V
V. F. Yakushev
Researcher at Russian Academy of Sciences
Publications - 102
Citations - 2185
V. F. Yakushev is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Neutrino & Large Volume Detector. The author has an hindex of 25, co-authored 98 publications receiving 2060 citations.
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Journal ArticleDOI
The OPERA experiment in the CERN to Gran Sasso neutrino beam
R. Acquafredda,T. Adam,N. Agafonova,P. Alvarez Sanchez,M. Ambrosio,A. M. Anokhina,Shigeki Aoki,Akitaka Ariga,Tomoko Ariga,L. Arrabito,C. Aufranc,D. Autiero,A. Badertscher,A. V. Bagulya,Eric Baussan,A. Bergnoli,F. Bersani Greggio,A. Bertolin,M. Besnier,D. Biaré,D. Bick,S. Blin,K. Borer,J. Boucrot,D. Boutigny,V. Boyarkin,Cristiano Bozza,T. Brugière,R. Brugnera,G. Brunetti,S. Buontempo,J. E. Campagne,B. Carlus,E. Carrara,A. Cazes,L. Chaussard,M. M. Chernyavsky,V. Chiarella,N. Chon-Sen,Artem Chukanov,Robert Ciesielski,L. Consiglio,M. Cozzi,G. D'Amato,F. Dal Corso,Nicola D'Ambrosio,J. Damet,C. De La Taille,G. Delellis,Y. Déclais,T. Descombes,M. Deserio,F. Di Capua,D. Di Ferdinando,A. Di Giovanni,N. Di Marco,C. Di Troia,N. Dick,S. Dmitrievski,A. Dominjon,Marcos Dracos,D. Duchesneau,B. Dulach,S. Dusini,J. Ebert,Ilias Efthymiopoulos,O. Egorov,K. Elsener,R. I. Enikeev,Antonio Ereditato,Luigi Salvatore Esposito,C. Fanin,J. Favier,G. Felici,Torben Ferber,R. A. Fini,L. Fournier,A. Franceschi,D. Frekers,T. Fukuda,C. Fukushima,V. I. Galkin,V. A. Galkin,R. Gallet,S. Gardien,A. Garfagnini,G. Gaudiot,G. Giacomelli,M. Giorgini,C. Girerd,C. Goellnitz,T. Goeltzenlichter,J. Goldberg,Dmitry Golubkov,Y. A. Gornushkin,J.-N. Grapton,G. Grella,F. Grianti,Edda Gschwendtner,Christophe Guérin,Murat Guler,C. Gustavino,J.L. Guyonnet,Caren Hagner,T. Hamane,T. Hara,M. Hauger,M. Hess,M. Hierholzer,K. Hoshino,M. Ieva,M. Incurvati,Krešimir Jakovčić,J. Janicsko Csathy,B. Janutta,Cécile Jollet,F. Juget,M. Kazuyama,Seok Kim,N. Khovansky,M. Kimura,B. Klicek,J. Knuesel,Koichi Kodama,D. Kolev,Masahiro Komatsu,U. Kose,Alexey Krasnoperov,I. Kreslo,Z. Krumstein,V. V. Kutsenov,Andrei Kuznetsov,Imad Baptiste Laktineh,M. Lavy,C Lazzaro,T. D. Le,T. Le Flour,J. Lenkeit,J Lewis,S. Lieunard,Ante Ljubičić,A. Longhin,Guillaume Lutter,A. S. Malgin,K. Manai,G. Mandrioli,A. Marotta,J. Marteau,G. Martin-Chassard,V. A. Matveev,N. Mauri,M. Meddahi,F. Meisel,Anselmo Meregaglia,A. Meschini,M. Messina,P. Migliozzi,P. Monacelli,I. Monteiro,F. Moreau,Kunihiro Morishima,U. Moser,M. T. Muciaccia,P. Mugnier,Naotaka Naganawa,Mitsuhiro Nakamura,Toshiyuki Nakano,T. Napolitano,V. Nikitina,Kimio Niwa,Y. Nonoyama,A. Nozdrin,S. Ogawa,A. G. Olchevski,D. Orlandi,G. I. Orlova,V. I. Osedlo,D. Ossetski,M. Paniccia,Alessandro Paoloni,B. D. Park,I. G. Park,Alessandra Pastore,L. Patrizii,L. Pellegrino,E. Pennacchio,H. Pessard,V. Pilipenko,C. Pistillo,N. G. Polukhina,M. Pozzato,K. Pretzl,P. A. Publichenko,F. Pupilli,L. Raux,J. P. Repellin,R. Rescigno,D. Rizhikov,T. M. Roganova,G. Romano,G. Rosa,I. Rostovtseva,André Rubbia,A. Russo,V. G. Ryasny,O. G. Ryazhskaya,A. Sadovski,C. Sanelli,Osamu Sato,Y. Sato,V. Saveliev,G. P. Sazhina,A. Schembri,W. Schmidt Parzefall,H. Schroeder,H. U. Schütz,J. Schuler,L. Scotto Lavina,J. Serrano,H. Shibuya,S. Simone,Maximiliano Sioli,C. Sirignano,G. Sirri,J. S. Song,M. Spinetti,Luca Stanco,N. I. Starkov,Mario Stipčević,T. Strauss,P. Strolin,V. Sugonyaev,Satoru Takahashi,V. P. Talochkin,M. Tenti,V. Tereschenko,F. Terranova,I. Tezuka,V. Tioukov,P. Tolun,V. A. Tsarev,R. Tsenov,S. Tufanli,U. Ugolino,N. Ushida,G. Van Beek,V. Verguilov,T. Viant,Pierre Vilain,M. S. Vladimirov,Lucia Votano,J. L. Vuilleumier,T. Waelchli,Marc Weber,Gaston Wilquet,Björn Wonsak,J. Wurtz,V. F. Yakushev,C. S. Yoon,Yu. Zaitsev,Amina Zghiche,R. Zimmermann +261 more
TL;DR: The OPERA neutrino oscillation experiment has been designed to prove the appearance of ντ in a nearly pure νμ beam (CNGS) produced at CERN and detected in the underground Hall C of the Gran Sasso Laboratory, 730 km away from the source as discussed by the authors.
Journal ArticleDOI
On the Event Observed in the Mont Blanc Underground Neutrino Observatory during the Occurrence of Supernova 1987a
Marco Aglietta,Giovanni Badino,G. Bologna,C. Castagnoli,Antonella Castellina,V. L. Dadykin,W. Fulgione,P. Galeotti,F. F. Kalchukov,B. V. Kortchaguin,P. V. Kortchaguin,A. S. Malguin,V. G. Ryassny,O. G. Ryazhskaya,O. Saavedra,V. P. Talochkin,G. C. Trinchero,S. Vernetto,G. T. Zatsepin,V. F. Yakushev +19 more
TL;DR: In this article, the characteristics of the event detected in the Mont Blanc Underground Neutrino Observatory on February 23, 1987, consisting of 5 interactions recorded during 7s are discussed, and it is shown that the event can be explained in terms of detection of neutrinos emitted during the stellar collapse in the Large Magellanic Cloud.
Journal ArticleDOI
Observation of a first ντ candidate event in the OPERA experiment in the CNGS beam
N. Agafonova,A. B. Aleksandrov,O Altinok,M. Ambrosio,A. M. Anokhina,Shigeki Aoki,Akitaka Ariga,Tomoko Ariga,D. Autiero,A. Badertscher,A. V. Bagulya,A. Bendhabi,A. Bertolin,M. Besnier,D. Bick,V. Boyarkin,Cristiano Bozza,T. Brugière,R. Brugnera,F. Brunet,G. Brunetti,G. Brunetti,S. Buontempo,A. Cazes,L. Chaussard,M. M. Chernyavsky,V. Chiarella,N. Chon-Sen,Artem Chukanov,Robert Ciesielski,F. Dal Corso,Nicola D'Ambrosio,Y. Déclais,P. Del Amo Sanchez,G. De Lellis,M. De Serio,F. Di Capua,A. Di Crescenzo,D. Di Ferdinando,N. Di Marco,A. Di Giovanni,S. Dmitrievsky,Marcos Dracos,D. Duchesneau,S. Dusini,Timur Dzhatdoev,J. Ebert,O. Egorov,R. I. Enikeev,Antonio Ereditato,Luigi Salvatore Esposito,J. Favier,Torben Ferber,R. A. Fini,D. Frekers,T. Fukuda,V. I. Galkin,A. Garfagnini,G. Giacomelli,M. Giorgini,J. Goldberg,C. Göllnitz,Dmitry Golubkov,L. Goncharova,Y. A. Gornushkin,G. Grella,F. Grianti,A. M. Guler,C. Gustavino,Caren Hagner,K. Hamada,T. Hara,M. Hierholzer,K. Hoshino,M. Ieva,H. Ishida,Katsumi Ishiguro,Krešimir Jakovčić,Cécile Jollet,F. Juget,M. Kamiscioglu,J. Kawada,M. Kazuyama,Seok Kim,M. Kimura,Nobuko Kitagawa,B. Klicek,J. Knuesel,K. Kodama,Masahiro Komatsu,U. Kose,I. Kreslo,H. Kubota,C Lazzaro,J. Lenkeit,Ivano Lippi,Ante Ljubičić,A. Longhin,Guillaume Lutter,A. S. Malgin,G. Mandrioli,K Mannai,A. Marotta,J. Marteau,T. Matsuo,V. A. Matveev,N. Mauri,E. Medinaceli,F. Meisel,Anselmo Meregaglia,P. Migliozzi,S. Mikado,S. Miyamoto,P. Monacelli,Kunihiro Morishima,U. Moser,M. T. Muciaccia,Naotaka Naganawa,Tatsuhiro Naka,M. Nakamura,Toshiyuki Nakano,Y. Nakatsuka,Dmitry V. Naumov,V. Nikitina,Kimio Niwa,Y. Nonoyama,S. Ogawa,A. Olchevsky,T. Omura,G. I. Orlova,V. I. Osedlo,M. Paniccia,Alessandro Paoloni,B. D. Park,I. G. Park,Alessandra Pastore,L. Patrizii,E. Pennacchio,H. Pessard,V. Pilipenko,C. Pistillo,N. G. Polukhina,M. Pozzato,K. Pretzl,P. A. Publichenko,F. Pupilli,J.P. Repellin,R. Rescigno,T. M. Roganova,Hiroki Rokujo,G. Romano,G. Rosa,I. Rostovtseva,André Rubbia,A. Russo,V. G. Ryasny,O. G. Ryazhskaya,Y. Sakatani,Osamu Sato,Yoshihiro Sato,A. Schembri,W. Schmidt-Parzefall,H. Schroeder,L. Scotto Lavina,A. Sheshukov,H. Shibuya,S. Simone,Maximiliano Sioli,C. Sirignano,G. Sirri,J. S. Song,M. Spinetti,Luca Stanco,N. I. Starkov,Mario Stipčević,T. Strauss,P. Strolin,K. Suzuki,Satoru Takahashi,M. Tenti,F. Terranova,I. Tezuka,V. Tioukov,P. Tolun,A. Trabelsi,T. Tran,S. Tufanli,Pierre Vilain,M. S. Vladimirov,Lucia Votano,J. L. Vuilleumier,Gaston Wilquet,Björn Wonsak,V. F. Yakushev,C. S. Yoon,J. Yoshida,T. Yoshioka,Yu. Zaitsev,S. Zemskova,Amina Zghiche,R. Zimmermann +200 more
TL;DR: The OPERA neutrino detector in the underground Gran Sasso Laboratory (LNGS) has been designed to perform the first detection of neutrinos oscillations in direct appearance mode through the study of the $
u_mu\rightarrow
u_\tau$ channel.
Journal ArticleDOI
The most powerful scintillator supernovae detector: LVD
Marco Aglietta,Behcet Alpat,E. D. Alyea,P. Antonioli,G. Anzivino,Giovanni Badino,Y. Ban,G. Bari,M. Basile,A. Benelli,V. S. Berezinsky,L. Bergamasco,Stefano Bianco,A. Bizzetti,G. Bruni,Y. Cao,G. Cara Romeo,R. Casaccia,Carlotta Castagnoli,Antonella Castellina,K. Chen,R. Chen,Jose Chinellato,Luisa Cifarelli,G. Cini,Shuang Cong,A. Contin,V. L. Dadikin,M. Dardo,A. De Silva,M. Deutsch,L. G. Dos Santos,R. I. Enikeev,Fabrizio Fabbri,W. Fulgione,P. Galeotti,Piera Luisa Ghia,P. Giusti,F. Grianti,S. Gu,E. S. Hafen,P. Haridas,Giuseppe Iacobucci,N. Inoue,F. F. Khalchukov,E. V. Korolkova,P. V. Kortchaguin,V. B. Kortchaguin,V. A. Kudryavtsev,G. Landi,K. Lau,X. Lin,L. Lu,J. Ma,Z. Ma,G. Maccarrone,A. S. Malguin,Z. Mao,M. A. Markov,T. Massam,B. Mayes,N. Mengotti Silva,Akeo Misaki,G. H. Mo,B. Monteleoni,C. Morello,J. H. Moromisato,Rosario Nania,G. Navarra,L. Panaro,D. Parks,P.G. Pelfer,L. Periale,P. Picchi,P. Pinna,Lawrence Pinsky,I. A. Pless,M. Pu,J. Pyrlyk,J. Qiu,V. G. Ryasny,O. G. Ryazhskaya,O. Saavedra,K. Saitoh,D. Sanders,Gabriella Sartorelli,S. Sarwar,D. Shen,V. P. Talochkin,H. Tang,J. Tang,W. D. Tian,G. C. Trinchero,A. Turtelli,I. Uman,P. Vallania,S. Vernetto,E. von Goeler,L. Votano,Tomonori Wada,F. Wang,H. Wang,S. Wang,R. Weathers,Roy Weinstein,M. Widgoff,L. Xu,Z. Xu,V. F. Yakushev,Isao Yamamoto,G. Yi,A. Zallo,G. T. Zatsepin,X. Zhou,Q. Zhu,X. Zhu,B. Zhuan,Antonino Zichichi +117 more
TL;DR: The Large Volume Detector (LVD) as discussed by the authors is a multipurpose detector consisting of a large volume of liquid scintillator interleaved with limited streamer tubes.
Journal ArticleDOI
Muon ''depth-intensity'' relation measured by the LVD underground experiment and cosmic-ray muon spectrum at sea level
Marco Aglietta,Behcet Alpat,E. D. Alyea,Pietro Antonioli,Giovanni Badino,G. Bari,M. Basile,V. S. Berezinsky,F. Bersani,M. E. Bertaina,R. Bertoni,G. Bonoli,A. Bosco,G. Bruni,G. Cara Romeo,C. Castagnoli,Antonella Castellina,A. Chiavassa,Jose Chinellato,Luisa Cifarelli,F. Cindolo,G. Conforto,Andrea Contin,V. L. Dadykin,A. De Silva,M. Deutsch,P. Dominici,L. G. Dos Santos,L. Emaldi,R. I. Enikeev,Fabrizio Fabbri,W. Fulgione,P. Galeotti,C. Ghetti,P. L. Ghia,P. Giusti,R. Granella,F. Grianti,G. Guidi,E. S. Hafen,P. Haridas,Giuseppe Iacobucci,N. Inoue,E. Kemp,F. F. Khalchukov,Elena Korolkova,P. V. Korchaguin,V. B. Korchaguin,V. A. Kudryavtsev,K. Lau,M. Luvisetto,G. Maccarone,A. S. Malguin,R. Mantovani,T. Massam,B. W. Mayes,Antonella Megna,C. Melagrana,N. Mengotti Silva,C. Morello,J. H. Moromisato,Rosario Nania,G. Navarra,L. Panaro,L. Periale,A. Pesci,P. Picchi,Lawrence Pinsky,I. A. Pless,J. Pyrlik,V. G. Ryasny,O. G. Ryazhskaya,O. Saavedra,K. Saitoh,Stefano Santini,G. Sartorelli,M. Selvi,N. Taborgna,V. P. Talochkin,J. Tang,G. C. Trinchero,S. Tsuji,A. Turtelli,I. Uman,P. Vallania,G. Van Buren,S. Vernetto,F. Vetrano,Carlo Vigorito,E. von Goeler,L. Votano,Tomonori Wada,Roy Weinstein,M. Widgoff,V. F. Yakushev,Isao Yamamoto,G. T. Zatsepin,Antonino Zichichi +97 more
TL;DR: In this article, an analysis of muon events with all muon multiplicities collected during 21804 h of operation of the first Large Volume Detector tower was presented, where the measured angular distribution of the muon intensity has been converted to the ''depth-vertical-intensity'' relation in the depth range from 3 to 12 km w.r.t.