Literature DB >> 24877929

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

P Adamson1, I Anghel2, A Aurisano3, G Barr4, M Bishai5, A Blake6, G J Bock1, D Bogert1, S V Cao7, C M Castromonte8, D Cherdack9, S Childress1, J A B Coelho10, L Corwin11, D Cronin-Hennessy12, J K de Jong4, A V Devan13, N E Devenish14, M V Diwan5, C O Escobar15, J J Evans16, E Falk14, G J Feldman17, M V Frohne18, H R Gallagher9, R A Gomes8, M C Goodman19, P Gouffon20, N Graf21, R Gran22, K Grzelak23, A Habig22, S R Hahn1, J Hartnell14, R Hatcher1, A Himmel24, A Holin25, J Huang7, J Hylen1, G M Irwin26, Z Isvan27, C James1, D Jensen1, T Kafka9, S M S Kasahara12, G Koizumi1, M Kordosky13, A Kreymer1, K Lang7, J Ling5, P J Litchfield28, P Lucas1, W A Mann9, M L Marshak12, N Mayer29, C McGivern30, M M Medeiros8, R Mehdiyev7, J R Meier12, M D Messier11, D G Michael24, W H Miller12, S R Mishra31, S Moed Sher1, C D Moore1, L Mualem24, J Musser11, D Naples30, J K Nelson13, H B Newman24, R J Nichol25, J A Nowak12, J O'Connor25, M Orchanian24, R B Pahlka1, J Paley19, R B Patterson24, G Pawloski32, A Perch25, S Phan-Budd19, R K Plunkett1, N Poonthottathil1, X Qiu26, A Radovic33, B Rebel1, C Rosenfeld31, H A Rubin34, M C Sanchez2, J Schneps9, A Schreckenberger35, P Schreiner19, R Sharma1, A Sousa36, N Tagg37, R L Talaga19, J Thomas25, M A Thomson6, X Tian31, A Timmons16, S C Tognini8, R Toner38, D Torretta1, G Tzanakos39, J Urheim11, P Vahle13, B Viren5, A Weber40, R C Webb41, C White34, L Whitehead42, L H Whitehead25, S G Wojcicki26, R Zwaska1.   

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.

Year:  2014        PMID： 24877929     DOI： 10.1103/PhysRevLett.112.191801

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN： 0031-9007            Impact factor:   9.161


  3 in total

1.  Neutrino physics: A deliberate mix-up in flavour.

Authors:  Helen O'Keeffe
Journal:  Nature       Date:  2016-05-19       Impact factor: 49.962

2.  Prospects for beyond the Standard Model physics searches at the Deep Underground Neutrino Experiment: DUNE Collaboration.

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Journal:  Eur Phys J C Part Fields       Date:  2021-04-16       Impact factor: 4.590

Review 3.  Neutrino oscillation studies with reactors.

Authors:  P Vogel; L J Wen; C Zhang
Journal:  Nat Commun       Date:  2015-04-27       Impact factor: 14.919
  3 in total

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