Details

Autor(en) / Beteiligte

• 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, G J
• 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

Titel

Combined analysis of νμ disappearance and νμ→νe appearance in MINOS using accelerator and atmospheric neutrinos

Ist Teil von

• Physical review letters, 2014-05, Vol.112 (19), p.191801-191801

Ort / Verlag

United States: American Physical Society (APS)

Erscheinungsjahr

2014

Quelle

PROLA

Beschreibungen/Notizen

• We report on a new analysis of neutrino oscillations in MINOS using the complete set of accelerator and atmospheric data. The analysis combines the ν(μ) disappearance and ν(e) appearance data using the three-flavor formalism. We measure |Δm(32)(2)| = [2.28-2.46] × 10(-3) eV(2) (68% C.L.) and sin(2)θ(23) = 0.35-0.65 (90% C.L.) in the normal hierarchy, and |Δm(32)(2)| = [2.32-2.53] × 10(-3) eV(2) (68% C.L.) and sin(2)θ(23) = 0.34-0.67 (90% C.L.) in the inverted hierarchy. The data also constrain δ(CP), the θ(23} octant degeneracy and the mass hierarchy; we disfavor 36% (11%) of this three-parameter space at 68% (90%) C.L.