A
A. Marotta
Researcher at University of Naples Federico II
Publications - 41
Citations - 1650
A. Marotta is an academic researcher from University of Naples Federico II. The author has contributed to research in topics: Neutrino & Nuclear emulsion. The author has an hindex of 20, co-authored 41 publications receiving 1583 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
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
Measurement of nucleon structure functions in neutrino scattering
Gulsen Onengut,R. van Dantzig,M. de Jong,Rudolf Oldeman,Murat Guler,S. Kama,U. Kose,M. Serin-Zeyrek,P. Tolun,M. G. Catanesi,M. T. Muciaccia,A. Bülte,K. Winter,B. Van de Vyver,Pierre Vilain,Gaston Wilquet,Biagio Saitta,E. Di Capua,S. Ogawa,H. Shibuya,Ivana Hristova,A. Kayis-Topaksu,T. Kawamura,D. Kolev,M. Litmaath,H. Meinhard,J. Panman,Alexandre Rozanov,R. Tsenov,J. W. E. Uiterwijk,Piero Zucchelli,J. Goldberg,Michiyuki Chikawa,J. S. Song,C. S. Yoon,Koichi Kodama,N. Ushida,Shigeki Aoki,T. Hara,Th. Delbar,Denis Favart,Ghislain Grégoire,S. Kalinin,I. Makhlioueva,A. Artamonov,P. Gorbunov,V. Khovansky,V. Shamanov,Ilya Tsukerman,N. Bruski,D. Frekers,D. Rondeshagen,T. Wolff,K. Hoshino,J. Kawada,Masahiro Komatsu,Motoaki Miyanishi,M. Nakamura,Toshiyuki Nakano,K. Narita,K. Niu,K. Niwa,N. Nonaka,Osamu Sato,T. Toshito,Salvatore Buontempo,A. G. Cocco,Nicola D'Ambrosio,G. De Lellis,G. De Rosa,F. Di Capua,G. Fiorillo,A. Marotta,M. Messina,P. Migliozzi,R. Santorelli,L. Scotto Lavina,P. Strolin,V. Tioukov,T. Okusawa,U. Dore,P. F. Loverre,L. Ludovici,G. Rosa,R. Santacesaria,A. Satta,F. R. Spada,E. Barbuto,Cristiano Bozza,G. Grella,G. Romano,C. Sirignano,S. Sorrentino,Yoshihiro Sato,I. Tezuka +94 more
TL;DR: In this article, the neutrino-nucleon and anti-neutrino−nucleons differential cross-sections are measured in the range 0.01 x 0.7, 0.05 y 0.95, 10 E ν 200 GeV.
Journal ArticleDOI
High-speed particle tracking in nuclear emulsion by last-generation automatic microscopes
N. Armenise,M. De Serio,M. Ieva,M. T. Muciaccia,Alessandra Pastore,S. Simone,J. Damet,I. Kreslo,N. Savvinov,T. Waelchli,L. Consiglio,M. Cozzi,D. Di Ferdinando,Luigi Salvatore Esposito,G. Giacomelli,M. Giorgini,G. Mandrioli,L. Patrizii,Maximiliano Sioli,G. Sirri,L. Arrabito,Imad Baptiste Laktineh,P. Royole-Degieux,S. Buontempo,Nicola D'Ambrosio,G. De Lellis,G. De Rosa,F. Di Capua,D. Coppola,F. Formisano,A. Marotta,P. Migliozzi,C. Pistillo,L. Scotto Lavina,G. Sorrentino,P. Strolin,V. Tioukov,Frédéric Juget,M. Hauger,G. Rosa,E. Barbuto,Cristiano Bozza,G. Grella,G. Romano,C. Sirignano +44 more
TL;DR: The European Scanning System (ES) as discussed by the authors is a last-generation automatic microscope working at a scanning speed of 20 cm 2 / h, designed to unambigously detect ν μ → ν τ oscillations in nuclear emulsions.
Journal ArticleDOI
Hardware performance of a scanning system for high speed analysis of nuclear emulsions
L. Arrabito,E. Barbuto,Cristiano Bozza,Salvatore Buontempo,L. Consiglio,D. Coppola,M. Cozzi,J. Damet,Nicola D'Ambrosio,G. De Lellis,M. De Serio,F. Di Capua,D. Di Ferdinando,D. Di Marco,Luigi Salvatore Esposito,G. Giacomelli,G. Grella,M. Hauger,F. Juget,I. Kreslo,M. Giorgini,M. Ieva,Imad Baptiste Laktineh,K. Manai,G. Mandrioli,A. Marotta,Shahid Manzoor,P. Migliozzi,P. Monacelli,M. T. Muciaccia,Alessandra Pastore,L. Patrizii,C. Pistillo,M. Pozzato,P. Royole-Degieux,G. Romano,G. Rosa,N. Savvinov,A. Schembri,L. Scotto Lavina,S. Simone,Maximiliano Sioli,C. Sirignano,G. Sirri,G. Sorrentino,P. Strolin,V. Tioukov,T. Waelchli +47 more
TL;DR: The European Scanning System (ESS) as discussed by the authors is a very fast automatic system developed for the mass scanning of the emulsions of the OPERA experiment, which requires microscopes with scanning speeds of 20 cm 2 =h in an emulsion volume of 44mm thickness.