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1. Final results on oscillation from the CHORUS experiment

Author: O. Melzer, K. Niu, T. Wolff, N. Nonaka, Antonio Ereditato, V. Shamanov, C. Sirignano, M. van Beuzekom, Yoshihiro Sato, T. Okusawa, P. Strolin, R. Santacesaria, Alexandre Rozanov, H. Shibuya, E. Pesen, G. Brooijmans, B. Van de Vyver, D. Bonekämper, Piero Zucchelli, S. Di Liberto, M. Kazuno, J. Hérin, Ramazan Sever, Mitsuhiro Nakamura, P. Gorbunov, K. Nakamura, Pierre Vilain, T. Hara, A. Mailov, Mathieu Doucet, G. Piredda, Y. Ishii, M. Messina, M. A. Mazzoni, J. Panman, M. De Serio, J. Kawada, A. Maslennikov, G. Romano, M. Serin-Zeyrek, A. Bülte, M. de Jong, E. Di Capua, Gulsen Onengut, Y. Kotaka, G. Fiorillo, D. Rondeshagen, Toshiyuki Nakano, N. Ushida, Mehmet Zeyrek, Shigeki Aoki, I. Tezuka, S. Buontempo, E. Arik, G. De Lellis, P. Migliozzi, K. Narita, S. Simone, E. Barbuto, N. Armenise, Michiyuki Chikawa, F. Di Capua, J. Konijn, S. Kalinin, U. Dore, V. Palladino, M. Vander Donckt, T. Kozaki, Ivana Hristova, C.A.F.J. van der Poel, L. Ludovici, Nicola D'Ambrosio, Mihail Chizhov, E. Eskut, C. Luppi, Masahiro Komatsu, T. Toshito, A. Artamonov, R. Tsenov, H. Meinhard, D. Frekers, David Saltzberg, Antonio Capone, D. Kolev, N. Bruski, I.M. Papadopoulos, G. Grégoire, P. F. Loverre, Koichi Kodama, S. Sorrentino, L. Scotto Lavina, S. Ogawa, Jean-Paul Fabre, J. Goldberg, A. Satta, C. S. Yoon, Henry T. Wong, Denis Favart, M. Litmaath, M. T. Muciaccia, T. Kawamura, Ch. Weinheimer, Rudolf Oldeman, R. van Dantzig, Ilya Tsukerman, J. W. E. Uiterwijk, M. G. Catanesi, G. De Rosa, V. Khovansky, A. Kayis-Topaksu, D. De Pedis, K. Winter, Murat Guler, G. Grella, Y. Obayashi, K. Niwa, Th. Delbar, H. Øverȧs, David Cussans, Motoaki Miyanishi, W. Flegel, K. Hoshino, F. R. Spada, U. Kose, E. Niu, F. Cassol, G. Rosa, Gaston Wilquet, P. Tolun, S. Ricciardi, I. Makhlioueva, J. S. Song, Cristiano Bozza, E. Radicioni, Jürgen Brunner, Osamu Sato, L. Vivolo, A. G. Cocco, Jan Visschers, P. Righini, Biagio Saitta, V. Tioukov, A. Marotta, Çukurova Üniversitesi, Eskut, E., Kayis Topaksu, A., Önengüt, G., van Beuzekom, M. G., van Dantzig, R., de Jong, M., Konijn, J., Melzer, O., Oldeman, R. G. C., Pesen, E., van der Poel, C. A. F. J., Visschers, J. L., Güler, M., Köse, U., Serin Zeyrek, M., Sever, R., Tolun, P., Zeyrek, M. T., Armenise, N., Cassol, F., Catanesi, M. G., De Serio, M., Muciaccia, M. T., Radicioni, E., Righini, P., Simone, S., Vivolo, L., Bülte, A., Winter, K., Vander Donckt, M., Van de Vyver, B., Vilain, P., Wilquet, G., Saitta, B., Di Capua, E., Luppi, C., Ishii, Y., Kazuno, M., Ogawa, S., Shibuya, H., Brunner, J., Chizhov, M., Cussans, D., Doucet, M., Fabre, J. P., Flegel, W., Hristova, I. R., Kawamura, T., Kolev, D., Litmaath, M., Meinhard, H., Niu, E., Øverȧs, H., Panman, J., Papadopoulos, I. M., Ricciardi, S., Rozanov, A., Saltzberg, D., Tsenov, R., Uiterwijk, J. W. E., Weinheimer, C., Wong, H., Zucchelli, P., Goldberg, J., Chikawa, M., Arik, E., Mailov, A. A., Song, J. S., Yoon, C. S., Kodama, K., Ushida, N., Aoki, S., Hara, T., Brooijmans, G., Delbar, T., Favart, D., Grégoire, G., Hérin, J., Kalinin, S., Makhlioueva, I., Artamonov, A., Gorbunov, P., Khovansky, V., Shamanov, V., Tsukerman, I., Bonekämper, D., Bruski, N., Frekers, D., Rondeshagen, D., Wolff, T., Hoshino, K., Kawada, J., Komatsu, M., Kotaka, Y., Kozaki, T., Miyanishi, M., Nakamura, M., Nakano, T., Narita, K., Niu, K., Niwa, K., Nonaka, N., Obayashi, Y., Sato, O., Toshito, T., Buontempo, S., Cocco, A. G., D'Ambrosio, N., De Lellis, G., De Rosa, G., DI CAPUA, Francesco, Ereditato, A., Fiorillo, Giuliana, Marotta, A., Messina, M., Migliozzi, P., Palladino, V., Scotto Lavina, L., Strolin, P., Tioukov, V., Nakamura, K., Okusawa, T., Capone, A., De Pedis, D., Di Liberto, S., Dore, U., Loverre, P. F., Ludovici, L., Maslennikov, A., Mazzoni, M. A., Piredda, G., Rosa, G., Santacesaria, R., Satta, A., Spada, F. R., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sirignano, C., Sorrentino, S., Sato, Y., and Tezuka, I.
Subjects: Physics, Nuclear and High Energy Physics, Muon, biology, Oscillation, Chorus, Weinberg angle, biology.organism_classification, Tau lepton appearance, Nuclear physics, Neutrino, Neutrino oscillation, Lepton, Event reconstruction
Abstract: The final oscillation analysis of the complete set of data collected by CHORUS in the years 1994-1997 is presented. Reconstruction algorithms of data extracted by electronic detectors were improved and the data recorded in the emulsion target were analysed by new automated scanning systems, allowing the use of a new method for event reconstruction in emulsion. CHORUS has applied these new techniques to the sample of 1996-1997 events for which no muons were observed in the electronic detectors. Combining the new sample with the data analysed in previous papers, the overall sensitivity of the experiment to the ?? appearance is thus improved. In a two-neutrino mixing scheme, a 90% C.L. upper limit of sin2 2 ?µ ? < 4.4 × 10-4 is set for large ? m2, improving by a factor 1.5 the previously published CHORUS result. © 2007 Elsevier B.V. All rights reserved. Bundesministerium für Bildung und Forschung: 05 7MS12P, 05 6BU11P Grant Foundation: KRF-2003-005-C00014 Promotion and Mutual Aid Corporation for Private Schools of Japan CERN Israel Science Foundation: 328/94 Brussels Instituut voor Milieubeheer Istituto Nazionale di Fisica Nucleare Foundation for Fundamental Research on Matter Korean Foundation for Cancer Research Walter Burke Institute for Theoretical Physics We gratefully acknowledge the help and support of the neutrino beam staff and of the numerous technical collaborators who contributed to the detector construction, operation, emulsion pouring, development, and scanning. The experiment has been made possible by grants from the Institut Interuniversitaire des Sciences Nucléaires and the Interuniversitair Instituut voor Kernwetenschappen (Belgium), the Israel Science Foundation (grant 328/94) and the Technion Vice President Fund for the Promotion of Research (Israel), CERN (Geneva, Switzerland), the German Bundesministerium für Bildung und Forschung (contract numbers 05 6BU11P and 05 7MS12P) (Germany), the Institute of Theoretical and Experimental Physics (Moscow, Russia), the Istituto Nazionale di Fisica Nucleare (Italy), the Promotion and Mutual Aid Corporation for Private Schools of Japan and Japan Society for the Promotion of Science (Japan), the Korea Research Foundation Grant (KRF-2003-005-C00014) (Republic of Korea), the Foundation for Fundamental Research on Matter FOM and the National Scientific Research Organization NWO (The Netherlands), and the Scientific and Technical Research Council of Turkey (Turkey). We gratefully acknowledge their support.
Published: 2008

2. Measurement of the Z/A dependence of neutrino charged-current total cross-sections

Author: Kayis Topaksu, A. a, Onengüt, G. a, van Dantzig, R. b, de Jong, M. b, Konijn, J. b, Melzer, O. b, Oldeman, R. G. C. bz, Pesen, E. b, van der Poel, C. A. F. J. b, Spada, F. R. baa, Visschers, J. L. b, Güler, M. cab, Serin Zeyrek, M. c, Kama, S. c, Sever, R. c, Tolun, P. c, Zeyrek, M. T. c, Armenise, N. d, Catanesi, M. G. d, de Serio, M. d, leva, M. d, Muciaccia, M. T. d, Radicioni, E. d, Simone, S. d, Bülte, A. e, Winter, K. e, El Aidi, R. f, van de Vyver, B. fabac, Vilain, P. fad, Wilquet, G. fad, Saitta, B. g, Di Capua, E. h, Ogawa, S. i, Shibuya, H. i, Artamonov, A. j, Brunner, J. jae, Chizhov, M. jaf, Cussans, D. jag, Doucet, M. jah, Fabre, J. P. j, Hristova, I. R. jaf, Kawamura, T. j, Kolev, D. jaf, Litmaath, M. jai, Meinhard, H. j, Panman, J. j, Papadopoulos, I. M. j, Ricciardi, S. jaj, Rozanov, A. jae, Saltzberg, D. jak, Tsenov, R. jaf, Uiterwijk, J. W. E. j, Zucchelli, P. j, Goldberg, J. k, Chikawa, M. l, Arik, E. m, Song, J. S. n, Yoon, C. S. n, Kodama, K. o, Ushida, N. o, Aoki, S. p, Hara, T. p, Delbar, T. q, Favart, D. q, Grégoire, G. q, Kalinin, S. q, Makhlyoueva, I. q, Gorbunov, P. rac, Khovansky, V. r, Shamanov, V. r, Tsukerman, I. r, Bruski, N. s, Frekers, D. s, Rondeshagen, D. s, Wolff Westfälische, T. s, Hoshino, K. t, Kawada, J. t, Komatsu, M. t, Miyanishi, M. t, Nakamura, M. t, Nakano, T. t, Narita, K. t, Niu, K. t, Niwa, K. t, Nonaka, N. t, Sato, O. t, Toshito, T. t, Buontempo, S. u, Cocco, A. G. u, D'Ambrosio, N. u, de Lellis, G. u, de Rosa, Ereditato, A. u, Fiorillo, G. u, Marotta, A. u, Messina, M. u, Migliozzi, P. u, Pistillo, C. u, Santorelli, R. u, Scotto Lavina, L. u, Strolin, P. u, Tioukov, V. u, Nakamura, K. v, Okusawa, T. v, Dore, U. w, Loverre, P. F. w, Ludovici, L. w, Maslennikov, A. wal, Righini, P. w, Rosa, G. w, Santacesaria, R. w, Satta, A. w, Barbuto, E. x, Bozza, C. x, Grella, G. x, Romano, G. x, F. , Sorrentino, S. x, Sato, Y. y, Tezuka, I. y., DI CAPUA, FRANCESCO, Çukurova Üniversitesi, K., Narita, K., Niu, K., Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, F. D., Capua, A., Ereditato, Fiorillo, Giuliana, A., Marotta, M., Messina, P., Migliozzi, C., Pistillo, R., Santorelli, L. S., Lavina, P., Strolin, V., Tioukov, K., Nakamura, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, A., Maslennikov, P., Righini, G., Rosa, R., Santacesaria, A., Satta, E., Barbuto, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, I., Tezuka, Kayis, Topaksu, A. a, Onengüt, G., A., Van, Dantzig, R., B., De, Jong, M. b, Konijn, J. b, Melzer, O. b, Oldeman, R. G. C., Bz, Pesen, E. b, van der, Poel, C. A. F. J. b, Spada, F. R., Baa, Visschers, J. L. b, Güler, M., Cab, Serin, Zeyrek, M. c, Kama, S. c, Sever, R. c, Tolun, P. c, Zeyrek, M. T. c, Armenise, N. d, Catanesi, M. G., D., De, Serio, M. d, Leva, M. d, Muciaccia, M. T. d, Radicioni, E. d, Simone, S. d, Bülte, A. e, Winter, K., E., El, Aidi, R., F., van de, Vyver, B., Fabac, Vilain, P., Fad, Wilquet, G., Fad, Saitta, B. g, Di, Capua, E. h, Ogawa, S. i, Shibuya, H. i, Artamonov, A. j, Brunner, J., Jae, Chizhov, M., Jaf, Cussans, D., Jag, Doucet, M., Jah, Fabre, J. P. j, Hristova, I. R., Jaf, Kawamura, T. j, Kolev, D., Jaf, Litmaath, M., Jai, Meinhard, H. j, Panman, J. j, Papadopoulos, I. M. j, Ricciardi, S., Jaj, Rozanov, A., Jae, Saltzberg, D., Jak, Tsenov, R., Jaf, Uiterwijk, J. W. E. j, Zucchelli, P. j, Goldberg, J. k, Chikawa, M. l, Arik, E. m, Song, J. S. n, Yoon, C. S. n, Kodama, K. o, Ushida, N. o, Aoki, S. p, Hara, T. p, Delbar, T. q, Favart, D. q, Grégoire, G. q, Kalinin, S. q, Makhlyoueva, I. q, Gorbunov, P., Rac, Khovansky, V. r, Shamanov, V. r, Tsukerman, I. r, Bruski, N., Frekers, D., Rondeshagen, D., Wolff, Westfälische, T. s, Hoshino, K. t, Kawada, J. t, Komatsu, M. t, Miyanishi, M. t, Nakamura, M. t, Nakano, T. t, Narita, K. t, Niu, K. t, Niwa, K. t, Nonaka, N. t, Sato, O. t, Toshito, T. t, Buontempo, S. u, Cocco, A. G. u, D'Ambrosio, N., U., De, Lelli, G., U., De, Rosa, DI CAPUA, Francesco, Ereditato, A. u, Fiorillo, G. u, Marotta, A. u, Messina, M. u, Migliozzi, P. u, Pistillo, C. u, Santorelli, R. u, Scotto, Lavina, L. u, Strolin, P. u, Tioukov, V. u, Nakamura, K. v, Okusawa, T. v, Dore, U. w, Loverre, P. F. w, Ludovici, L. w, Maslennikov, A., Wal, Righini, P. w, Rosa, G. w, Santacesaria, R. w, Satta, A. w, Barbuto, E. x, Bozza, C. x, Grella, G. x, Romano, G. x, F., Sorrentino, S. x, Sato, Y. y, Tezuka, and I., Y.
Subjects: Physics, CHORUS EXPERIMENT, Large Hadron Collider, Physics and Astronomy (miscellaneous), Period (periodic table), Physics::Instrumentation and Detectors, Detector, RATIOS, Calorimeter, Nuclear physics, Flux (metallurgy), High Energy Physics::Experiment, Neutrino, Atomic physics, CALORIMETER, Engineering (miscellaneous), Particle Physics - Experiment, Charged current, Beam (structure)
Abstract: A relative measurement of total cross-sections is reported for polyethylene, marble, iron, and lead targets for the inclusive charged-current reaction nu(mu) + N --> mu- + X. The targets, passive blocks of similar to100 kg each, were exposed simultaneously to the CERN SPS wide-band muon-neutrino beam over a period of 18 weeks. Systematic effects due to differences in the neutrino flux and detector efficiency for the different target locations were minimised by changing the position of the four targets on their support about every two weeks. The relative neutrino fluxes on the targets were monitored within the same experiment using charged-current interactions in the calorimeter positioned directly downstream of the four targets. From a fit to the Z/A dependence of the total cross-sections a value is deduced for the effective neutron-to-proton cross-section ratio.
Published: 2003

3. Charge identification of highly ionizing particles in desensitized nuclear emulsion using high speed read-out system

Author: Masanobu Ozaki, M. Natsume, H. Shibuya, Tatsumi Koi, Taku Nakamura, Koichi Kodama, Takashi Sasaki, S. Kameoka, Masataka Komori, S. Ogawa, Nobuyuki Kanematsu, Satoru Takahashi, K. Murakami, Naotaka Naganawa, Shinji Sato, M. Shibasaki, T. Fukuda, Mitsutaka Kanazawa, Ken Yusa, C. Fukushima, K. Amako, T. Toshito, Shigeki Aoki, Kimio Niwa, Makoto Asai, and T. Ban
Subjects: Physics, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Dynamic range, Track (disk drive), chemistry.chemical_element, Charged particle, Ion, chemistry, Ionization, Emulsion, Nuclear emulsion, Atomic physics, Nuclear Experiment, Instrumentation, Helium
Abstract: We performed an experimental study of charge identification of heavy ions from helium to carbon having energy of about 290 MeV/u using an emulsion chamber. Emulsion was desensitized by means of forced fading (refreshing) to expand a dynamic range of response to highly charged particles. For the track reconstruction and charge identification, the fully automated high speed emulsion read-out system, which was originally developed for identifying minimum ionizing particles, was used without any modification. Clear track by track charge identification up to Z=6 was demonstrated. The refreshing technique has proved to be a powerful technique to expand response of emulsion film to highly ionizing particles.
Published: 2006

4. Measurement of neutrino oscillation by the K2K experiment

Author: S. Andringa, T. Nakadaira, R. Gran, Tadayuki Takahashi, Yoshitaka Itow, Makoto Sakuda, F. Nakata, K. Fujii, A. Rodriguez, D. Kerr, M. H. Ahn, U. Dore, S. Likhoded, S P Mikheyev, K. Martens, Y. Totsuka, Y. Takubo, Kate Scholberg, Y. Takeuchi, Yu. Kudenko, Shinya Yamada, H. I. Jang, S. C. Boyd, M. Okumura, A. Blondel, A. Ikeda, K. Tashiro, Itsuo Nakano, C. K. Jung, M. Sekiguchi, H. Yokoyama, F. Pierre, Minoru Yoshida, M. Kitamura, L. Whitehead, K. Taki, S. Nawang, N. Yershov, Shogo Nishiyama, O. V. Mineev, E. Sharkey, K. Kaneyuki, Hirokazu Ishino, D. Kielczewska, Shoei Nakayama, Taichi Morita, Y. Kurimoto, Hiroyuki Noumi, T. Otaki, R. Schroeter, L. Ludovici, E. J. Jeon, Takashi Kobayashi, J. Kameda, M. Onchi, Y. Yamanoi, C. Cavata, M. Sorel, Katsuki Hiraide, H. C. Bhang, P. F. Loverre, J. Bouchez, M. Y. Pac, G. Sitjes, S. Mine, C. O. Kim, I. Kato, E. Seo, A. Shima, T. Kutter, K. Hayashi, H. So, S. M. Oser, T. Ishida, J. Hill, J. Catala, A. K. Ichikawa, Tomoyuki Maruyama, T. Hara, K. K. Joo, Lawrence Sulak, P. Novella, Susumu Noda, S. Fukuda, K. Takenaka, Yoshitaka Kuno, T. Ishii, Masaaki Tanaka, F. Nova, John G. Learned, Y. Yamada, B. H. Kang, Y. Obayashi, M. Takasaki, A. Minamino, A. Tornero-Lopez, J.J. Gómez-Cadenas, Takanori Sasaki, M. Fechner, S. Echigo, C. Yanagisawa, J. Zalipska, C. McGrew, G. Jover, J.H. Kim, K. Nakamura, K. B. McConnel Mahn, S. B. Kim, V. A. Matveev, M. Minakawa, A. Cervera, C. W. Walter, Y. Takenaga, Y. Hayato, Yuichi Oyama, Masaya Hasegawa, M. Miura, G. Kume, M. Tada, David William Casper, Takehisa Hasegawa, C. Mitsuda, K. Sato, J. Hosaka, A. Suzuki, R. L. Helmer, Hyosun Kim, Katsuhiro Kobayashi, A. Sakai, Nobuyuki Sakurai, Yusuke Koshio, S. Ueda, Shoji Yamamoto, J. Mallet, S. Matsuno, H. Takeuchi, T. Ooyabu, Masayuki Nakahata, Y. Aoyama, R. Terri, R. Ashie, H. Ishii, Y. Suga, Masashi Yokoyama, J. S. Jang, G. Mitsuka, E. Aliu, H. Tanaka, A. Sarrat, Mark R. Vagins, K. K. Shiraishi, Takaaki Kajita, Masaki Ishitsuka, Kenichi Tanaka, Yoshihiro Suzuki, H. Park, Masaharu Ieiri, X. Espinal, Y. Moriguchi, Beom Jun Kim, Michael B. Smy, Y. Fukuda, T. Iwashita, R. J. Wilkes, I. Higuchi, I. T. Lim, Y. Kato, W. R. Kropp, Federico Sanchez, Toshio Namba, C. Mariani, H. Maesaka, Ko Okumura, E. Kearns, Shigeki Aoki, T. Toshito, Hiroshi Sato, K. Asakura, P. Kitching, C. Mauger, J. Argyriades, H. Nishino, S. H. Lim, A. Okada, M. Kohama, M. Takatsuki, F. Berghaus, Tsuyoshi Nakaya, C. Saji, J. Kubota, Jordi Burguet-Castell, H. G. Berns, W. Wang, Masataka Iinuma, E. Hirose, J. Yoo, K. Nishikawa, J. Y. Kim, Henry W. Sobel, K. Nitta, Y. Tanaka, Masato Shiozawa, Shaomin Chen, A. Konaka, Shigetaka Moriyama, K. O. Cho, R. Nambu, N. Tamura, Silvia Borghi, J. L. Stone, T. Inagaki, A. N. Khotjantsev, Y. Fujii, J. H. Choi, M. M. Khabibullin, Stephane T'Jampens, E. Fernandez, I. S. Jeong, and K. Ishihara
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Tamura, Norio, 010308 nuclear & particles physics, Oscillation, T2K experiment, FOS: Physical sciences, Física, Elementary particle, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, Massless particle, High Energy Physics - Experiment (hep-ex), K2K experiment, 0103 physical sciences, 田村, 詔生, Neutrino, 010306 general physics, Neutrino oscillation, Lepton
Abstract: We present measurements of nu_mu disappearance in K2K, the KEK to Kamioka long-baseline neutrino oscillation experiment. One hundred and twelve beam-originated neutrino events are observed in the fiducial volume of Super-Kamiokande with an expectation of 158.1^{+9.2}_{-8.6} events without oscillation. A distortion of the energy spectrum is also seen in 58 single-ring muon-like events with reconstructed energies. The probability that the observations are explained by the expectation for no neutrino oscillation is 0.0015% (4.3sigma). In a two flavor oscillation scenario, the allowed Delta m^2 region at sin^2(2theta) is between 1.9 and 3.5 x 10^{-3} eV^2 at the 90% C.L. with a best-fit value of 2.8 x 10^{-3} eV^2., Comment: 40 pages, 48 figures
Published: 2006

5. Measurements of D0 production and of decay branching fractions in neutrino–nucleon scattering

Author: Motoaki Miyanishi, Yoshihiro Sato, Nicola D'Ambrosio, V. Khovansky, M. T. Muciaccia, T. Kawamura, Alfredo G. Cocco, G. Rosa, A. Kayis-Topaksu, F. Di Capua, F. R. Spada, I. Tezuka, Ghislain Grégoire, Salvatore Buontempo, K. Hoshino, Toshiyuki Nakano, Th. Delbar, E. Barbuto, Denis Favart, G. De Lellis, P. Migliozzi, M. Messina, P. F. Loverre, G. Romano, Pierre Vilain, S. Sorrentino, L. Ludovici, E. Di Capua, L. Scotto Lavina, R. Santacesaria, M. Nakamura, P. Gorbunov, G. Fiorillo, Chiara Sirignano, A. Artamonov, M. de Jong, Gaston Wilquet, H. Shibuya, C. S. Yoon, P. Tolun, I. Makhlioueva, H. Meinhard, M. Sorrentino, Ilya Tsukerman, Murat Guler, R. van Dantzig, Alexandre Rozanov, S. Kalinin, Kimio Niwa, G. Grella, Masahiro Komatsu, Shigeki Aoki, Utku Kose, A. Satta, B. Van de Vyver, U. Dore, T. Toshito, N. Ushida, K. Winter, K. Narita, Piero Zucchelli, D. Frekers, K. Kodama, J. W. E. Uiterwijk, Rudolf Oldeman, J. Goldberg, Osamu Sato, Cristiano Bozza, N. Nonaka, V. Shamanov, D. Kolev, Biagio Saitta, Jiro Kawada, V. Tioukov, G. De Rosa, Gulsen Onengut, A. Marotta, Michiyuki Chikawa, K. Niu, T. Okusawa, P. Strolin, S. Ogawa, R. Tsenov, T. Hara, J. S. Song, N. Bruski, M. G. Catanesi, J. Panman, and Ivana Hristova
Subjects: Nuclear physics, Physics, Nuclear and High Energy Physics, Particle physics, Large Hadron Collider, Scattering, Branching fraction, Nuclear emulsion, Neutrino, Nucleon, Charged current, Charged particle
Abstract: During the years 1994–1997, the emulsion target of the CHORUS detector was exposed to the wide-band neutrino beam of the CERN SPS of 27 GeV average neutrino energy. In total about 100 000 charged-current neutrino interactions were located in the nuclear emulsion target and fully reconstructed. From this sample of events which was based on the data acquired by new automatic scanning systems, 1048 charged-current interactions with a D 0 in the final state were selected by a pattern recognition program and confirmed as neutral-particle decays through visual inspection. The ratio of decay branching fractions of the D 0 into four charged particles to two charged particles was measured to be B ( D 0 → V 4 ) / B ( D 0 → V 2 ) = 0.207 ± 0.016 ± 0.004 . The inclusive measurement of the observed production rate of the D 0 with a decay into four charged prongs in combination with external measurements of this topological branching ratio was used to determine the total D 0 production rate by neutrinos without additional assumption on the branching fractions. The value of this rate relative to the charged-current cross-section was found to be σ ( D 0 ) / σ ( CC ) = 0.0269 ± 0.0018 ± 0.0013 . In addition, the same normalization method was used to deduce the inclusive topological decay rate into final states with neutral particles only. A value of 0.218 ± 0.049 ± 0.036 was found for this branching fraction. From an observed number of three charged six-prong events the branching ratio into six charged particles was determined to be ( 1.2 −0.9 +1.3 ± 0.2 ) × 10 −3 . A measurement of the energy dependence of the D 0 production by neutrinos relative to the total charged-current cross-section is also reported. This measurement was used to deduce for m c , the effective charm-quark mass, a value of ( 1.42 ± 0.08 ) GeV / c 2 .
Published: 2005

6. Measurement of D*+ production in charged-current neutrino interactions

Author: I. Tezuka, Osamu Sato, Mitsuhiro Nakamura, Yoshihiro Sato, H. Meinhard, N. Nonaka, S. Buontempo, Gulsen Onengut, F. Di Capua, Koichi Kodama, Piero Zucchelli, V. Shamanov, G. Grella, K. Niu, T. Okusawa, P. Strolin, D. Kolev, Cristiano Bozza, S. Sorrentino, Biagio Saitta, G. De Rosa, Ilya Tsukerman, J. W. E. Uiterwijk, L. Scotto Lavina, S. Ogawa, Pierre Vilain, H. Shibuya, Nicola D'Ambrosio, Jiro Kawada, V. Tioukov, C. S. Yoon, Alexandre Rozanov, G. Grégoire, A. Kayis-Topaksu, P. F. Loverre, A. Satta, M. T. Muciaccia, B. Van de Vyver, M. Messina, L. Ludovici, K. Winter, T. Kawamura, Alfredo G. Cocco, A. Marotta, P. Gorbunov, J. Panman, Rudolf Oldeman, G. Romano, G. Fiorillo, N. Ushida, A. Artamonov, G. Rosa, J. S. Song, Gaston Wilquet, P. Tolun, K. Hoshino, M. de Jong, Masahiro Komatsu, T. Toshito, J. Goldberg, F. R. Spada, U. Kose, Murat Guler, I. Makhlioueva, Toshiyuki Nakano, R. van Dantzig, K. Narita, E. Barbuto, G. De Lellis, E. Di Capua, Chiara Sirignano, V. Khovansky, Shigeki Aoki, K. Niwa, N. Bruski, Th. Delbar, R. Tsenov, M. G. Catanesi, Ivana Hristova, Michiyuki Chikawa, P. Migliozzi, T. Hara, Motoaki Miyanishi, S. Kalinin, U. Dore, D. Frekers, Denis Favart, and R. Santacesaria
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Large Hadron Collider, Physics::Instrumentation and Detectors, Hadron, Neutrino beam, Nuclear physics, High Energy Physics::Experiment, Nuclear emulsion, Production (computer science), Neutrino, Nuclear Experiment, Neutrino oscillation, Charged current
Abstract: During the years 1994–1997, the emulsion target of the CHORUS detector was exposed to the wide-band neutrino beam of the CERN SPS of 27 GeV average neutrino energy. In total about 100 000 charged-current neutrino interactions were located in the nuclear emulsion target and fully reconstructed. A high-statistics sample of neutrino interactions with a D 0 in the final state was collected. Using the decay mode D * + → D 0 π + a production cross-section measurement of the D * + in neutrino–nucleon charged-current interactions was performed. The low Q-value of the decay was used to isolate a sample of candidate events containing a positive hadron with a small p T with respect to the D 0 direction. A signal of 22.1 ± 5.5 D * + events was obtained. The D * + production cross-section relative to the D 0 production cross-section, σ ( D * + ) / σ ( D 0 ) , was estimated to be 0.38 ± 0.09 ( stat ) ± 0.05 ( syst ) . From this result, the fraction of D 0 's produced via the decay of a D * was deduced to be 0.63 ± 0.17 . The D * + production cross-section relative to the ν μ charged-current interaction, σ ( D * + ) / σ ( CC ) , was estimated to be [ 1.02 ± 0.25 ( stat ) ± 0.15 ( syst ) ] % .
Published: 2005

7. Indications of Neutrino Oscillation in a 250 km Long-Baseline Experiment

Author: David William Casper, C. W. Walter, Makoto Sakuda, C. Yanagisawa, Toshio Namba, M. H. Ahn, K. Martens, W. R. Kropp, Nobuyuki Sakurai, H. W. Sobel, S. Fukuda, Atsumu Suzuki, H. Maesaka, Takehisa Hasegawa, T. Iwashita, Minoru Yoshida, Y. Fukuda, S. H. Lim, S. B. Boyd, K. Nishikawa, S. Mine, J. L. Stone, Y. Takeuchi, K. Kaneyuki, Yuichi Oyama, E. Kearns, T. Inagaki, Shinya Yamada, Y. Totsuka, E. J. Jeon, M. Kohama, Shoei Nakayama, Koji Nakamura, S. Matsuno, H. I. Jang, Kazumasa Miyano, J. Hill, C. K. Jung, Masaya Hasegawa, M. Miura, S. B. Kim, Tomoyuki Maruyama, J. H. Choi, D. Kielczewska, Hwangseo Park, I. Kato, John G. Learned, Itsuo Nakano, L. R. Sulak, T. Ishida, A. Obayashi, E. Sharkey, Susumu Noda, H. C. Bhang, T. Ishii, N. Tamura, M. Y. Pac, Yasunari Suzuki, C. O. Kim, N. Sasao, J. S. Jang, H. Yokoyama, W. Gajewski, Kate Scholberg, Ken-ichiro Kobayashi, A. K. Ichikawa, T. Toshito, R. J. Wilkes, Shigetaka Moriyama, A. Kibayashi, J. Y. Kim, I. T. Lim, T. Hara, Shogo Nishiyama, J. Kameda, C. McGrew, M. Ishitsuka, H. So, Shigeki Aoki, J. Yoo, J. Zalipska, Takashi Kobayashi, A. Ikeda, Y. Hayato, A. L. Stachyra, Mark R. Vagins, Masato Shiozawa, Shoji Yamamoto, Tsuyoshi Nakaya, Y. Suga, F. Nakata, Beom Jun Kim, Yoshitaka Itow, Yusuke Koshio, T. Ooyabu, Masayuki Nakahata, Takaaki Kajita, C. Mauger, and A. Okada
Subjects: Physics, Tamura, Norio, Physics::Instrumentation and Detectors, Oscillation, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, High Energy Physics::Phenomenology, FOS: Physical sciences, General Physics and Astronomy, Solar neutrino problem, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), K2K experiment, Measurements of neutrino speed, High Energy Physics::Experiment, 田村, 詔生, Neutrino, Neutrino oscillation, Charged current
Abstract: The K2K experiment observes indications of neutrino oscillation: a reduction of $\nu_\mu$ flux together with a distortion of the energy spectrum. Fifty-six beam neutrino events are observed in Super-Kamiokande (SK), 250 km from the neutrino production point, with an expectation of $80.1^{+6.2}_{-5.4}$. Twenty-nine one ring $\mu$-like events are used to reconstruct the neutrino energy spectrum, which is better matched to the expected spectrum with neutrino oscillation than without. The probability that the observed flux at SK is explained by statistical fluctuation without neutrino oscillation is less than 1%., Comment: 5 pages, 3 figures embedded, LaTeX with RevTeX style, accepted for publication in PRL on December 13, 2002
Published: 2003

8. Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data

Author: Masatoshi Koshiba, Takashi Kobayashi, M. Ishitsuka, Shoichi Yamada, Takaaki Kajita, A. Kibayashi, L. R. Sulak, Shantanu Desai, Y. Ichikawa, K. Kobayashi, M. D. Messier, Y. Totsuka, T. Shibata, K. Kaneyuki, M. Takita, J. Shirai, S. Tasaka, W. E. Keig, Atsumu Suzuki, M. Earl, D. W. Liu, John G. Learned, M. Etoh, R. Nishimura, Makoto Sakuda, G. W. Sullivan, A. L. Stachyra, K. Miyano, C. W. Walter, Y. Nagashima, S. Matsuno, E. Sharkey, S. Dazeley, Hyosun Kim, D. Takemori, R. Svoboda, G. Guillian, R. W. Ellsworth, C. McGrew, A. M. Gago, K. Martens, S. Moriyama, C. Saji, J. Kameda, J. L. Stone, David William Casper, S. Nakayama, Yoshihiro Suzuki, T. Ishii, Kunio Inoue, Yoshitaka Itow, M. L. Chen, D. Turč, Y. Obayashi, J. A. Goodman, C. Mitsuda, K. S. Ganezer, T. Inagaki, Y. Kajiyama, S. Hatakeyama, R. J. Wilkes, M. Goldhaber, Y. Gando, M. Koike, Toshio Namba, Henry W. Sobel, K. Nitta, M. Ackermann, Y. Fukuda, E. Kearns, B. Viren, Koji Nakamura, S. Mine, Kyoshi Nishijima, Masayuki Nakahata, K. Nishikawa, M. Miura, Y. Takeuchi, Todd Haines, M. B. Smy, S. C. Boyd, T. Ishizuka, S. Fukuda, A. K. Ichikawa, Minoru Yoshida, C. Yanagisawa, H. Okazawa, K. Ishihara, A. Suzuki, M. Kohama, T. Iwashita, J. Hill, A. Okada, N. Sakurai, H. G. Berns, Alec Habig, Y. Watanabe, Mikio Morii, E. Blaufuss, Tsuyoshi Nakaya, C. K. Jung, C. Mauger, T. Toshito, J. Yoo, D. Kielczewska, Magdalena Malek, T. Maruyama, Masato Shiozawa, I. Kato, T. Barszczak, H. Takeuchi, Y. Hatakeyama, S. B. Kim, W. R. Kropp, Y. Oyama, Y. Hayato, Yusuke Koshio, Takehisa Hasegawa, Hirokazu Ishino, M. R. Vagins, W. Gajewski, and Kate Scholberg
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Standard solar model, Solar neutrino, High Energy Physics::Phenomenology, Solar neutrino problem, High Energy Physics - Experiment, Nuclear physics, Neutrino detector, High Energy Physics::Experiment, Neutrino, GALLEX, Super-Kamiokande, Neutrino oscillation
Abstract: A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two allowed areas at large neutrino mixing when combined with either the solar $^8$B flux prediction of the standard solar model or the SNO interaction rate measurements. A global fit combining SK data with the solar neutrino interaction rates measured by Homestake, SNO, Gallex/GNO and SAGE prefers a single allowed area, the Large Mixing Angle solution, at the 98.9% confidence level. The mass square difference $\Delta m^2$ between the two mass eigenstates ranges from about 3 to $19\times10^{-5}$eV$^2$, while the mixing angle $\theta$ is in the range of $\tan^2\theta\approx$0.25--0.65., Comment: 10 Pages, 4 figures, submitted to Physics Letters B
Published: 2002

9. Detection of accelerator-produced neutrinos at a distance of 250 km

Author: S.H Ahn, S An, S Aoki, H.G Berns, H.C Bhang, S Boyd, D Casper, T Chikamatsu, J.H Choi, S Echigo, M Etoh, K Fujii, S Fukuda, Y Fukuda, W Gajewski, U Golebiewska, T Hara, T Hasegawa, Y Hayato, J Hill, S.J Hong, M Ieiri, T Inada, T Inagaki, T Ishida, H Ishii, T Ishii, H Ishino, M Ishitsuka, Y Itow, T Iwashita, H.I Jang, J.S Jang, E.J Jeon, E.M Jeong, C.K Jung, T Kadowaki, T Kajita, J Kameda, K Kaneyuki, I Kato, Y Kato, E Kearns, S Kenmochi, B.H Khang, A Kibayashi, D Kielczewska, B.J Kim, C.O Kim, H.I Kim, J.H Kim, J.Y Kim, S.B Kim, S Kishi, M Kitamura, K Kobayashi, T Kobayashi, Y Kobayashi, M Kohama, D.G Koo, Y Koshio, W Kropp, G Kume, E Kusano, J.G Learned, H.K Lee, J.W Lee, S.B Lee, I.T Lim, S.H Lim, H Maesaka, K Martens, T Maruyama, S Matsuno, C Mauger, C McGrew, M Minakawa, S Mine, M Miura, S Miyamoto, K Miyano, S Moriyama, S Mukai, M Nakahata, K Nakamura, M Nakamura, I Nakano, T Nakaya, S Nakayama, K Nakayoshi, K Nishijima, K Nishikawa, S Nishiyama, S Noda, H Noumi, Y Obayashi, J.K Oh, A Okada, M Onchi, T Otaki, Y Oyama, M.Y Pac, H Park, S.H Park, S.K Park, A Sakai, M Sakuda, N Sakurai, N Sasao, K Sato, K Scholberg, E Seo, E Sharkey, K Shiino, A Shima, M Shiozawa, H So, H Sobel, A Stachyra, J.L Stone, L.R Sulak, A Suzuki, Y Suzuki, M Takasaki, M Takatsuki, K Takenaka, H Takeuchi, Y Takeuchi, N Tamura, K.H Tanaka, Y Tanaka, K Tashiro, K Tauchi, T Toshito, Y Totsuka, V Tumakov, T Umeda, M Vagins, C.W Walter, R.J Wilkes, S Yamada, T Yamaguchi, Y Yamanoi, C Yanagisawa, H Yokoyama, J Yoo, M Yoshida, and S.Y You
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, High Energy Physics::Phenomenology, Detector, Extrapolation, FOS: Physical sciences, Coincidence, High Energy Physics - Experiment, High Energy Physics - Phenomenology, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), Pion, K2K experiment, High Energy Physics::Experiment, Nuclear Experiment (nucl-ex), Neutrino, Neutrino oscillation, Nuclear Experiment, Beam (structure)
Abstract: The KEK to Kamioka long-baseline neutrino experiment (K2K) has begun its investigation of neutrino oscillations suggested by atmospheric neutrino observations. Twenty-eight neutrino events have been detected in coincidence with the expected arrival time of the beam in the 22.5 kt fiducial volume of Super--Kamiokande, the far detector at 250 km distance. The expectation is 37.8+3.5-3.8, derived using measurements of neutrino interactions in a near detector and extrapolation using a beam simulation validated by a measurement of pion kinematics after production and focusing. The background is of order 10^-3 events., Comment: 6 pages, 3 embedded figures, LaTeX with RevTeX style, submitted to PRL. This version is As Submitted
Published: 2001

10. SolarB8and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data

Author: Y. Watanabe, J. Hill, M. Morii, T. Toshito, Minoru Yoshida, Y. Nagashima, J. A. Goodman, Y. Oyama, S. Tasaka, W. E. Keig, Y. Hayato, C. W. Walter, Atsumu Suzuki, Yusuke Koshio, B. Lee, K. Kaneyuki, Magdalena Malek, Soo-Bong Kim, M. B. Smy, Y. Fukuda, E. Kearns, Yoshitaka Itow, K. Nishikawa, M. Takita, L. R. Price, J. Shirai, M. Koike, H. Takeuchi, A. Suzuki, B. Viren, C. Saji, E. Sharkey, S. Dazeley, G. Guillian, S. Moriyama, M. Kohama, K. Ishihara, C. Mitsuda, C. McGrew, S. Matsuno, C. K. Jung, Tsuyoshi Nakaya, Heekyong Kim, H. Okazawa, D. Kielczewska, Yoshihiro Suzuki, C. Mauger, J. Yoo, Y. Totsuka, T. Ishii, M. Goldhaber, Kunio Inoue, Masato Shiozawa, Y. Takeuchi, R. J. Wilkes, T. Barszczak, U. Golebiewska, Alec Habig, M. Earl, D. W. Liu, R. Svoboda, J. Kameda, G. W. Sullivan, Takehisa Hasegawa, Masayuki Nakahata, Y. Gando, M. Ishitsuka, Hirokazu Ishino, Y. Hatakeyama, S. Mine, Shantanu Desai, Y. Ichikawa, A. L. Stachyra, K. Miyano, Takashi Kobayashi, W. R. Kropp, Tomoyuki Maruyama, R. W. Ellsworth, J. L. Stone, Henry W. Sobel, K. Nitta, H. Fujiyasu, E. Blaufuss, Kyoshi Nishijima, T. Inagaki, M. R. Vagins, Koji Nakamura, Masatoshi Koshiba, M. Miura, W. Gajewski, Kate Scholberg, A. Kibayashi, L. R. Sulak, T. Shibata, M. D. Messier, Makoto Sakuda, S. C. Boyd, T. Ishizuka, Y. Obayashi, K. Martens, John G. Learned, K. Kobayashi, Y. Kajiyama, Shoichi Yamada, Takaaki Kajita, M. Etoh, K. S. Ganezer, Todd Haines, D. Turcan, C. Yanagisawa, A. Okada, N. Sakurai, S. Nakayama, David William Casper, A. Sakai, and D. Takemori
Subjects: Physics, Sudbury Neutrino Observatory, Particle physics, Recoil, Solar neutrino, General Physics and Astronomy, Flux, Electron, Neutrino, Super-Kamiokande, Energy (signal processing)
Abstract: Solar neutrino measurements from 1258days of data from the Super-Kamiokande detector are presented. The measurements are based on recoil electrons in the energy range 5.0{endash}20.0MeV. The measured solar neutrino flux is 2.32{+-}0.03(stat){sup +0.08}{sub {minus}0.07}(syst){times}10{sup 6} cm{sup {minus}2}s{sup {minus}1} , which is 45.1{+-}0.5(stat ){sup +1.6}{sub {minus}1.4}(syst) % of that predicted by the BP2000 SSM. The day vs night flux asymmetry ({Phi}{sub n}{minus}{Phi}{sub d})/ {Phi}{sub average} is 0.033{+-}0.022(stat){sup +0.013}{sub {minus}0.012}(syst) . The recoil electron energy spectrum is consistent with no spectral distortion. For the hep neutrino flux, we set a 90% C.L.upper limit of 40{times}10{sup 3} cm{sup {minus}2}s{sup {minus}1} , which is 4.3times the BP2000 SSM prediction.
Published: 2001

11. Constraints on Neutrino Oscillations Using 1258 Days of Super-Kamiokande Solar Neutrino Data

Author: Hirokazu Ishino, H. Takeuchi, K. Kaneyuki, Makoto Sakuda, M. Ishitsuka, K. Martens, K. Kobayashi, S. Matsuno, T. Shibata, Minoru Yoshida, David William Casper, Shantanu Desai, Y. Ichikawa, A. Sakai, Y. Takeuchi, J. L. Stone, E. Blaufuss, S. Nakayama, John G. Learned, Henry W. Sobel, K. Nitta, D. Turcan, R. W. Ellsworth, Kyoshi Nishijima, A. L. Stachyra, K. Miyano, Y. Watanabe, D. Takemori, M. Etoh, G. Guillian, S. Moriyama, T. Ishii, Kunio Inoue, Tomoyuki Maruyama, C. W. Walter, T. Inagaki, Y. Hatakeyama, M. Goldhaber, B. Viren, J. Hill, M. Morii, S. Tasaka, W. E. Keig, Shoichi Yamada, Takaaki Kajita, Koji Nakamura, T. Toshito, Soo-Bong Kim, M. Takita, L. R. Price, J. Shirai, C. Yanagisawa, D. W. Liu, Yoshitaka Itow, C. K. Jung, Y. Fukuda, E. Kearns, Todd Haines, Atsumu Suzuki, D. Kielczewska, M. Miura, Takehisa Hasegawa, E. Sharkey, G. W. Sullivan, S. Fukuda, M. Koike, S. Dazeley, Masayuki Nakahata, K. Nishikawa, C. McGrew, Magdalena Malek, M. R. Vagins, N. Sakurai, A. Okada, H. Okazawa, K. Ishihara, W. Gajewski, Kate Scholberg, Yoshihiro Suzuki, H. Fujiyasu, Y. Nagashima, Y. Kajiyama, J. Kameda, K. S. Ganezer, K. B. Lee, Alec Habig, Y. Totsuka, C. Saji, J. A. Goodman, M. Earl, Takashi Kobayashi, S. C. Boyd, T. Ishizuka, Masatoshi Koshiba, Y. Obayashi, A. Kibayashi, L. R. Sulak, C. Mitsuda, R. Svoboda, R. J. Wilkes, U. Golebiewska, K. K. Young, S. Mine, M. B. Smy, M. D. Messier, M. Kohama, Heekyong Kim, C. Mauger, J. Yoo, Masato Shiozawa, T. Barszczak, Y. Gando, W. R. Kropp, A. Suzuki, Tsuyoshi Nakaya, Y. Oyama, Y. Hayato, and Yusuke Koshio
Subjects: Physics, Particle physics, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, High Energy Physics::Phenomenology, General Physics and Astronomy, Flux, Solar neutrino problem, High Energy Physics - Experiment, Nuclear physics, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, Super-Kamiokande, Neutrino oscillation, Zenith
Abstract: We report the result of a search for neutrino oscillations using precise measurements of the recoil electron energy spectrum and zenith angle variations of the solar neutrino flux from 1258 days of neutrino-electron scattering data in Super-Kamiokande. The absence of significant zenith angle variation and spectrum distortion places strong constraints on neutrino mixing and mass difference in a flux-independent way. Using the Super-Kamiokande flux measurement in addition, two allowed regions at large mixing are found., Comment: 6 pages, 4 figures, submitted to PRL
Published: 2001

12. Leading order analysis of neutrino induced dimuon events in the CHORUS experiment

Author: M. Serin-Zeyrek, S. Kalinin, U. Dore, B. Saitta, Shigeki Aoki, Motoaki Miyanishi, K. Hoshino, I. Tezuka, S. Sorrentino, S. Kama, D. Frekers, I. Makhlioueva, Masahiro Komatsu, Toshiyuki Nakano, Ghislain Grégoire, D. Kolev, J. S. Song, E. Barbuto, H. Meinhard, T. Okusawa, T. Toshito, D. Rondeshagen, S. Ogawa, P. F. Loverre, R. Santorelli, P. Migliozzi, G. Rosa, Gaston Wilquet, P. Tolun, G. Romano, P. Zucchelli, Ilya Tsukerman, L. Scotto Lavina, A. Rozanov, N. Bruski, A. Satta, A. G. Cocco, C. S. Yoon, J. Panman, T. Hara, A. Kayis-Topaksu, Pierre Vilain, Osamu Sato, M. Litmaath, T. Kawamura, E. Di Capua, A. Artamonov, Rudolf Oldeman, N. Nonaka, Denis Favart, L. Ludovici, V. Shamanov, C. Sirignano, Koichi Kodama, Michiyuki Chikawa, K. Winter, P. Strolin, A. Bülte, V. Tioukov, Cristiano Bozza, J. W. E. Uiterwijk, R. Tsenov, Nicola D'Ambrosio, A. Marotta, J. Goldberg, Ivana Hristova, M. Messina, G. De Rosa, K. Narita, R. van Dantzig, S. Buontempo, G. De Lellis, Y. Sato, G. Fiorillo, F. R. Spada, U. Kose, R. Santacesaria, V. Khovansky, F. Di Capua, J. Kawada, Murat Guler, G. Grella, Gulsen Onengut, K. Niwa, B. Van de Vyver, N. Ushida, Th. Delbar, H. Shibuya, M. T. Muciaccia, T. Wolff, Mitsuhiro Nakamura, P. Gorbunov, M. de Jong, K. Niu, M. G. Catanesi, UCL - SC/PHYS - Département de physique, Çukurova Üniversitesi, A., Kayis Topaksu, G., Onengut, R. v., Dantzig, M. d., Jong, R. G., C., A., Guler, S., Kama, U., Kose, M., Serin Zeyrek, P., Tolun, M. G., Catanesi, M. T., Muciaccia, A., Bulte, K., Winter, B. V., De, P., Vilain, G., Wilquet, B., Saitta, E. D., Capua, S., Ogawa, H., Shibuya, I. R., Hristova, T., Kawamura, D., Kolev, M., Litmaath, H., Meinhard, J., Panman, A., Rozanov, R., Tsenov, J. W., E., P., Zucchelli, J., Goldberg, M., Chikawa, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, T., Delbar, D., Favart, G., Gregoire, S., Kalinin, I., Makhlioueva, A., Artamonov, P., Gorbunov, V., Khovansky, V., Shamanov, I., Tsukerman, N., Bruski, D., Freker, D., Rondeshagen, T., Wolff, K., Hoshino, J., Kawada, M., Komatsu, A., Miyanishi, M., Nakamura, T., Nakano, K., Narita, K., Niu, K., Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, DI CAPUA, Francesco, Fiorillo, Giuliana, A., Marotta, M., Messina, P., Migliozzi, R., Santorelli, L. S., Lavina, Strolin, PAOLO EMILIO, V., Tioukov, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, G., Rosa, R., Santacesaria, A., Satta, F. R., Spada, E., Barbuto, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, and I., Tezuka
Subjects: Quark, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, FOS: Physical sciences, Charm quark, High Energy Physics - Experiment, PHYSICS, Nuclear physics, charm production, High Energy Physics - Experiment (hep-ex), neutrino, CHARGED-CURRENT INTERACTIONS, LEPTOPRODUCTION, OPPOSITE-SIGN DIMUONS, Neutrino, SCATTERING, QCD ANALYSIS, NUCLEON, Neutrino oscillation, Nuclear Experiment, OSCILLATION, Physics, Muon, dimuon, High Energy Physics::Phenomenology, Dimuon, Baryon, Charm production, PARTON DISTRIBUTIONS, Physique des particules élémentaires, High Energy Physics::Experiment, HEAVY QUARKS, Nucleon, Particle Physics - Experiment, Lepton
Abstract: We present a leading order QCD analysis of a sample of neutrino induced charged-current events with two muons in the final state originating in the lead-scintillating fibre calorimeter of the CHORUS detector. The results are based on a sample of 8910 neutrino and 430 antineutrino induced opposite-sign dimuon events collected during the exposure of the detector to the CERN Wide Band Neutrino Beam between 1995 and 1998. The analysis yields a value of the charm quark mass of mc = (1.26 ± 0.16 ± 0.09) GeV / c2 and a value of the ratio of the strange to non-strange sea in the nucleon of κ = 0.33 ± 0.05 ± 0.05, improving the results obtained in similar analyses by previous experiments. © 2008 Elsevier B.V. All rights reserved., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2008

13. Tau Neutrinos Favored over Sterile Neutrinos in Atmospheric Muon Neutrino Oscillations

Author: C. Yanagisawa, Y. Takeuchi, S. Nakayama, H. Fujiyasu, Minoru Yoshida, S. Inaba, N. Sakurai, Y. Totsuka, K. S. Ganezer, M. Etoh, H. Takeuchi, C. Mitsuda, K. Kaneyuki, Y. Gando, C. W. Walter, R. J. Wilkes, U. Golebiewska, B. K. Kim, R. W. Ellsworth, Hirokazu Ishino, H. Okazawa, K. Kobayashi, K. K. Young, S. Fukuda, M. L. Chen, R. Svoboda, S. Mine, Todd Haines, M. Earl, T. Maruyama, T. Inagaki, J. Hill, Atsumu Suzuki, Koji Nakamura, Soo-Bong Kim, M. Takita, L. R. Price, J. Shirai, E. Blaufuss, A. Suzuki, M. Miura, Y. Fukuda, E. Kearns, Y. Obayashi, John G. Learned, Masatoshi Koshiba, A. Kibayashi, E. Sharkey, A. Okada, L. R. Sulak, J. L. Stone, G. W. Sullivan, Shoichi Yamada, Takaaki Kajita, C. Mauger, Masato Shiozawa, C. Saji, Henry W. Sobel, K. Nitta, T. Barszczak, J. Kameda, Y. Nagashima, Kyoshi Nishijima, K. Nishikawa, S. C. Boyd, T. Ishizuka, C. McGrew, Y. Watanabe, R. Sanford, M. D. Messier, J. A. Goodman, Yoshihiro Suzuki, M. Morii, K. Ishihara, T. Toshito, M. B. Smy, S. Matsuno, Osamu Sasaki, M. Kohama, Magdalena Malek, Ko Okumura, Takehisa Hasegawa, T. Ishii, Kunio Inoue, Alec Habig, Takashi Kobayashi, M. R. Vagins, W. Gajewski, Kate Scholberg, Masayuki Nakahata, G. Guillian, S. Moriyama, M. Takahashi, M. Goldhaber, M. Ishitsuka, Y. Ichikawa, A. L. Stachyra, K. Miyano, Y. Oyama, Y. Hayato, B. Viren, Yusuke Koshio, C. K. Jung, M. Takahata, D. Kielczewska, W. R. Kropp, Makoto Sakuda, K. Martens, David William Casper, A. Sakai, Yoshitaka Itow, M. Kirisawa, M. Koike, D. Takemori, S. Tasaka, W. E. Keig, and Y. Hatakeyama
Subjects: Physics, Sterile neutrino, Particle physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, High Energy Physics::Phenomenology, General Physics and Astronomy, Solar neutrino problem, High Energy Physics - Experiment, Cosmic neutrino background, Neutrino detector, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, Neutrino astronomy
Abstract: The previously published atmospheric neutrino data did not distinguish whether muon neutrinos were oscillating into tau neutrinos or sterile neutrinos, as both hypotheses fit the data. Using data recorded in 1100 live-days of the Super-Kamiokande detector, we use three complementary data samples to study the difference in zenith angle distribution due to neutral currents and matter effects. We find no evidence favoring sterile neutrinos, and reject the hypothesis at the 99% confidence level. On the other hand, we find that oscillation between muon and tau neutrinos suffices to explain all the results in hand., Comment: 9 pages with 2 figures, submitted to PRL
Published: 2000

14. Charged-particle multiplicities in charged-current neutrino and anti-neutrino-nucleus interactions

Author: S. Kalinin, E. Di Capua, U. Dore, E. Barbuto, Toshiyuki Nakano, A. Rozanov, K. Winter, G. De Lellis, A. Kayis-Topaksu, Ghislain Grégoire, Cristiano Bozza, Shigeki Aoki, K. Niu, I. Tezuka, M. T. Muciaccia, A. Satta, S. Sorrentino, C. S. Yoon, N. Nonaka, D. Frekers, V. Shamanov, C. Sirignano, G. De Rosa, G. Romano, Nicola D'Ambrosio, J. Panman, P. Strolin, S. Ogawa, Osamu Sato, Y. Sato, G. Fiorillo, Pierre Vilain, H. Meinhard, Mitsuhiro Nakamura, J. Kawada, Masahiro Komatsu, T. Okusawa, T. Toshito, Gulsen Onengut, F. R. Spada, U. Kose, Rudolf Oldeman, A. G. Cocco, Denis Favart, T. Hara, D. Kolev, Michiyuki Chikawa, H. Shibuya, N. Ushida, G. Grella, L. Ludovici, L. Scotto Lavina, K. Narita, Ivana Hristova, P. Gorbunov, Koichi Kodama, R. Santacesaria, G. Rosa, M. de Jong, P. Migliozzi, Gaston Wilquet, P. Tolun, J. W. E. Uiterwijk, Murat Guler, N. Bruski, P. Zucchelli, T. Kawamura, Ilya Tsukerman, K. Niwa, Th. Delbar, B. Van de Vyver, A. Artamonov, R. Tsenov, J. Goldberg, B. Saitta, R. van Dantzig, S. Buontempo, F. Di Capua, I. Makhlioueva, V. Khovansky, P. F. Loverre, J. S. Song, M. G. Catanesi, Motoaki Miyanishi, K. Hoshino, V. Tioukov, A. Marotta, Çukurova Üniversitesi, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), CHORUS, A., Kayis Topaksu, G., Onengut, R. v., Dantzig, M. d., Jong, R. G., C., M., Guler, U., Kose, P., Tolun, M. G., Catanesi, M. T., Muciaccia, K., Winter, B. v., De, P., Vilain, G., Wilquet, B., Saitta, E. D., Capua, S., Ogawa, H., Shibuya, I. R., Hristovalo, T., Kawamura, D., Kolev, H., Meinhard, J., Panman, A., Rozanov, R., Tsenov, J. W., E., P., Zucchelli, J., Goldberg, M., Chikawa, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, T., Delbar, D., Favart, G., Gregoire, S., Kalinin, I., Makhlioueva, A., Artamonov, P., Gorbunov, V., Khovansky, V., Shamanov, I., Tsukerman, N., Bruski, D., Freker, K., Hoshino, J., Kawada, M., Komatsu, M., Miyanishi, M., Nakamura, T., Nakano, K., Narita, K., Niu, K., Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosi, DE LELLIS, Giovanni, DE ROSA, Gianfranca, F. D., Capua, Fiorillo, Giuliana, A., Marotta, P., Migliozzi, L. S., 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, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, and I., Tezuka
Subjects: HIGH-ENERGY, COLLISIONS, Particle physics, Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, Monte Carlo method, FOS: Physical sciences, PROTON INTERACTIONS, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), neutrino interactions, multiplicity, SEARCH, Ionization, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], DISTRIBUTIONS, Nuclear emulsion, 010306 general physics, Engineering (miscellaneous), Scaling, Charged current, Physics, CHORUS EXPERIMENT, 010308 nuclear & particles physics, NU-P, HADRONS, Multiplicity (mathematics), Charged particle, 3. Good health, High Energy Physics::Experiment, Neutrino, Particle Physics - Experiment, EMULSION, SYSTEM
Abstract: The CHORUS experiment, designed to search for $\nu_{\mu}\to\nu_{\tau}$ oscillations, consists of a nuclear emulsion target and electronic detectors. In this paper, results on the production of charged particles in a small sample of charged-current neutrino-- and anti-neutrino--nucleus interactions at high energy are presented. For each event, the emission angle and the ionization features of the charged particles produced in the interaction are recorded, while the standard kinematic variables are reconstructed using the electronic detectors. The average multiplicities for charged tracks, the pseudo-rapidity distributions, the dispersion in the multiplicity of charged particles and the KNO scaling are studied in different kinematical regions. A study of quasi-elastic topologies performed for the first time in nuclear emulsions is also reported. The results are presented in a form suitable for use in the validation of Monte Carlo generators of neutrino--nucleus interactions., Comment: 17 pages, 5 figures
Published: 2007

15. Associated charm production in neutrino-nucleus interactions

Author: A. G. Cocco, N. Nonaka, H. Meinhard, Denis Favart, V. Shamanov, C. Sirignano, P. Strolin, L. Ludovici, A. Kayis-Topaksu, M. T. Muciaccia, B. Van de Vyver, Motoaki Miyanishi, K. Hoshino, S. Sorrentino, Y. Sato, S. Ogawa, J. Panman, J. Kawada, Ghislain Grégoire, S. Buontempo, P. Zucchelli, Ilya Tsukerman, F. Di Capua, T. Hara, P. Gorbunov, D. Kolev, Osamu Sato, A. Rozanov, G. Romano, M. de Jong, Gulsen Onengut, N. Ushida, Mitsuhiro Nakamura, E. Di Capua, M. G. Catanesi, A. Artamonov, K. Niu, Koichi Kodama, Emiliano Barbuto, V. Tioukov, Murat Guler, G. Rosa, R. Tsenov, Gaston Wilquet, J. Goldberg, A. Marotta, P. Tolun, Nicola D'Ambrosio, K. Narita, R. van Dantzig, P. Migliozzi, A. Satta, C. S. Yoon, Cristiano Bozza, Michiyuki Chikawa, J. W. E. Uiterwijk, J. S. Song, F. R. Spada, B. Saitta, U. Kose, I. Makhlioueva, G. Fiorillo, Ivana Hristova, R. Santacesaria, G. De Rosa, S. Kalinin, U. Dore, I. Tezuka, N. Bruski, D. Frekers, T. Kawamura, K. Winter, H. Shibuya, G. Grella, Toshiyuki Nakano, G. De Lellis, K. Niwa, Th. Delbar, Masahiro Komatsu, T. Okusawa, T. Toshito, L. Scotto Lavina, Rudolf Oldeman, Shigeki Aoki, P. F. Loverre, V. Khovansky, Pierre Vilain, Çukurova Üniversitesi, A., Kayis Topaksu, G., Onengut, R. v., Dantzig, M. d., Jong, R. G., C., M., Guler, U., Kose, P., Tolun, M. G., Catanesi, M. T., Muciaccia, K., Winter, B. v., De, P., Vilain, G., Wilquet, B., Saitta, E. D., Capua, S., Ogawa, H., Shibuya, I. R., Hristova, T., Kawamura, D., Kolev, H., Meinhard, J., Panman, A., Rozanov, R., Tsenov, J. W., E., P., Zucchelli, J., Goldberg, M., Chikawa, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, T., Delbar, D., Favart, G., Gregoire, S., Kalinin, I., Makhlioueva, A., Artamonov, P., Gorbunov, V., Khovansky, V., Shamanov, I., Tsukerman, N., Bruski, D., Freker, K., Hoshino, J., Kawada, M., Komatsu, M., Miyanishi, M., Nakamura, T., Nakano, K., Narita, K., Niu, K., Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, F. D., Capua, Fiorillo, Giuliana, A., Marotta, P., Migliozzi, L. S., 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, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, I., Tezuka, UCL - SC/PHYS - Département de physique, Kayis Topaksu, A., Önengüt, G., van Dantzig, R., de Jong, M., Oldeman, R. G. C., Güler, M., Köse, U., Tolun, P., Catanesi, M. G., Muciaccia, M. T., Winter, K., Van de Vyver, B., Vilain, P., Wilquet, G., Saitta, B., Di Capua, E., Ogawa, S., Shibuya, H., Hristova, I. R., Kawamura, T., Kolev, D., Meinhard, H., Panman, J., Rozanov, A., Tsenov, R., Uiterwijk, J. W. E., Zucchelli, P., Goldberg, J., Chikawa, M., Song, J. S., Yoon, C. S., Kodama, K., Ushida, N., Aoki, S., Hara, T., Delbar, T., Favart, D., Grégoire, G., Kalinin, S., Makhlioueva, I., Artamonov, A., Gorbunov, P., Khovansky, V., Shamanov, V., Tsukerman, I., Bruski, N., Frekers, D., Hoshino, K., Kawada, J., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Narita, K., Niu, K., Niwa, K., Nonaka, N., Sato, O., Toshito, T., Buontempo, S., Cocco, A. G., D’Ambrosio, N., De Lellis, G., De Rosa, G., DI CAPUA, Francesco, Marotta, A., Migliozzi, P., Scotto Lavina, L., Strolin, P., Tioukov, V., Okusawa, T., Dore, U., Loverre, P. F., Ludovici, L., Rosa, G., Santacesaria, R., Satta, A., Spada, F. R., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sirignano, C., Sorrentino, S., Sato, Y., and Tezuka, I.
Subjects: Quark, Particle physics, Physics and Astronomy (miscellaneous), FOS: Physical sciences, High Energy Physics - Experiment, Nuclear physics, EVENTS, High Energy Physics - Experiment (hep-ex), SEARCH, SCATTERING, PARTICLES, Nuclear emulsion, TRIMUON PRODUCTION, Charm (quantum number), TEVATRON, Engineering (miscellaneous), OSCILLATION, Physics, Muon, Neutral current, ELECTROWEAK PARAMETERS, CHORUS, Pair production, Neutrino, Particle Physics - Experiment, Lepton
Abstract: In this paper a search for associated charm production both in neutral and charged current $\nu$-nucleus interactions is presented. The improvement of automatic scanning systems in the {CHORUS} experiment allows an efficient search to be performed in emulsion for short-lived particles. Hence a search for rare processes, like the associated charm production, becomes possible through the observation of the double charm-decay topology with a very low background. About 130,000 $\nu$ interactions located in the emulsion target have been analysed. Three events with two charm decays have been observed in the neutral-current sample with an estimated background of 0.18$\pm$0.05. The relative rate of the associated charm cross-section in deep inelastic $\nu$ interactions, $\sigma(c\bar{c}\nu)/\sigma_\mathrm{NC}^\mathrm{DIS}= (3.62^{+2.95}_{-2.42}({stat})\pm 0.54({syst}))\times 10^{-3}$ has been measured. One event with two charm decays has been observed in charged-current $\nu_\mu$ interactions with an estimated background of 0.18$\pm$0.06 and the upper limit on associated charm production in charged-current interactions at 90% C.L. has been found to be $\sigma (c\bar{c} \mu^-)/\sigma_\mathrm{CC} < 9.69 \times 10^{-4}$., Comment: 10 pages, 4 figures
Published: 2007

16. Measurement of nucleon structure functions in neutrino scattering

Author: M. Messina, Koichi Kodama, J. W. E. Uiterwijk, G. Fiorillo, E. Barbuto, Motoaki Miyanishi, D. Kolev, F. Di Capua, S. Kalinin, R. Santacesaria, Cristiano Bozza, U. Dore, E. Di Capua, H. Shibuya, K. Niwa, Yoshihiro Sato, M. T. Muciaccia, Th. Delbar, Salvatore Buontempo, T. Wolff, J. Goldberg, Osamu Sato, L. Ludovici, K. Winter, Alexandre Rozanov, G. Rosa, D. Rondeshagen, P. Migliozzi, B. Van de Vyver, D. Frekers, Toshiyuki Nakano, G. De Lellis, C. S. Yoon, Masahiro Komatsu, T. Hara, M. Nakamura, P. Gorbunov, G. Grella, Rudolf Oldeman, P. F. Loverre, A. G. Cocco, Denis Favart, Piero Zucchelli, T. Toshito, Nicola D'Ambrosio, N. Nonaka, M. de Jong, Murat Guler, V. Shamanov, C. Sirignano, V. Khovansky, A. Artamonov, A. Bülte, I. Makhlioueva, J. S. Song, R. Tsenov, I. Tezuka, R. van Dantzig, A. Satta, Pierre Vilain, N. Ushida, L. Scotto Lavina, H. Meinhard, Biagio Saitta, V. Tioukov, Gaston Wilquet, R. Santorelli, F. R. Spada, U. Kose, A. Marotta, P. Tolun, M. Serin-Zeyrek, Shigeki Aoki, K. Narita, S. Sorrentino, S. Kama, S. Ogawa, J. Kawada, Gulsen Onengut, K. Niu, T. Okusawa, P. Strolin, G. De Rosa, Michiyuki Chikawa, Ivana Hristova, A. Kayis-Topaksu, Ghislain Grégoire, K. Hoshino, N. Bruski, G. Romano, M. Litmaath, T. Kawamura, M. G. Catanesi, Ilya Tsukerman, J. Panman, Önengüt, G., van Dantzig, R., de Jong, M., Oldeman, R. G. C., Güler, M., Kama, S., Köse, U., Serin Zeyrek, M., Tolun, P., Catanesi, M. G., Muciaccia, M. T., Bülte, A., Winter, K., Van de Vyver, B., Vilain, P., Wilquet, G., Saitta, B., Di Capua, E., Ogawa, S., Shibuya, H., Hristova, I. R., Kayis Topaksu, A., Kawamura, T., Kolev, D., Litmaath, M., Meinhard, H., Panman, J., Rozanov, A., Tsenov, R., Uiterwijk, J. W. E., Zucchelli, P., Goldberg, J., Chikawa, M., Song, J. S., Yoon, C. S., Kodama, K., Ushida, N., Aoki, S., Hara, T., Delbar, T., Favart, D., Grégoire, G., Kalinin, S., Makhlioueva, I., Artamonov, A., Gorbunov, P., Khovansky, V., Shamanov, V., Tsukerman, I., Bruski, N., Frekers, D., Rondeshagen, D., Wolff, T., Hoshino, K., Kawada, J., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Narita, K., Niu, K., Niwa, K., Nonaka, N., Sato, O., Toshito, T., Buontempo, S., Cocco, A. G., D'Ambrosio, N., De Lellis, G., De Rosa, G., DI CAPUA, Francesco, Fiorillo, Giuliana, Marotta, A., Messina, M., Migliozzi, P., Santorelli, R., Scotto Lavina, L., Strolin, P., Tioukov, V., Okusawa, T., Dore, U., Loverre, P. F., Ludovici, L., Rosa, G., Santacesaria, R., Satta, A., Spada, F. R., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sirignano, C., Sorrentino, S., Sato, Y., Tezuka, I., UCL - SC/PHYS - Département de physique, Çukurova Üniversitesi, G., Onengut, R. v., Dantzig, M. d., Jong, R. G., C., M., Guler, S., Kama, U., Kose, M., Serin Zeyrek, P., Tolun, M. G., Catanesi, M. T., Muciaccia, A., Bulte, K., Winter, B. V., De, P., Vilain, G., Wilquet, B., Saitta, E. D., Capua, S., Ogawa, H., Shibuya, I. R., Hristova, A., Kayis Topaksu, T., Kawamura, D., Kolev, M., Litmaath, H., Meinhard, J., Panman, A., Rozanov, R., Tsenov, J. W., E., P., Zuechelli, J., Goldberg, M., Chikawa, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, T., Delbar, D., Favart, G., Gregoire, S., Kalinin, I., Makhlioueva, A., Artamonov, P., Gorbunov, V., Khovansky, V., Shamanov, I., Tsukerman, N., Bruski, D., Freker, D., Rondeshagen, T., Wolff, K., Hoshino, J., Kawada, M., Komatsu, M., Miyanishi, M., Nakamura, T., Nakano, K., Narita, K., Niu, K., Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, F. D., Capua, A., Marotta, M., Messina, P., Mighozzi, R., Santorelli, L. S., Lavina, Strolin, PAOLO EMILIO, V., Tioukov, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, G., Rosa, R., Santacesaria, A., Satta, F. R., Spada, E., Barbuto, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, and I., Tezuka
Subjects: Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Nuclear Theory, CROSS-SECTIONS, Nuclear physics, Pion, Alte energie, fisica del neutrino, DEPENDENCE, SEARCH, Nuclear Experiment, Charged current, OSCILLATION, Physics, CHORUS EXPERIMENT, Large Hadron Collider, Muon, Oscillation, High Energy Physics::Phenomenology, High Energy Physics::Experiment, Neutrino, Nucleon, Particle Physics - Experiment, SYSTEM, Beam (structure)
Abstract: After completion of the data taking for the ?µ›?? oscillation search, the CHORUS lead-scintillator calorimeter was used in the 1998 run as an active target. High-statistics samples of charged-current interactions were collected in the CERN SPS west area neutrino beam. This beam contained predominantly muon (anti-)neutrinos from sign-selected pions and kaons. We measure the flux and energy spectrum of the incident neutrinos and compare them with beam simulations. The neutrino-nucleon and anti-neutrino-nucleon differential cross-sections are measured in the range 0.01
Published: 2006

17. First events from the CNGS neutrino beam detected in the OPERA experiment

Author: R Acquafredda, N Agafonova, M Ambrosio, A Anokhina, S Aoki, A Ariga, L Arrabito, D Autiero, A Badertscher, E Baussan, A Bergnoli, F Bersani Greggio, M Besnier, M Beyer, S Bondil-Blin, K Borer, J Boucrot, V Boyarkin, C Bozza, R Brugnera, S Buontempo, Y Caffari, J E Campagne, B Carlus, E Carrara, A Cazes, L Chaussard, M Chernyavsky, V Chiarella, N Chon-Sen, A Chukanov, R Ciesielski, L Consiglio, M Cozzi, F Dal Corso, N D'Ambrosio, J Damet, G De Lellis, Y Déclais, T Descombes, M De Serio, F Di Capua, D Di Ferdinando, A Di Giovanni, N Di Marco, C Di Troia, S Dmitrievski, M Dracos, D Duchesneau, B Dulach, S Dusini, J Ebert, R Enikeev, A Ereditato, L S Esposito, C Fanin, J Favier, G Felici, T Ferber, L Fournier, A Franceschi, D Frekers, T Fukuda, C Fukushima, V I Galkin, V A Galkin, R Gallet, A Garfagnini, G Gaudiot, G Giacomelli, O Giarmana, M Giorgini, L Girard, C Girerd, C Goellnitz, J Goldberg, Y Gornoushkin, G Grella, F Grianti, C Guerin, M Guler, C Gustavino, C Hagner, T Hamane, T Hara, M Hauger, M Hess, K Hoshino, M Ieva, M Incurvati, K Jakovcic, J Janicsko Csathy, B Janutta, C Jollet, F Juget, M Kazuyama, S H Kim, M Kimura, J Knuesel, K Kodama, D Kolev, M Komatsu, U Kose, A Krasnoperov, I Kreslo, Z Krumstein, I Laktineh, C de La Taille, T Le Flour, S Lieunard, A Ljubicic, A Longhin, A Malgin, K Manai, G Mandrioli, U Mantello, A Marotta, J Marteau, G Martin-Chassard, V Matveev, M Messina, L Meyer, S Micanovic, P Migliozzi, S Miyamoto, P Monacelli, I Monteiro, K Morishima, U Moser, M T Muciaccia, P Mugnier, N Naganawa, M Nakamura, T Nakano, T Napolitano, M Natsume, K Niwa, Y Nonoyama, A Nozdrin, S Ogawa, A Olchevski, D Orlandi, D Ossetski, A Paoloni, B D Park, I G Park, A Pastore, L Patrizii, L Pellegrino, H Pessard, V Pilipenko, C Pistillo, N Polukhina, M Pozzato, K Pretzl, P Publichenko, L Raux, J P Repellin, T Roganova, G Romano, G Rosa, A Rubbia, V Ryasny, O Ryazhskaya, D Ryzhikov, A Sadovski, C Sanelli, O Sato, Y Sato, V Saveliev, N Savvinov, G Sazhina, A Schembri, W Schmidt Parzefall, H Schroeder, H U Schütz, L Scotto Lavina, J Sewing, H Shibuya, S Simone, M Sioli, C Sirignano, G Sirri, J S Song, R Spaeti, M Spinetti, L Stanco, N Starkov, M Stipcevic, P Strolin, V Sugonyaev, S Takahashi, V Tereschenko, F Terranova, I Tezuka, V Tioukov, I Tikhomirov, P Tolun, T Toshito, V Tsarev, R Tsenov, U Ugolino, N Ushida, G Van Beek, V Verguilov, P Vilain, L Votano, J L Vuilleumier, T Waelchli, R Waldi, M Weber, G Wilquet, B Wonsak, R Wurth, J Wurtz, V Yakushev, C S Yoon, Y Zaitsev, I Zamboni, R Zimmermann, Acquafredda, R, Agafonova, N, Ambrosio, M, Anokhina, A, Aoki, S, Ariga, A, Arrabito, L, Autiero, D, Badertscher, A, Baussan, E, Bergnoli, A, Greggio, F, Besnier, M, Beyer, M, Bondil Blin, S, Borer, K, Boucrot, J, Boyarkin, V, Bozza, C, Brugnera, R, Buontempo, S, Caffari, Y, Campagne, J, Carlus, B, Carrara, E, Cazes, A, Chaussard, L, Chernyavsky, M, Chiarella, V, Chon Sen, N, Chukanov, A, Ciesielski, R, Consiglio, L, Cozzi, M, Corso, F, D'Ambrosio, N, Damet, J, Lellis, G, Déclais, Y, Descombes, T, Serio, M, Capua, F, Ferdinando, D, Giovanni, A, Marco, N, Troia, C, Dmitrievski, S, Dracos, M, Duchesneau, D, Dulach, B, Dusini, S, Ebert, J, Enikeev, R, Ereditato, A, Esposito, L, Fanin, C, Favier, J, Felici, G, Ferber, T, Fournier, L, Franceschi, A, Frekers, D, Fukuda, T, Fukushima, C, Galkin, V, Gallet, R, Garfagnini, A, Gaudiot, G, Giacomelli, G, Giarmana, O, Giorgini, M, Girard, L, Girerd, C, Goellnitz, C, Goldberg, J, Gornoushkin, Y, Grella, G, Grianti, F, Guerin, C, Guler, M, Gustavino, C, Hagner, C, Hamane, T, Hara, T, Hauger, M, Hess, M, Hoshino, K, Ieva, M, Incurvati, M, Jakovcic, K, Csathy, J, Janutta, B, Jollet, C, Juget, F, Kazuyama, M, Kim, S, Kimura, M, Knuesel, J, Kodama, K, Kolev, D, Komatsu, M, Kose, U, Krasnoperov, A, Kreslo, I, Krumstein, Z, Laktineh, I, Taille, C, Flour, T, Lieunard, S, Ljubicic, A, Longhin, A, Malgin, A, Manai, K, Mandrioli, G, Mantello, U, Marotta, A, Marteau, J, Martin Chassard, G, Matveev, V, Messina, M, Meyer, L, Micanovic, S, Migliozzi, P, Miyamoto, S, Monacelli, P, Monteiro, I, Morishima, K, Moser, U, Muciaccia, M, Mugnier, P, Naganawa, N, Nakamura, M, Nakano, T, Napolitano, T, Natsume, M, Niwa, K, Nonoyama, Y, Nozdrin, A, Ogawa, S, Olchevski, A, Orlandi, D, Ossetski, D, Paoloni, A, Park, B, Park, I, Pastore, A, Patrizii, L, Pellegrino, L, Pessard, H, Pilipenko, V, Pistillo, C, Polukhina, N, Pozzato, M, Pretzl, K, Publichenko, P, Raux, L, Repellin, J, Roganova, T, Romano, G, Rosa, G, Rubbia, A, Ryasny, V, Ryazhskaya, O, Ryzhikov, D, Sadovski, A, Sanelli, C, Sato, O, Sato, Y, Saveliev, V, Savvinov, N, Sazhina, G, Schembri, A, Parzefall, W, Schroeder, H, Schütz, H, Lavina, L, Sewing, J, Shibuya, H, Simone, S, Sioli, M, Sirignano, C, Sirri, G, Song, J, Spaeti, R, Spinetti, M, Stanco, L, Starkov, N, Stipcevic, M, Strolin, P, Sugonyaev, V, Takahashi, S, Tereschenko, V, Terranova, F, Tezuka, I, Tioukov, V, Tikhomirov, I, Tolun, P, Toshito, T, Tsarev, V, Tsenov, R, Ugolino, U, Ushida, N, Beek, G, Verguilov, V, Vilain, P, Votano, L, Vuilleumier, J, Waelchli, T, Waldi, R, Weber, M, Wilquet, G, Wonsak, B, Wurth, R, Wurtz, J, Yakushev, V, Yoon, C, Zaitsev, Y, Zamboni, I, Zimmermann, R, Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), OPERA, R. ACQUAFREDDA, N. AGAFONOVA, M. AMBROSIO, A. ANOKHINA, S. AOKI, A. ARIGA, L. ARRABITO, D. AUTIERO, A. BADERTSCHER, E. BAUSSAN, A. BERGNOLI, F. BERSANI GREGGIO, M. BESNIER, M. BEYER, S. BONDIL-BLIN, K. BORER, J. BOUCROT, V. BOYARKIN, C. BOZZA, R. BRUGNERA, S. BUONTEMPO, Y. CAFFARI, J. E. CAMPAGNE, B. CARLUS, E. CARRARA, A. CAZES, L. CHAUSSARD, M. CHERNYAVSKY, V. CHIARELLA, N. CHON-SEN, A. CHUKANOV, R. CIESIELSKI, L. CONSIGLIO, M. COZZI, F. DAL CORSO, N. D'AMBROSIO, J. DAMET, G. DE LELLIS, Y. DÉCLAIS, T. DESCOMBES, M. DE SERIO, F. DI CAPUA, D. DI FERDINANDO, A. DI GIOVANNI, N. DI MARCO, C. DI TROIA, S. DMITRIEVSKI, M. DRACOS, D. DUCHESNEAU, B. DULACH, S. DUSINI, J. EBERT, R. ENIKEEV, A. EREDITATO, L. S. ESPOSITO, C. FANIN, J. FAVIER, G. FELICI, T. FERBER, L. FOURNIER, A. FRANCESCHI, D. FREKERS, T. FUKUDA, C. FUKUSHIMA, V. I. GALKIN, V. A. GALKIN, R. GALLET, A. GARFAGNINI, G. GAUDIOT, G. GIACOMELLI, O. GIARMANA, M. GIORGINI, L. GIRARD, C. GIRERD, C. GOELLNITZ, J. GOLDBERG, Y. GORNOUSHKIN, G. GRELLA, F. GRIANTI, C. GUERIN, M. GULER, C. GUSTAVINO, C. HAGNER, T. HAMANE, T. HARA, M. HAUGER, M. HESS, K. HOSHINO, M. IEVA, M. INCURVATI, K. JAKOVCIC, J. JANICSKO CSATHY, B. JANUTTA, C. JOLLET, F. JUGET, M. KAZUYAMA, S. H. KIM, M. KIMURA, J. KNUESEL, K. KODAMA, D. KOLEV, M. KOMATSU, U. KOSE, A. KRASNOPEROV, I. KRESLO, Z. KRUMSTEIN, I. LAKTINEH, C. DE LA TAILLE, T. LE FLOUR, S. LIEUNARD, A. LJUBICIC, A. LONGHIN, A. MALGIN, K. MANAI, G. MANDRIOLI, U. MANTELLO, A. MAROTTA, J. MARTEAU, G. MARTIN-CHASSARD, V. MATVEEV, M. MESSINA, L. MEYER, S. MICANOVIC, P. MIGLIOZZI, S. MIYAMOTO, P. MONACELLI, I. MONTEIRO, K. MORISHIMA, U. MOSER, M. T. MUCIACCIA, P. MUGNIER, N. NAGANAWA, M. NAKAMURA, T. NAKANO, T. NAPOLITANO, M. NATSUME, K. NIWA, Y. NONOYAMA, A. NOZDRIN, S. OGAWA, A. OLCHEVSKI, D. ORLANDI, D. OSSETSKI, A. PAOLONI, B. D. PARK, I. G. PARK, A. PASTORE, L. PATRIZII, L. PELLEGRINO, H. PESSARD, V. PILIPENKO, C. PISTILLO, N. POLUKHINA, M. POZZATO, K. PRETZL, P. PUBLICHENKO, L. RAUX, J. P. REPELLIN, T. ROGANOVA, G. ROMANO, G. ROSA, A. RUBBIA, V. RYASNY, O. RYAZHSKAYA, D. RYZHIKOV, A. SADOVSKI, C. SANELLI, O. SATO, Y. SATO, V. SAVELIEV, N. SAVVINOV, G. SAZHINA, A. SCHEMBRI, W. SCHMIDT PARZEFALL, H. SCHROEDER, H. U. SCHÜTZ, L. SCOTTO LAVINA, J. SEWING, H. SHIBUYA, S. SIMONE, M. SIOLI, C. SIRIGNANO, G. SIRRI, J. S. SONG, R. SPAETI, M. SPINETTI, L. STANCO, N. STARKOV, M. STIPCEVIC, P. STROLIN, V. SUGONYAEV, S. TAKAHASHI, V. TERESCHENKO, F. TERRANOVA, I. TEZUKA, V. TIOUKOV, I. TIKHOMIROV, P. TOLUN, T. TOSHITO, V. TSAREV, R. TSENOV, U. UGOLINO, N. USHIDA, G. VAN BEEK, V. VERGUILOV, P. VILAIN, L. VOTANO, J. L. VUILLEUMIER, T. WAELCHLI, R. WALDI, M. WEBER, G. WILQUET, B. WONSAK, R. WURTH, J. WURTZ, V. YAKUSHEV, C. S. YOON, Y. ZAITSEV, I. ZAMBONI, R. ZIMMERMANN, Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), R., Acquafredda, DE LELLIS, Giovanni, and Strolin, PAOLO EMILIO
Subjects: Particle physics, LONG BASELINE EXPERIMENTS, NEUTRINO OSCILLATIONS, Physics::Instrumentation and Detectors, neutrino oscilations, OPERA experiment, muon neutrino, tau neutrino, FOS: Physical sciences, General Physics and Astronomy, Elementary particle, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, High energy physic, Nuclear physics, High Energy Physics - Experiment (hep-ex), neutrino, Alte energie, fisica del neutrino, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Neutrino events Engineering controlled terms: Data reduction, 010306 general physics, Neutrino oscillation, Nuclear Experiment, NUCLEAR EMULSIONS, Charged current, ICARUS, Physics, Large Hadron Collider, 010308 nuclear & particles physics, Emulsion, Targets Engineering main heading: Particle detectors, Particle beam, Oscillation, FIS/01 - FISICA SPERIMENTALE, Neutrino detector, Electronic detector, Measurements of neutrino speed, PARTICLE PHYSICS, High Energy Physics::Experiment, Emulsion film target, Neutrino, Integrated beam intensity, Particle Physics - Experiment, Beam (structure)
Abstract: The OPERA neutrino detector at the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in appearance mode, through the study of nu_mu to nu_tau oscillations. The apparatus consists of a lead/emulsion-film target complemented by electronic detectors. It is placed in the high-energy, long-baseline CERN to LNGS beam (CNGS) 730 km away from the neutrino source. In August 2006 a first run with CNGS neutrinos was successfully conducted. A first sample of neutrino events was collected, statistically consistent with the integrated beam intensity. After a brief description of the beam and of the various sub-detectors, we report on the achievement of this milestone, presenting the first data and some analysis results., Submitted to the New Journal of Physics
Published: 2006

18. Search for νμ→ντ oscillation using the τ decay modes into a single charged particle

Author: E. Eskut, A. Kayis, G. Onengüt, R. van Dantzig, M. de Jong, J. Konijn, O. Melzer, R.G.C. Oldeman, C.A.F.J. van der Poel, J.W.E. Uiterwijk, J.L. Visschers, M. Guler, M. Serin-Zeyrek, R. Sever, P. Tolun, M.T. Zeyrek, N. Armenise, F. Cassol, M.G. Catanesi, M.T. Muciaccia, E. Radicioni, S. Simone, L. Vivolo, A. Bülte, T. Patzak, K. Winter, P. Annis, R. El Aidi, M. Gruwé, C. Mommaert, M. Vander Donckt, B. Van de Vyver, P. Vilain, G. Wilquet, P. Righini, B. Saitta, E. Di Capua, C. Luppi, P. Zucchelli, Y. Ishii, T. Kawamura, M. Kazuno, S. Ogawa, H. Shibuya, J. Brunner, D. Cussans, J.P. Fabre, R. Ferreira, W. Flegel, M. Litmaath, D. Macina, R. Meijer Drees, H. Meinhard, P. Migliozzi, E. Niu, H. Øverȧs, J. Panman, I.M. Papadopoulos, E. Pesen, F. Riccardi, S. Ricciardi, A. Rozanov, D. Saltzberg, P. Strolin, R. Tsenov, Ch. Weinheimer, H. Wong, J. Goldberg, K. Hoepfner, M. Chikawa, E. Arik, A.A. Mailov, H.I. Jang, I.G. Park, J.S. Song, C.S. Yoon, K. Kodama, N. Ushida, S. Aoki, T. Hara, G. Brooijmans, D. Favart, G. Grégoire, J. Hérin, A. Artamonov, P. Gorbunov, V. Khovansky, V. Shamanov, D. Bonekämper, D. Frekers, D. Rondeshagen, T. Wolff, K. Hoshino, M. Kobayashi, M. Komatsu, Y. Kotaka, T. Kozaki, M. Miyanishi, M. Nakamura, K. Nakazawa, T. Nakano, K. Niu, K. Niwa, Y. Obayashi, O. Sato, T. Toshito, S. Buontempo, A. Cocco, N. D'Ambrosio, G. De Lellis, A. Ereditato, G. Fiorillo, F. Garufi, M. Messina, V. Palladino, S. Sorrentino, V. Tioukov, K. Nakamura, T. Okusawa, T. Yoshida, A. Capone, D. De Pedis, S. Di Liberto, U. Dore, P.F. Loverre, L. Ludovici, A. Maslennikov, M.A. Mazzoni, G. Piredda, R. Santacesaria, A. Satta, E. Barbuto, A. di Bartolomeo, C. Bozza, G. Grella, G. Iovane, G. Romano, G. Rosa, Y. Sato, and I. Tezuka
Subjects: Physics, Nuclear physics, Nuclear and High Energy Physics, Particle physics, Muon, Tau neutrino, Hadron, High Energy Physics::Experiment, Muon neutrino, Neutrino, Charged particle, Charged current, Lepton
Abstract: Part of the neutrino events collected in 1994-1995 by the CHORUS experiment has been analysed. A search was performed for ντ charged current interactions followed by the τ lepton decay into a single charged negative hadron, a possible indication for νμ→ντ oscillation. A sample of 6844 events without an identified muon has been located in the emulsion target. Within the selection criteria, no τ− candidate has been found. Combining this result with the one from the search for ντ interactions using the muonic decay mode (36 182 events with an identified muon), a 90% C.L. limit on the mixing angle sin22θμτ
Published: 1998

19. A search for νμ→ντ oscillation

Author: A. Meyer-Sievers, W. Flegel, F. Cassol, K. Niu, Yoshihiro Sato, G. Grégoire, M. Nakamura, C. Luppi, T. Toshito, D. Bonekämper, M. T. Muciaccia, D. De Pedis, I. Tezuka, M. A. Mazzoni, T. Wolff, K. Hoshino, Inanc Birol, T. Okusawa, Toshiyuki Nakano, A. Bülte, P. Strolin, A. S. Ayan, J. S. Song, David Saltzberg, Y. Ishii, M. Messina, U. Dore, G. De Lellis, E. Pesen, A. Maslennikov, C. S. Yoon, G. Stefanini, C. Mommaert, A. Artamonov, D. Rondeshagen, G. Iovane, O. Melzer, K. Nakamura, Vincent Lemaitre, Ramazan Sever, P. Gorbunov, J. L. Visschers, L. Ludovici, G. Fiorillo, R. Tsenov, Ch. Weinheimer, J. Panman, M. de Jong, C. H. Hahn, D. Frekers, J. Konijn, E. Radicioni, Jürgen Brunner, Rudolf Oldeman, R. Beyer, S. Sorrentino, T. Kozaki, T. Hara, Gulsen Onengut, R. van Dantzig, Antonio Capone, E. Di Capua, R. Ferreira, Pierre Vilain, Denis Favart, Michiyuki Chikawa, Y. Kotaka, F. Marchetti-Stasi, M. Vander Donckt, V. Khovansky, F. Garufi, G. Piredda, Gaston Wilquet, T. Yoshida, I.M. Papadopoulos, Franco Meddi, P. Righini, P. Tolun, N. Ushida, Cristiano Bozza, H. I. Jang, Kerstin Hoepfner, Nicola D'Ambrosio, G. Romano, Biagio Saitta, A. Di Bartolomeo, Alexandre Rozanov, S. Simone, Kimio Niwa, R. Santacesaria, M. Gruwe, R. Gurin, T. Kawamura, Alfredo G. Cocco, Kazuma Nakazawa, S. Ogawa, B. Van de Vyver, David Cussans, Piero Zucchelli, Makoto Kobayashi, M. Kazuno, M. Litmaath, Mehmet Zeyrek, R. Meijer Drees, M. Serin-Zeyrek, A. Mailov, M. G. Catanesi, J. Goldberg, Osamu Sato, L. Vivolo, Antonio Ereditato, T. Patzak, V. Shamanov, Shigeki Aoki, N. Armenise, H. Øverasolars, F. Riccardi, S. Ricciardi, G. Rosa, P. Lendermann, H. Meinhard, Koichi Kodama, V. Smirnitsky, Henry T. Wong, J. W. E. Uiterwijk, Jean-Paul Fabre, G. Brooijmans, A. Kayis, I. G. Park, Motoaki Miyanishi, P. Annis, E. Niu, P. F. Loverre, Salvatore Buontempo, Y. Obayashi, K. Winter, S. Di Liberto, G. Grella, J. Hérin, M. S. Park, E. Arik, P. Migliozzi, V. Palladino, H. Shibuya, D. Macina, C.A.F.J. van der Poel, and E. Eskut
Subjects: Physics, Nuclear and High Energy Physics, Atomic physics
Published: 1998

20. Experimental study of trimuon events in neutrino charged-current interactions

Author: T. Wolff, Nicola D'Ambrosio, David Cussans, E. Radicioni, C.A.F.J. van der Poel, Jürgen Brunner, David Saltzberg, P. Gorbunov, A. Satta, M. de Jong, Y. Sato, F. R. Spada, U. Kose, T. Hara, J. Kawada, Gulsen Onengut, N. Ushida, Mitsuhiro Nakamura, S. Sorrentino, S. Kama, K. Nakamura, E. Di Capua, G. Fiorillo, I.M. Papadopoulos, M. T. Muciaccia, A. Ereditato, O. Melzer, Michiyuki Chikawa, S. Ogawa, G. De Lellis, D. Rondeshagen, Ramazan Sever, K. Niu, Ghislain Grégoire, P. Zucchelli, Ilya Tsukerman, Mathieu Doucet, S. Kalinin, A. G. Cocco, U. Dore, P. Strolin, G. De Rosa, Pierre Vilain, E. Pesen, A. Kayis-Topaksu, Ivana Hristova, Masahiro Komatsu, V Tioukov, Toshiyuki Nakano, Osamu Sato, R. Santacesaria, P. F. Loverre, T. Okusawa, T. Toshito, A. Marotta, Rudolf Oldeman, Denis Favart, P. Migliozzi, I. Tezuka, L. Ludovici, D. Kolev, D. Frekers, E. Arik, P. Righini, B. Saitta, R. Santorelli, M. Ieva, Koichi Kodama, Mihail Chizhov, G. Romano, N. Nonaka, Jan Visschers, V. Shamanov, C. Sirignano, J. S. Song, Murat Guler, J. W. E. Uiterwijk, M. G. Catanesi, I. Makhlyoueva, H. Shibuya, M Messina, Cristiano Bozza, N. Bruski, Motoaki Miyanishi, K. Hoshino, M. Litmaath, T. Kawamura, M. De Serio, M. Serin-Zeyrek, A. Bülte, K. Niwa, Jean-Paul Fabre, Shigeki Aoki, G. Rosa, Gaston Wilquet, P. Tolun, S. Ricciardi, K. Winter, L. Scotto Lavina, Th. Delbar, C. S. Yoon, V. Khovansky, C. Pistillo, A. Maslennikov, H. Meinhard, J. Konijn, G. Grella, A. Rozanov, Mehmet Zeyrek, S. Simone, B. Van de Vyver, E. Barbuto, S. Buontempo, J. Panman, F. Di Capua, K. Narita, A. Artamonov, R. Tsenov, J. Goldberg, R. van Dantzig, Other Research IHEF (IoP, FNWI), Kayis Topaksu, A., Onengüt, G., van Dantzig, R., de Jong, M., Konijn, J., Melzer, O., Oldeman, R. G. C., Pesen, E., van der Poel, C. A. F. J., Visschers, J. L., Güler, M., Köse, U., Serin Zeyrek, M., Kama, S., Sever, R., Tolun, P., Zeyrek, M. T., Catanesi, M. G., De Serio, M., Ieva, M., Muciaccia, M. T., Radicioni, E., Simone, S., Bülte, A., Winter, K., Van de Vyver, B., Vilain, P., Wilquet, G., Saitta, B., Di Capua, E., Ogawa, S., Shibuya, H., Artamonov, A., Brunner, J., Chizhov, M., Cussans, D., Doucet, M., Fabre, J. P., Hristova, I. R., Kawamura, T., Kolev, D., Litmaath, M., Meinhard, H., Panman, J., Papadopoulos, I. M., Ricciardi, S., Rozanov, A., Saltzberg, D., Tsenov, R., Uiterwijk, J. W. E., Zucchelli, P., Goldberg, J., Chikawa, M., Arik, E., Song, J. S., Yoon, C. S., Kodama, K., Ushida, N., Aoki, S., Hara, T., Delbar, T., Favart, D., Grégoire, G., Kalinin, S., Makhlyoueva, I., Gorbunov, P., Khovansky, V., Shamanov, V., Tsukerman, I., Bruski, N., Frekers, D., Rondeshagen, D., Wolff, T., Hoshino, K., Kawada, J., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Narita, K., Niu, K., Niwa, K., Nonaka, N., Sato, O., Toshito, T., Buontempo, S., Cocco, A. G., D'Ambrosio, N., De Lellis, G., De Rosa, G., DI CAPUA, Francesco, Ereditato, A., Fiorillo, Giuliana, Marotta, A., Messina, M., Migliozzi, P., Pistillo, C., Santorelli, R., Scotto Lavina, L., Strolin, P., Tioukov, V., Nakamura, K., Okusawa, T., Dore, U., Loverre, P. F., Ludovici, L., Maslennikov, A., Righini, P., Rosa, G., Santacesaria, R., Satta, A., Spada, F. R., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sirignano, C., Sorrentino, S., Sato, Y., Tezuka, I., T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, F. D., Capua, A., Ereditato, A., Marotta, M., Messina, P., Migliozzi, C., Pistillo, R., Santorelli, L. S., Lavina, P., Strolin, V., Tioukov, K., Nakamura, T., Okusawa, U., Dore, R., Loverre, L., Ludovici, A., Maslennikov, P., Righini, G., Rosa, R., Santacesaria, A., Satta, F. R., Spada, E., Barbuto, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, I., Tezuka, UCL - SC/PHYS - Département de physique, and Çukurova Üniversitesi
Subjects: Physics, CHORUS EXPERIMENT, Nuclear and High Energy Physics, Particle physics, INCLUSIVE RHO-0 PRODUCTION, Muon, Large Hadron Collider, Meson, Physics::Instrumentation and Detectors, Branching fraction, NU-P, MESON PRODUCTION, Bremsstrahlung, Virtual particle, NEON, ANTINEUTRINO, J/PSI, Nuclear physics, SCATTERING, High Energy Physics::Experiment, CALORIMETER, Neutrino, Particle Physics - Experiment, Charged current
Abstract: WOS: 000223122600006 This Letter reports on a study of trimuon events induced by neutrino interactions in the CHORUS calorimeter exposed to the CERN SPS wide-band v(mu) beam. Among the multimuon events produced in the calorimeter, 42 mu(-) mu(-) mu(+) events were selected and their kinematical properties investigated. In the past, several groups collected a sample of about one hundred events of this type but their source was largely unknown. Taking advantage of experimental data presently available on the production and muonic branching ratios of light neutral mesons and resonances, we make absolute predictions for the expected rates in our experiment. Detailed Monte Carlo simulations described in this article show that more than half of the trimuon events can be attributed to this source. Muons from pi- and K- decays in charm dimuon events are responsible for an additional approximate to 25% contribution to the total mu(-)mu(-)mu(+) rate. The remaining 25% of events are likely to come from the internal bremsstrahlung of virtual photons into a muon pair. Associated-charm production with subsequent decays of both charmed particles into muons is a negligible source of trimuon events. (C) 2004 Elsevier B.V. All rights reserved.
Published: 2004

21. Cross-section measurement for quasi-elastic production of charmed baryons in νN interactions

Author: I Maklioueva, O. Melzer, M. Serin-Zeyrek, Michiyuki Chikawa, E. Arik, C. Pistillo, M. T. Muciaccia, Shigeki Aoki, Ivana Hristova, E. Di Capua, S. Kalinin, R. Santacesaria, V. Khovansky, U. Dore, H. Meinhard, P. Strolin, E. Pesen, S. Sorrentino, I. Tezuka, G. L. Pittoni, Toshiyuki Nakano, J. S. Song, Motoaki Miyanishi, S. Buontempo, G. De Lellis, K. Niwa, F. Di Capua, D. Frekers, Mathieu Doucet, Y. Sato, Mitsuhiro Nakamura, S. Ogawa, K. Nakamura, Ramazan Sever, Nicola D'Ambrosio, D. Kolev, K. Hoshino, A. G. Cocco, Denis Favart, J. Kawada, Gulsen Onengut, N. Ushida, T. Hara, K. Winter, B. Saitta, Rudolf Oldeman, P. Migliozzi, F. R. Spada, C. S. Yoon, U. Kose, G. De Rosa, Pierre Vilain, N. Bruski, T. Kawamura, I.M. Papadopoulos, Mihail Chizhov, Ghislain Grégoire, M. G. Catanesi, V. Tioukov, K. Niu, G. Romano, A. Artamonov, H. Shibuya, L. Ludovici, A. Marotta, Osamu Sato, N. Nonaka, E. Radicioni, M. Ieva, Antonio Ereditato, P. Righini, V. Shamanov, C. Sirignano, P. Gorbunov, A. Satta, M. de Jong, R. Tsenov, J. Goldberg, Jan Visschers, G. Rosa, R. van Dantzig, Gaston Wilquet, S. Simone, M. De Serio, P. Tolun, A. Bülte, B. Van de Vyver, S. Ricciardi, Koichi Kodama, Murat Guler, J. W. E. Uiterwijk, L. Scotto Lavina, M. Messina, Th. Delbar, A. Rozanov, G. Fiorillo, G. Grella, Mehmet Zeyrek, Masahiro Komatsu, Cristiano Bozza, T. Okusawa, T. Toshito, P. F. Loverre, K. Narita, E. Barbuto, J. Panman, P. Zucchelli, Ilya Tsukerman, A. Kayis-Topaksu, Çukurova Üniversitesi, Kayis Topaksu, A., Onengüt, G., van Dantzig, R., de Jong, M., Melzer, O., Oldeman, R. G. C., Pesen, E., Spada, F. R., Visschers, J. L., Güler, M., Köse, U., Serin Zeyrek, M., Sever, R., Tolun, P., Zeyrek, M. T., Catanesi, M. G., De Serio, M., Ieva, M., Muciaccia, M. T., Radicioni, E., Simone, S., Bülte, A., Winter, K., Van de Vyver, B., Vilain, P., Wilquet, G., Pittoni, G. L., Saitta, B., Di Capua, E., Ogawa, S., Shibuya, H., Artamonov, A., Chizhov, M., Doucet, M., Hristova, I. R., Kawamura, T., Kolev, D., Meinhard, H., Panman, J., Papadopoulos, I. M., Ricciardi, S., Rozanov, A., Tsenov, R., Uiterwijk, J. W. E., Zucchelli, P., Goldberg, J., Chikawa, M., Arik, E., Song, J. S., Yoon, C. S., Kodama, K., Ushida, N., Aoki, S., Hara, T., Delbar, T., Favart, D., Grégoire, G., Kalinin, S., Maklioueva, I., Gorbunov, P., Khovansky, V., Shamanov, V., Tsukerman, I., Bruski, N., Frekers, D., Hoshino, K., Kawada, J., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Narita, K., Niu, K., Niwa, K., Nonaka, N., Sato, O., Toshito, T., Buontempo, S., Cocco, A. G., D'Ambrosio, N., De Lellis, G., De Rosa, G., DI CAPUA, Francesco, Ereditato, A., Fiorillo, Giuliana, Marotta, A., Messina, M., Migliozzi, P., Pistillo, C., Scotto lavina, L., Strolin, P., Tioukov, V., Nakamura, K., Okusawa, T., Dore, U., Loverre, P. F., Ludovici, L., Righini, P., Rosa, G., Santacesaria, R., Satta, A., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sirignano, C., Sorrentino, S., Sato, Y., Tezuka, I., T., Nakano, K., Narita, K., Niu, K., Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, F. D., Capua, A., Ereditato, A., Marotta, M., Messina, P., Migliozzi, C., Pistillo, L. S., Lavina, P., Strolin, V., Tioukov, K., Nakamura, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, P., Righini, G., Rosa, R., Santacesaria, A., Satta, E., Barbuto, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, and I., Tezuka
Subjects: Physics, Particle physics, Nuclear and High Energy Physics, CHORUS EXPERIMENT, High Energy Physics::Phenomenology, Physique atomique et nucléaire, Baryon, Nuclear physics, Charmed baryons, Cross section (physics), NEUTRINO-PRODUCTION, CHARGED-CURRENT INTERACTIONS, Nuclear emulsion, Production (computer science), High Energy Physics::Experiment, Charm (quantum number), Neutrino, Nuclear Experiment, Charged current, Particle Physics - Experiment
Abstract: A study of quasi-elastic production of charmed baryons in charged-current interactions of neutrinos with the nuclear emulsion target of CHORUS is presented. In a sample of about 46 000 interactions located in the emulsion, candidates for decays of short-lived particles were identified by using new automatic scanning systems and later confirmed through visual inspection. Criteria based both on the topological and kinematical characteristics of quasi-elastic charm production allowed a clear separation between events of this type and those in which charm is produced in deep inelastic processes. A final sample containing 13 candidates consistent with quasi-elastic production of a charmed baryon with an estimated background of 1.7 events was obtained. At the average neutrino energy of 27 GeV the cross-section for the total quasi-elastic production of charmed baryons relative to the νN charged-current cross-section was measured to be σ(QE)/σ(CC) = (0.23-0.06+0.02(stat)×10-2. Through an analysis of the topology at the production and decay vertices the relative cross-sections were measured separately for singly (Λc +, ∑c+, ∑c +*) and doubly (∑c++, ∑ c++*) charged baryons. © 2003 Published by Elsevier B.V., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2003

22. Measurement of Lambda(+)(c) production in neutrino charged-current interactions

Author: E. Barbuto, S. Simone, A. Satta, B. Van de Vyver, E. Radicioni, Jiro Kawada, P. Zucchelli, Ilya Tsukerman, S. Kalinin, U. Dore, Nicola D'Ambrosio, J. Panman, C. S. Yoon, V. Tioukov, Mitsuhiro Nakamura, K. Nakamura, Osamu Sato, P. F. Loverre, Ghislain Grégoire, S. Sorrentino, K. Niu, A. Marotta, T. Kawamura, A. Kayis-Topaksu, M. Miyanishi, I. Tezuka, J. S. Song, F. R. Spada, G. Romano, D. Frekers, A. Artamonov, S. Ogawa, M. De Serio, A. Bülte, Jan Visschers, K. Niwa, B. Saitta, Th. Delbar, T. Hara, R. Tsenov, D. Kolev, M. Messina, Cristiano Bozza, N. Bruski, V. Khovansky, C. Pistillo, Utku Kose, M. G. Catanesi, J. Goldberg, I. Papadopoulos, M. T. Muciaccia, G. Fiorillo, N. Nonaka, K. Narita, R. van Dantzig, S. Buontempo, A. G. Cocco, Michiyuki Chikawa, F. Di Capua, Antonio Ereditato, E. Di Capua, Denis Favart, V. Shamanov, Murat Guler, H. Shibuya, Chiara Sirignano, G. De Rosa, K. Hoshino, R. El-Aidi, Ramazan Sever, S. Ricciardi, Mathieu Doucet, M. Ieva, K. Winter, Koichi Kodama, G. Grella, P. Gorbunov, Toshiyuki Nakano, I Maklioueva, Ivana Hristova, R. Santacesaria, L. Scotto Lavina, G. De Lellis, M. de Jong, E. Arik, J. W. E. Uiterwijk, L. Ludovici, G. Rosa, Masahiro Komatsu, Gaston Wilquet, P. Tolun, T. Okusawa, T. Toshito, Y. Sato, A. Rozanov, Gulsen Onengut, N. Ushida, H. Meinhard, P. Migliozzi, Mehmet Zeyrek, Mihail Chizhov, O. Melzer, P. Strolin, E. Pesen, M. Serin-Zeyrek, Shigeki Aoki, Rudolf Oldeman, Pierre Vilain, P. Righini, N. Armenise, Çukurova Üniversitesi, A., Kayis Topaksu, G., Onengut, R. v., Dantzig, A. d., Jong, O., Melzer, R. G., C., E., Pesen, F. R., Spada, J. L., Visscher, M., Guler, U., Kose, A., Serin Zeyrek, R., Sever, P., Tolun, M. T., Zeyrek, N., Armenise, M. G., Catanesi, M. D., Serio, M., Leva, M. T., Muciaccia, A., Bulte, K., Winter, R., El Aidi, B. V., De, P., Vilain, G., Wilquet, B., Saitta, E. D., Capua, S., Ogawa, H., Shibuya, A., Artamonov, M., Chizhov, M., Doucet, I. R., Hristova, T., Kawamura, D., Kolev, H., Meinhard, J., Panman, I. M., Papadopoulo, S., Ricciardi, A., Rozanov, R., Tsenov, J. W., E., P., Zucchelli, J., Goldberg, M., Chikawa, E., Arik, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, T., Delbar, D., Favart, G., Gregoire, S., Kalinin, I., Maklioueva, P., Gorbunov, V., Khovansky, V., Shamanov, I., Tsukerman, N., Bruski, D., Freker, K., Hoshino, J., Kawada, M., Komatsu, M., Miyanishi, M., Nakamura, T., Nakano, K., Narita, K., Niu, K., Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, DI CAPUA, Francesco, A., Ereditato, Fiorillo, Giuliana, A., Marotta, M., Messina, P., Migliozzi, C., Pistillo, L. S., Lavina, Strolin, PAOLO EMILIO, V., Tioukov, K., Nakamura, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, P., Righini, G., Rosa, R., Santacesaria, A., Satta, E., Barbuto, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, I., Tezuka, Kayis Topaksu, A, Onengüt, G, van Dantzig, R, de Jong, M, Melzer, O, Oldeman, R. G. C, Pesen, E, Spada, F. R, Visschers, J. L, Güler, M, Köse, U, Serin Zeyrek, M, Sever, R, Tolun, P, Zeyrek, M. T, Armenise, N, Catanesi, M. G, De Serio, M, Ieva, M, Muciaccia, M. T, Radicioni, E, Simone, S, Bülte, A, Winter, K, El Aidi, R, Van de Vyver, B, Vilain, P, Wilquet, G, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Artamonov, A, Chizhov, M, Doucet, M, Hristova, I. R, Kawamura, T, Kolev, D, Meinhard, H, Panman, J, Papadopoulos, I. M, Ricciardi, S, Rozanov, A, Tsenov, R, Uiterwijk, J. W. E, Zucchelli, P, Goldberg, J, Chikawa, M, Arik, E, Song, J. S, Yoon, C. S, Kodama, K, Ushida, N, Aoki, S, Hara, T, Delbar, T, Favart, D, Grégoire, G, Kalinin, S, Maklioueva, I, Gorbunov, P, Khovansky, V, Shamanov, V, Tsukerman, I, Bruski, N, Frekers, D, Hoshino, K, Kawada, J, Komatsu, M, Miyanishi, M, Nakamura, M, Nakano, T, Narita, K, Niu, K, Niwa, K, Nonaka, N, Sato, O, Toshito, T, Buontempo, S, Cocco, A. G, D'Ambrosio, N, De Lellis, G, De Rosa, G, Ereditato, A, Marotta, A, Messina, M, Migliozzi, P, Pistillo, C, Scotto lavina, L, Strolin, P, Tioukov, V, Nakamura, K, Okusawa, T, Dore, U, Loverre, P. F, Ludovici, L, Righini, P, Rosa, G, Santacesaria, R, Satta, A, Barbuto, E, Bozza, C, Grella, G, Romano, G, Sirignano, C, Sorrentino, S, Sato, Y, and Tezuka, I.
Subjects: Physics, Nuclear and High Energy Physics, Large Hadron Collider, Lambda, Lambda baryon, CROSS-SECTIONS, Nuclear physics, EVENTS, OPPOSITE-SIGN DIMUONS, Production (computer science), High Energy Physics::Experiment, Charm (quantum number), Neutrino, Nucleon, Nuclear Experiment, Charged current
Abstract: A measurement of ?c+ production in neutrino nucleon charged-current interactions is presented. In a subsample of about 50 000 interactions located in the emulsion target of the CHORUS detector, exposed to the wide band neutrino beam of the CERN SPS, candidates for decays of short-lived particles were identified using new automatic scanning systems and later confirmed through visual inspection. Criteria based on the flight length allowed a statistical separation among the different charm species thus enabling a sample particularly rich in A+ to be defined. At an average neutrino energy of 27 GeV, the product ?(?c+)/?(CC) × BR(?c+ › 3p) was measured to be (0.37 ± 0.10(stat) ± 0.02(syst)) × 10-2, while the values of (1.54 ± 0.35(stat) ± 0.18(syst)) × 10-2 and of 0.24 ± 0.07(stat) ± 0.04(syst) were obtained for ?(?c+)/?(CC) and BR(?c+ › 3p), respectively. © 2003 Elsevier Science B.V. All rights reserved. KRF-2001-005-D00006 Israel Science Foundation: 328/94 Japan Society for the Promotion of Science CERN Bundesministerium für Bildung und Forschung Instituto Nazionale di Fisica Nucleare Foundation for Fundamental Research on Matter Korean Foundation for Cancer Research We gratefully acknowledge the help and support of the neutrino-beam staff and of the numerous technical collaborators who contributed to the detector construction, operation, emulsion pouring, development, and scanning. The experiment has been made possible by grants from the Institut Interuniversitaire des Sciences Nucl e ´ aires and the Interuniversitair Instituut voor Kernwetenschappen (Belgium); the Israel Science Foundation (Grant 328/94) and the Technion Vice President Fund for the Promotion of Research (Israel); CERN (Geneva, Switzerland); the German Bundesministerium f u ¨ r Bildung und Forschung (Germany); the Institute of Theoretical and Experimental Physics (Moscow, Russia); the Istituto Nazionale di Fisica Nucleare (Italy); the Promotion and Mutual Aid Corporation for Private Schools of Japan and Japan Society for the Promotion of Science (Japan); the Korea Research Foundation (Grant KRF-2001-005-D00006) (Republic of Korea); the Foundation for Fundamental Research on Matter FOM and the National Scientific Research Organization NWO (The Netherlands); and the Scientific and Technical Research Council of Turkey (Turkey). We gratefully acknowledge their support.
Published: 2003

23. Observation of one event with the characteristics of associated charm production in neutrino charged-current interactions

Author: A. Kayis-Topaksu, A. G. Cocco, M. Messina, I Maklioueva, Denis Favart, G. Fiorillo, P. F. Loverre, G. De Rosa, K. Niu, E. Arik, V. Palladino, B. Saitta, Osamu Sato, K. Niwa, Th. Delbar, Murat Guler, M. Miyanishi, G. Grella, Michiyuki Chikawa, G. De Lellis, Y. Sato, Masahiro Komatsu, T. Wolff, M. G. Catanesi, Nicola D'Ambrosio, T. Okusawa, D. Kolev, V. Khovansky, T. Toshito, S. Kalinin, Gulsen Onengut, Jan Visschers, N. Armenise, Koichi Kodama, T. Kawamura, U. Dore, S. Sorrentino, N. Ushida, David Cussans, M. De Serio, A. Bülte, K. Hoshino, P. Gorbunov, J. W. E. Uiterwijk, S. Ogawa, Toshiyuki Nakano, O. Melzer, M. de Jong, Ivana Hristova, S. Simone, R. Santacesaria, P. Zucchelli, Ilya Tsukerman, F. R. Spada, A. Maslennikov, P. Strolin, Cristiano Bozza, B. Van de Vyver, S. Ricciardi, E. Pesen, I. Tezuka, A. Satta, R. El-Aidi, P. Migliozzi, L. Ludovici, E. Di Capua, J. Konijn, N. Nonaka, P Righini, M. Ieva, Mihail Chizhov, Antonio Ereditato, V. Shamanov, Ramazan Sever, G. Rosa, Gaston Wilquet, P. Tolun, D. Frekers, A. Artamonov, H. Shibuya, T. Hara, R. Tsenov, J. Goldberg, N. Bruski, R. van Dantzig, S. Buontempo, F. Di Capua, Mathieu Doucet, K. Winter, Mitsuhiro Nakamura, K. Nakamura, C. S. Yoon, I.M. Papadopoulos, M. T. Muciaccia, K. Narita, E. Barbuto, Valeri Tioukov, Pierre Vilain, J. Panman, M. Serin-Zeyrek, Shigeki Aoki, Mehmet Zeyrek, A. Rozanov, H. Meinhard, Rudolf Oldeman, Ghislain Grégoire, G. Romano, J. S. Song, E. Radicioni, Jürgen Brunner, D. Rondeshagen, Kayis Topaksu, A, Onengüt, G, van Dantzig, R, de Jong, M, Konijn, J, Melzer, O, Oldeman, R. G. C, Pesen, E, Visschers, J. L, Güler, M, Serin Zeyrek, M, Sever, R, Tolun, P, Zeyrek, M. T, Armenise, N, Catanesi, M. G, De Serio, M, Ieva, M, Muciaccia, M. T, Radicioni, E, Simone, S, Bülte, A, Winter, K, El Aidi, R, Van de Vyver, B, Vilain, P, Wilquet, G, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Artamonov, A, Brunner, J, Chizhov, M, Cussans, D, Doucet, M, Hristova, I. R, Kolev, D, Meinhard, H, Panman, J, Papadopoulos, I. M, Ricciardi, S, Rozanov, A, Tsenov, R, Uiterwijk, J. W. E, Zucchelli, P, Goldberg, J, Chikawa, M, Arik, E, Song, J. S, Yoon, C. S, Kodama, K, Ushida, N, Aoki, S, Hara, T, Delbar, T, Favart, D, Grégoire, G, Kalinin, S, Maklioueva, I, Gorbunov, P, Khovansky, V, Shamanov, V, Tsukerman, I, Bruski, N, Frekers, D, Rondeshagen, D, Wolff, T, Hoshino, K, Komatsu, M, Miyanishi, M, Nakamura, M, Nakano, T, Narita, K, Niu, K, Niwa, K, Nonaka, N, Sato, O, Toshito, T, Buontempo, S, Cocco, A. G, D'Ambrosio, N, De lellis, G, De Rosa, G, DI CAPUA, Francesco, Ereditato, A, Fiorillo, Giuliana, Kawamura, T, Messina, M, Migliozzi, P, Palladino, V, Strolin, P, Tioukov, V, Nakamura, K, Okusawa, T, Dore, U, Loverre, P. F, Ludovici, L, Maslennikov, A, Righini, P, Rosa, G, Santacesaria, R, Satta, A, Spada, F. R, Barbuto, E, Bozza, C, Grella, G, Romano, G, Sorrentino, S, Sato, Y, Tezuka, I., UCL - SC/PHYS - Département de physique, Çukurova Üniversitesi, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, F. D., Capua, A., Ereditato, T., Kawamura, M., Messina, P., Migliozzi, Palladino, Vittorio, Strolin, PAOLO EMILIO, V., Tioukov, K., Nakamura, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, A., Maslennikov, P., Righini, G., Rosa, R., Santacesaria, A., Satta, F. R., Spada, E., Barbuto, C., Bozza, G., Grella, G., Romano, S., Sorrentino, Y., Sato, and I., Tezuka
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Muon, High Energy Physics::Phenomenology, Hadron, Nuclear physics, SEARCH, High Energy Physics::Experiment, Production (computer science), Nuclear emulsion, Charm (quantum number), Neutrino, Nuclear Experiment, Event (particle physics), Particle Physics - Experiment, Charged current, OSCILLATION
Abstract: We report on a search for associated charm production in neutrino charged-current interactions in the CHORUS experiment, based on the visual observation of charmed-particle decays. The search differs from those carried out so far in which the production of cc has been inferred from measurements of events with two or three muons in the final state, resulting from the decay of charmed hadrons. One event with a double charm-decay topology has been found and a corresponding background of 0.04 events has been evaluated. © 2002 Elsevier Science B.V. All rights reserved. CERN Promotion and Mutual Aid Corporation for Private Schools of Japan Bundesministerium für Bildung und Forschung Grant Foundation: KRF-2001-005-D00006 Israel Science Foundation: 328/94 Instituto Nazionale di Fisica Nucleare Foundation for Fundamental Research on Matter Korean Foundation for Cancer Research We gratefully acknowledge the help and support of the neutrino-beam staff and of the numerous technical collaborators who contributed to the detector construction, operation, emulsion pouring, development and scanning. The experiment has been made possible by grants from the Institut Interuniversitaire des Sciences Nucléaires and the Interuniversitair Instituut voor Kernwetenschappen (Belgium); the Israel Science Foundation (grant 328/94) and the Technion Vice President Fund for the Promotion of Research (Israel); CERN (Geneva, Switzerland); the German Bundesministerium für Bildung und Forschung (Germany); the Institute of Theoretical and Experimental Physics (Moscow, Russia); the Istituto Nazionale di Fisica Nucleare (Italy); the Promotion and Mutual Aid Corporation for Private Schools of Japan and Japan Society for the Promotion of Science (Japan); the Korea Research Foundation Grant (KRF-2001-005-D00006) (Republic of Korea); the Foundation for Fundamental Research on Matter FOM and the National Scientific Research Organization NWO (The Netherlands); and the Scientific and Technical Research Council of Turkey (Turkey). We gratefully acknowledge their support.
Published: 2002

24. Measurement of D0 production in neutrino charged-current interactions

Author: Motoaki Miyanishi, A. Artamonov, E. Di Capua, K. Hoshino, R. Tsenov, J. Goldberg, S. Ricciardi, G. De Rosa, M. De Serio, A. Bülte, R. van Dantzig, O. Melzer, R. El-Aidi, S. Kalinin, H. Meinhard, Murat Guler, L. Scotto Lavina, Nicola D'Ambrosio, G. Fiorillo, Osamu Sato, Masahiro Komatsu, U. Dore, T. Okusawa, S. Simone, T. Toshito, A. G. Cocco, M. Serin-Zeyrek, B. Van de Vyver, P. Gorbunov, M. G. Catanesi, P. Strolin, Denis Favart, M. de Jong, Shigeki Aoki, I. Tezuka, Pierre Vilain, E. Pesen, F. R. Spada, U. Kose, K. Niu, S. Buontempo, F. Di Capua, N. Armenise, I Maklioueva, Jan Visschers, D. Frekers, P Righini, B. Saitta, A. Rozanov, Koichi Kodama, E. Arik, K. Winter, V. Khovansky, T. Hara, Ghislain Grégoire, A. Ereditato, N. Bruski, P. Migliozzi, J. W. E. Uiterwijk, S. Sorrentino, L. Ludovici, T. Kawamura, G. Romano, M. Ieva, C. S. Yoon, Michiyuki Chikawa, S. Ogawa, Mihail Chizhov, A. Satta, Cristiano Bozza, M Messina, Rudolf Oldeman, Ivana Hristova, Mathieu Doucet, Y. Sato, R. Santacesaria, Mehmet Zeyrek, G. Rosa, K. Narita, P. F. Loverre, J. Kawada, Ramazan Sever, Gaston Wilquet, Gulsen Onengut, P. Tolun, E. Barbuto, N. Ushida, H. Shibuya, N. Nonaka, V. Shamanov, C. Sirignano, J. Panman, P. Zucchelli, Ilya Tsukerman, M. T. Muciaccia, A. Kayis-Topaksu, Mitsuhiro Nakamura, K. Nakamura, Toshiyuki Nakano, G. De Lellis, I.M. Papadopoulos, D. Kolev, E. Radicioni, K. Niwa, Th. Delbar, C. Pistillo, V Tioukov, A. Marotta, G. Grella, J. S. Song, UCL - SC/PHYS - Département de physique, Çukurova Üniversitesi, Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, L., Castagneto, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, F. D., Capua, DE ROSA, Gianfranca, A., Ereditato, Fiorillo, Giuliana, T., Kawamura, M., Messina, P., Migliozzi, Palladino, Vittorio, P., Strolin, V., Tioukov, K., Nakamura, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, P., Righini, G., Rosa, R., Santacesaria, A., Satta, F. R., Spada, E., Barbuto, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, and I., Tezuka
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Meson, Physics::Instrumentation and Detectors, High Energy Physics::Phenomenology, Detector, CHORUS, Neutrino beam, Vertex (geometry), EVENTS, Nuclear physics, OPPOSITE-SIGN DIMUONS, SEARCH, Physique des particules élémentaires, High Energy Physics::Experiment, Nuclear emulsion, QUARKS, Neutrino, Nuclear Experiment, Neutrino oscillation, Particle Physics - Experiment, Charged current
Abstract: During the years 1994-1997, the emulsion target of the CHORUS detector was exposed to the Wide Band Neutrino Beam from the CERN-SPS. About 170 000 neutrino interactions were successfully located in the emulsion. Improvements in the automatic emulsion scanning systems and application of different criteria allowed the sample of located events to be used for studies of charm production. We present a measurement of the production rate of D 0 mesons based on a sample of 25 693 located v μ charged-current (CC) interactions analysed so far. After reconstruction of the event topology in the vertex region, 283 D 0 decays were observed with an estimated background of 9.2 K 0 and Λ decays. The ratio of cross-section of D 0 production and v μ CC interactions is found to be (1.99 ± 0.13(stat.) ± 0.17(syst.)) × 10 -2 at 27 GeV average v μ energy. © 2002 Elsevier Science B. V. All rights reserved., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2002

25. Validation and verification of Geant4 standard electromagnetic physics

Author: Alexander Bagulya, J. Jacquemier, T Toshito, M. Maire, John Apostolakis, Vladimir Ivanchenko, L. Urbán, S Elles, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), and GEANT4
Subjects: Physics::Computational Physics, History, 010308 nuclear & particles physics, business.industry, Physics::Instrumentation and Detectors, Physics::Medical Physics, Experimental data, computer.software_genre, 01 natural sciences, [INFO.INFO-MO]Computer Science [cs]/Modeling and Simulation, Computer Science Applications, Education, Software, 0103 physical sciences, Verification, Data mining, 010306 general physics, business, computer
Abstract: International audience; The standard electromagnetic physics packages of Geant4 are used for simulation of particle transport and HEP detector response. The requirements to the precision and stability of computations are strong, for example, calorimeter response for ATLAS and CMS should be reproduced well within 1%. To keep and control long-stand quality of the package the software suites for validation and verification have been developed. In this work we describe main approaches for the validation, the structure of validation software and show examples of comparison between Geant4 simulation and the data.
Published: 2009

26. Recent progress in emulsion technology to study fragmentation reactions of high energetic ion beams

Author: Nakahiro Yasuda, H. Kubota, Masataka Komori, T. Toshito, Satoshi Kodaira, Nobuyuki Kanematsu, Ken'ichi Kuge, Shuya Ota, and TOSHITO, Toshiyuki
Subjects: Nuclear and High Energy Physics, Chemistry, [PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex], Nuclear engineering, Ion source, heavy ion, Nuclear physics, charge identification, Ion beam deposition, Fragmentation (mass spectrometry), nuclear emulsion, Ionization, Ionization chamber, Emulsion, Carbon Ion Radiotherapy, Nuclear emulsion, Instrumentation
Abstract: The R&D project to study nuclear fragmentation using emulsion in attempt to improve the accuracy of dose calculation in carbon ion radiotherapy has been carried out at NIRS-HIMAC since 2003. Based on the developed techniques, we are accumulating experimental data of fragmentation reactions for various beams and target combinations. In this programme we are also developing the practical application of hybrid apparatus of emulsion and CR-39, and performing basic study of gold deposition development in order to improve measurement of ionization.
Published: 2008

27. Measurement of atmospheric neutrino oscillation parameters by Super-Kamiokande I

Author: G. Guillian, C. Yanagisawa, M. Goldhaber, A. K. Ichikawa, K. Kaneyuki, A. Minamino, Y. Watanabe, S. Mine, D. W. Liu, Atsumu Suzuki, S. Matsuno, E. Kearns, T. Toshito, Hirokazu Ishino, M. Ishitsuka, Y. Totsuka, A. Suzuki, C. W. Walter, Ko Okumura, R. Svoboda, D. Turcan, Shantanu Desai, Y. Nakajima, K. Ishihara, J. P. Cravens, Y. Ashie, C. McGrew, S. Clark, R. J. Wilkes, Tsuyoshi Nakaya, Kunio Inoue, Y. Hayato, K. Taki, T. Sasaki, C. Saji, J. Yoo, A. L. Stachyra, K. Nishikawa, I. T. Lim, Masato Shiozawa, A. Kibayashi, K. S. Ganezer, J. Kameda, Shoji Yamamoto, T. Kato, N. Tamura, L. R. Sulak, C. W. Sterner, E. Blaufuss, J. Shirai, Y. Fukuda, Magdalena Malek, J. L. Stone, E. Sharkey, S. Dazeley, Yoshitaka Itow, Takashi Kobayashi, K. Hayashi, Y. Gando, Yusuke Koshio, Koji Nakamura, Y. Takeuchi, K. Washburn, Mark R. Vagins, John G. Learned, T. Iwashita, H. Okazawa, S. Ueda, T. Maruyama, S. Likhoded, Shinya Yamada, R. Nambu, W. Wang, S. Hatakeyama, Y. Kuno, R. Gran, Kazumasa Miyano, Henry W. Sobel, K. Nitta, Michael B. Smy, H. Seo, Takehisa Hasegawa, Kyoshi Nishijima, J. A. Goodman, Alec Habig, W. R. Kropp, G. W. Sullivan, John Hill, C. K. Jung, D. Kielczewska, Shigetaka Moriyama, J. S. Jang, D. Takemori, Yuichi Oyama, I. Kato, Shoei Nakayama, Katsuhiro Kobayashi, Minoru Yoshida, Y. Obayashi, T. Harada, S. Tasaka, W. E. Keig, T. Ishii, W. Gajewski, Kate Scholberg, S. B. Kim, David William Casper, Masayuki Nakahata, C. Mitsuda, J. Hosaka, Y. Takenaga, Masaya Hasegawa, M. Miura, K. K. Shiraishi, Yoshihiro Suzuki, Masatoshi Koshiba, J. Ishii, J. Zalipska, T. Ishida, Makoto Sakuda, A. Sarrat, Todd Haines, M. D. Messier, C. Mauger, A. Okada, H. G. Berns, T. Ishizuka, Taichi Morita, R. W. Ellsworth, Takaaki Kajita, Y. Choi, J. Y. Kim, Toshio Namba, and H. Maesaka
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Muon, High Energy Physics::Phenomenology, Monte Carlo method, High Energy Physics - Experiment, Nuclear physics, Neutrino detector, High Energy Physics::Experiment, Neutrino, Neutrino oscillation, Super-Kamiokande, Charged current, Energy (signal processing)
Abstract: We present a combined analysis of fully-contained, partially-contained and upward-going muon atmospheric neutrino data from a 1489 day exposure of the Super--Kamiokande detector. The data samples span roughly five decades in neutrino energy, from 100 MeV to 10 TeV. A detailed Monte Carlo comparison is described and presented. The data is fit to the Monte Carlo expectation, and is found to be consistent with neutrino oscillations of $\nu_\mu \leftrightarrow \nu_\tau$ with $\sin^22\theta > 0.92$ and $1.5\times 10^{-3} < \Delta m^2 < 3.4\times 10^{-3}{\rm eV}^2$ at 90% confidence level., Comment: 32 pages, 44 figures. As accepted for publication in Physical Review D
Published: 2005

28. Publisher's Note: Search for dark matter WIMPs using upward through-going muons in Super-Kamiokande [Phys. Rev. D70, 083523 (2004)]

Author: S. Desai, Y. Ashie, S. Fukuda, Y. Fukuda, K. Ishihara, Y. Itow, Y. Koshio, A. Minamino, M. Miura, S. Moriyama, M. Nakahata, T. Namba, R. Nambu, Y. Obayashi, N. Sakurai, M. Shiozawa, Y. Suzuki, H. Takeuchi, Y. Takeuchi, S. Yamada, M. Ishitsuka, T. Kajita, K. Kaneyuki, S. Nakayama, A. Okada, T. Ooyabu, C. Saji, M. Earl, E. Kearns, J. L. Stone, L. R. Sulak, C. W. Walter, W. Wang, M. Goldhaber, T. Barszczak, D. Casper, J. P. Cravens, W. Gajewski, W. R. Kropp, S. Mine, D. W. Liu, M. B. Smy, H. W. Sobel, C. W. Sterner, M. R. Vagins, K. S. Ganezer, J. Hill, W. E. Keig, J. Y. Kim, I. T. Lim, R. W. Ellsworth, S. Tasaka, G. Guillian, A. Kibayashi, J. G. Learned, S. Matsuno, D. Takemori, M. D. Messier, Y. Hayato, A. K. Ichikawa, T. Ishida, T. Ishii, T. Iwashita, J. Kameda, T. Kobayashi, T. Maruyama, K. Nakamura, K. Nitta, Y. Oyama, M. Sakuda, Y. Totsuka, A. T. Suzuki, M. Hasegawa, K. Hayashi, T. Inagaki, I. Kato, H. Maesaka, T. Morita, T. Nakaya, K. Nishikawa, T. Sasaki, S. Ueda, S. Yamamoto, T. J. Haines, S. Dazeley, S. Hatakeyama, R. Svoboda, E. Blaufuss, J. A. Goodman, G. W. Sullivan, D. Turcan, K. Scholberg, A. Habig, C. K. Jung, T. Kato, K. Kobayashi, M. Malek, C. Mauger, C. McGrew, A. Sarrat, E. Sharkey, C. Yanagisawa, T. Toshito, C. Mitsuda, K. Miyano, T. Shibata, Y. Kajiyama, Y. Nagashima, M. Takita, M. Yoshida, H. I. Kim, S. B. Kim, J. Yoo, H. Okazawa, T. Ishizuka, Y. Choi, H. K. Seo, Y. Gando, T. Hasegawa, K. Inoue, J. Shirai, A. Suzuki, M. Koshiba, T. Hashimoto, Y. Nakajima, K. Nishijima, T. Harada, H. Ishino, M. Morii, R. Nishimura, Y. Watanabe, D. Kielczewska, J. Zalipska, R. Gran, K. K. Shiraishi, K. Washburn, and R. J. Wilkes
Subjects: Nuclear physics, Physics, Nuclear and High Energy Physics, Particle physics, Weakly interacting massive particles, Dark matter, Cosmic ray, Elementary particle, Neutrino, Super-Kamiokande, Light dark matter, Particle identification
Published: 2004

29. Limits on the Neutrino Magnetic Moment using 1496 Days of Super-Kamiokande-I Solar Neutrino Data

Author: G. Guillian, Atsumu Suzuki, K. Hayashi, C. McGrew, Y. Hayato, K. Nishikawa, T. J. Haines, E. Kearns, Toshio Namba, Y. Watanabe, John G. Learned, Y. Totsuka, S. B. Kim, J. L. Stone, T. Inagaki, Kenzo Nakamura, D. Takemori, Shoji Yamamoto, C. Saji, Yusuke Koshio, H. Maesaka, G. W. Sullivan, T. Toshito, M. Earl, M. Ishitsuka, C. K. Jung, D. Kielczewska, C. W. Walter, Katsuhiro Kobayashi, M. D. Messier, H. W. Sobel, T. Hashimoto, T. Ooyabu, Masayuki Nakahata, Takaaki Kajita, C. Mauger, Shantanu Desai, S. Ueda, Michael B. Smy, H. Seo, T. Maruyama, S. Fukuda, Yoshitaka Kuno, I. Kato, A. Okada, W. Wang, Y. Ashie, H. Okazawa, Kunio Inoue, Minoru Yoshida, M. Takita, J. Y. Kim, Mikio Morii, Takehisa Hasegawa, Yuichi Oyama, Y. Obayashi, K. S. Ganezer, K. Kaneyuki, R. Nishimura, Makoto Sakuda, Magdalena Malek, Y. Fukuda, A. K. Ichikawa, Hyosun Kim, T. Ishizuka, T. Shibata, J. Zalipska, K. Martens, S. Mine, A. Minamino, T. Sasaki, J. Kameda, Y. Takeuchi, Shinya Yamada, S. Matsuno, T. Ishida, Taichi Morita, R. W. Ellsworth, L. R. Sulak, M. Ackermann, T. Kobayashi, Y. Kajiyama, Masatoshi Koshiba, Yoshihiro Suzuki, D. W. Liu, B. Viren, Alec Habig, T. Kato, C. W. Sterner, A. Kibayashi, J. Ishii, J. A. Goodman, J. P. Cravens, E. Blaufuss, W. R. Kropp, W. Gajewski, Kate Scholberg, T. Iwashita, K. Nitta, Kyoshi Nishijima, D. Turcan, Hirokazu Ishino, Y. Nakajima, K. Ishihara, David William Casper, J. Shirai, Shigetaka Moriyama, Y. Nagashima, H. Takeuchi, Masaya Hasegawa, M. Miura, Nobuyuki Sakurai, Shoei Nakayama, K. K. Shiraishi, Shigeki Tasaka, E. Sharkey, S. Dazeley, K. Washburn, S. Hatakeyama, R. Gran, C. Mitsuda, Yoshitaka Itow, R. J. Wilkes, I. T. Lim, C. Yanagisawa, J. Yoo, Kazumasa Miyano, Masato Shiozawa, Y. Choi, T. Barszczak, J. Hill, Y. Gando, T. Ishii, R. Nambu, A. Suzuki, R. Svoboda, Tsuyoshi Nakaya, W. E. Keig, and Mark R. Vagins
Subjects: Physics, Particle physics, Magnetic moment, Physics::Instrumentation and Detectors, Solar neutrino, High Energy Physics::Phenomenology, General Physics and Astronomy, Electron, Solar neutrino problem, High Energy Physics - Experiment, Nuclear physics, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, Super-Kamiokande, Neutrino oscillation
Abstract: A search for a non-zero neutrino magnetic moment has been conducted using 1496 live days of solar neutrino data from {\SK}. Specifically, we searched for distortions to the energy spectrum of recoil electrons arising from magnetic scattering due to a non-zero neutrino magnetic moment. In the absence of clear signal, we found $\mu_{\nu} \leq 3.6 \times 10^{-10}$ $\mu_{B}$ at 90% C.L. by fitting to the Super-Kamiokande day/night spectra. The fitting took into account the effect of neutrino oscillation on the shapes of energy spectra. With additional information from other solar neutrino and KamLAND experiments constraining the oscillation region, a limit of $\mu_{\nu} \leq 1.1 \times 10^{-10}$ $\mu_{B}$ at 90% C.L. was obtained., Comment: 5 pages, 4 figures
Published: 2004

30. Evidence for an oscillatory signature in atmospheric neutrino oscillations

Author: Toshio Namba, J. Yoo, J. P. Cravens, Masato Shiozawa, Shantanu Desai, Atsumu Suzuki, W. Gajewski, Kate Scholberg, Y. Totsuka, H. Maesaka, T. Sasaki, E. Kearns, Mark R. Vagins, Y. Takeuchi, Shinya Yamada, E. Blaufuss, Y. Nagashima, Masaki Ishitsuka, A. L. Stachyra, J. Zalipska, C. McGrew, J. Shirai, A. Suzuki, Takaaki Kajita, R. Nishimura, Makoto Sakuda, Y. Hayato, K. Taki, R. Svoboda, G. Guillian, A. Kibayashi, E. Sharkey, S. Dazeley, Y. Watanabe, Hirokazu Ishino, L. R. Sulak, J. Kameda, Ko Okumura, C. Yanagisawa, S. Likhoded, Yoshitaka Itow, W. R. Kropp, Shoji Yamamoto, C. W. Walter, M. Goldhaber, C. Saji, Y. Kuno, M. Takita, Y. Ashie, C. W. Sterner, Tsuyoshi Nakaya, K. Nakamura, T. Toshito, K. Washburn, K. Hayashi, S. Mine, Kunio Inoue, S. Hatakeyama, R. Gran, Y. Gando, H. Okazawa, Tomoyuki Maruyama, T. Ooyabu, A. Minamino, T. Ishida, John G. Learned, H. W. Sobel, W. Wang, Masayuki Nakahata, T. Iwashita, K. Kaneyuki, Y. Fukuda, R. Nambu, A. Sarrat, D. W. Liu, T. Ishizuka, C. K. Jung, Alec Habig, S. Matsuno, S. Ueda, Minoru Yoshida, D. Takemori, D. Kielczewska, Magdalena Malek, Todd Haines, N. Tamura, Yasunari Suzuki, Y. Choi, M. D. Messier, K. Nishikawa, G. W. Sullivan, J. L. Stone, T. Inagaki, Kazumasa Miyano, Taichi Morita, R. W. Ellsworth, T. Kobayashi, C. Mauger, Takehisa Hasegawa, Masatoshi Koshiba, J. S. Jang, T. Ishii, A. Okada, I. Kato, H. G. Berns, Yusuke Koshio, John Hill, Michael B. Smy, Katsuhiro Kobayashi, J. Ishii, Y. Takenaga, H. Seo, Masaya Hasegawa, M. Miura, David William Casper, T. Harada, C. Mitsuda, R. J. Wilkes, Y. Obayashi, J. Hosaka, K. Nitta, S. Tasaka, W. E. Keig, S. B. Kim, Kyoshi Nishijima, J. Y. Kim, D. Turcan, I. T. Lim, Y. Nakajima, K. K. Shiraishi, K. Ishihara, T. Kato, Shigetaka Moriyama, Yuichi Oyama, J. A. Goodman, Shoei Nakayama, A. K. Ichikawa, and K. S. Ganezer
Subjects: Physics, Particle physics, Tamura, Norio, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, General Physics and Astronomy, High Energy Physics - Experiment, Distribution (mathematics), Measurements of neutrino speed, 田村, 詔生, High Energy Physics::Experiment, Muon neutrino, Atmospheric neutrino, Neutrino, Signature (topology), Neutrino oscillation, Energy (signal processing)
Abstract: Muon neutrino disappearance probability as a function of neutrino flight length L over neutrino energy E was studied. A dip in the L/E distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation. The observed L/E distribution constrained nu_mu nu_tau neutrino oscillation parameters; 1.9x10^-3 < Delta m^2 < 3.0x10^-3 eV^2 and \sin^2(2theta) > 0.90 at 90% confidence level., Comment: 5 pages, 5 figures, submitted to PRL
Published: 2004

31. Search for Dark Matter WIMPs using Upward Through-going Muons in Super-Kamiokande

Author: K. Kaneyuki, G. Guillian, H. W. Sobel, Atsumu Suzuki, S. Mine, M. Goldhaber, J. Y. Kim, Mikio Morii, Takaaki Kajita, Magdalena Malek, E. Kearns, Y. Nagashima, H. Takeuchi, Hyosun Kim, M. Ishitsuka, Shoei Nakayama, Lawrence Sulak, C. Saji, David William Casper, Shantanu Desai, Nobuyuki Sakurai, Yoshihiro Suzuki, Todd Haines, Masatoshi Koshiba, C. McGrew, Y. Totsuka, E. Blaufuss, Y. Ashie, Y. Hayato, S. Ueda, Y. Takeuchi, Shinya Yamada, R. Nishimura, Makoto Sakuda, Minoru Yoshida, M. D. Messier, J. L. Stone, A. Kibayashi, T. Kobayashi, Kunio Inoue, Michael B. Smy, K. K. Shiraishi, W. R. Kropp, W. Wang, Y. Kajiyama, T. Inagaki, Toshio Namba, M. Earl, K. Nitta, Kenzo Nakamura, Yoshitaka Itow, Kyoshi Nishijima, C. W. Sterner, T. Ishii, C. Yanagisawa, C. Mauger, H. Seo, H. Maesaka, A. Minamino, Yusuke Koshio, Shigetaka Moriyama, T. Iwashita, Mark R. Vagins, Masaya Hasegawa, M. Miura, A. Okada, K. Hayashi, Kazumasa Miyano, John Hill, C. W. Walter, T. Hashimoto, J. G. Learned, T. Ishizuka, K. Washburn, T. Shibata, A. K. Ichikawa, D. Takemori, T. Ooyabu, G. W. Sullivan, C. Mitsuda, S. Hatakeyama, Masayuki Nakahata, R. Gran, C. K. Jung, D. Turcan, D. Kielczewska, Taichi Morita, R. W. Ellsworth, Katsuhiro Kobayashi, D. W. Liu, J. Kameda, M. Takita, R. J. Wilkes, I. Kato, Y. Nakajima, Hirokazu Ishino, I. T. Lim, A. Sarrat, Y. Fukuda, K. Ishihara, Y. Obayashi, S. Tasaka, W. E. Keig, J. A. Goodman, T. Harada, T. Kato, K. Nishikawa, Yuichi Oyama, Tomoyuki Maruyama, S. B. Kim, J. Zalipska, K. S. Ganezer, J. P. Cravens, T. Ishida, Takehisa Hasegawa, T. Sasaki, Y. Choi, W. Gajewski, Kate Scholberg, Y. Watanabe, T. Toshito, Shoji Yamamoto, J. Shirai, E. Sharkey, S. Dazeley, S. Fukuda, H. Okazawa, Alec Habig, S. Matsuno, Y. Gando, R. Nambu, J. Yoo, Masato Shiozawa, T. Barszczak, A. Suzuki, R. Svoboda, and Tsuyoshi Nakaya
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Muon, Physics::Instrumentation and Detectors, Dark matter, Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), WIMP, Neutrino detector, Weakly interacting massive particles, High Energy Physics::Experiment, Neutrino, Super-Kamiokande, Light dark matter
Abstract: We present the results of indirect searches for Weakly Interacting Massive Particles (WIMPs) with 1679.6 live days of data from the Super-Kamiokande detector using neutrino-induced upward through-going muons. The search is performed by looking for an excess of high energy muon neutrinos from WIMP annihilations in the Sun, the core of the Earth, and the Galactic Center, as compared to the number expected from the atmospheric neutrino background. No statistically significant excess was seen. We calculate flux limits in various angular cones around each of the above celestial objects. We obtain conservative model-independent upper limits on WIMP-nucleon cross-section as a function of WIMP mass and compare these results with the corresponding results from direct dark matter detection experiments., 10 pages, 14 figures, Submitted to Phys. Rev. D
Published: 2004

32. Search for periodic modulations of the solar neutrino flux in Super-Kamiokande-I

Author: J. Yoo, Y. Ashie, S. Fukuda, Y. Fukuda, K. Ishihara, Y. Itow, Y. Koshio, A. Minamino, M. Miura, S. Moriyama, M. Nakahata, T. Namba, R. Nambu, Y. Obayashi, N. Sakurai, M. Shiozawa, Y. Suzuki, H. Takeuchi, Y. Takeuchi, S. Yamada, M. Ishitsuka, T. Kajita, K. Kaneyuki, S. Nakayama, A. Okada, T. Ooyabu, C. Saji, S. Desai, M. Earl, E. Kearns, M. D. Messier, J. L. Stone, L. R. Sulak, C. W. Walter, M. Goldhaber, T. Barszczak, D. Casper, W. Gajewski, W. R. Kropp, S. Mine, D. W. Liu, M. B. Smy, H. W. Sobel, M. R. Vagins, A. Gago, K. S. Ganezer, J. Hill, W. E. Keig, J. Y. Kim, I. T. Lim, R. W. Ellsworth, S. Tasaka, A. Kibayashi, J. G. Learned, S. Matsuno, D. Takemori, Y. Hayato, A. K. Ichikawa, T. Ishii, J. Kameda, T. Kobayashi, T. Maruyama, K. Nakamura, K. Nitta, Y. Oyama, M. Sakuda, Y. Totsuka, M. Yoshida, M. Kohama, T. Iwashita, A. T. Suzuki, T. Inagaki, I. Kato, T. Nakaya, K. Nishikawa, T. J. Haines, S. Dazeley, S. Hatakeyama, R. Svoboda, E. Blaufuss, M. L. Chen, J. A. Goodman, G. Guillian, G. W. Sullivan, D. Turcan, K. Scholberg, A. Habig, M. Ackermann, C. K. Jung, T. Kato, K. Kobayashi, K. Martens, M. Malek, C. Mauger, C. McGrew, E. Sharkey, B. Viren, C. Yanagisawa, T. Toshito, C. Mitsuda, K. Miyano, T. Shibata, Y. Kajiyama, Y. Nagashima, M. Takita, H. I. Kim, S. B. Kim, H. Okazawa, T. Ishizuka, Y. Choi, H. K. Seo, M. Etoh, Y. Gando, T. Hasegawa, K. Inoue, J. Shirai, A. Suzuki, M. Koshiba, Y. Hatakeyama, Y. Ichikawa, M. Koike, K. Nishijima, H. Ishino, M. Morii, R. Nishimura, Y. Watanabe, D. Kielczewska, H. G. Berns, S. C. Boyd, A. L. Stachyra, and R. J. Wilkes
Subjects: Physics, Nuclear and High Energy Physics, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, Detector, FOS: Physical sciences, Flux, Astrophysics, Solar neutrino problem, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Neutrino detector, Astrophysics::Solar and Stellar Astrophysics, Measurements of neutrino speed, High Energy Physics::Experiment, Super-Kamiokande, Neutrino oscillation
Abstract: A search for periodic modulations of the solar neutrino flux was performed using the Super-Kamiokande-I data taken from May 31st, 1996 to July 15th, 2001. The detector's capability of measuring the exact time of events, combined with a relatively high yield of solar neutrino events, allows a search for short-time variations in the observed flux. We employed the Lomb test to look for periodic modulations of the observed solar neutrino flux. The obtained periodogram is consistent with statistical fluctuation and no significant periodicity was found.
Published: 2003

33. Search for Supernova Relic Neutrinos at Super-Kamiokande

Author: M. Malek, M. Morii, S. Fukuda, Y. Fukuda, M. Ishitsuka, Y. Itow, T. Kajita, J. Kameda, K. Kaneyuki, K. Kobayashi, Y. Koshio, M. Miura, S. Moriyama, M. Nakahata, S. Nakayama, T. Namba, A. Okada, T. Ooyabu, C. Saji, N. Sakurai, M. Shiozawa, Y. Suzuki, H. Takeuchi, Y. Takeuchi, Y. Totsuka, S. Yamada, S. Desai, M. Earl, E. Kearns, M. D. Messier, J. L. Stone, L. R. Sulak, C. W. Walter, M. Goldhaber, T. Barszczak, D. Casper, W. Gajewski, W. R. Kropp, S. Mine, D. W. Liu, M. B. Smy, H. W. Sobel, M. R. Vagins, A. Gago, K. S. Ganezer, W. E. Keig, R. W. Ellsworth, S. Tasaka, A. Kibayashi, J. G. Learned, S. Matsuno, D. Takemori, Y. Hayato, T. Ishii, T. Kobayashi, T. Maruyama, K. Nakamura, Y. Obayashi, Y. Oyama, M. Sakuda, M. Yoshida, M. Kohama, T. Iwashita, A. T. Suzuki, A. Ichikawa, T. Inagaki, I. Kato, T. Nakaya, K. Nishikawa, T. J. Haines, S. Dazeley, S. Hatakeyama, R. Svoboda, E. Blaufuss, J. A. Goodman, G. Guillian, G. W. Sullivan, D. Turcan, K. Scholberg, A. Habig, M. Ackermann, J. Hill, C. K. Jung, K. Martens, C. Mauger, C. McGrew, E. Sharkey, B. Viren, C. Yanagisawa, T. Toshito, C. Mitsuda, K. Miyano, T. Shibata, Y. Kajiyama, Y. Nagashima, K. Nitta, M. Takita, H. I. Kim, S. B. Kim, J. Yoo, H. Okazawa, T. Ishizuka, M. Etoh, Y. Gando, T. Hasegawa, K. Inoue, K. Ishihara, J. Shirai, A. Suzuki, M. Koshiba, Y. Hatakeyama, Y. Ichikawa, M. Koike, K. Nishijima, H. Ishino, R. Nishimura, Y. Watanabe, D. Kielczewska, H. G. Berns, S. C. Boyd, A. L. Stachyra, and R. J. Wilkes
Subjects: Physics, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, General Physics and Astronomy, Flux, Cosmic ray, Astrophysics, Upper and lower bounds, High Energy Physics - Experiment, Nuclear physics, Supernova, Positron, High Energy Physics::Experiment, Neutrino, Super-Kamiokande, Charged current
Abstract: A search for the relic neutrinos from all past core-collapse supernovae was conducted using 1496 days of data from the Super-Kamiokande detector. This analysis looked for electron-type anti-neutrinos that had produced a positron with an energy greater than 18 MeV. In the absence of a signal, 90% C.L. upper limits on the total flux were set for several theoretical models; these limits ranged from 20 to 130 nu_e bar cm^-2 s^-1. Additionally, an upper bound of 1.2 nu_e bar cm^-2 s^-1 was set for the supernova relic neutrino flux in the energy region E_nu > 19.3 MeV., Comment: 4 pages, 2 figures. Submitted to Physical Review Letters. New version includes corrections to Figure 1. Also, text has been shortened to conform with the space limitations of PRL
Published: 2003

34. Search for nu(e) from the sun at Super-Kamiokande-I

Author: M. Ishitsuka, T. J. Haines, A. T. Suzuki, C. W. Walter, Shantanu Desai, Y. Ichikawa, R. Nishimura, Makoto Sakuda, J. Shirai, J. L. Stone, T. Inagaki, Hyosun Kim, Ken-ichiro Kobayashi, Yoshitaka Itow, K. Martens, Shigeki Tasaka, E. Sharkey, S. Dazeley, T. Shibata, A. L. Stachyra, M. Ackermann, E. Blaufuss, J. A. Goodman, M. D. Messier, D. W. Liu, M. Koike, Y. Fukuda, C. Mitsuda, G. Guillian, C. Mauger, D. Turcan, Y. Totsuka, Y. Takeuchi, Y. Kajiyama, K. Nishikawa, K. Nitta, A. Okada, M. L. Chen, H. G. Berns, M. Miura, S. Mine, R. J. Wilkes, Yuichi Oyama, M. Earl, A. K. Ichikawa, M. Goldhaber, L. R. Sulak, T. Ishii, Takehisa Hasegawa, K. Ishihara, M. Koshiba, Y. Nagashima, H. Takeuchi, Kazumasa Miyano, Hirokazu Ishino, S. Fukuda, M. B. Smy, Y. Hatakeyama, A. Gago, H. W. Sobel, John G. Learned, S. Nakayama, H. Okazawa, K. Kaneyuki, S. C. Boyd, T. Ishizuka, D. Takemori, S. Hatakeyama, M. Etoh, Magdalena Malek, K. S. Ganezer, R. W. Ellsworth, Mikio Morii, T. Kobayashi, Michitoshi Yoshida, Tomoyuki Maruyama, Takaaki Kajita, Kunio Inoue, Alec Habig, C. Saji, S. Matsuno, A. Kibayashi, G. W. Sullivan, Yasunari Suzuki, Y. Watanabe, David William Casper, Toshio Namba, C. Yanagisawa, W. Gajewski, Kate Scholberg, Nobuyuki Sakurai, T. Toshito, M. R. Vagins, K. Nishijima, M. Takita, J. Kameda, C. McGrew, M. Kohama, Y. Hayato, K. Nakamura, S. Moriyama, T. Ooyabu, Masayuki Nakahata, Yusuke Koshio, E. Kearns, A. Suzuki, R. Svoboda, Tsuyoshi Nakaya, Y. Gando, S. B. Kim, C. K. Jung, J. Yoo, W. E. Keig, Masato Shiozawa, T. Barszczak, J. Hill, B. Viren, D. Kielczewska, I. Kato, Y. Obayashi, W. R. Kropp, S. Yamada, and T. Iwashita
Subjects: Physics, Standard solar model, Particle physics, Solar neutrino, General Physics and Astronomy, Flux, Cosmic ray, Limit (mathematics), Monochromatic color, Neutrino, Super-Kamiokande
Abstract: We present the results of a search for low energy nu(e) from the Sun using 1496 days of data from Super-Kamiokande-I. We observe no significant excess of events and set an upper limit for the conversion probability to nu(e) of the 8B solar neutrino. This conversion limit is 0.8% (90% C.L.) of the standard solar model's neutrino flux for total energy=8-20 MeV. We also set a flux limit for monochromatic nu(e) for E(nu(e))=10-17 MeV.
Published: 2002

35. Determination of the semi-leptonic branching fraction of charm hadrons produced in neutrino charged current interactions

Author: Nicola D'Ambrosio, S. Sorrentino, A. Rozanov, Michiyuki Chikawa, F. R. Spada, M. T. Muciaccia, S. Ogawa, A. G. Cocco, O. Melzer, Mitsuhiro Nakamura, K. Nakamura, Rudolf Oldeman, Masahiro Komatsu, Ivana Hristova, K. Hoshino, Denis Favart, T. Okusawa, C. Pistillo, Ghislain Grégoire, T. Toshito, K. Narita, I.M. Papadopoulos, M Messina, R. Santacesaria, E. Barbuto, H. Meinhard, G. Romano, S. Simone, E. Di Capua, V Tioukov, P. Strolin, M. De Serio, A. Bülte, J. Panman, S. Ricciardi, J. S. Song, P. Zucchelli, Ilya Tsukerman, A. Ereditato, G. De Rosa, D. Kolev, E. Pesen, Mathieu Doucet, P. Migliozzi, N. Bruski, L. Scotto Lavina, M. G. Catanesi, S. Kalinin, R. El-Aidi, Murat Guler, B. Van de Vyver, T. Kawamura, Ramazan Sever, U. Dore, Mehmet Zeyrek, E. Radicioni, Mihail Chizhov, B. Saitta, I. Tezuka, D. Frekers, H. Shibuya, I Maklioueva, T. Hara, L. Ludovici, Y. Sato, A. Kayis-Topaksu, S. Buontempo, K. Winter, N. Nonaka, G. Rosa, M. Ieva, V. Shamanov, C. Sirignano, P. F. Loverre, E. Arik, Gulsen Onengut, Gaston Wilquet, P. Tolun, Pierre Vilain, G. Grella, N. Armenise, F. Di Capua, C. S. Yoon, N. Ushida, K. Niwa, Th. Delbar, A. Artamonov, R. Tsenov, J. Goldberg, R. van Dantzig, P Righini, V. Khovansky, M. Serin-Zeyrek, Shigeki Aoki, M. Miyanishi, Toshiyuki Nakano, P. Gorbunov, G. De Lellis, M. de Jong, K. Niu, A. Satta, Cristiano Bozza, Osamu Sato, Koichi Kodama, J. W. E. Uiterwijk, Jan Visschers, G. Fiorillo, UCL - SC/PHYS - Département de physique, Kayis Topaksu, A, Onengüt, G, de Jong, M, Melzer, O, Oldeman, R. G. C, Pesen, E, Spada, F. R, van Dantzig, R, Visschers, J. L, Güler, M, Serin Zeyrek, M, Sever, R, Tolun, P, Zeyrek, M. T, Armenise, N, Catanesi, M. G, De Serio, M, Ieva, M, Muciaccia, M. T, Radicioni, E, Simone, S, Bülte, A, Winter, K, El Aidi, R, Van de Vyver, B, Vilain, P, Wilquet, G, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Artamonov, A, Chizhov, M, Doucet, M, Hristova, I. R, Kawamura, T, Kolev, D, Meinhard, H, Panman, J, Papadopoulos, I. M, Ricciardi, S, Rozanov, A, Tsenov, R, Uiterwijk, J. W. E, Zucchelli, P, Goldberg, J, Chikawa, M, Arik, E, Song, J. S, Yoon, C. S, Kodama, K, Ushida, N, Aoki, S, Hara, T, Delbar, T, Favart, D, Grégoire, G, Kalinin, S, Maklioueva, I, Gorbunov, P, Khovansky, V, Shamanov, V, Tsukerman, I, Bruski, N, Frekers, D, Hoshino, K, Komatsu, M, Miyanishi, M, Nakamura, M, Nakano, T, Narita, K, Niu, K, Niwa, K, Nonaka, N, Sato, O, Toshito, T, Buontempo, S, Cocco, A. G, D'Ambrosio, N, De Lellis, G, DI CAPUA, Francesco, De Rosa, G, Ereditato, A, Fiorillo, Giuliana, Messina, M, Migliozzi, P, Pistillo, C, Scotto lavina, L, Strolin, P, Tioukov, V, Nakamura, K, Okusawa, T, Dore, U, Loverre, P. F, Ludovici, L, Righini, P, Rosa, G, Santacesaria, R, Satta, A, Barbuto, E, Bozza, C, Grella, G, Romano, G, Sirignano, C, Sorrentino, S, Sato, Y, Tezuka, I., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, F. D., Capua, DE ROSA, Gianfranca, A., Ereditato, M., Messina, P., Migliozzi, C., Pistillo, L. S., Lavina, P., Strolin, V., Tioukov, K., Nakamura, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, P., Righini, G., Rosa, R., Santacesaria, A., Satta, E., Barbuto, C., Ozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, I., Tezuka, and Çukurova Üniversitesi
Subjects: Physics, Particle physics, Nuclear and High Energy Physics, Branching fraction, Detector, Hadron, CHORUS, Visible energy, CROSS-SECTIONS, PHYSICS, EVENTS, Nuclear physics, OPPOSITE-SIGN DIMUONS, SEARCH, Yield (chemistry), Physique des particules élémentaires, Charm (quantum number), Neutrino, Particle Physics - Experiment, Charged current
Abstract: During the years 1994-1997, the emulsion target of the CHORUS detector was exposed to the CERN-SPS Wide Band Neutrino Beam. The improvements of the past few years in the automatic emulsion scanning systems allowed a sample of events located in emulsion to be used for studies of charm production. Based on a sample of 56172vμu charged-current interactions analysed so far, we find a value of Bμ = 0.093 ± 0.009(stat.) ± 0.009(syst.) for the semi-leptonic branching fraction of charm hadrons. The result for events with visible energy larger than 30 GeV, Bμ = 0.102 ± 0.016(stat.) ± 0.010(syst.), can be combined with the existing measurements of the dimuon rate to yield a value of 0.219 ± 0.022 for the magnitude of the Cabibbo-Kobayashi-Maskawa matrix element \Vcd\. © 2002 Elsevier Science B.V. All rights reserved., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2002

36. Design, construction, and operation of SciFi tracking detector for K2K experiment

Author: A Suzuki, H Park, S Aoki, S Echigo, K Fujii, T Hara, T Iwashita, M Kitamura, M Kohama, G Kume, M Onchi, T Otaki, K Sato, M Takatsuki, K Takenaka, Y Tanaka, K Tashiro, T Inagaki, I Kato, S Mukai, T Nakaya, K Nishikawa, N Sasao, A Shima, H Yokoyama, T Chikamatsu, Y Hayato, T Ishida, T Ishii, H Ishino, E.J Jeon, T Kobayashi, S.B Lee, K Nakamura, Y Oyama, A Sakai, M Sakuda, V Tumakov, S Fukuda, Y Fukuda, M Ishizuka, Y Itow, T Kajita, J Kameda, K Kaneyuki, K Kobayashi, Y Kobayashi, Y Koshio, M Miura, S Moriyama, M Nakahata, S Nakayama, Y Obayashi, A Okada, N Sakurai, M Shiozawa, Y Suzuki, H Takeuchi, Y Takeuchi, Y Totsuka, T Toshito, S Yamada, K Miyano, M Nakamura, N Tamura, I Nakano, M Yoshida, T Kadowaki, S Kishi, T Maruyama, M Etoh, K Nishijima, H.C Bhang, B.H Khang, B.J Kim, H.I Kim, J.H Kim, S.B Kim, H So, J.H Yoo, J.H Choi, H.I Jang, J.S Jang, J.Y Kim, I.T Lim, M.Y Pac, E Kearns, K Scholberg, J.L Stone, L.R Sulak, C.W Walter, D Casper, W Gajewski, W Kropp, S Mine, H Sobel, M Vagins, S Matsuno, J Hill, C.K Jung, K Martens, C Mauger, C McGrew, E Sharkey, C Yanagisawa, H Berns, S Boyd, J Wilkes, D Kielczewska, and U Golebiewska
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Muon, business.industry, Physics::Instrumentation and Detectors, Track (disk drive), Noise reduction, Detector, FOS: Physical sciences, Tracking (particle physics), Particle identification, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Optics, K2K experiment, High Energy Physics::Experiment, business, Neutrino oscillation, Instrumentation
Abstract: We describe the construction and performance of a scintillating fiber detector used in the near detector for the K2K (KEK to Kamioka, KEK E362) long baseline neutrino oscillation experiment. The detector uses 3.7 m long and 0.692 mm diameter scintillating fiber coupled to image-intensifier tubes (IIT), and a CCD camera readout system. Fiber sheet production and detector construction began in 1997, and the detector was commissioned in March, 1999. Results from the first K2K runs confirm good initial performance : position resolution is estimated to be about 0.8 mm, and track finding efficiency is $98 \pm 2$ % for long tracks (i.e., those which intersect more than 5 fiber planes). The hit efficiency was estimated to be $92 \pm 2$ % using cosmic-ray muons, after noise reduction at the offline stage. The possibility of using the detector for particle identification is also discussed., Comment: In total 21 pages with 18 figures. THis is the proceedings for "The 7th International Conference on Instrumentation for Colliding Beam Physics", held on Hamamatsu, Japan, Nov. 15-19, 1999
Published: 2000
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37. 16-N as a calibration source for Super-Kamiokande

Author: E Blaufuss, G Guillian, Y Fukuda, S Fukuda, M Ishitsuka, Y Itow, T Kajita, J Kameda, K Kaneyuki, K Kobayashi, Y Kobayashi, Y Koshio, M Miura, S Moriyama, M Nakahata, S Nakayama, Y Obayashi, A Okada, K Okumura, N Sakurai, M Shiozawa, Y Suzuki, H Takeuchi, Y Takeuchi, T Toshito, Y Totsuka, S Yamada, M Earl, A Habig, E Kearns, M.D Messier, K Scholberg, J.L Stone, L.R Sulak, C.W Walter, M Goldhaber, T Barszczak, D Casper, W Gajewski, W.R Kropp, S Mine, L.R Price, M Smy, H.W Sobel, M.R Vagins, K.S Ganezer, W.E Keig, R.W Ellsworth, S Tasaka, A Kibayashi, J.G Learned, S Matsuno, D Takemori, Y Hayato, T Ishii, T Kobayashi, K Nakamura, Y Oyama, A Sakai, M Sakuda, O Sasaki, S Echigo, M Kohama, A.T Suzuki, T Inagaki, K Nishikawa, T.J Haines, B.K Kim, R Sanford, R Svoboda, M.L Chen, J.A Goodman, G.W Sullivan, J Hill, C.K Jung, K Martens, M Malek, C Mauger, C McGrew, E Sharkey, B Viren, C Yanagisawa, M Kirisawa, S Inaba, C Mitsuda, K Miyano, H Okazawa, C Saji, M Takahashi, M Takahata, Y Nagashima, K Nitta, M Takita, M Yoshida, S.B Kim, M Etoh, Y Gando, T Hasegawa, K Inoue, K Ishihara, T Maruyama, J Shirai, A Suzuki, M Koshiba, Y Hatakeyama, Y Ichikawa, M Koike, K Nishijima, H Fujiyasu, H Ishino, M Morii, Y Watanabe, U Golebiewska, D Kielczewska, S.C Boyd, A.L Stachyra, R.J Wilkes, and K.K Young
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Scale (ratio), Physics::Instrumentation and Detectors, Solar neutrino, Detector, Isotropy, FOS: Physical sciences, Linear particle accelerator, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Neutron generator, Calibration, Physics::Accelerator Physics, Super-Kamiokande, Instrumentation
Abstract: The decay of 16-N is used to cross check the absolute energy scale calibration for solar neutrinos established by the electron linear accelerator (LINAC). A deuterium-tritium neutron generator was employed to create 16-N via the (n,p) reaction on 16-O in the water of the detector. This technique is isotropic and has different systematic uncertainties than the LINAC. The results from this high statistics data sample agree with the absolute energy scale of the LINAC to better than 1%. A natural source of 16-N from the capture of mu^- on 16-O, which is collected as a background to the solar neutrino analysis, is also discussed., Comment: 20 pages, 10 figures, Submitted to NIM A, published version
Published: 2000
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38. The CHORUS experiment to search for ν_μ→ν_τ oscillation

Author: K. Hoepfner, Motoaki Miyanishi, P. Annis, A. Capone, G. Grella, E. Niu, Nicola D'Ambrosio, B. Saitta, G. Grégoire, T. Kawamura, Alfredo G. Cocco, Salvatore Buontempo, David Saltzberg, M. Litmaath, Kimio Niwa, Y. Obayashi, F. Riccardi, G. Rosa, E. Arik, R. Santacesaria, U. Dore, Matteo Ferroni, M. G. Catanesi, C. Mommaert, S. Sorrentino, N. Ushida, S. N. Kim, H. Chikawa, Vincent Lemaitre, M. Komatzu, K. Nakamura, F. Marchetti-Stasi, S. Ogawa, D. Frekers, L. Ludovici, J. Panman, D. C. Kim, Franco Meddi, M. Vander Donckt, Mehmet Zeyrek, Koichi Kodama, T. Kozaki, V. Khovansky, E. Pesen, T. Hara, Y. Kotaka, C. H. Hahn, Pierre Vilain, M. S. Park, G. Carnevale, K. Winter, Jean-Paul Fabre, V. Smirnitsky, D. Eckstein, D. Macina, M. Nakamura, D. Rondeshagen, E. Radicioni, Jürgen Brunner, P. Migliozzi, V. Palladino, Ch. Weinheimer, K. Hoshino, R. Gurin, Rudolf Oldeman, D. De Pedis, H. I. Jang, Henry T. Wong, J. W. E. Uiterwijk, R. Beyer, A. Artamonov, M. A. Mazzoni, Y. Ishii, A. S. Ayan, A. Maslennikov, G. Brooijmans, A. Kayis, F. Garufi, P. Lendermann, E. Di Capua, R. Ferreira, T. Yoshida, M. Messina, I. G. Park, G. Iovane, A. Meyer-Sievers, W. Flegel, C. S. Yoon, F. Cassol, Denis Favart, G. Romano, R. Tzenov, H. Øverȧs, R. van Dantzig, A. Di Bartolomeo, M. Serin-Zeyrek, Alexandre Rozanov, S. Simone, G. Fiorillo, H. Meinhard, S. Di Liberto, J. Konijn, V. Epstein, B. Van de Vyver, J. Hérin, A. Mailov, P. Zucchelli, J. S. Song, Shigeki Aoki, H. Shibuya, M. Kazuno, C. Luppi, J. L. Visschers, R. Meijer Drees, T. Patzak, K. Niu, T. Toshito, I. Tezuka, T. Okusawa, P. Strolin, T. Wolff, L. Casagrande, Gulsen Onengut, J. Y. Kim, P. Gorbunov, M. de Jong, J. Goldberg, Osamu Sato, L. Vivolo, Cristiano Bozza, Ramazan Sever, G. Piredda, Yoshihiro Sato, P. Righini, D. Bonekämper, M. T. Muciaccia, N. Armenise, Toshiyuki Nakano, S. Ricciardi, M. Gruwe, Inanc Birol, Antonio Ereditato, V. Shamanov, G. Stefanini, C.A.F.J. van der Poel, E. Eskut, Gaston Wilquet, P. Tolun, Makoto Kobayashi, and P. F. Loverre
Subjects: Physics, Nuclear and High Energy Physics, biology, Calorimeter (particle physics), Physics::Instrumentation and Detectors, Oscillation, Detector, Chorus, biology.organism_classification, Nuclear physics, Nuclear magnetic resonance, Muon spectrometer, Magnet, High Energy Physics::Experiment, Sensitivity (control systems), Neutrino oscillation, Instrumentation
Abstract: A new experimental apparatus, designed principally for a high sensitivity search for ν μ → ν τ oscillation, has been successlly constructed and made operational by the CHORUS Collaboration for the CERN-WA95 experiment. It consists of a large emulsion target, a scintillating fiber tracker system with optoelectronics read-out, an air-core magnet, a set of trigger hodoscopes, a calorimeter based on the lead/scintillating-fiber technique, and a muon spectrometer. The design, construction and performance of the entire apparatus and of the different detectors are described.
Published: 1997

39. Search for Nucleon Decay via Modes Favored by Supersymmetric Grand Unification Models in Super-Kamiokande-I

Author: Masatoshi Koshiba, Shoei Nakayama, Yuichi Oyama, A. Kibayashi, J. Ishii, K. Kaneyuki, J. Hill, Y. Gando, S. Matsuno, Yasunari Suzuki, Makoto Sakuda, Y. Takeuchi, Shinya Yamada, Toshio Namba, Y. Totsuka, Yusuke Koshio, R. Nambu, Mark R. Vagins, T. Ishizuka, H. Maesaka, M. Goldhaber, Taichi Morita, R. W. Ellsworth, A. Suzuki, M. Earl, Masashi Yokoyama, J. A. Goodman, R. Svoboda, Magdalena Malek, J. Zalipska, T. Harada, Tsuyoshi Nakaya, T. Ishida, C. McGrew, M. Ishitsuka, C. W. Walter, Y. Hayato, S. B. Kim, J. Y. Kim, J. Yoo, Shantanu Desai, Masato Shiozawa, Y. Choi, N. Tamura, T. Sasaki, J. L. Stone, L. R. Sulak, Henry W. Sobel, K. Nitta, Shoji Yamamoto, Koji Nakamura, A. Minamino, Kyoshi Nishijima, Michael B. Smy, T. Ooyabu, Masayuki Nakahata, Takaaki Kajita, H. Seo, Shigetaka Moriyama, Y. Fukuda, A. L. Stachyra, T. J. Haines, A. Sarrat, David William Casper, C. Mitsuda, J. Hosaka, A. K. Ichikawa, M. D. Messier, K. K. Shiraishi, D. W. Liu, C. Mauger, D. Takemori, K. Taki, A. Okada, H. G. Berns, J. Kameda, C. W. Sterner, D. Turcan, Y. Nakajima, K. Ishihara, T. Kobayashi, K. Hayashi, S. Ueda, T. Maruyama, Ko Okumura, John G. Learned, Y. Ashie, G. W. Sullivan, Katsuhiro Kobayashi, Kunio Inoue, J. S. Jang, K. Nishikawa, Y. Watanabe, S. Mine, T. Toshito, J. P. Cravens, W. R. Kropp, G. Guillian, T. Iwashita, S. Likhoded, Yoshitaka Itow, Y. Kuno, T. Kato, C. K. Jung, Minoru Yoshida, D. Kielczewska, Kazumasa Miyano, K. S. Ganezer, I. Kato, Y. Obayashi, W. E. Keig, Y. Takenaga, Masaya Hasegawa, M. Miura, K. Washburn, S. Hatakeyama, R. Gran, E. Blaufuss, C. Yanagisawa, Atsumu Suzuki, E. Kearns, T. Nakadaira, Takehisa Hasegawa, C. Saji, Hirokazu Ishino, W. Wang, H. Okazawa, Alec Habig, J. Shirai, Shigeki Tasaka, E. Sharkey, S. Dazeley, W. Gajewski, Kate Scholberg, T. Ishii, R. J. Wilkes, and I. T. Lim
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, High Energy Physics::Phenomenology, Supersymmetry, High Energy Physics - Experiment, Particle decay, TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY, Mass spectrum, Grand Unified Theory, High Energy Physics::Experiment, Neutron, Neutrino, Nucleon, Super-Kamiokande
Abstract: We report the results for nucleon decay searches via modes favored by supersymmetric grand unified models in Super-Kamiokande. Using 1489 days of full Super-Kamiokande-I data, we searched for $p \to \bar{\nu} K^+$, $n \to \bar{\nu} K^0$, $p \to \mu^+ K^0$ and $p \to e^+ K^0$ modes. We found no evidence for nucleon decay in any of these modes. We set lower limits of partial nucleon lifetime 2.3$\times10^{33}$, 1.3$\times10^{32}$, 1.3$\times10^{33}$ and 1.0$\times10^{33}$ years at 90% confidence level for $p \to \bar{\nu} K^+$, $n \to \bar{\nu} K^0$, $p \to \mu^+ K^0$ and $p \to e^+ K^0$ modes, respectively. These results give a strong constraint on supersymmetric grand unification models., Comment: 14 pages, 13 figures
Published: 2005

40. Observation of weak neutral current neutrino production of J/psi

Author: Nicola D'Ambrosio, T. Kawamura, K. Winter, Valeri Tioukov, T. Wolff, Alfredo G. Cocco, Michiyuki Chikawa, Pierre Vilain, David Cussans, O. Melzer, C. S. Yoon, N. Ushida, G. Onenguet, K. Niu, F. R. Spada, S. Di Liberto, E. Barbuto, J. Hérin, P. Gorbunov, T. Okusawa, P. Strolin, Antonio Ereditato, E. Pesen, V. Shamanov, Mathieu Doucet, M. de Jong, Osamu Sato, H. Veraes, L. Vivolo, Ch. Weinheimer, J. Panman, R. Santacesaria, Rudolf Oldeman, Jean-Paul Fabre, G. Romano, Y. Kotaka, Jan Visschers, Ramazan Sever, H. Shibuya, Mihail Chizhov, E. Di Capua, Piero Zucchelli, Murat Guler, David Saltzberg, A. Satta, M. Serin-Zeyrek, M. Kazuno, G. Piredda, Yoshihiro Sato, Mitsuhiro Nakamura, K. Nakamura, Shigeki Aoki, U. Dore, G. Rosa, Gaston Wilquet, P. Righini, S. Sorrentino, S. Simone, D. Rondeshagen, A. Kayis-Topaksu, Koichi Kodama, P. Tolun, N. Bruski, Cristiano Bozza, Mehmet Zeyrek, M. Litmaath, S. Ogawa, K. Hoshino, Ioannis Papadopoulos, T. Kozaki, R. Listone, D. Frekers, M. G. Catanesi, Henry T. Wong, J. W. E. Uiterwijk, Toshiyuki Nakano, N. Armenise, Denis Favart, T. Hara, G. De Lellis, H. Meinhard, D. Bonekaemper, I. G. Park, Y. Ishii, M. Messina, W. Flegel, S. Ricciardi, M. T. Muciaccia, L. Ludovici, F. Cassol, G. Fiorillo, I. Tezuka, D. De Pedis, Antonio Capone, A. Buelte, G. Grella, C.A.F.J. van der Poel, E. Eskut, R. El-Aidi, Y. Obayashi, K. Niwa, M. De Serio, Masahiro Komatsu, T. Toshito, S. Buontempo, F. Di Capua, M. Vander Donckt, Alexandre Rozanov, B. Van de Vyver, A. Mailov, V. Khovansky, A. Artamonov, R. Tsenov, J. Goldberg, R. van Dantzig, G. Grégoire, P. F. Loverre, A. Maslennikov, J. Konijn, G. Brooijmans, E. Radicioni, Jürgen Brunner, J. S. Song, Biagio Saitta, Motoaki Miyanishi, P. Annis, E. Niu, I S. Tsukerman, E. Arik, P. Migliozzi, V. Palladino, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), CHORUS, UCL - SC/PHYS - Département de physique, Çukurova Üniversitesi, E., Eskut, A., Kayis Topaksu, G., Onengut, R. v., Dantzig, M. d., Jong, J., Konijn, O., Melzer, R. G., C., E., Pesen, C. A. F., J. W. E., J. L., Visscher, M., Guler, M., Serin Zeyrek, R., Sever, P., Tolun, M. T., Zeyrek, N., Armenise, F., Cassol, M. G., Catanesi, R. D., Serio, M. T., Muciaccia, E., Radicioni, S., Simone, L., Vivolo, A., Bulte, K., Winter, P., Anni, R., El Aidi, M. V., Donckt, B. V., De, P., Vilain, G., Wilquet, P., Righini, B., Saitta, E. D., Capua, Y., Ishii, T., Kawamura, M., Kazuno, S., Ogawa, H., Shibuya, J., Brunner, M., Chizhov, D., Cussan, M., Doucet, J. P., Fabre, W., Flegel, M., Litmaath, H., Meinhard, E., Niu, H., Overa, J., Panman, I. M., Papadopoulo, S., Ricciardi, A., Rozanov, D., Saltzberg, P., Strolin, R., Tsenov, C., Weinheimer, H., Wong, P., Zucchelli, J., Goldberg, M., Chikawa, E., Arik, A. A., Mailov, I. G., Park, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, G., Brooijman, D., Favart, G., Gregoire, J., Herin, A., Artamonov, P., Gorbunov, V., Khovansky, V., Shamanov, I., Tsukerman, D., Bonekamper, N., D'Ambrosio, D., Freker, D., Rondeshagen, T., Wolff, K., Hoshino, M., Komatsu, Y., Kotaka, T., Kozaki, M., Miyanishi, M., Nakamura, T., Nakano, K., Niu, K., Niwa, Y., Obayashi, O., Sato, T., Toshito, N., Bruski, S., Buontempo, A. G., Cocco, G. D., Lelli, F. D., Capua, A., Ereditato, Fiorillo, Giuliana, R., Listone, M., Messina, P., Migliozzi, Palladino, Vittorio, V., Tioukov, K., Nakamura, T., Okusawa, A., Capone, D. D., Pedi, S. D., Liberto, U., Dore, P. F., Loverre, L., Ludovici, A., Maslennikov, G., Piredda, G., Rosa, R., Santacesaria, A., Satta, F. R., Spada, E., Barbuto, C., Bozza, G., Grella, G., Romano, S., Sorrentino, Y., Sato, I., Tezuka, and Damoiseaux, Magali
Subjects: Nuclear and High Energy Physics, Particle physics, [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], Physics::Instrumentation and Detectors, 01 natural sciences, Nucleon, Nuclear physics, PHYSICS, Neutral currents, 0103 physical sciences, Neutrino, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], CALORIMETER, 010306 general physics, Nuclear Experiment, Quantum chromodynamics, Physics, CHORUS EXPERIMENT, Large Hadron Collider, Neutral current, 010308 nuclear & particles physics, CHARM PRODUCTION, High Energy Physics::Phenomenology, Calorimeter, J/?, Production (computer science), High Energy Physics::Experiment, Particle Physics - Experiment
Abstract: Observation of J/? production by neutrinos in the calorimeter of the CHORUS detector exposed to the CERN SPS wide-band ?µ beam is reported. A spectrum-averaged cross section ?J/? = (6.3 ± 3.0) × 10-41 cm2 is obtained for 20 GeV ? E? ? 200 GeV. The data are compared with the theoretical model based on the QCD Z-gluon fusion mechanism. © 2001 Published by Elsevier Science B.V. Foundation for Fundamental Research on Matter Promotion and Mutual Aid Corporation for Private Schools of Japan Bundesministerium für Bildung und Forschung: 057MS12P Brussels Instituut voor Milieubeheer CERN Israel Science Foundation: 328/94 Instituto Nazionale di Fisica Nucleare Nederlandse Organisatie voor Wetenschappelijk Onderzoek National Council for Scientific Research Korean Foundation for Cancer Research: KRF-99-005-D00004 Stichting voor Fundamenteel Onderzoek der Materie We would like to thank A. Kaidalov, S. Kruchinin and V. Lemaitre for fruitful discussions. We gratefully acknowledge the help and support of our numerous technical collaborators who contributed to the detector construction and operation. We thank the neutrino beam staff for their competent assistance, ensuring the excellent performance of the facility. The accumulation of a large data sample in this experiment was also made possible thanks to the efforts of the crew operating the CERN PS and SPS. The general technical support from EP, ECP and IT Divisions is gratefully acknowledged. We thank S. Anthony for help in preparation of the text. The experiment has been made possible by grants from our funding agencies: the Institut Interuniversitaire des Sciences Nucléaires and the Interuniversitair Instituut voor Kernwetenschappen (Belgium); the Israel Science Foundation (Grant 328/94) and the Technion Vice President Fund for the Promotion of Research (Israel); CERN (Geneva, Switzerland); the German Bundesministerium für Bildung und Forschung (Grant 057MS12P(0)) (Germany); the Institute of Theoretical and Experimental Physics (Moscow, Russia); the Istituto Nazionale di Fisica Nucleare (Italy); the Promotion and Mutual Aid Corporation for Private Schools of Japan and Japan Society for the Promotion of Science (Japan); the Korea Research Foundation (Grant KRF-99-005-D00004) (Republic of Korea); the Foundation for Fundamental Research on Matter (FOM) and the National Scientific Research Organization (NWO) (The Netherlands); and the Scientific and Technical Research Council of Turkey (Turkey).

41. Emulsion Cloud Chamber technique to measure the fragmentation of a high-energy carbon beam

Author: Naotaka Naganawa, A. Russo, C. Pistillo, Yoshiya Furusawa, P. Migliozzi, G. De Lellis, T. Toshito, Yu.P. Petukhov, F. Di Capua, Salvatore Buontempo, L. Scotto Lavina, P. Strolin, Akitaka Ariga, Nakahiro Yasuda, V. Tioukov, and A. Marotta
Subjects: Materials science, Physics - Instrumentation and Detectors, Hydrogen, Detector, FOS: Physical sciences, chemistry.chemical_element, Instrumentation and Detectors (physics.ins-det), Molecular physics, Physics - Medical Physics, law.invention, chemistry, law, Emulsion, Nuclear emulsion, Medical Physics (physics.med-ph), Cloud chamber, Nucleon, Boron, Nuclear Experiment, Instrumentation, Mathematical Physics, Helium
Abstract: Beams of Carbon nuclei are used or planned to be used in various centers for cancer treatment around the world because of their therapeutic advantages over proton beams. The knowledge of the fragmentation of Carbon nuclei when they interact with the human body is important to evaluate the spatial profile of their energy deposition in the tissues, hence the damage to the tissues neighboring the tumor. In this respect, the identification of the fragmentation products is a key element. We present in this paper the charge measurement of about 3000 fragments produced by the interaction of $^{12}$C nuclei with an energy of 400 MeV/nucleon in a detector simulating the density of the human body. The nuclear emulsion technique is used, by means of the so-called Emulsion Cloud Chamber. In order to achieve the large dynamical range required for the charge measurement, the recently developed techniques of the emulsion controlled fading are used. The nuclear emulsions are inspected using fast automated microscopes recently developed. A charge assignment efficiency of more than 99% is achieved. The separation of Hydrogen, Helium, Lithium, Berillium, Boron and Carbon can be achieved at two standard deviations or considerably more, according to the track length available for the measurement., 15 pages, 8 figures

42. Progress in Geant4 Electromagnetic Physics Modelling and Validation.

Author: J Apostolakis, M Asai, A Bagulya, J M C Brown, H Burkhardt, N Chikuma, M A Cortes-Giraldo, S Elles, V Grichine, S Guatelli, S Incerti, V N Ivanchenko, J Jacquemier, O Kadri, M Maire, L Pandola, D Sawkey, T Toshito, L Urban, and T Yamashita
Published: 2015
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43. Measurement of charm production in antineutrino charged-current interactions

Author: Onengüt, G, Van Dantzig, R, De Jong, M, Konijn, J, Melzer, O, Oldeman, R G C, Pesen, E, Van der Poel, C A F J, Visschers, J L, Güler, M, Köse, U, Serin-Zeyrek, M, Kama, S, Sever, R, Tolun, P, Zeyrek, M T, Catanesi, M G, De Serio, M, Ieva, M, Muciaccia, M T, Radicioni, E, Simone, S, Bülte, A, Winter, Klaus, Van de Vyver, B, Vilain, P, Wilquet, G, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Artamonov, A V, Brunner, J, Chizhov, M, Cussans, D G, Doucet, M, Fabre, Jean-Paul, Hristova, I R, Kawamura, T, Kolev, D, Litmaath, M, Meinhard, H, Panman, J, Papadopoulos, I M, Ricciardi, S, Rozanov, A, Saltzberg, D, Tsenov, R V, Uiterwijk, J W E, Zucchelli, P, Goldberg, J, Chikawa, M, Arik, E, Song, J S, Yoon, C S, Kodama, K, Ushida, N, Aoki, S, Hara, T, Delbar, T, Favart, D, Grégoire, G, Kalinin, S, Makhlyoueva, I V, Gorbunov, P, Khovanskii, V D, Shamanov, V V, Tsukerman, I, Bruski, N, Frekers, D, Rondeshagen, D, Wolff, T, Hoshino, K, Kawada, J, Komatsu, M, Miyanishi, M, Nakamura, M, Nakano, T, Narita, K, Niu, K, Niwa, K, Nonaka, N, Sato, O, Toshito, T, Buontempo, S, Cocco, A G, D'Ambrosio, N, De Lellis, G, De Rosa, G, Di Capua, F, Ereditato, A, Fiorillo, G, Marotta, A, Messina, M, Migliozzi, P, Pistillo, C, Santorelli, R, Scotto-Lavina, L, Strolin, P, Tioukov, V, Nakamura, K, Okusawa, T, Dore, U, FLoverre, P, Ludovici, L, Maslennikov, A L, Righini, P, Rosa, G, Santacesaria, R, Satta, A, Spada, F R, Barbuto, E, Bozza, C, Grella, G, Romano, G, Sirignano, C, Sorrentino, S, Sato, Y, Tezuka, I, Other Research IHEF (IoP, FNWI), UCL - SC/PHYS - Département de physique, Çukurova Üniversitesi, Önengüt, G., van Dantzig, R., de Jong, M., Melzer, O., Oldeman, R. G. C., Pesen, E., Visschers, J. L., Güler, M., Köse, U., Serin Zeyrek, M., Sever, R., Tolun, P., Zeyrek, M. T., Catanesi, M. G., De Serio, M., Ieva, M., Muciaccia, M. T., Radicioni, E., Simone, S., Bülte, A., Winter, K., Van de Vyver, B., Vilain, P., Wilquet, G., Saitta, B., Di Capua, E., Ogawa, S., Shibuya, H., Artamonov, A., Chizhov, M., Doucet, M., Hristova, I. R., Kayis Topaksu, A., Kawamura, T., Kolev, D., Meinhard, H., Panman, J., Papadopoulos, I. M., Ricciardi, S., Rozanov, A., Tsenov, R., Uiterwijk, J. W. E., Zucchelli, P., Goldberg, J., Chikawa, M., Arik, E., Song, J. S., Yoon, C. S., Kodama, K., Ushida, N., Aoki, S., Hara, T., Delbar, T., Favart, D., Grégoire, G., Kalinin, S., Makhlioueva, I., Gorbunov, P., Khovansky, V., Shamanov, V., Tsukerman, I., Bruski, N., Frekers, D., Hoshino, K., Kawada, J., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Narita, K., Niu, K., Niwa, K., Nonaka, N., Sato, O., Toshito, T., Buontempo, S., Cocco, A. G., D'Ambrosio, N., De Lellis, G., De Rosa, G., DI CAPUA, Francesco, Ereditato, A., Fiorillo, Giuliana, Marotta, A., Messina, M., Migliozzi, P., Pistillo, C., Scotto Lavina, L., Strolin, P., Tioukov, V., Nakamura, K., Okusawa, T., Dore, U., Loverre, P. F., Ludovici, L., Righini, P., Rosa, G., Santacesaria, R., Satta, A., Spada, F. R., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sirignano, C., Sorrentino, S., Sato, Y., Tezuka, I., G., Onengut, R. v., Dantzig, M. d., Jong, O., Melzer, R. G., C., E., Pesen, J. L., Visscher, M., Guler, U., Kose, M., Serin Zeyrek, R., Sever, P., Tolun, M. T., Zeyrek, M. G., Catanesi, M. D., Serio, M., Ieva, M. T., Muciaccia, E., Radicioni, S., Simone, A., Bulte, K., Winter, B. V., De, P., Vilain, G., Wilquet, B., Saitta, E. D., Capua, S., Ogawa, H., Shibuya, A., Artamonov, M., Chizhov, M., Doucet, I. R., Hristova, A., Kayis Topaksu, T., Kawamura, D., Kolev, H., Meinhard, J., Panman, I. M., Papadopoulo, S., Ricciardi, A., Rozanov, R., Tsenov, J. W., E., P., Zucchelli, J., Goldberg, M., Chikawa, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, T., Delbar, D., Favart, G., Gregoire, S., Kalinin, I., Makhlioueva, P., Gorbunov, V., Khovansky, V., Shamanov, I., Tsukerman, N., Bruski, D., Freker, K., Hoshino, J., Kawada, M., Komatsu, M., Miyanishi, M., Nakamura, T., Nakano, K., Narita, K., Niu, K., Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, A., Ereditato, A., Marotta, M., Messina, P., Migliozzi, C., Pistillo, L. S., Lavina, P., Strolin, V., Tioukov, K., Nakamura, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, P., Righini, G., Rosa, R., Santacesaria, A., Satta, F. R., Spada, E., Barbuto, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, and I., Tezuka
Subjects: Physics, NEUTRINO INTERACTIONS, CHORUS EXPERIMENT, Nuclear and High Energy Physics, Particle physics, Muon, Large Hadron Collider, Physics::Instrumentation and Detectors, High Energy Physics::Phenomenology, Charge (physics), BEAMS, EVENTS, Nuclear physics, OPPOSITE-SIGN DIMUONS, High Energy Physics::Experiment, Production (computer science), Charm (quantum number), Neutrino, Nuclear Experiment, Particle Physics - Experiment, Charged current, Beam (structure)
Abstract: During the years 1994-1997, the emulsion target of the CHORUS detector was exposed to the wide-band neutrino beam of the CERN SPS collecting about 10 6 neutrino interactions. A measurement of ?¯µ-induced charm production is performed by using the presence of a 5% ?¯µ component in the ?µ beam. The measurement takes advantage of the capability to observe the decay topology in the emulsion. The analysis is based on a sample of charged-current interactions with at least one identified muon. About 100000 were located in the emulsion target and fully reconstructed. By requiring a positive muon charge as determined by the CHORUS muon spectrometer, 32?¯µ-induced charm events were observed with an estimated background of 3.2 events. At an average antineutrino energy in the neutrino beam of 18 GeV, the charm production rate induced by antineutrinos is measured to be ?(?¯µN›µ+c¯X)/?(?¯µN›µ+X) =(5.0-0.9+1.4(stat)±0.7(syst))%. The ratio between neutral and charged charm production rates in this process is (2.6-1.0+1.7(stat)±0.8(syst)). The charm production rate as a function of the antineutrino energy is found to be in good agreement with previous results derived from di-lepton data. © 2004 Elsevier B.V. All rights reserved. Bundesministerium für Bildung und Forschung Promotion and Mutual Aid Corporation for Private Schools of Japan Grant Foundation: KRF-2003-005-C00014 Israel Science Foundation: 328/94 CERN Brussels Instituut voor Milieubeheer Instituto Nazionale di Fisica Nucleare Foundation for Fundamental Research on Matter Korean Foundation for Cancer Research We gratefully acknowledge the help and support of the neutrino-beam staff and of the numerous technical collaborators who contributed to the detector construction, operation, emulsion pouring, development, and scanning. The experiment was made possible by grants from the Institut Interuniversitaire des Sciences Nucléaires and the Interuniversitair Instituut voor Kernwetenschappen (Belgium); the Israel Science Foundation (Grant 328/94) and the Technion Vice President Fund for the Promotion of Research (Israel); CERN (Geneva, Switzerland); the German Bundesministerium für Bildung und Forschung (Germany); the Institute of Theoretical and Experimental Physics (Moscow, Russia); the Istituto Nazionale di Fisica Nucleare (Italy); the Promotion and Mutual Aid Corporation for Private Schools of Japan and Japan Society for the Promotion of Science (Japan); Korea Research Foundation Grant (KRF-2003-005-C00014) (Republic of Korea); the Foundation for Fundamental Research on Matter FOM and the National Scientific Research Organization NWO (The Netherlands); and the Scientific, and Technical Research Council of Turkey (Turkey). We gratefully acknowledge their support.
Published: 2004

44. Measurement of charm production in neutrino charged-current interactions

Author: Kayis Topaksu, A., Onengut, G., Dantzig, R. V., Jong, M. D., Van Dantzig, R., De Jong, M., Oldeman, P. G. C., Oldeman, R. G. C., Guler, M., Kose, U., Tolun, P., Catanesi, M. G., Muciaccia, M. T., Winter, K., B. V., De, Van De Vyver, B., Vilain, P., Wilquet, G., Saitta, B., Capua, E. D., Di Capua, E., Ogawa, S., Shibuya, H., Hristova, I. R., Kawamura, T., Kolev, D., Meinhard, H., Panman, J., Rozanov, A., Tsenov, R., Uiterwijk, J. W. E., Zucchelli, P., Goldbergll, Goldberg, J., Chikawa, M., Song, J. S., Yoon, C. S., Kodama, K., Ushida, N., Aoki, S., Hara, T., Delbar, T., Favart, D., Gregoire, G., Kalinin, S., Makhlioueva, I., Artamonov, A., Gorbunov, P., Khovansky, V., Shamanov, V., Tsukerman, I., Bruski, N., Frekers, D., Hoshino, K., Kawada, J., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Narita, K., Niu, K., Niwa, K., Nonaka, N., Sato, O., Toshito, T., Buontempo, S., Cocco, A. G., D'Ambrosio, N., Lellis, G. D., De Lellis, G., De Rosa, G., Di Capua, F., Fiorillo, G., Marotta, A., Messina, M., Migliozzi, P., Lavina, L. S., Scotto Lavina, L., Strolin, P., Tioukov, V., Okusawa, T., Dore, U., Loverre, Pier Ferruccio, Ludovici, L., Rosa, Giovanni, Capua, F. D., Dore, Ubaldo, Loverre, P. F., Rosa, G., Santacesaria, R., Satta, A., Spada, F. R., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sirignano, C., Sorrentino, S., Sato, Y., Tezuka, I., Çukurova Üniversitesi, A., Kayis Topaksu, G., Önengüt, R., van Dantzig, M., de Jong, R. G. C., Oldeman, M., Güler, U., Köse, P., Tolun, M. G., Catanesi, M. T., Muciaccia, K., Winter, B., Van de Vyver, P., Vilain, G., Wilquet, B., Saitta, E., Di Capua, S., Ogawa, H., Shibuya, I. R., Hristova, T., Kawamura, D., Kolev, H., Meinhard, J., Panman, A., Rozanov, R., Tsenov, J. W. E., Uiterwijk, P., Zucchelli, J., Goldberg, M., Chikawa, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, T., Delbar, D., Favart, G., Grégoire, S., Kalinin, I., Makhlioueva, A., Artamonov, P., Gorbunov, V., Khovansky, V., Shamanov, I., Tsukerman, N., Bruski, D., Freker, K., Hoshino, J., Kawada, M., Komatsu, M., Miyanishi, M., Nakamura, T., Nakano, K., Narita, K., Niu, K., Niwa, N., Nonaka, O., Sato, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, DI CAPUA, Francesco, Fiorillo, Giuliana, A., Marotta, M., Messina, P., Migliozzi, L., Scotto Lavina, Strolin, PAOLO EMILIO, V., Tioukov, T., Okusawa, U., Dore, P. F., Loverre, L., Ludovici, G., Rosa, R., Santacesaria, A., Satta, F. R., Spada, E., Barbuto, C., Bozza, G., Grella, G., Romano, C., Sirignano, S., Sorrentino, Y., Sato, and I., Tezuka
Subjects: Physics, Particle physics, Muon, Large Hadron Collider, Physics::Instrumentation and Detectors, Hadron, High Energy Physics::Phenomenology, General Physics and Astronomy, FOS: Physical sciences, Hadronization, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Nuclear emulsion, High Energy Physics::Experiment, Charm (quantum number), Neutrino, Nuclear Experiment, Charged current, Particle Physics - Experiment
Abstract: The nuclear emulsion target of the CHORUS detector was exposed to the wide-band neutrino beam of the CERN SPS of 27 GeV average neutrino energy from 1994 to 1997. In total about 100000 charged-current neutrino interactions with at least one identified muon were located in the emulsion target and fully reconstructed, using newly developed automated scanning systems. Charmed particles were searched for by a program recognizing particle decays. The observation of the decay in nuclear emulsion makes it possible to select a sample with very low background and minimal kinematical bias. 2013 charged-current interactions with a charmed hadron candidate in the final state were selected and confirmed through visual inspection. The charm production rate induced by neutrinos relative to the charged-current cross-section is measured to be sigma(nu_mu N -> mu- C X)/sigma(CC) = (5.75 +-0.32 stat +-0.30 syst)%. The charm production cross-section as a function of the neutrino energy is also obtained. The results are in good agreement with previous measurements. The charm-quark hadronization produces the following charmed hadrons with relative fractions (in %): f_Dzero = 43.7+-4.5, f_Lambda_c^plus = 19.2+-4.2, f_Dplus = 25.3+-4.2, and f_D_splus = 11.8+-4.7., 16 pages, 5 figures
Published: 2011

45. A survey of practice patterns for adaptive particle therapy for interfractional changes.

Author: Trnkova P, Zhang Y, Toshito T, Heijmen B, Richter C, Aznar MC, Albertini F, Bolsi A, Daartz J, Knopf AC, and Bertholet J
Abstract: Background and Purpose: Anatomical changes may compromise the planned target coverage and organs-at-risk dose in particle therapy. This study reports on the practice patterns for adaptive particle therapy (APT) to evaluate current clinical practice and wishes and barriers to further implementation., Materials and Methods: An institutional questionnaire was distributed to PT centres worldwide (7/2020-6/2021) asking which type of APT was used, details of the workflow, and what the wishes and barriers to implementation were. Seventy centres from 17 countries participated. A three-round Delphi consensus analysis (10/2022) among the authors followed to define recommendations on required actions and future vision., Results: Out of the 68 clinically operational centres, 84% were users of APT for at least one treatment site with head and neck being most common. APT was mostly performed offline with only two online APT users (plan-library). No centre used online daily re-planning. Daily 3D imaging was used for APT by 19% of users. Sixty-eight percent of users had plans to increase their use or change their technique for APT. The main barrier was "lack of integrated and efficient workflows". Automation and speed, reliable dose deformation for dose accumulation and higher quality of in-room volumetric imaging were identified as the most urgent task for clinical implementation of online daily APT., Conclusion: Offline APT was implemented by the majority of PT centres. Joint efforts between industry research and clinics are needed to translate innovations into efficient and clinically feasible workflows for broad-scale implementation of online APT., Competing Interests: The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper., (© 2023 The Authors.)
Published: 2023
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46. A survey of practice patterns for real-time intrafractional motion-management in particle therapy.

Author: Zhang Y, Trnkova P, Toshito T, Heijmen B, Richter C, Aznar M, Albertini F, Bolsi A, Daartz J, Bertholet J, and Knopf A
Abstract: Background and Purpose: Organ motion compromises accurate particle therapy delivery. This study reports on the practice patterns for real-time intrafractional motion-management in particle therapy to evaluate current clinical practice and wishes and barriers to implementation., Materials and Methods: An institutional questionnaire was distributed to particle therapy centres worldwide (7/2020-6/2021) asking which type(s) of real-time respiratory motion management (RRMM) methods were used, for which treatment sites, and what were the wishes and barriers to implementation. This was followed by a three-round DELPHI consensus analysis (10/2022) to define recommendations on required actions and future vision. With 70 responses from 17 countries, response rate was 100% for Europe (23/23 centres), 96% for Japan (22/23) and 53% for USA (20/38)., Results: Of the 68 clinically operational centres, 85% used RRMM, with 41% using both rescanning and active methods. Sixty-four percent used active-RRMM for at least one treatment site, mostly with gating guided by an external marker. Forty-eight percent of active-RRMM users wished to expand or change their RRMM technique. The main barriers were technical limitations and limited resources. From the DELPHI analysis, optimisation of rescanning parameters, improvement of motion models, and pre-treatment 4D evaluation were unanimously considered clinically important future focus. 4D dose calculation was identified as the top requirement for future commercial treatment planning software., Conclusion: A majority of particle therapy centres have implemented RRMM. Still, further development and clinical integration were desired by most centres. Joint industry, clinical and research efforts are needed to translate innovation into efficient workflows for broad-scale implementation., Competing Interests: The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper., (© 2023 The Authors.)
Published: 2023
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47. Outcomes of proton therapy for non-small cell lung cancer in patients with interstitial pneumonia.

Author: Hashimoto S, Iwata H, Hattori Y, Nakajima K, Nomura K, Hayashi K, Toshito T, Yamamori E, Akita K, Mizoe JE, Ogino H, and Shibamoto Y
Subjects: Aged, Aged, 80 and over, Carcinoma, Non-Small-Cell Lung pathology, Female, Humans, Lung Neoplasms pathology, Male, Neoplasm Staging, Retrospective Studies, Carcinoma, Non-Small-Cell Lung radiotherapy, Lung Diseases, Interstitial complications, Lung Neoplasms radiotherapy, Proton Therapy
Abstract: Background: Interstitial pneumonia (IP) is a disease with a poor prognosis. In addition, IP patients are more likely to develop lung cancer. Since IP patients frequently develop toxicities during cancer treatment, minimally invasive cancer treatment is warranted for such patients to maintain their quality of life. This study retrospectively investigated the efficacy and safety of proton therapy (PT) for non-small cell lung cancer (NSCLC) in patients with IP., Methods: Twenty-nine NSCLC patients with IP were treated with PT between September 2013 and December 2019. The patients had stage IA to IIIB primary NSCLC. Ten of the 29 patients exhibited the usual interstitial pneumonia pattern. The prescribed dose was 66-74 Grays (relative biological effectiveness) in 10-37 fractions., Results: The median follow-up period was 21.1 months [interquartile range (IQR), 15.6-37.3] for all patients and 37.2 months (IQR, 24.0-49.9) for living patients. The median patient age was 77 years (IQR, 71-81). The median planning target volume was 112.0 ml (IQR, 56.1-246.3). The 2-year local control, progression-free survival, and overall survival rates were 85% (95% confidence interval: 57-95), 30% (15-47), and 45% (26-62), respectively. According to the Common Terminology Criteria for Adverse Events (version 4.0), grade 3 acute radiation pneumonitis (RP) was observed in 1 patient. Two patients developed grade 3 late RP, but no other patients experienced serious toxicities. The patients' quality of life (European Organization for Research and Treatment of Cancer QLQ-C30 and QLQ-LC13 and SF-36) scores had not changed after 3 months., Conclusions: PT may be a relatively safe treatment for NSCLC patients with IP, without deteriorating quality of life scores within 3 months., (© 2022. The Author(s).)
Published: 2022
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48. Patient-Reported Quality of Life Outcomes after Moderately Hypofractionated and Normofractionated Proton Therapy for Localized Prostate Cancer.

Author: Nakajima K, Iwata H, Hattori Y, Nomura K, Hayashi K, Toshito T, Umemoto Y, Hashimoto S, Ogino H, and Shibamoto Y
Abstract: We retrospectively evaluated the three-year patient-reported quality of life (QOL) after moderately hypofractionated proton therapy (MHPT) for localized prostate cancer in comparison with that after normofractionated PT (NFPT) using the Expanded Prostate Cancer Index Composite-50. Patients who received MHPT (60-63 Gy (relative biological effectiveness equivalents; RBE)/20-21 fractions) ( n = 343) or NFPT (74-78 Gy (RBE)/37-39 fractions) ( n = 296) between 2013 and 2016 were analyzed. The minimum clinically important difference (MCID) threshold was defined as one-half of a standard deviation of the baseline value. The median follow-up was 56 months and 83% completed questionnaires at 36 months. Clinically meaningful score deterioration was observed in the urinary domain at 1 month in both groups and in the sexual domain at 6-36 months in the NFPT group, but not observed in the bowel domain. At 36 months, the mean score change for urinary summary was -0.3 (MHPT) and -1.6 points (NFPT), and that for bowel summary was +0.1 and -2.0 points; the proportion of patients with MCID was 21% and 24% for urinary summary and 18% and 29% for bowel summary. Overall, MHPT had small negative impacts on QOL over three years, and the QOL after MHPT and NFPT was similar.
Published: 2022
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49. Spot Scanning Proton Therapy for Sinonasal Malignant Tumors.

Author: Nakajima K, Iwata H, Hattori Y, Nomura K, Hashimoto S, Toshito T, Hayashi K, Kuroda Y, Fukano H, Ogino H, and Shibamoto Y
Abstract: Purpose: Treatment of sinonasal malignant tumors is challenging, and evidence to establish a standard treatment is limited. Our objective was to evaluate the efficacy and safety of spot scanning proton therapy (SSPT) for sinonasal malignant tumors., Patients and Methods: We retrospectively analyzed patients with sinonasal malignant tumors (T1-4bN0-2M0) who underwent SSPT between May 2014 and September 2019. The prescription dose was typically either 60 GyRBE in 15 fractions or 60.8 GyRBE in 16 fractions for mucosal melanoma and 70.2 GyRBE in 26 fractions for other histologic subtypes. Endpoints included local control (LC), progression-free survival, overall survival (OS), and incidence of toxicity. Prognostic factors were analyzed using the Kaplan-Meier method and log-rank test., Results: Of 62 enrolled patients, the common histologic subtypes were mucosal melanoma (35%), squamous cell carcinoma (27%), adenoid cystic carcinoma (16%), and olfactory neuroblastoma (10%). Locally advanced stages were common (T3 in 42% and T4 in 53%). Treatment-naïve tumors and postsurgical recurrent tumors accounted for 73% and 27%, respectively. No patient had previous radiotherapy. The median follow-up was 17 months (range, 6-66) for all patients and 21.5 months (range, 6-66) for survivors. The 2-year LC, progression-free survival, and OS rates of all patients were 92%, 50%, and 76%, respectively. Univariate analysis revealed histology as a prognostic factor for OS, being higher in adenoid cystic carcinoma and olfactory neuroblastoma than in other tumors. Sixteen grade ≥3 late toxicities were observed in 12 patients (19%), including 11 events resulting in visual impairment; the most common was cataract. There was 1 grade 4 toxicity, and there were no grade 5 toxicities., Conclusion: SSPT was well tolerated and yielded good LC for sinonasal malignant tumors. Although we consider SSPT to be a leading treatment modality, further studies are required to establish its status as a standard treatment., Competing Interests: Conflicts of Interest: The authors have no relevant conflicts of interest to disclose., (©Copyright 2021 The Author(s).)
Published: 2021
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50. Changes in sexual function and serum testosterone levels in patients with prostate cancer after image-guided proton therapy.

Author: Hattori Y, Iwata H, Nakajima K, Nomura K, Hayashi K, Toshito T, Hashimoto S, Umemoto Y, Mizoe JE, Ogino H, and Shibamoto Y
Subjects: Aged, Aged, 80 and over, Humans, Male, Middle Aged, Penile Erection physiology, Prostate-Specific Antigen blood, Prostatic Neoplasms radiotherapy, Risk Factors, Prostatic Neoplasms blood, Prostatic Neoplasms physiopathology, Proton Therapy, Radiotherapy, Image-Guided, Testosterone blood
Abstract: Since sexual function and testosterone levels after image-guided proton therapy (IGPT) have not yet been examined in detail, we prospectively evaluated changes before and after IGPT. Among patients treated with IGPT with or without combined androgen blockade (CAB) therapy between February 2013 and September 2014, patients who agreed to participate in the study and were followed up for >3 years after IGPT were evaluated. Serum testosterone levels were regularly measured together with prostate-specific antigen (PSA) levels before and after IGPT. The Erection Hardness Score (EHS) and the sexual domain summary, function subscale and bother subscale of the sexual domain in the Expanded Prostate Cancer Index Composite (EPIC) were assessed. There were 38 low-risk, 46 intermediate-risk and 43 high- or very-high-risk patients (NCCN classification). Although serum testosterone levels in low-risk patients did not decrease after IGPT, reductions were observed in the average EHS and the sexual domain summary score of the EPIC. In intermediate-, high- and very-high-risk patients, testosterone and PSA levels both increased following the termination of CAB after IGPT, and the average EHS increased. The sexual domain summary score gradually increased, but not above minimally important differences. In intermediate-risk patients, the function subscale increased from 4.4 to 14.8 (P < 0.05) 12 months after IGPT and reached a plateau after 60 months. The results of the present study would suggest the potential of IGPT, and further prospective studies to directly compare IGPT with other modalities are warranted., (© The Author(s) 2021. Published by Oxford University Press on behalf of The Japanese Radiation Research Society and Japanese Society for Radiation Oncology.)
Published: 2021
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