Charge-separated atmospheric neutrino-induced muons in the MINOS far detector

Autor: Adamson, P. Andreopoulos, C. Arms, K. E. Armstrong, R. and Auty, D. J. Avvakumov, S. Ayres, D. S. Baller, B. and Barish, B. Barnes, Jr., P. D. Barr, G. Barrett, W. L. and Beall, E. Becker, B. R. Belias, A. Bergfeld, T. and Bernstein, R. H. Bhattacharya, D. Bishai, M. Blake, A. and Bock, B. Bock, G. J. Boehm, J. Boehnlein, D. J. Bogert, D. Border, P. M. Bower, C. Buckley-Geer, E. Cabrera, A. and Chapman, J. D. Cherdack, D. Childress, S. Choudhary, B. C. Cobb, J. H. Culling, A. J. de Jong, J. K. De Santo, A. Dierckxsens, M. Diwan, M. V. Dorman, M. Drakoulakos, D. Durkin, T. Erwin, A. R. Escobar, C. O. Evans, J. J. and Harris, E. Falk Feldman, G. J. Fields, T. H. Ford, R. and Frohne, M. V. Gallagher, H. R. Giurgiu, G. A. Godley, A. and Gogos, J. Goodman, M. C. Gouffon, P. Gran, R. and Grashorn, E. W. Grossman, N. Grzelak, K. Habig, A. and Harris, D. Harris, P. G. Hartnell, J. Hartouni, E. P. and Hatcher, R. Heller, K. Holin, A. Howcroft, C. Hylen, J. and Indurthy, D. Irwin, G. M. Ishitsuka, M. Jaffe, D. E. and James, C. Jenner, L. Jensen, D. Joffe-Minor, T. Kafka, T. Kang, H. J. Kasahara, S. M. S. Kim, M. S. Koizumi, G. and Kopp, S. Kordosky, M. Koskinen, D. J. Kotelnikov, S. K. and Kreymer, A. Kumaratunga, S. Lang, K. Lebedev, A. and Lee, R. Ling, J. Liu, J. Litchfield, P. J. Litchfield, R. P. Lucas, P. Mann, W. A. Marchionni, A. Marino, A. D. and Marshak, M. L. Marshall, J. S. Mayer, N. McGowan, A. M. and Meier, J. R. Merzon, G. I. Messier, M. D. Michael, D. G. and Milburn, R. H. Miller, J. L. Miller, W. H. Mishra, S. R. and Mislivec, A. Miyagawa, P. S. Moore, C. D. Morfin, J. and Mualem, L. Mufson, S. Murgia, S. Musser, J. Naples, D. and Nelson, J. K. Newman, H. B. Nichol, R. J. Nicholls, T. C. Ochoa-Ricoux, J. P. Oliver, W. P. Osiecki, T. and Ospanov, R. Paley, J. Paolone, V. Para, A. Patzak, T. and Pavlovic, Z. Pearce, G. F. Peck, C. W. Peterson, E. A. and Petyt, D. A. Ping, H. Piteira, R. Pittam, R. and Plunkett, R. K. Rahman, D. Rameika, R. A. Raufer, T. M. and Rebel, B. Reichenbacher, J. Reyna, D. E. Rosenfeld, C. and Rubin, H. A. Ruddick, K. Ryabov, V. A. Saakyan, R. and Sanchez, M. C. Saoulidou, N. Schneps, J. Schreiner, P. and Semenov, V. K. Seun, S.-M. Shanahan, P. Smart, W. and Smirnitsky, V. Smith, C. Sousa, A. Speakman, B. and Stamoulis, P. Symes, P. A. Tagg, N. Talaga, R. L. and Tetteh-Lartey, E. Thomas, J. Thompson, J. Thomson, M. A. and Thron, J. L. Tinti, G. Trostin, I. Tsarev, V. A. and Tzanakos, G. Urheim, J. Vahle, P. Verebryusov, V. Viren, B. Ward, C. P. Ward, D. R. Watabe, M. Weber, A. and Webb, R. C. Wehmann, A. West, N. White, C. Wojcicki, S. G. Wright, D. M. Wu, Q. K. Yang, T. Yumiceva, F. X. and Zheng, H. Zois, M. Zwaska, R. MINOS Collaboration
Jazyk: angličtina
Rok vydání: 2007
Předmět:
Popis: We found 140 neutrino-induced muons in 854.24 live days in the MINOS far detector, which has an acceptance for neutrino-induced muons of 6.91x10(6) cm(2) sr. We looked for evidence of neutrino disappearance in this data set by computing the ratio of the number of low momentum muons to the sum of the number of high momentum and unknown momentum muons for both data and Monte Carlo expectation in the absence of neutrino oscillations. The ratio of data and Monte Carlo ratios, R, is R=0.65(-0.12)(+0.15)(stat)+/- 0.09(syst), a result that is consistent with an oscillation signal. A fit to the data for the oscillation parameters sin(2)2 theta(23) and Delta m(23)(2) excludes the null oscillation hypothesis at the 94% confidence level. We separated the muons into mu(-) and mu(+) in both the data and Monte Carlo events and found the ratio of the total number of mu(-) to mu(+) in both samples. The ratio of those ratios, R boolean AND(CPT), is a test of CPT conservation. The result R boolean AND(CPT)=0.72(-0.18)(+0.24)(stat)(-0.04)(+0.08)(syst) is consistent with CPT conservation.
Databáze: OpenAIRE