First observations of separated atmospheric νμ and (ν)over-barμ events in the MINOS detector

被引:66
作者
Adamson, P
Alexopoulos, T
Allison, WWM
Alner, GJ
Anderson, K
Andreopoulos, C
Andrews, M
Andrews, R
Arroyo, C
Avvakumov, S
Ayres, DS
Baller, B
Barish, B
Barker, MA
Barnes, PD
Barr, G
Barrett, WL
Beall, E
Becker, BR
Belias, A
Bergfeld, T
Bernstein, RH
Bhattacharya, D
Bishai, M
Blake, A
Bocean, V
Bock, B
Bock, GJ
Boehm, J
Boehnlein, DJ
Bogert, D
Border, PM
Bower, C
Boyd, S
Buckley-Geer, E
Byon-Wagner, A
Cabrera, A
Chapman, JD
Chase, TR
Chernichenko, SK
Childress, S
Choudhary, BC
Cobb, JH
Cossairt, JD
Courant, H
Crane, DA
Culling, AJ
Dawson, JW
DeMuth, DM
De Santo, A
机构
[1] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[2] Argonne Natl Lab, Argonne, IL 60439 USA
[3] Univ Athens, Dept Phys, GR-15771 Athens, Greece
[4] Benedictine Univ, Dept Phys, Lisle, IL 60532 USA
[5] Brookhaven Natl Lab, Upton, NY 11973 USA
[6] CALTECH, Lauritsen Lab, Pasadena, CA 91125 USA
[7] Univ Cambridge, Cavendish Lab, Dept Phys, Cambridge CB3 0HE, England
[8] Univ Estadual Campinas, IF, BR-13083970 Campinas, SP, Brazil
[9] Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China
[10] Coll France, APC, F-75231 Paris 05, France
[11] Columbia Univ, Dept Phys, New York, NY 10027 USA
[12] Harvard Univ, High Energy Phys Lab, Cambridge, MA 02138 USA
[13] IIT, Div Phys, Chicago, IL 60616 USA
[14] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA
[15] Inst High Energy Phys, RU-140284 Protvino, Moscow Region, Russia
[16] Inst Theoret & Expt Phys, High Energy Expt Phys Dept, Moscow 117218, Russia
[17] James Madison Univ, Dept Phys, Harrisonburg, VA 22807 USA
[18] Joint Inst Nucl Res, RU-141980 Dubna, Moscow Region, Russia
[19] PN Lebedev Phys Inst, Dept Nucl Phys, Moscow 117924, Russia
[20] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[21] Univ Minnesota, Minneapolis, MN 55455 USA
[22] Univ Minnesota, Dept Phys, Duluth, MN 55812 USA
[23] Univ Oxford, Subdept Particle Phys, Oxford OX1 3RH, England
[24] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
[25] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England
[26] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil
[27] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA
[28] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[29] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England
[30] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA
[31] Univ Texas, Dept Phys, Austin, TX 78712 USA
[32] Tufts Univ, Dept Phys, Medford, MA 02155 USA
[33] UCL, Dept Phys & Astron, London WC1E 6BT, England
[34] Western Washington Univ, Dept Phys, Bellingham, WA 98225 USA
[35] Coll William & Mary, Dept Phys, Williamsburg, VA 23187 USA
[36] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
来源
PHYSICAL REVIEW D | 2006年 / 73卷 / 07期
基金
英国科学技术设施理事会;
关键词
D O I
10.1103/PhysRevD.73.072002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The complete 5.4 kton MINOS far detector has been taking data since the beginning of August 2003 at a depth of 2070 meters water-equivalent in the Soudan mine, Minnesota. This paper presents the first MINOS observations of nu(mu) and (nu) over bar (mu) charged-current atmospheric neutrino interactions based on an exposure of 418 days. The ratio of upward- to downward-going events in the data is compared to the Monte Carlo expectation in the absence of neutrino oscillations, giving R-up/down(data)/R-up/down(MC)=0.62(-0.14)(+0.19)(stat.)+/- 0.02(sys.). An extended maximum likelihood analysis of the observed L/E distributions excludes the null hypothesis of no neutrino oscillations at the 98% confidence level. Using the curvature of the observed muons in the 1.3 T MINOS magnetic field nu(mu) and (nu) over bar (mu) interactions are separated. The ratio of (nu) over bar (mu) to nu(mu) events in the data is compared to the Monte Carlo expectation assuming neutrinos and antineutrinos oscillate in the same manner, giving R-(nu) over bar mu/nu(data)(mu)/R-(nu) over bar mu/nu(MC)(mu)=0.96(-0.27)(+0.38)(stat.)+/- 0.15(sys.), where the errors are the statistical and systematic uncertainties. Although the statistics are limited, this is the first direct observation of atmospheric neutrino interactions separately for nu(mu) and (nu) over bar (mu).
引用
收藏
页数:18
相关论文
共 40 条
[1]   On the linearity of the MINOS light-injection calibration system [J].
Adamson, P ;
Barrett, L ;
Belias, A ;
Blake, A ;
Cabrera, A ;
Falk, E ;
Harris, PG ;
Hartnell, J ;
Howcroft, C ;
Kordosky, M ;
Lang, K ;
Lee, R ;
Liu, J ;
Michael, D ;
Morse, R ;
Nelson, JK ;
Nichol, R ;
Pearce, G ;
Ruddick, K ;
Smith, PN ;
Symes, PA ;
Thomas, J ;
Vahle, PL ;
Webb, R ;
Weber, A ;
White, RF .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2004, 521 (2-3) :361-366
[2]  
ADAMSON P, IN PRESS MINOS CALIF
[3]  
ADAMSON P, 1998, 1337 MINOS
[4]   GEANT4-a simulation toolkit [J].
Agostinelli, S ;
Allison, J ;
Amako, K ;
Apostolakis, J ;
Araujo, H ;
Arce, P ;
Asai, M ;
Axen, D ;
Banerjee, S ;
Barrand, G ;
Behner, F ;
Bellagamba, L ;
Boudreau, J ;
Broglia, L ;
Brunengo, A ;
Burkhardt, H ;
Chauvie, S ;
Chuma, J ;
Chytracek, R ;
Cooperman, G ;
Cosmo, G ;
Degtyarenko, P ;
Dell'Acqua, A ;
Depaola, G ;
Dietrich, D ;
Enami, R ;
Feliciello, A ;
Ferguson, C ;
Fesefeldt, H ;
Folger, G ;
Foppiano, F ;
Forti, A ;
Garelli, S ;
Giani, S ;
Giannitrapani, R ;
Gibin, D ;
Cadenas, JJG ;
González, I ;
Abril, GG ;
Greeniaus, G ;
Greiner, W ;
Grichine, V ;
Grossheim, A ;
Guatelli, S ;
Gumplinger, P ;
Hamatsu, R ;
Hashimoto, K ;
Hasui, H ;
Heikkinen, A ;
Howard, A .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2003, 506 (03) :250-303
[5]   Atmospheric neutrino flux above 1 GeV [J].
Agrawal, V ;
Gaisser, TK ;
Lipari, P ;
Stanev, T .
PHYSICAL REVIEW D, 1996, 53 (03) :1314-1323
[6]  
Aguilar A, 2001, PHYS REV D, V64, DOI 10.1103/PhysRevD.64.112007
[7]   Evidence for muon neutrino oscillation in an accelerator-based experiment [J].
Aliu, E ;
Andringa, S ;
Aoki, S ;
Argyriades, J ;
Asakura, K ;
Ashie, R ;
Berns, H ;
Bhang, H ;
Blondel, A ;
Borghi, S ;
Bouchez, J ;
Burguet-Castell, J ;
Casper, D ;
Cavata, C ;
Cervera, A ;
Cho, KO ;
Choi, JH ;
Dore, U ;
Espinal, X ;
Fechner, M ;
Fernandez, E ;
Fukuda, Y ;
Gomez-Cadenas, J ;
Gran, R ;
Hara, T ;
Hasegawa, M ;
Hasegawa, T ;
Hayashi, K ;
Hayato, Y ;
Helmer, RL ;
Hill, J ;
Hiraide, K ;
Hosaka, J ;
Ichikawa, AK ;
Iinuma, M ;
Ikeda, A ;
Inagaki, T ;
Ishida, T ;
Ishihara, K ;
Ishii, T ;
Ishitsuka, M ;
Itow, Y ;
Iwashita, T ;
Jang, HI ;
Jeon, EJ ;
Jeong, IS ;
Joo, K ;
Jover, G ;
Jung, CK ;
Kajita, T .
PHYSICAL REVIEW LETTERS, 2005, 94 (08)
[8]   Neutrino oscillation effects in Soudan 2 upward-stopping muons [J].
Allison, WWM ;
Alner, GJ ;
Ayres, DS ;
Barr, GD ;
Barrett, WL ;
Border, PM ;
Cobb, JH ;
Cockerill, DJA ;
Courant, H ;
Demuth, DM ;
Fields, TH ;
Gallagher, HR ;
Goodman, MC ;
Kafka, T ;
Kasahara, SMS ;
Litchfield, PJ ;
Mann, WA ;
Marshak, ML ;
Miller, WH ;
Mualem, L ;
Nelson, JK ;
Napier, A ;
Oliver, WP ;
Pearce, GF ;
Peterson, EA ;
Petyt, DA ;
Ruddick, K ;
Sanchez, M ;
Schneps, J ;
Sousa, A ;
Thron, JL ;
West, N .
PHYSICAL REVIEW D, 2005, 72 (05)
[9]   Atmospheric neutrino oscillations from upward throughgoing muon multiple scattering in MACRO [J].
Ambrosio, M ;
Antolini, R ;
Bakari, D ;
Baldini, A ;
Barbarino, GC ;
Barish, BC ;
Battistoni, G ;
Becherini, Y ;
Bellotti, R ;
Bemporad, C ;
Bernardini, P ;
Bilokon, H ;
Bloise, C ;
Bower, C ;
Brigida, M ;
Bussino, S ;
Cafagna, E ;
Calicchio, M ;
Campana, D ;
Carboni, M ;
Caruso, R ;
Cecchini, S ;
Cei, F ;
Chiarella, V ;
Chiarusi, T ;
Choudhary, BC ;
Coutu, S ;
Cozzi, M ;
De Cataldo, G ;
Dekhissi, H ;
De Marzo, C ;
De Mitri, I ;
Derkaoui, J ;
De Vincenzi, M ;
Di Credico, A ;
Favuzzi, C ;
Forti, C ;
Fusco, P ;
Giacomelli, G ;
Giannini, G ;
Giglietto, N ;
Giorgini, M ;
Grassi, M ;
Grillo, A ;
Gustavino, C ;
Habig, A ;
Hanson, K ;
Heinz, R ;
Iarocci, E ;
Katsavounidis, E .
PHYSICS LETTERS B, 2003, 566 (1-2) :35-44
[10]   Total cross section measurements for upsilon(mu), (upsilon)over-bar-(mu) charged current interactions in 3-30 GeV energy range with IHEP-JINR neutrino detector [J].
Anikeev, VB ;
Belikov, SV ;
Borisov, AA ;
Bozhko, NI ;
Bugorsky, AP ;
Chernichenko, SK ;
Goryachev, VN ;
Gurgiev, SN ;
Kirsanov, MM ;
Kononov, AI ;
Kozhin, AS ;
Kravtsov, VI ;
Kulikov, VA ;
Lipaev, VV ;
Mukhin, AI ;
Mukhin, SA ;
Perelygin, VF ;
Salomatin, YI ;
Sapunov, YI ;
Sidorov, AV ;
Spiridonov, AA ;
Sviridov, YM ;
Sytnik, VV ;
Shestermanov, KE ;
Shchukin, GL ;
Tumakov, VL ;
Vovenko, AS ;
Zhigunov, VP ;
Barabash, LS ;
Baranov, SA ;
Batusov, YA ;
Bunyatov, SA ;
Denisov, OA ;
Karev, AG ;
Kazarinov, MY ;
Klimov, OL ;
Lyukov, VV ;
Nefedov, YA ;
Prakhov, SN ;
Snyatkov, VI ;
Vovenko, AA .
ZEITSCHRIFT FUR PHYSIK C-PARTICLES AND FIELDS, 1996, 70 (01) :39-46