar 140306 Indian Institute of Technology Guwahati Assam 781039 Faculty of Mathematics and Physics Charles University 121 16 Prague Budker Institute of Nuclear Physics SB RAS Novosibirsk 630090 Novosibirsk State University Novosibirsk 630090 P.N. Lebedev Physical Institute of the Russian Academy of Sciences Moscow 119991 H. Niewodniczanski Institute of Nuclear Physics Krakow 31-342 Faculty of Chemistry and Chemical Engineering University of Maribor 2000 Maribor J. Stefan Institute 1000 Ljubljana INFN—Sezione di Roma Tre I-00146 Roma INFN—Sezione di Napoli I-80126 Napoli Università di Napoli Federico II I-80126 Napoli Department of Physics Fu Jen Catholic University Taipei 24205 Department of Physics National Taiwan University Taipei 10617 National Central University Chung-li 32054 Department of Physics and Institute of Natural Sciences Hanyang University Seoul 04763 Korea Institute of Science and Technology Inform

We report results from the first search for the rare penguin-dominated decay mode B0→KS0KS0γ, which can result from the production of tensor mesons f(1270) and f′(1525) in association with a photon. The search uses the full data sample of 772×106 BB¯ pairs collected with the Belle detector at the KEKB asymmetric-energy e+e− collider. No statistically significant signals are observed in the KS0KS0 invariant mass range 1 GeV/c2

关键词： Electroweak interaction Flavor changing neutral currents Bottom mesons Lepton colliders

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