{"paper":{"title":"Combined analysis of $\\nu_{\\mu}$ disappearance and $\\nu_{\\mu} \\rightarrow \\nu_{e}$ appearance in MINOS using accelerator and atmospheric neutrinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-ex","authors_text":"A. Aurisano, A. Blake, A. Habig, A. Himmel, A. Holin, A. Kreymer, A. Perch, A. Radovic, A. Schreckenberger, A. Sousa, A. Timmons, A. V. Devan, A. Weber, B. Rebel, B. Viren, C. D. Moore, C. James, C. M. Castromonte, C. McGivern, C. O. Escobar, C. Rosenfeld, C. White, D. Bogert, D. Cherdack, D. Cronin-Hennessy, D. G. Michael, D. Jensen, D. Naples, D. Torretta, E. Falk, G. Barr, G. J. Bock, G. J. Feldman, G. Koizumi, G. M. Irwin, G. Pawloski, G. Tzanakos, H. A. Rubin, H. B. Newman, H. R. Gallagher, I. Anghel, J. A. B. Coelho, J. A. Nowak, J. Hartnell, J. Huang, J. Hylen, J. J. Evans, J. K. de Jong, J. K. Nelson, J. Ling, J. Musser, J. O'Connor, J. Paley, J. R. Meier, J. Schneps, J. Thomas, J. Urheim, K. Grzelak, K. Lang, L. Corwin, L. H. Whitehead, L. Mualem, L. Whitehead, M. A. Thomson, M. Bishai, M. C. Goodman, M. C. Sanchez, M. D. Messier, MINOS Collaboration: P. Adamson, M. Kordosky, M. L. Marshak, M. M. Medeiros, M. Orchanian, M. V. Diwan, M. V. Frohne, N. E. Devenish, N. Graf, N. Mayer, N. Poonthottathil, N. Tagg, P. Gouffon, P. J. Litchfield, P. Lucas, P. Schreiner, P. Vahle, R. A. Gomes, R. B. Pahlka, R. B. Patterson, R. C. Webb, R. Gran, R. Hatcher, R. J. Nichol, R. K. Plunkett, R. L. Talaga, R. Mehdiyev, R. Sharma, R. Toner, R. Zwaska, S. Childress, S. C. Tognini, S. G. Wojcicki, S. Moed Sher, S. M. S. Kasahara, S. Phan-Budd, S. R. Hahn, S. R. Mishra, S. V. Cao, T. Kafka, W. A. Mann, W. H. Miller, X. Qiu, X. Tian, Z. Isvan","submitted_at":"2014-03-04T17:25:19Z","abstract_excerpt":"We report on a new analysis of neutrino oscillations in MINOS using the complete set of accelerator and atmospheric data. The analysis combines the $\\nu_{\\mu}$ disappearance and $\\nu_{e}$ appearance data using the three-flavor formalism. We measure $|\\Delta m^{2}_{32}|=[2.28-2.46]\\times10^{-3}\\mbox{\\,eV}^{2}$ (68% C.L.) and $\\sin^{2}\\theta_{23}=0.35-0.65$ (90% C.L.) in the normal hierarchy, and $|\\Delta m^{2}_{32}|=[2.32-2.53]\\times10^{-3}\\mbox{\\,eV}^{2}$ (68% C.L.) and $\\sin^{2}\\theta_{23}=0.34-0.67$ (90% C.L.) in the inverted hierarchy. The data also constrain $\\delta_{CP}$, the $\\theta_{23}"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.0867","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}