1. Combined Analysis of νμ Disappearance and νμ→νe Appearance in MINOS Using Accelerator and Atmospheric Neutrinos
- Author
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Adamson, P., Anghel, I., Aurisano, A., Barr, G., Bishai, M., Blake, A., Bock, G. J., Bogert, D., Cao, S. V., Castromonte, C. M., Cherdack, D., Childress, S., Coelho, J. A. B., Corwin, L., Cronin-Hennessy, D., de Jong, J. K., Devan, A. V., Devenish, N. E., Diwan, M. V., Escobar, C. O., Evans, J. J., Falk, E., Feldman, Gary, Frohne, M. V., Gallagher, H. R., Gomes, R. A., Goodman, M. C., Gouffon, P., Graf, N., Gran, R., Grzelak, K., Habig, A., Hahn, S. R., Hartnell, J., Hatcher, R., Himmel, A., Holin, A., Huang, J., Hylen, J., Irwin, G. M., Isvan, Z., James, C., Jensen, D., Kafka, T., Kasahara, S. M. S., Koizumi, G., Kordosky, M., Kreymer, A., Lang, K., Ling, J., Litchfield, P. J., Lucas, P., Mann, W. A., Marshak, M. L., Mayer, N., McGivern, C., Medeiros, M. M., Mehdiyev, R., Meier, J. R., Messier, M. D., Michael, D. G., Miller, W. H., Mishra, S. R., Moed Sher, S., Moore, C. D., Mualem, L., Musser, J., Naples, D., Nelson, J. K., Newman, H. B., Nichol, R. J., Nowak, J. A., O’Connor, J., Orchanian, M., Pahlka, R. B., Paley, J., Patterson, R. B., Pawloski, G., Perch, A., Phan-Budd, S., Plunkett, R. K., Poonthottathil, N., Qiu, X., Radovic, A., Rebel, B., Rosenfeld, C., Rubin, H. A., Sanchez, M. C., Schneps, J., Schreckenberger, A., Schreiner, P., Sharma, R., Sousa, A., Tagg, N., Talaga, R. L., Thomas, J., Thomson, M. A., Tian, X., Timmons, A., Tognini, S. C., Toner, Ruth, Torretta, D., Tzanakos, G., Urheim, J., Vahle, P., Viren, B., Weber, A., Webb, R. C., White, C., Whitehead, L., Whitehead, L. H., Wojcicki, S. G., and Zwaska, R.
- Subjects
eutrino: mass: hierarchy ,neutrino: atmosphere ,neutrino: oscillation ,MINOS ,neutrino/mu: beam ,neutrino/mu: flux ,neutrino/e: particle identification ,flavor: 3 ,neutrino: mass difference ,neutrino: mixing angle ,CP: violation ,experimental results - Abstract
We report on a new analysis of neutrino oscillations in MINOS using the complete set of accelerator and atmospheric data. The analysis combines the νμ disappearance and νe appearance data using the three-flavor formalism. We measure |Δm232|=[2.28–2.46]×10−3 eV2 (68% C.L.) and sin2θ23=0.35–0.65 (90% C.L.) in the normal hierarchy, and |Δm232|=[2.32–2.53]×10−3 eV2 (68% C.L.) and sin2θ23=0.34–0.67 (90% C.L.) in the inverted hierarchy. The data also constrain δCP, the θ23 octant degeneracy and the mass hierarchy; we disfavor 36% (11%) of this three-parameter space at 68% (90%) C.L., Physics, Accepted Manuscript
- Published
- 2014
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