BibTex format

author = {Acero, MA and Adamson, P and Aliaga, L and Anfimov, N and Antoshkin, A and Arrieta-Diaz, E and Asquith, L and Aurisano, A and Back, A and Backhouse, C and Baird, M and Balashov, N and Baldi, P and Bambah, BA and Bashar, S and Bays, K and Bernstein, R and Bhatnagar, V and Bhattarai, D and Bhuyan, B and Bian, J and Blair, J and Booth, AC and Bowles, R and Bromberg, C and Buchanan, N and Butkevich, A and Calvez, S and Carroll, TJ and Catano-Mur, E and Choudhary, BC and Christensen, A and Coan, TE and Colo, M and Cremonesi, L and Davies, GS and Derwent, PF and Ding, P and Djurcic, Z and Dolce, M and Doyle, D and Dueñas, Tonguino D and Dukes, EC and Duyang, H and Ehrlich, R and Elkins, M and Ewart, E and Feldman, GJ and Filip, P and Franc, J and Frank, MJ and Gallagher, HR and Gandrajula, R and Gao, F and Giri, A and Gomes, RA and Goodman, MC and Grichine, V and Groh, M and Group, R and Guo, B and Habig, A and Hakl, F and Hall, A and Hartnell, J and Hatcher, R and Hausner, H and He, M and H},
doi = {10.1103/PhysRevD.106.032004},
journal = {Physical Review D},
title = {Improved measurement of neutrino oscillation parameters by the NOvA experiment},
url = {},
volume = {106},
year = {2022}

RIS format (EndNote, RefMan)

AB - We present new νμ→νe, νμ→νμ, ν¯μ→ν¯e, and ν¯μ→ν¯μ oscillation measurements by the NOvA experiment, with a 50% increase in neutrino-mode beam exposure over the previously reported results. The additional data, combined with previously published neutrino and antineutrino data, are all analyzed using improved techniques and simulations. A joint fit to the νe, νμ, ν¯e, and ν¯μ candidate samples within the 3-flavor neutrino oscillation framework continues to yield a best-fit point in the normal mass ordering and the upper octant of the θ23 mixing angle, with Δm322=(2.41±0.07)×10-3 eV2 and sin2θ23=0.57-0.04+0.03. The data disfavor combinations of oscillation parameters that give rise to a large asymmetry in the rates of νe and ν¯e appearance. This includes values of the charge parity symmetry (CP) violating phase in the vicinity of δCP=π/2 which are excluded by >3σ for the inverted mass ordering, and values around δCP=3π/2 in the normal ordering which are disfavored at 2σ confidence.
AU - Acero,MA
AU - Adamson,P
AU - Aliaga,L
AU - Anfimov,N
AU - Antoshkin,A
AU - Arrieta-Diaz,E
AU - Asquith,L
AU - Aurisano,A
AU - Back,A
AU - Backhouse,C
AU - Baird,M
AU - Balashov,N
AU - Baldi,P
AU - Bambah,BA
AU - Bashar,S
AU - Bays,K
AU - Bernstein,R
AU - Bhatnagar,V
AU - Bhattarai,D
AU - Bhuyan,B
AU - Bian,J
AU - Blair,J
AU - Booth,AC
AU - Bowles,R
AU - Bromberg,C
AU - Buchanan,N
AU - Butkevich,A
AU - Calvez,S
AU - Carroll,TJ
AU - Catano-Mur,E
AU - Choudhary,BC
AU - Christensen,A
AU - Coan,TE
AU - Colo,M
AU - Cremonesi,L
AU - Davies,GS
AU - Derwent,PF
AU - Ding,P
AU - Djurcic,Z
AU - Dolce,M
AU - Doyle,D
AU - Dueñas,Tonguino D
AU - Dukes,EC
AU - Duyang,H
AU - Ehrlich,R
AU - Elkins,M
AU - Ewart,E
AU - Feldman,GJ
AU - Filip,P
AU - Franc,J
AU - Frank,MJ
AU - Gallagher,HR
AU - Gandrajula,R
AU - Gao,F
AU - Giri,A
AU - Gomes,RA
AU - Goodman,MC
AU - Grichine,V
AU - Groh,M
AU - Group,R
AU - Guo,B
AU - Habig,A
AU - Hakl,F
AU - Hall,A
AU - Hartnell,J
AU - Hatcher,R
AU - Hausner,H
AU - He,M
AU - Heller,K
AU - Hewes,J
AU - Himmel,A
AU - Holin,A
AU - Huang,J
AU - Jargowsky,B
AU - Jarosz,J
AU - Jediny,F
AU - Johnson,C
AU - Judah,M
AU - Kakorin,I
AU - Kaplan,DM
AU - Kalitkina,A
AU - Keloth,R
AU - Klimov,O
AU - Koerner,LW
AU - Kolupaeva,L
AU - Kotelnikov,S
AU - Kralik,R
AU - Kullenberg,C
AU - Kubu,M
AU - Kumar,A
AU - Kuruppu,CD
AU - Kus,V
AU - Lackey,T
AU - Lang,K
AU - Lasorak,P
AU - Lesmeister,J
AU - Lin,S
AU - Lister,A
AU - Liu,J
AU - Lokajicek,M
DO - 10.1103/PhysRevD.106.032004
PY - 2022///
SN - 2470-0010
TI - Improved measurement of neutrino oscillation parameters by the NOvA experiment
T2 - Physical Review D
UR -
VL - 106
ER -