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

نویسندگان

  • P Adamson
  • I Anghel
  • A Aurisano
  • G Barr
  • M Bishai
  • A Blake
  • G J Bock
  • D Bogert
  • S V Cao
  • C M Castromonte
  • D Cherdack
  • S Childress
  • J A B Coelho
  • L Corwin
  • D Cronin-Hennessy
  • J K de Jong
  • A V Devan
  • N E Devenish
  • M V Diwan
  • C O Escobar
  • J J Evans
  • E Falk
  • G J Feldman
  • M V Frohne
  • H R Gallagher
  • R A Gomes
  • M C Goodman
  • P Gouffon
  • N Graf
  • R Gran
  • K Grzelak
  • A Habig
  • S R Hahn
  • J Hartnell
  • R Hatcher
  • A Himmel
  • A Holin
  • J Huang
  • J Hylen
  • G M Irwin
  • Z Isvan
  • C James
  • D Jensen
  • T Kafka
  • S M S Kasahara
  • G Koizumi
  • M Kordosky
  • A Kreymer
  • K Lang
  • J Ling
  • P J Litchfield
  • P Lucas
  • W A Mann
  • M L Marshak
  • N Mayer
  • C McGivern
  • M M Medeiros
  • R Mehdiyev
  • J R Meier
  • M D Messier
  • D G Michael
  • W H Miller
  • S R Mishra
  • S Moed Sher
  • C D Moore
  • L Mualem
  • J Musser
  • D Naples
  • J K Nelson
  • H B Newman
  • R J Nichol
  • J A Nowak
  • J O'Connor
  • M Orchanian
  • R B Pahlka
  • J Paley
  • R B Patterson
  • G Pawloski
  • A Perch
  • S Phan-Budd
  • R K Plunkett
  • N Poonthottathil
  • X Qiu
  • A Radovic
  • B Rebel
  • C Rosenfeld
  • H A Rubin
  • M C Sanchez
  • J Schneps
  • A Schreckenberger
  • P Schreiner
  • R Sharma
  • A Sousa
  • N Tagg
  • R L Talaga
  • J Thomas
  • M A Thomson
  • X Tian
  • A Timmons
  • S C Tognini
  • R Toner
  • D Torretta
  • G Tzanakos
  • J Urheim
  • P Vahle
  • B Viren
  • A Weber
  • R C Webb
  • C White
  • L Whitehead
  • L H Whitehead
  • S G Wojcicki
  • R Zwaska
چکیده

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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عنوان ژورنال:
  • Physical review letters

دوره 112 19  شماره 

صفحات  -

تاریخ انتشار 2014