New constraints on oscillation parameters from νe appearance and νμ disappearance in the NOvA experiment

dc.contributor.author Acero, M. A.
dc.contributor.author Adamson, P.
dc.contributor.author Aliaga, L.
dc.contributor.author Alion, T.
dc.contributor.author Allakhverdian, V.
dc.contributor.author Anfimov, N.
dc.contributor.author Antoshkin, A.
dc.contributor.author Arrieta-Diaz, E.
dc.contributor.author Aurisano, A.
dc.contributor.author Back, A.
dc.contributor.author Backhouse, C.
dc.contributor.author Baird, M.
dc.contributor.author Balashov, N.
dc.contributor.author Bambah, B. A.
dc.contributor.author Bays, K.
dc.contributor.author Behera, B.
dc.contributor.author Bending, S.
dc.contributor.author Bernstein, R.
dc.contributor.author Bhatnagar, V.
dc.contributor.author Bhuyan, B.
dc.contributor.author Bian, J.
dc.contributor.author Blackburn, T.
dc.contributor.author Blair, J.
dc.contributor.author Bolshakova, A.
dc.contributor.author Bour, P.
dc.contributor.author Bromberg, C.
dc.contributor.author Brown, J.
dc.contributor.author Buchanan, N.
dc.contributor.author Butkevich, A.
dc.contributor.author Bychkov, V.
dc.contributor.author Campbell, M.
dc.contributor.author Carroll, T. J.
dc.contributor.author Catano-Mur, E.
dc.contributor.author Cedeno, A.
dc.contributor.author Childress, S.
dc.contributor.author Choudhary, B. C.
dc.contributor.author Chowdhury, B.
dc.contributor.author Coan, T. E.
dc.contributor.author Colo, M.
dc.contributor.author Cooper, J.
dc.contributor.author Corwin, L.
dc.contributor.author Cremonesi, L.
dc.contributor.author Cronin-Hennessy, D.
dc.contributor.author Davies, G. S.
dc.contributor.author Davies, J. P.
dc.contributor.author De Rijck, S.
dc.contributor.author Derwent, P. F.
dc.contributor.author Dharmapalan, R.
dc.contributor.author Ding, P.
dc.contributor.author Djurcic, Z.
dc.contributor.author Dukes, E. C.
dc.contributor.author Dung, P.
dc.contributor.author Duyang, H.
dc.contributor.author Edayath, S.
dc.contributor.author Ehrlich, R.
dc.contributor.author Feldman, G. J.
dc.contributor.author Frank, M. J.
dc.contributor.author Gallagher, H. R.
dc.contributor.author Gandrajula, R.
dc.contributor.author Gao, F.
dc.contributor.author Germani, S.
dc.contributor.author Giri, A.
dc.contributor.author Gomes, R. A.
dc.contributor.author Goodman, M. C.
dc.contributor.author Grichine, V.
dc.contributor.author Groh, M.
dc.contributor.author Group, R.
dc.contributor.author Grover, D.
dc.contributor.author Guo, B.
dc.contributor.author Habig, A.
dc.contributor.author Hakl, F.
dc.contributor.author Hartnell, J.
dc.contributor.author Hatcher, R.
dc.contributor.author Hatzikoutelis, A.
dc.contributor.author Heller, K.
dc.contributor.author Himmel, A.
dc.contributor.author Holin, A.
dc.contributor.author Howard, B.
dc.contributor.author Huang, J.
dc.contributor.author Hylen, J.
dc.contributor.author Jediny, F.
dc.contributor.author Judah, M.
dc.contributor.author Kakorin, I.
dc.contributor.author Kalra, D.
dc.contributor.author Kaplan, D. M.
dc.contributor.author Keloth, R.
dc.contributor.author Klimov, O.
dc.contributor.author Koerner, L. W.
dc.contributor.author Kolupaeva, L.
dc.contributor.author Kotelnikov, S.
dc.contributor.author Kourbanis, I.
dc.contributor.author Kreymer, A.
dc.contributor.author Kulenberg, Ch
dc.contributor.author Kumar, A.
dc.contributor.author Kuruppu, C.
dc.contributor.author Kus, V.
dc.contributor.author Lackey, T.
dc.contributor.author Lang, K.
dc.contributor.author Lin, S.
dc.contributor.author Lokajicek, M.
dc.date.accessioned 2022-03-27T11:55:21Z
dc.date.available 2022-03-27T11:55:21Z
dc.date.issued 2018-08-01
dc.description.abstract We present updated results from the NOvA experiment for νμ→νμ and νμ→νe oscillations from an exposure of 8.85×1020 protons on target, which represents an increase of 46% compared to our previous publication. The results utilize significant improvements in both the simulations and analysis of the data. A joint fit to the data for νμ disappearance and νe appearance gives the best-fit point as normal mass hierarchy, Δm322=2.44×10-3 eV2/c4, sin2θ23=0.56, and δCP=1.21π. The 68.3% confidence intervals in the normal mass hierarchy are Δm322[2.37,2.52]×10-3 eV2/c4, sin2θ23[0.43,0.51][0.52,0.60], and δCP[0,0.12π][0.91π,2π]. The inverted mass hierarchy is disfavored at the 95% confidence level for all choices of the other oscillation parameters.
dc.identifier.citation Physical Review D. v.98(3)
dc.identifier.issn 24700010
dc.identifier.uri 10.1103/PhysRevD.98.032012
dc.identifier.uri https://link.aps.org/doi/10.1103/PhysRevD.98.032012
dc.identifier.uri https://dspace.uohyd.ac.in/handle/1/15000
dc.title New constraints on oscillation parameters from νe appearance and νμ disappearance in the NOvA experiment
dc.type Journal. Article
dspace.entity.type
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