{"paper":{"title":"Electron neutrino and antineutrino appearance in the full MINOS data sample","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ex","authors_text":"A. Blake, A. Habig, A. Himmel, A. Holin, A. Kreymer, A. Radovic, A. Schreckenberger, A. Sousa, A. V. Devan, A. Weber, B. Rebel, B. Viren, C. Backhouse, C. D. Moore, C. James, C. O. Escobar, C. Rosenfeld, C. White, D. Bogert, D. Cherdack, D. Cronin-Hennessy, D. E. Jaffe, D. Jensen, D. Naples, D. Torretta, E. Falk, G. Barr, G. J. Bock, G. J. Feldman, G. Koizumi, G. M. Irwin, G. Pawloski, G. Tinti, G. Tzanakos, H. A. Rubin, H. B. Newman, H. R. Gallagher, I. Anghel, J. A. B. Coelho, J. A. Nowak, J. Hartnell, J. Hylen, J. J. Evans, J. K. de Jong, J. K. Nelson, J. Ling, J. Musser, J. O'Connor, J. Paley, J. P. Ochoa-Ricoux, J. R. Meier, J. Schneps, J. Thomas, J. Urheim, K. Grzelak, K. Lang, L. Corwin, L. Mualem, L. Whitehead, M. A. Thomson, M. Bishai, M. C. Goodman, M. C. Sanchez, M. D. Messier, M. Kordosky, M. L. Marshak, M. Mathis, M. M. Medeiros, M. Orchanian, M. V. Diwan, M. V. Frohne, N. E. Devenish, N. Graf, N. Mayer, N. Tagg, P. Adamson, 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. G. Wojcicki, S. Moed Sher, S. M. S. Kasahara, S. Phan-Budd, S. R. Hahn, S. R. Mishra, S. V. Cao, T. Kafka, T. Yang, W. A. Mann, W. H. Miller, W. P. Oliver, X. Qiu, Z. Isvan","submitted_at":"2013-01-19T18:08:06Z","abstract_excerpt":"We report on $\\nu_e$ and $\\bar{\\nu}_e$ appearance in $\\nu_\\mu$ and $\\bar{\\nu}_\\mu$ beams using the full MINOS data sample. The comparison of these $\\nu_e$ and $\\bar{\\nu}_e$ appearance data at a 735 km baseline with $\\theta_{13}$ measurements by reactor experiments probes $\\delta$, the $\\theta_{23}$ octant degeneracy, and the mass hierarchy. This analysis is the first use of this technique and includes the first accelerator long-baseline search for $\\bar{\\nu}_\\mu\\rightarrow\\bar{\\nu}_e$. Our data disfavor 31% (5%) of the three-parameter space defined by $\\delta$, the octant of the $\\theta_{23}$,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.4581","kind":"arxiv","version":3},"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"}