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. 2014 May 16;112(19):191801.
doi: 10.1103/PhysRevLett.112.191801. Epub 2014 May 12.

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

P Adamson  1 I Anghel  2 A Aurisano  3 G Barr  4 M Bishai  5 A Blake  6 G J Bock  1 D Bogert  1 S V Cao  7 C M Castromonte  8 D Cherdack  9 S Childress  1 J A B Coelho  10 L Corwin  11 D Cronin-Hennessy  12 J K de Jong  4 A V Devan  13 N E Devenish  14 M V Diwan  5 C O Escobar  15 J J Evans  16 E Falk  14 G J Feldman  17 M V Frohne  18 H R Gallagher  9 R A Gomes  8 M C Goodman  19 P Gouffon  20 N Graf  21 R Gran  22 K Grzelak  23 A Habig  22 S R Hahn  1 J Hartnell  14 R Hatcher  1 A Himmel  24 A Holin  25 J Huang  7 J Hylen  1 G M Irwin  26 Z Isvan  27 C James  1 D Jensen  1 T Kafka  9 S M S Kasahara  12 G Koizumi  1 M Kordosky  13 A Kreymer  1 K Lang  7 J Ling  5 P J Litchfield  28 P Lucas  1 W A Mann  9 M L Marshak  12 N Mayer  29 C McGivern  30 M M Medeiros  8 R Mehdiyev  7 J R Meier  12 M D Messier  11 D G Michael  24 W H Miller  12 S R Mishra  31 S Moed Sher  1 C D Moore  1 L Mualem  24 J Musser  11 D Naples  30 J K Nelson  13 H B Newman  24 R J Nichol  25 J A Nowak  12 J O'Connor  25 M Orchanian  24 R B Pahlka  1 J Paley  19 R B Patterson  24 G Pawloski  32 A Perch  25 S Phan-Budd  19 R K Plunkett  1 N Poonthottathil  1 X Qiu  26 A Radovic  33 B Rebel  1 C Rosenfeld  31 H A Rubin  34 M C Sanchez  2 J Schneps  9 A Schreckenberger  35 P Schreiner  19 R Sharma  1 A Sousa  36 N Tagg  37 R L Talaga  19 J Thomas  25 M A Thomson  6 X Tian  31 A Timmons  16 S C Tognini  8 R Toner  38 D Torretta  1 G Tzanakos  39 J Urheim  11 P Vahle  13 B Viren  5 A Weber  40 R C Webb  41 C White  34 L Whitehead  42 L H Whitehead  25 S G Wojcicki  26 R Zwaska  1
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Free article

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

P Adamson et al. Phys Rev Lett. .
Free article

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 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.

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