116 results on '"T. Toshito"'
Search Results
2. Final results on oscillation from the CHORUS experiment
- Author
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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
3. Low-velocity ion tracks in fine grain emulsion
- Author
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Kimio Niwa, M. Natsume, Toshiyuki Nakano, K. Hoshino, M. Nakamura, T. Toshito, T. Tani, Osamu Sato, and K. Kuwabara
- Subjects
Physics ,Nuclear and High Energy Physics ,Range (particle radiation) ,Number density ,Scanning electron microscope ,Ion track ,Emulsion ,Nuclear emulsion ,Atomic physics ,Nuclear Experiment ,Tracking (particle physics) ,Instrumentation ,Ion - Abstract
We have studied low-velocity Kr ion responses of nuclear emulsions for the possibility of tracking Ag and Br recoils from galactic dark matter particles. Tracks of 680–1180 km/s Kr ions have been observed in a 40 nm-sized AgBr grain emulsion with scanning electron microscopy. The tracks have a linear energy-dependency in range, angles biased along the incident direction, and a high developed-grain number density with respect to expected electronic stopping. We find that the fine grain emulsion is sensitive enough to low-velocity heavy ions whose energy losses are mainly governed by nuclear stopping.
- Published
- 2007
4. Measurement of the Z/A dependence of neutrino charged-current total cross-sections
- Author
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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
5. Charge identification of highly ionizing particles in desensitized nuclear emulsion using high speed read-out system
- Author
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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
6. Measurement of neutrino oscillation by the K2K experiment
- Author
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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
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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
7. Measurements of D0 production and of decay branching fractions in neutrino–nucleon scattering
- Author
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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 .
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- 2005
8. Measurement of D*+ production in charged-current neutrino interactions
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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
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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
9. π/p separation at by an emulsion cloud chamber
- Author
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M. Nakamura, Naotaka Naganawa, Akitaka Ariga, Masahiro Komatsu, T. Toshito, Taku Nakamura, Toshiyuki Nakano, T. Ban, K. Hoshino, and K. Niwa
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Physics ,Nuclear and High Energy Physics ,Detector ,Separation (aeronautics) ,Proton Synchrotron ,Particle identification ,law.invention ,Momentum ,Nuclear physics ,law ,Emulsion ,Cloud chamber ,Instrumentation ,Beam (structure) - Abstract
We have performed an experimental study of π/p separation at a momentum of 1.2 GeV / c using an Emulsion Cloud Chamber (ECC) detector with secondary beam produced by the proton synchrotron at KEK. The separation is greater than 3 standard deviations using dE/dx measurements of 2.6 mm long tracks with an automatic emulsion read-out system.
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- 2004
10. Identification of neutrino interactions using the DONUT spectrometer
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V. Paolone, Mitsuhiro Nakamura, Masahiro Komatsu, T. Toshito, J. S. Song, B. Baller, Koichi Kodama, T. Kafka, N. Nonaka, G. Tzanakos, B. Lundberg, S. Yoshida, Roger Rusack, D. J. Boehnlein, K. Narita, R. A. Rameika, Osamu Sato, T. Hara, M. A. Kubantsev, N. R. Stanton, Takayoshi Kawai, Niki Saoulidou, M. Skender, C. Erickson, D. P. Ciampa, S. H. Chung, K. Okada, N. Giokaris, W. P. Oliver, C. Rosenfeld, H. Matsuoka, J. Kawada, J. Trammell, C. Andreopoulos, P. Berghaus, Reinhard Schwienhorst, C. S. Yoon, R. A. Sidwell, Shigeki Aoki, Ken Heller, H. Jiko, T. Akdogan, Toshiyuki Nakano, M. Miyanishi, Matt W. Graham, N. W. Reay, J. Sielaff, A. Kulik, J. Wilcox, K. Hoshino, J. Schneps, and K. Niwa
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Physics ,Nuclear and High Energy Physics ,Scintillation ,Particle physics ,Muon ,Spectrometer ,Physics::Instrumentation and Detectors ,High Energy Physics::Phenomenology ,Detector ,Nuclear physics ,Tau neutrino ,High Energy Physics::Experiment ,Nuclear emulsion ,Neutrino ,Instrumentation ,Lepton - Abstract
The experimental apparatus used for the first direct observation of the tau neutrino (the DONUT experiment) is described. Its main features consisted of a target system composed of nuclear emulsion targets and scintillation fiber trackers, a magnetic charged-particle spectrometer and detectors for lepton identification. This paper will concentrate on the description of the electronic detectors and their performance in selecting neutrino interactions, making the vertex predictions necessary for locating events in the emulsion target and lepton identification.
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- 2004
11. The Super-Kamiokande detector
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Kimihiro Okumura, Makoto Sakuda, B. K. Kim, S. Fukuda, K. Martens, S. Moriyama, Toshio Suzuki, Todd Haines, S. B. Boyd, M. L. Chen, T. Hasegawa, Z. Conner, M. Kitaguchi, K. Nishikawa, K. S. Ganezer, Alec Habig, M. Earl, B. Viren, J. Kameda, M. Koga, H. Okazawa, R. W. Ellsworth, A. Okada, M. Takahashi, J. S. George, K. Ishihara, Atsumu Suzuki, T. Inagaki, Shoichi Yamada, Takaaki Kajita, S. Matsuno, T. Iwashita, K. Fujita, H. G. Berns, M. Ishitsuka, S. Desai, Koji Nakamura, M. Miura, Y. Ichikawa, Mikio Morii, E. Guillian, C. K. Jung, M. Takahata, H. Nishihama, J. Hsu, K. Ito, Toshio Namba, D. Kielczewska, T. Ishii, Kunio Inoue, S. Nakayama, John G. Learned, I. Kato, M. Etoh, I. Nishiyama, T. Futagami, A. L. Stachyra, K. Miyano, C. Saji, Y. Hatakeyama, T. Hayakawa, H. Maesaka, R. A. Doyle, Florian Goebel, M. B. Smy, J. L. Stone, D. W. Liu, David William Casper, E. Ichihara, T. Hashimoto, A. K. Ichikawa, C. Yanagisawa, K. Nishijima, S. Hatakeyama, M. Kohama, Akira Hasegawa, G. W. Sullivan, Henry W. Sobel, K. Nitta, Y. Kobayashi, A. Sakai, M. Takita, M. Ackerman, Frederick Reines, L. R. Price, J. Shirai, W. Wang, T. Horiuchi, H. Takeda, V. J. Stenger, M. Masuzawa, E. Sharkey, Minoru Yoshida, Yoshitaka Itow, D. Turcan, S. Inaba, N. Sakurai, T. Takayama, Y. Kanaya, M. Kirisawa, R. Svoboda, M. Koike, J. Hill, Shuji Yamamoto, A. Kusano, K. Higuchi, Hiroaki Nishimura, Masaya Hasegawa, Y. Watanabe, K. Kaneyuki, T. Kobayashi, R. Sanford, Osamu Sasaki, Magdalena Malek, Y. Kajiyama, A. Kibayashi, L. R. Sulak, W. Doki, S. Tasaka, T. Toshito, W. E. Keig, Y. Nagashima, H. Fujiyasu, J. A. Goodman, J. T. Hong, Y. Takeuchi, F. Tsushima, C. W. Walter, Soo-Bong Kim, S. Kasuga, Y. Fukuda, E. Kearns, Y. Totsuka, M. Koshiba, Hyosun Kim, C. McGrew, Yoshihiro Suzuki, K. Kobayashi, M. Nemoto, D. Kerr, T. Maruyama, Takashi Yamaguchi, M. D. Messier, S. Echigo, T. Kato, C. Mitsuda, P. G. Halverson, R. J. Wilkes, U. Golebiewska, K. K. Young, S. Mine, Y. Obayashi, Y. Gando, E. Blaufuss, Junichi Kanzaki, C. Mauger, J. Yoo, Masato Shiozawa, T. Barszczak, T. Oyabu, A. Suzuki, Tsuyoshi Nakaya, Masayuki Nakahata, Hirokazu Ishino, L. Wai, M. Oketa, J. W. Flanagan, Hiroshi Ogawa, M. R. Vagins, H. Kobayashi, W. Gajewski, Kate Scholberg, W. R. Kropp, Y. Oyama, Y. Hayato, T. Iwamoto, and Yusuke Koshio
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Physics ,Nuclear and High Energy Physics ,Particle physics ,Physics::Instrumentation and Detectors ,Cherenkov detector ,Solar neutrino ,High Energy Physics::Phenomenology ,T2K experiment ,law.invention ,Neutrino detector ,law ,High Energy Physics::Experiment ,Neutrino astronomy ,Neutrino ,Super-Kamiokande ,Neutrino oscillation ,Instrumentation - Abstract
Super-Kamiokande is the world's largest water Cherenkov detector, with net mass 50,000 tons. During the period April, 1996 to July, 2001, Super-Kamiokande I collected 1678 live-days of data, observing neutrinos from the Sun, Earth's atmosphere, and the K2K long-baseline neutrino beam with high efficiency. These data provided crucial information for our current understanding of neutrino oscillations, as well as setting stringent limits on nucleon decay. In this paper, we describe the detector in detail, including its site, configuration, data acquisition equipment, online and offline software, and calibration systems which were used during Super-Kamiokande I.
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- 2003
12. Study of electron identification in a few GeV region by an emulsion cloud chamber
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M. Miyanishi, K. Narita, Toshiyuki Nakano, Mitsuhiro Nakamura, N. Nonaka, K. Niwa, T. Uetake, Masahiro Komatsu, T. Toshito, Takafumi Nakamura, Osamu Sato, Koichi Kodama, and K. Hoshino
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Physics ,Large Hadron Collider ,Physics::Instrumentation and Detectors ,Detector ,Proton Synchrotron ,Electron ,law.invention ,Nuclear physics ,Pion ,law ,Physics::Accelerator Physics ,High Energy Physics::Experiment ,Cloud chamber ,Nuclear Experiment ,Neutrino oscillation ,Instrumentation ,Cherenkov radiation - Abstract
We have performed an experimental study of electron identification using an emulsion cloud chamber detector with electron-enriched π− beams at 2 and 4 GeV/c produced by the proton synchrotron source at CERN. This study shows that the efficiency of electron identification is about 90% with little (6%) contamination from pions. These results are in agreement with those obtained using a Cherenkov counter and are reproduced well by the simulation.
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- 2003
13. Indications of Neutrino Oscillation in a 250 km Long-Baseline Experiment
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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
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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
14. Detection and analysis of tau–neutrino interactions in DONUT emulsion target
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J. Sielaff, Koichi Kodama, K. Hoshino, Mitsuhiro Nakamura, J. S. Song, C. Erickson, B. Lundberg, V. Paolone, C. S. Yoon, Reinhard Schwienhorst, K. Narita, Masahiro Komatsu, T. Toshito, T. Kafka, H. Matsuoka, Niki Saoulidou, Shigeki Aoki, T. Hara, Osamu Sato, Ken Heller, Takayoshi Kawai, K. Niwa, H. Jiko, B. Baller, N. Nonaka, J. Kawada, S. H. Chung, G. Tzanakos, K Okada, J. Trammell, R. A. Rameika, M. Miyanishi, and Toshiyuki Nakano
- Subjects
Physics ,Nuclear and High Energy Physics ,Particle physics ,Physics::Instrumentation and Detectors ,Nuclear physics ,Coulomb scattering ,Tau neutrino ,Emulsion ,Particle ,High Energy Physics::Experiment ,Nuclear emulsion ,Neutrino ,Instrumentation ,Charged current ,Analysis method - Abstract
The DONUT experiment used an emulsion/counter-hybrid-detector, which succeeded in detecting tau–neutrino charged-current interactions. A new method of emulsion analysis, NETSCAN, was used to locate neutrino events and detect tau decays. It is based on a fully automated emulsion readout system (Ultra Track Selector) developed at Nagoya University. The achieved plate-to-plate alignment accuracy of ∼0.2 μm over an area of 2.6 mm ×2.6 mm permitted an efficient and systematic tau decay search using emulsion data. Moreover, this accuracy allowed measurement of particle momenta by multiple Coulomb scattering, and contributed to the efficient background rejection for the ντ candidates. This paper describes details of our emulsion analysis methods.
- Published
- 2002
15. Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data
- Author
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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
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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
16. Detection of accelerator-produced neutrinos at a distance of 250 km
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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
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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
17. SolarB8and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data
- Author
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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
18. Constraints on Neutrino Oscillations Using 1258 Days of Super-Kamiokande Solar Neutrino Data
- Author
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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
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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
19. Leading order analysis of neutrino induced dimuon events in the CHORUS experiment
- Author
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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
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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
20. Tau Neutrinos Favored over Sterile Neutrinos in Atmospheric Muon Neutrino Oscillations
- Author
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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
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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
21. Charged-particle multiplicities in charged-current neutrino and anti-neutrino-nucleus interactions
- Author
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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
22. Associated charm production in neutrino-nucleus interactions
- Author
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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
23. Measurement of nucleon structure functions in neutrino scattering
- Author
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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
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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
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- 2006
24. First events from the CNGS neutrino beam detected in the OPERA experiment
- Author
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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
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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
25. Measurements of D-0 production and of decay branching fractions in neutrino-nucleon scattering
- Author
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T. Toshito, S. Buontempo, A. G. Cocco, N. D'Ambrosio, DE LELLIS, GIOVANNI, DE ROSA, GIANFRANCA, F. D. Capua, FIORILLO, GIULIANA, A. Marotta, M. Messina, P. Migliozzi, L. S. Lavina, M. Sorrentino, P. Strolin, V. Tioukov, T. Okusawa, U. Dore, R. 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, T., Toshito, S., Buontempo, A. G., Cocco, N., D'Ambrosio, DE LELLIS, Giovanni, DE ROSA, Gianfranca, F. D., Capua, Fiorillo, Giuliana, A., Marotta, M., Messina, P., Migliozzi, L. S., Lavina, M., Sorrentino, P., Strolin, V., Tioukov, T., Okusawa, U., Dore, R., 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
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CHARGED-CURRENT INTERACTIONS ,LEPTOPRODUCTION ,OPPOSITE-SIGN DIMUONS ,NOMAD EXPERIMENT ,LAMBDA-C+ ,PARTICLE-PRODUCTION ,HEAVY QUARKS ,CHARMED-BARYON PRODUCTION ,NU(MU) ,EMULSION - 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 Do 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 Do into four charged particles to two charged particles was measured to be B(D-0 &RARR; V4)/B(D-0 &RARR; V2) = 0.207 &PLUSMN; 0.016 &PLUSMN; 0.004. The inclusive measurement of the observed production rate of the Do with a decay into four charged prongs in combination with external measurements of this topological branching ratio was used to determine the total Do 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 &PLUSMN; 0.0018 &PLUSMN; 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 &PLUSMN; 0.049 &PLUSMN; 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) &PLUSMN; 0.2) x 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 &PLUSMN; 0.08) GeV/c(2). © 2005 Elsevier B.V. All rights reserved.
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- 2005
26. Search for νμ→ντ oscillation using the τ decay modes into a single charged particle
- Author
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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
27. 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
28. Experimental study of trimuon events in neutrino charged-current interactions
- Author
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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
29. Cross-section measurement for quasi-elastic production of charmed baryons in νN interactions
- Author
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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
30. 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.
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- 2003
31. Observation of one event with the characteristics of associated charm production in neutrino charged-current interactions
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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
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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
32. Measurement of D0 production in neutrino charged-current interactions
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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
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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
33. New results from a search for v(mu) -> v(tau) and v(e) -> v(tau) oscillation
- Author
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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. Visschers, M. Guler, M. Serin Zeyrek, R. Sever, P. Tolun, M. T. Zeyrek, N. Armenise, F. Cassol, M. G. Catanesi, M. D. Serio, M. T. Muciaccia, E. Radicioni, P. Righini, S. Simone, L. Vivolo, A. Bulte, K. Winter, P. Annis, R. El Aidi, M. V. Donckt, B. V. de, P. Vilain, G. Wilquet, B. Saitta, E. D. Capua, Y. Ishii, M. Kazuno, S. Ogawa, H. Shibuya, J. Brunner, M. Chizhou, D. Cussans, M. Doucet, J. P. Fabre, W. Flegel, M. Litmaath, H. Meinhard, E. Niu, H. Overas, J. Panman, I. M. Papdopoulos, 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, J. S. Song, C. S. Yoon, K. Kodama, N. Ushida, S. Aoki, T. Hara, G. Brooijmans, D. Favart, G. Gregoire, J. Herin, A. Artamonov, P. Gorbunov, V. Khovansky, V. Shamanov, I. Tsukerman, D. Bonekamper, N. D'Ambrosio, D. Frekers, 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. Lellis, F. D. Capua, A. Ereditato, T. Kawamura, R. Listone, M. Messina, P. Migliozzi, V. Tioukov, K. Nakamura, T. Okusawa, A. Capone, D. D. Pedis, 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, FIORILLO, GIULIANA, PALLADINO, VITTORIO, 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, M. D., Serio, M. T., Muciaccia, E., Radicioni, P., Righini, S., Simone, L., Vivolo, A., Bulte, K., Winter, P., Anni, R., El Aidi, M. V., Donckt, B. V., De, P., Vilain, G., Wilquet, B., Saitta, E. D., Capua, Y., Ishii, M., Kazuno, S., Ogawa, H., Shibuya, J., Brunner, M., Chizhou, D., Cussan, M., Doucet, J. P., Fabre, W., Flegel, M., Litmaath, H., Meinhard, E., Niu, H., Overa, J., Panman, I. M., Papdopoulo, 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, 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, T., Kawamura, 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, and I., Tezuka
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CHORUS EXPERIMENT ,LIMITS ,NU%28TAU%29+OSCILLATION%22">NU(MU)->NU(TAU) OSCILLATION ,SYSTEM - Abstract
A first analysis of the complete set of data collected by CHORUS in the years 1994-1997 is presented. The search for nu (tau) charged current events has been performed for both leptonic and hadronic decays of the tau lepton. No tau candidate has been found, A nu (tau) --> nu (tau) mixing is excluded down to sin(2)2 theta (mu tau) = 6.8 x 10(-4) for large Deltam(2) (90% C.L.). (C) 2001 Elsevier Science B.V. All rights reserved.
- Published
- 2001
34. Measurement of the fragmentation of Carbon nuclei used in hadron-therapy
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F. Di Capua, T. Toshito, A. Di Crescenzo, Yoshiya Furusawa, P. Migliozzi, G. De Lellis, P. Strolin, Marco Durante, Salvatore Buontempo, Akitaka Ariga, Yu.P. Petukhov, Naotaka Naganawa, A. Russo, V. Tioukov, C. Pistillo, Nakahiro Yasuda, DE LELLIS, Giovanni, Buontempo, S., DI CAPUA, Francesco, Di Crescenzo, A., Migliozzi, P., Petukhov, Y., Pistillo, C., Russo, A., Strolin, P., Tioukov, V., Durante, Marco, Furusawa, Y., Toshito, T., Yasuda, N., Ariga, A., and Naganawa, N.
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Physics ,Nuclear reaction ,Nuclear and High Energy Physics ,Fragmentation (mass spectrometry) ,Scattering ,Ionization ,Monte Carlo method ,Nuclear emulsion ,Multiplicity (chemistry) ,Atomic physics ,Electric charge - Abstract
The increasing use of Carbon nuclei in cancer therapy centres is motivated by their potential advantages as a very precise high LET radiation. 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 neighbouring the tumour. We report here a study of the fragmentation with the nuclear emulsion experimental technique. We have designed, built and exposed to a Carbon nuclei beam a chamber made of Lexan plates alternated with nuclear emulsion films. Lexan plates acted as passive material simulating human body tissues while nuclear emulsion films were used as both tracking devices with micrometric accuracy and ionisation detectors. Such a detector allowed the detection of Carbon interactions produced along their path, the identification of the fragments produced and the measurement of their scattering angle. We have measured the Carbon ion survival probability and studied their interactions. We report on the secondary particle multiplicity and the electrical charge distribution. We give results of the scattering angle of final state fragments as well as the range for H and He. Finally we give the total and partial charge-changing cross-sections for Δ z = 1 , 2 , 3 , 4 which are compared with previous results when available. The present work aims at providing data required as input to Monte Carlo simulations of Carbon ion interactions in the human body and ultimately of their therapeutic effectiveness.
- Published
- 2011
35. Validation and verification of Geant4 standard electromagnetic physics
- Author
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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
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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
36. A search for nu(mu)->nu(tau) oscillation
- Author
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E. Eskut, A. Kayis, G. Onengut, R. v. Dantzig, M. d. Jong, J. Konijn, O. Melzer, R. G. C. , C. A. F., J. W. E., J. L. Visschers, A. S. Ayan, E. Pesen, 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. Bulte, P. Lendermann, A. Meyer Sievers, T. Patzak, K. Winter, P. Annis, M. Gruwe, C. Mommaert, M. V. Donckt, B. V. de, P. Vilain, G. Wilquet, P. Righini, B. Saitta, E. D. Capua, C. Luppi, P. Zucchelli, Y. Ishii, T. Kawamura, M. Kazuno, S. Ogawa, H. Shibuya, R. Beyer, J. Brunner, D. Cussans, J. P. Fabre, R. Ferreira, W. Flegel, R. Gurin, M. Litmaath, L. Ludovici, D. Macina, R. M. Drees, H. Meinhard, P. Migliozzi, E. Niu, H. Overas, J. Panman, I. M. Papadopoulos, F. Riccardi, S. Ricciardi, A. Rozanov, D. Saltzberg, R. Santacesaria, G. Stefanini, R. Tsenov, C. Weinheimer, H. Wong, J. Goldberg, K. Hoepfner, M. Chikawa, E. Arik, I. Birol, A. A. Mailov, C. H. Hahn, H. I. Jang, I. G. Park, M. S. Park, J. S. Song, C. S. Yoon, K. Kodama, N. Ushida, S. Aoki, T. Hara, G. Brooijmans, D. Favart, G. Gregoire, J. Herin, V. Lemaitre, A. Artamonov, P. Gorbunov, V. Khovansky, V. Shamanov, V. Smirnitsky, D. Bonekamper, D. Frekers, D. Rondeshagen, T. Wolff, K. Hoshino, M. Kobayashi, 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. D. Lellis, A. Ereditato, F. Marchetti Stasi, M. Messina, PALLADINO, VITTORIO, S. Sorrentino, P. Strolin, K. Nakamura, T. Okusawa, T. Yoshida, A. Capone, D. D. Pedis, S. D. Liberto, U. Dore, P. F. Loverre, A. Maslennikov, M. A. Mazzoni, F. Meddi, G. Piredda, A. d. Bartolomeo, C. Bozza, G. Grella, G. Iovane, G. Romano, G. Rosa, Y. Sato, I. Tezuka, FIORILLO, GIULIANA, GARUFI, FABIO, E., Eskut, A., Kayi, G., Onengut, R. v., Dantzig, M. d., Jong, J., Konijn, O., Melzer, R. G. C., C. A. F., J. W., E., J. L., Visscher, A. S., Ayan, E., Pesen, 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., Bulte, P., Lendermann, A., Meyer Siever, T., Patzak, K., Winter, P., Anni, M., Gruwe, C., Mommaert, M. V., Donckt, B. V., De, P., Vilain, G., Wilquet, P., Righini, B., Saitta, E. D., Capua, C., Luppi, P., Zucchelli, Y., Ishii, T., Kawamura, M., Kazuno, S., Ogawa, H., Shibuya, R., Beyer, J., Brunner, D., Cussan, J. P., Fabre, R., Ferreira, W., Flegel, R., Gurin, M., Litmaath, L., Ludovici, D., Macina, R. M., Dree, H., Meinhard, P., Migliozzi, E., Niu, H., Overa, J., Panman, I. M., Papadopoulo, F., Riccardi, S., Ricciardi, A., Rozanov, D., Saltzberg, R., Santacesaria, G., Stefanini, R., Tsenov, C., Weinheimer, H., Wong, J., Goldberg, K., Hoepfner, M., Chikawa, E., Arik, I., Birol, A. A., Mailov, C. H., Hahn, H. I., Jang, I. G., Park, M. S., Park, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, G., Brooijman, D., Favart, G., Gregoire, J., Herin, V., Lemaitre, A., Artamonov, P., Gorbunov, V., Khovansky, V., Shamanov, V., Smirnitsky, D., Bonekamper, D., Freker, D., Rondeshagen, T., Wolff, K., Hoshino, M., Kobayashi, 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. D., Lelli, A., Ereditato, Fiorillo, Giuliana, Garufi, Fabio, F., Marchetti Stasi, M., Messina, Palladino, Vittorio, S., Sorrentino, P., Strolin, K., Nakamura, T., Okusawa, T., Yoshida, A., Capone, D. D., Pedi, S. D., Liberto, U., Dore, P. F., Loverre, A., Maslennikov, M. A., Mazzoni, F., Meddi, G., Piredda, A. d., Bartolomeo, C., Bozza, G., Grella, G., Iovane, G., Romano, G., Rosa, Y., Sato, and I., Tezuka
- Subjects
LIMITS ,LIGHT ,NEUTRINO - Abstract
CHORUS is an experiment searching for nu(mu) --> nu(tau) oscillation in the CERN wide band neutrino beam with a hybrid setup consisting of a nuclear emulsion target followed by electronic detectors. The experiment has been taking data from 1994 through 1997. A subset of the neutrino interactions collected in 1994 and 1995 have been analyzed, looking for nu(tau) charged current interactions where the tau lepton decays to mu(mu)nu(tau). In a sample of 31,423 nu(mu) charged current interactions, no nu(tau) candidates were found. For large Delta m(mu tau)(2) values, a limit on the mixing angle of sin(2)2 theta(mu tau) < 3.5 x 10(-3) at 90% C.L. can be set, thus improving the previous best result. (C) 1998 Elsevier Science B.V.
- Published
- 1998
37. Observation of neutrino induced diffractive D-s*(+) production and subsequent decay D-s*(+)-> D-s(+)->tau(+)->mu(+)
- Author
-
P. Annis, S. Aoki, A. Artamonov, E. Barbuto, A. d. Bartolomeo, D. Bonekamper, C. Bozza, C. Brooijmans, J. Brunner, A. Bulte, S. Buontempo, A. Capone, F. Cassol, M. G. Catanesi, M. Chikawa, A. Cocco, D. Cussans, N. D'Ambrosio, R. v. Dantzig, G. D. Lellis, D. D. Pedis, E. D. Capua, U. Dore, R. E. Aidi, A. Ereditato, D. Favart, R. Ferreira, D. Frekers, J. Goldberg, P. Gorbunov, G. Gregoire, G. Grella, T. Hara, J. Herin, K. Hoshino, G. Iovane, Y. Ishii, M. d. Jong, T. Kawamura, A. Kayis, M. Kazuno, V. Khovansky, K. Kodama, M. Komatsu, J. Konijn, Y. Kotaka, T. Kozaki, M. Litmaath, P. F. Loverre, L. Ludovici, M. Meinhard, O. Melzer, M. Messina, P. Migliozzi, M. Miyanishi, M. T. Muciaccia, K. Nakamura, M. Nakamura, T. Nakano, E. Niu, K. Niu, K. Niwa, Y. Obayashi, S. Ogawa, T. Okusawa, R. G. C., G. Onengut, H. Overas, J. Panman, I. M. Papadopoulos, I. G. Park, E. Pesen, G. Piredda, C. A. F., E. Radicioni, S. Ricciardi, P. Righini, G. Romano, D. Rondeshagen, G. Rosa, D. Saltzberg, B. Saitta, R. Santacesaria, O. Sato, Y. Sato, A. Satta, V. Shamanov, H. Shibuya, S. Simone, J. S. Song, S. Sorrentino, P. Strolin, I. Tezuka, V. Tioukov, P. Tolun, T. Toshito, R. Tsenov, J. W. E., N. Ushida, M. V. Dockt, B. V. de, P. Vilain, J. L. Visschers, L. Vivolo, C. Weinheimer, G. Wilquet, K. Winter, T. Wolff, H. Wong, C. S. Yoon, M. T. Zeyrek, P. Zucchelli, FIORILLO, GIULIANA, PALLADINO, VITTORIO, P., Anni, S., Aoki, A., Artamonov, E., Barbuto, A. d., Bartolomeo, D., Bonekamper, C., Bozza, C., Brooijman, J., Brunner, A., Bulte, S., Buontempo, A., Capone, F., Cassol, M. G., Catanesi, M., Chikawa, A., Cocco, D., Cussan, N., D'Ambrosio, R. v., Dantzig, G. D., Lelli, D. D., Pedi, E. D., Capua, U., Dore, R. E., Aidi, A., Ereditato, D., Favart, R., Ferreira, Fiorillo, Giuliana, D., Freker, J., Goldberg, P., Gorbunov, G., Gregoire, G., Grella, T., Hara, J., Herin, K., Hoshino, G., Iovane, Y., Ishii, M. d., Jong, T., Kawamura, A., Kayi, M., Kazuno, V., Khovansky, K., Kodama, M., Komatsu, J., Konijn, Y., Kotaka, T., Kozaki, M., Litmaath, P. F., Loverre, L., Ludovici, M., Meinhard, O., Melzer, M., Messina, P., Migliozzi, M., Miyanishi, M. T., Muciaccia, K., Nakamura, M., Nakamura, T., Nakano, E., Niu, K., Niu, K., Niwa, Y., Obayashi, S., Ogawa, T., Okusawa, R. G., C., G., Onengut, H., Overa, Palladino, Vittorio, J., Panman, I. M., Papadopoulo, I. G., Park, E., Pesen, G., Piredda, C. A., F., E., Radicioni, S., Ricciardi, P., Righini, G., Romano, D., Rondeshagen, G., Rosa, D., Saltzberg, B., Saitta, R., Santacesaria, O., Sato, Y., Sato, A., Satta, V., Shamanov, H., Shibuya, S., Simone, J. S., Song, S., Sorrentino, P., Strolin, I., Tezuka, V., Tioukov, P., Tolun, T., Toshito, R., Tsenov, J. W., E., N., Ushida, M. V., Dockt, B. V., De, P., Vilain, J. L., Visscher, L., Vivolo, C., Weinheimer, G., Wilquet, K., Winter, T., Wolff, H., Wong, C. S., Yoon, M. T., Zeyrek, and P., Zucchelli
- Subjects
PHYSICS ,FRAGMENTATION ,VECTOR-MESONS - Abstract
We report on the first direct observation of a neutrino induced charged-current interaction with two subsequent decays of short-lived particles close to the interaction vertex. This rare double-kink signature in the CHORUS emulsion target is interpreted as a D-s*(+) production followed by the decay chain D-s*(+) --> D-s(+) gamma, D-s(+) --> tau(+) v(tau),tau(+) --> mu(+) v(mu)v(tau). The event is characterised by small Q(2) and small four-momentum transfer squared t to the target nucleon, which indicates a diffractive production mechanism. A complete analysis of the event is presented. (C) 1998 Elsevier Science B.V. All rights reserved.
- Published
- 1998
38. Search for nu(mu) -> nu(tau) oscillation using the tau decay modes into a single charged particle
- Author
-
E. Eskut, A. Kayis, G. Onengut, R. v. Dantzig, M. d. Jong, J. Konijn, O. Melzer, R. G. C. , C. A. F., J. W. E., 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. Bulte, T. Patzak, K. Winter, P. Annis, R. E. Aidi, M. Gruwe, C. Mommaert, M. V. Donckt, B. V. de, P. Vilain, G. Wilquet, P. Righini, B. Saitta, E. D. 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. M. Drees, H. Meinhard, P. Migliozzi, E. Niu, H. Overas, J. Panman, I. M. Papadopoulos, E. Pesen, F. Riccardi, S. Ricciardi, A. Rozanov, D. Salzberg, P. Strolin, R. Tsenov, C. 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. Gregoire, J. Herin, A. Artamonov, P. Gorbunov, V. Khovansky, V. Shamanov, D. Bonekamper, 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. D. Lellis, A. Ereditato, M. Messina, S. Sorrentino, V. Tioukov, K. Nakamura, T. Okusawa, T. Yoshida, A. Capone, D. D. Pedis, S. D. Liberto, U. Dore, P. F. Loverre, L. Ludovici, A. Maslennikov, M. A. Mazzoni, G. Piredda, R. Santacesaria, A. Satta, E. Barbuto, A. d. Bartolomeo, C. Bozza, G. Grella, G. Iovane, G. Romano, G. Rosa, Y. Sato, I. Tezuka, FIORILLO, GIULIANA, GARUFI, FABIO, PALLADINO, VITTORIO, E., Eskut, A., Kayi, G., Onengut, R. v., Dantzig, M. d., Jong, J., Konijn, O., Melzer, R. G. C., 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, M. T., Muciaccia, E., Radicioni, S., Simone, L., Vivolo, A., Bulte, T., Patzak, K., Winter, P., Anni, R. E., Aidi, M., Gruwe, C., Mommaert, M. V., Donckt, B. V., De, P., Vilain, G., Wilquet, P., Righini, B., Saitta, E. D., Capua, C., Luppi, P., Zucchelli, Y., Ishii, T., Kawamura, M., Kazuno, S., Ogawa, H., Shibuya, J., Brunner, D., Cussan, J. P., Fabre, R., Ferreira, W., Flegel, M., Litmaath, D., Macina, R. M., Dree, H., Meinhard, P., Migliozzi, E., Niu, H., Overa, J., Panman, I. M., Papadopoulo, E., Pesen, F., Riccardi, S., Ricciardi, A., Rozanov, D., Salzberg, P., Strolin, R., Tsenov, C., 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., Brooijman, D., Favart, G., Gregoire, J., Herin, A., Artamonov, P., Gorbunov, V., Khovansky, V., Shamanov, D., Bonekamper, D., Freker, 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. D., Lelli, A., Ereditato, Fiorillo, Giuliana, Garufi, Fabio, M., Messina, Palladino, Vittorio, S., Sorrentino, V., Tioukov, K., Nakamura, T., Okusawa, T., Yoshida, A., Capone, D. D., Pedi, S. D., Liberto, U., Dore, P. F., Loverre, L., Ludovici, A., Maslennikov, M. A., Mazzoni, G., Piredda, R., Santacesaria, A., Satta, E., Barbuto, A. d., Bartolomeo, C., Bozza, G., Grella, G., Iovane, G., Romano, G., Rosa, Y., Sato, and I., Tezuka
- Abstract
Part of the neutrino events collected in 1994-1995 by the CHORUS experiment has been analysed. A search was performed for nu(tau) charged current interactions followed by the tau lepton decay into a single charged negative hadron, a possible indication for nu(mu) --> nu(tau) oscillation. A sample of 6844 events without an identified muon has been located in the emulsion target. Within the selection criteria, no tau(-) candidate has been found. Combining this result with the one from the search fur nu(tau) interactions using the muonic decay mode (36182 events with an identified muon), a 90% C.L. limit on the mixing angle sin(2)2 theta(mu tau) < 1.8.10(-3) (at large Delta m(2)) has been derived. (C) 1998 Published by Elsevier Science B.V. All rights reserved.
- Published
- 1998
39. 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
40. The CHORUS experiment to search for nu(mu)->nu(tau) oscillation
- Author
-
E. Eskut, A. Kayis, G. Onengut, R. vanDantzig, J. Konijn, R. G. C. , C. A. F., J. W. E., J. L. Visschers, A. S. Ayan, E. Pesen, M. SerinZeyrek, R. Sever, P. Tolun, M. T. Zeyrek, N. Armenise, F. Cassol, M. G. Catanesi, M. T. Muciaccia, E. Radicioni, S. Simone, L. Vivolo, D. Eckstein, P. Lendermann, A. MeyerSievers, T. Patzak, K. Winter, P. Righini, B. Saitta, P. Annis, M. Gruwe, C. Mommaert, M. VanderDonckt, B. VandeVyver, P. Vilain, G. Wilquet, E. DiCapua, M. Ferroni, C. Luppi, S. Ricciardi, Y. Ishii, T. Kawamura, M. Kazuno, S. Ogawa, H. Shibuya, R. Beyer, J. Brunner, G. Carnevale, J. P. Fabre, R. Ferreira, W. Flegel, R. Gurin, M. deJong, M. Litmaath, L. Ludovici, D. Macina, R. M. Drees, H. Meinhard, E. Niu, H. Overas, J. Panman, F. Riccardi, A. Rozanov, D. Saltzberg, G. Stefanini, R. Tzenov, C. Weinheimer, H. T. Wong, P. Zucchelli, J. Goldberg, K. Hoepfner, H. Chikawa, E. Arik, I. Birol, A. A. Mailov, C. H. Hahn, H. I. Jang, J. Y. Kim, S. N. Kim, I. G. Park, M. S. Park, J. S. Song, C. S. Yoon, K. Kodama, N. Ushida, S. Aoki, T. Hara, G. Brooijmans, D. Favart, G. Gregoire, J. Herin, V. Lemaitre, A. Artamonov, V. Epstein, P. Gorbunov, V. Khovansky, V. Shamanov, V. Smirnitsky, D. Bonekamper, D. Frekers, D. Rondeshagen, T. Wolff, K. Hoshino, M. Kobayashi, M. Komatzu, Y. Kotaka, T. Kozaki, M. Miyanishi, M. Nakamura, T. Nakano, K. Niu, K. Niwa, Y. Obayashi, O. Sato, T. Toshito, S. Buontempo, L. Casagrande, A. G. Cocco, N. DAmbrosio, A. Ereditato, F. MarchettiStasi, M. Messina, P. Migliozzi, S. Sorrentino, P. Strolin, K. Nakamura, T. Okusawa, T. Yoshida, A. Capone, D. DePedis, S. DiLiberto, U. Dore, P. F. Loverre, A. Maslennikov, M. A. Mazzoni, F. Meddi, G. Piredda, R. Santacesaria, A. D. Bartolomeo, C. Bozza, G. Grella, G. Iovane, G. Romano, G. Rosa, Y. Sato, I. Tezuka, FIORILLO, GIULIANA, GARUFI, FABIO, PALLADINO, VITTORIO, E., Eskut, A., Kayi, G., Onengut, R., Vandantzig, J., Konijn, R. G. C., C. A. F., J. W., E., J. L., Visscher, A. S., Ayan, E., Pesen, M., Serinzeyrek, R., Sever, P., Tolun, M. T., Zeyrek, N., Armenise, F., Cassol, M. G., Catanesi, M. T., Muciaccia, E., Radicioni, S., Simone, L., Vivolo, D., Eckstein, P., Lendermann, A., Meyersiever, T., Patzak, K., Winter, P., Righini, B., Saitta, P., Anni, M., Gruwe, C., Mommaert, M., Vanderdonckt, B., Vandevyver, P., Vilain, G., Wilquet, E., Dicapua, M., Ferroni, C., Luppi, S., Ricciardi, Y., Ishii, T., Kawamura, M., Kazuno, S., Ogawa, H., Shibuya, R., Beyer, J., Brunner, G., Carnevale, J. P., Fabre, R., Ferreira, W., Flegel, R., Gurin, M., Dejong, M., Litmaath, L., Ludovici, D., Macina, R. M., Dree, H., Meinhard, E., Niu, H., Overa, J., Panman, F., Riccardi, A., Rozanov, D., Saltzberg, G., Stefanini, R., Tzenov, C., Weinheimer, H. T., Wong, P., Zucchelli, J., Goldberg, K., Hoepfner, H., Chikawa, E., Arik, I., Birol, A. A., Mailov, C. H., Hahn, H. I., Jang, J. Y., Kim, S. N., Kim, I. G., Park, M. S., Park, J. S., Song, C. S., Yoon, K., Kodama, N., Ushida, S., Aoki, T., Hara, G., Brooijman, D., Favart, G., Gregoire, J., Herin, V., Lemaitre, A., Artamonov, V., Epstein, P., Gorbunov, V., Khovansky, V., Shamanov, V., Smirnitsky, D., Bonekamper, D., Freker, D., Rondeshagen, T., Wolff, K., Hoshino, M., Kobayashi, M., Komatzu, Y., Kotaka, T., Kozaki, M., Miyanishi, M., Nakamura, T., Nakano, K., Niu, K., Niwa, Y., Obayashi, O., Sato, T., Toshito, S., Buontempo, L., Casagrande, A. G., Cocco, N., Dambrosio, A., Ereditato, Fiorillo, Giuliana, Garufi, Fabio, F., Marchettistasi, M., Messina, P., Migliozzi, Palladino, Vittorio, S., Sorrentino, P., Strolin, K., Nakamura, T., Okusawa, T., Yoshida, A., Capone, D., Depedi, S., Diliberto, U., Dore, P. F., Loverre, A., Maslennikov, M. A., Mazzoni, F., Meddi, G., Piredda, R., Santacesaria, A. D., Bartolomeo, C., Bozza, G., Grella, G., Iovane, G., Romano, G., Rosa, Y., Sato, and I., Tezuka
- Subjects
CALIBRATION ,ELECTRON-SCATTERING ,LIMITS ,HYBRID EXPERIMENT ,PARTICLES ,NEUTRINO-ELECTRON ,CALORIMETER ,PERFORMANCE ,READOUT ,DETECTOR - Abstract
A new experimental apparatus, designed principally for a high sensitivity search for nu( --> mu(tau) oscillation, has been successfully 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
41. Validation of nuclear reaction models in Geant4 for the purpose of carbon ion radiotherapy
- Author
-
T. Toshito
- Subjects
Physics ,Nuclear reaction ,Nuclear physics ,Tissue equivalent ,Fragmentation (mass spectrometry) ,Nuclear engineering ,Monte Carlo method ,Dosimetry ,Carbon Ion Radiotherapy ,Nucleon ,Ion - Abstract
High energetic carbon beams are currently used for radiotherapy at several facilities in the world. Geant4 Monte Carlo simulation tool-kit has been introduced for dose calculation in carbon ion radiotherapy. Some models to treat nucleus-nucleus interactions are implemented in Geant4 to simulate nuclear fragmentation. Detailed physics validation for fragmentation models in Geant4 is indispensable in order to improve its dosimetric performance and establish its reliability. We validate fragmentation models in Geant4 using experimental data of 200 - 400 MeV/nucleon 12C ions, interacting with tissue equivalent materials of water and polycarbonate obtained by NIRS-HIMAC P152 experiment. This study is of importance both for persons to develop or improve the fragmentation models and for those to perform the dose calculation in carbon ion therapy using Geant4.
- Published
- 2007
42. Study on Nuclear Fragmentation by High Speed Emulsion Read-Out System
- Author
-
T. Toshito
- Subjects
Physics ,Nuclear reaction ,Nuclear physics ,Fragmentation (mass spectrometry) ,law ,Nuclear electronics ,Emulsion ,Heavy ion therapy ,Nuclear emulsion ,Cloud chamber ,Nuclear Experiment ,law.invention ,Ion - Abstract
Recent development of high speed nuclear emulsion read-out system is remarkable. Motivated by this, we started a project to apply it to studying the interactions of relativistic heavy ions in matter using HIMAC at National Institute of Radiological Sciences in Japan. We have developed the emulsion cloud chamber to study Carbon-Water interaction in the energy range from 400 MeV/n down to several 10 MeV/n. This measurement is quite important from a point of view of the heavy ion therapy. Our experimental results for total and partial charge-changing cross sections at E > 200 MeV/n agree well with the data available from past measurements. Detailed analysis by event-by-event basis is in progress. The new emulsion technology demonstrates the potential to study heavy ion fragmentation.
- Published
- 2006
43. Measurement of atmospheric neutrino oscillation parameters by Super-Kamiokande I
- Author
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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
44. Publisher's Note: Search for dark matter WIMPs using upward through-going muons in Super-Kamiokande [Phys. Rev. D70, 083523 (2004)]
- Author
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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
45. Limits on the Neutrino Magnetic Moment using 1496 Days of Super-Kamiokande-I Solar Neutrino Data
- Author
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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
46. Evidence for an oscillatory signature in atmospheric neutrino oscillations
- Author
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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
47. Search for Dark Matter WIMPs using Upward Through-going Muons in Super-Kamiokande
- Author
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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
48. Search for periodic modulations of the solar neutrino flux in Super-Kamiokande-I
- Author
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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
49. Search for Supernova Relic Neutrinos at Super-Kamiokande
- Author
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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
50. Search for nu(e) from the sun at Super-Kamiokande-I
- Author
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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
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