Title:
Constraints on Oscillation Parameters from νe Appearance and νμ Disappearance in NOvA

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dc.contributor.authorP. Adamson
dc.contributor.authorL. Aliaga
dc.contributor.authorD. Ambrose
dc.contributor.authorN. Anfimov
dc.contributor.authorA. Antoshkin
dc.contributor.authorE. Arrieta-Diaz
dc.contributor.authorK. Augsten
dc.contributor.authorA. Aurisano
dc.contributor.authorC. Backhouse
dc.contributor.authorM. Baird
dc.contributor.authorB.A. Bambah
dc.contributor.authorK. Bays
dc.contributor.authorB. Behera
dc.contributor.authorS. Bending
dc.contributor.authorR. Bernstein
dc.contributor.authorV. Bhatnagar
dc.contributor.authorB. Bhuyan
dc.contributor.authorJ. Bian
dc.contributor.authorT. Blackburn
dc.contributor.authorA. Bolshakova
dc.contributor.authorC. Bromberg
dc.contributor.authorJ. Brown
dc.contributor.authorG. Brunetti
dc.contributor.authorN. Buchanan
dc.contributor.authorA. Butkevich
dc.contributor.authorV. Bychkov
dc.contributor.authorM. Campbell
dc.contributor.authorE. Catano-Mur
dc.contributor.authorS. Childress
dc.contributor.authorB.C. Choudhary
dc.contributor.authorB. Chowdhury
dc.contributor.authorT.E. Coan
dc.contributor.authorJ.A.B. Coelho
dc.contributor.authorM. Colo
dc.contributor.authorJ. Cooper
dc.contributor.authorL. Corwin
dc.contributor.authorL. Cremonesi
dc.contributor.authorD. Cronin-Hennessy
dc.contributor.authorG.S. Davies
dc.contributor.authorJ.P. Davies
dc.contributor.authorP.F. Derwent
dc.contributor.authorR. Dharmapalan
dc.contributor.authorP. Ding
dc.contributor.authorZ. Djurcic
dc.contributor.authorE.C. Dukes
dc.contributor.authorH. Duyang
dc.contributor.authorS. Edayath
dc.contributor.authorR. Ehrlich
dc.contributor.authorG.J. Feldman
dc.contributor.authorM.J. Frank
dc.contributor.authorM. Gabrielyan
dc.contributor.authorH.R. Gallagher
dc.contributor.authorS. Germani
dc.contributor.authorT. Ghosh
dc.contributor.authorA. Giri
dc.contributor.authorR.A. Gomes
dc.contributor.authorM.C. Goodman
dc.contributor.authorV. Grichine
dc.contributor.authorR. Group
dc.contributor.authorD. Grover
dc.contributor.authorB. Guo
dc.contributor.authorA. Habig
dc.contributor.authorJ. Hartnell
dc.contributor.authorR. Hatcher
dc.contributor.authorA. Hatzikoutelis
dc.contributor.authorK. Heller
dc.contributor.authorA. Himmel
dc.contributor.authorA. Holin
dc.contributor.authorJ. Hylen
dc.contributor.authorF. Jediny
dc.contributor.authorM. Judah
dc.contributor.authorG.K. Kafka
dc.contributor.authorD. Kalra
dc.contributor.authorS.M.S. Kasahara
dc.contributor.authorS. Kasetti
dc.contributor.authorR. Keloth
dc.contributor.authorL. Kolupaeva
dc.contributor.authorS. Kotelnikov
dc.contributor.authorI. Kourbanis
dc.contributor.authorA. Kreymer
dc.contributor.authorA. Kumar
dc.contributor.authorS. Kurbanov
dc.contributor.authorK. Lang
dc.contributor.authorW.M. Lee
dc.contributor.authorS. Lin
dc.contributor.authorJ. Liu
dc.contributor.authorM. Lokajicek
dc.contributor.authorJ. Lozier
dc.contributor.authorS. Luchuk
dc.contributor.authorK. Maan
dc.contributor.authorS. Magill
dc.contributor.authorW.A. Mann
dc.contributor.authorM.L. Marshak
dc.contributor.authorK. Matera
dc.contributor.authorV. Matveev
dc.contributor.authorD.P. Méndez
dc.contributor.authorM.D. Messier
dc.contributor.authorH. Meyer
dc.contributor.authorT. Miao
dc.contributor.authorW.H. Miller
dc.contributor.authorS.R. Mishra
dc.contributor.authorR. Mohanta
dc.contributor.authorA. Moren
dc.contributor.authorL. Mualem
dc.contributor.authorM. Muether
dc.contributor.authorS. Mufson
dc.contributor.authorR. Murphy
dc.contributor.authorJ. Musser
dc.contributor.authorJ.K. Nelson
dc.contributor.authorR. Nichol
dc.contributor.authorE. Niner
dc.contributor.authorA. Norman
dc.contributor.authorT. Nosek
dc.contributor.authorY. Oksuzian
dc.contributor.authorA. Olshevskiy
dc.contributor.authorT. Olson
dc.contributor.authorJ. Paley
dc.contributor.authorP. Pandey
dc.contributor.authorR.B. Patterson
dc.contributor.authorG. Pawloski
dc.contributor.authorD. Pershey
dc.contributor.authorO. Petrova
dc.contributor.authorR. Petti
dc.contributor.authorS. Phan-Budd
dc.contributor.authorR.K. Plunkett
dc.contributor.authorR. Poling
dc.contributor.authorB. Potukuchi
dc.contributor.authorC. Principato
dc.contributor.authorF. Psihas
dc.contributor.authorA. Radovic
dc.contributor.authorR.A. Rameika
dc.contributor.authorB. Rebel
dc.contributor.authorB. Reed
dc.contributor.authorD. Rocco
dc.contributor.authorP. Rojas
dc.contributor.authorV. Ryabov
dc.contributor.authorK. Sachdev
dc.contributor.authorP. Sail
dc.contributor.authorO. Samoylov
dc.contributor.authorM.C. Sanchez
dc.contributor.authorR. Schroeter
dc.contributor.authorJ. Sepulveda-Quiroz
dc.contributor.authorP. Shanahan
dc.contributor.authorA. Sheshukov
dc.contributor.authorJ. Singh
dc.contributor.authorJ. Singh
dc.contributor.authorP. Singh
dc.contributor.authorV. Singh
dc.contributor.authorJ. Smolik
dc.contributor.authorN. Solomey
dc.contributor.authorE. Song
dc.contributor.authorA. Sousa
dc.contributor.authorK. Soustruznik
dc.contributor.authorM. Strait
dc.contributor.authorL. Suter
dc.contributor.authorR.L. Talaga
dc.contributor.authorM.C. Tamsett
dc.contributor.authorP. Tas
dc.contributor.authorR.B. Thayyullathil
dc.contributor.authorJ. Thomas
dc.contributor.authorX. Tian
dc.contributor.authorS.C. Tognini
dc.contributor.authorJ. Tripathi
dc.contributor.authorA. Tsaris
dc.contributor.authorJ. Urheim
dc.contributor.authorP. Vahle
dc.contributor.authorJ. Vasel
dc.contributor.authorL. Vinton
dc.contributor.authorA. Vold
dc.contributor.authorT. Vrba
dc.contributor.authorB. Wang
dc.contributor.authorM. Wetstein
dc.contributor.authorD. Whittington
dc.contributor.authorS.G. Wojcicki
dc.contributor.authorJ. Wolcott
dc.contributor.authorN. Yadav
dc.contributor.authorS. Yang
dc.contributor.authorJ. Zalesak
dc.contributor.authorB. Zamorano
dc.contributor.authorR. Zwaska
dc.date.accessioned2026-02-07T08:30:12Z
dc.date.issued2017
dc.description.abstractResults are reported from an improved measurement of νμ→νe transitions by the NOvA experiment. Using an exposure equivalent to 6.05×1020 protons on target, 33 νe candidates are observed with a background of 8.2±0.8 (syst.). Combined with the latest NOvA νμ disappearance data and external constraints from reactor experiments on sin22θ13, the hypothesis of inverted mass hierarchy with θ23 in the lower octant is disfavored at greater than 93% C.L. for all values of δCP. © 2017 American Physical Society.
dc.identifier.doi10.1103/PhysRevLett.118.231801
dc.identifier.issn319007
dc.identifier.urihttps://doi.org/10.1103/PhysRevLett.118.231801
dc.identifier.urihttps://dl.bhu.ac.in/bhuir/handle/123456789/30583
dc.publisherAmerican Physical Society
dc.titleConstraints on Oscillation Parameters from νe Appearance and νμ Disappearance in NOvA
dc.typePublication
dspace.entity.typeArticle

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