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Constraints on Oscillation Parameters from $\nu_e$ Appearance and $\nu_\mu$ Disappearance in NOvA

Authors :
The NOvA Collaboration
Adamson, P.
Aliaga, L.
Ambrose, D.
Anfimov, N.
Antoshkin, A.
Arrieta-Diaz, E.
Augsten, K.
Aurisano, A.
Backhouse, C.
Baird, M.
Bambah, B. A.
Bays, K.
Behera, B.
Bending, S.
Bernstein, R.
Bhatnagar, V.
Bhuyan, B.
Bian, J.
Blackburn, T.
Bolshakova, A.
Bromberg, C.
Brown, J.
Brunetti, G.
Buchanan, N.
Butkevich, A.
Bychkov, V.
Campbell, M.
Catano-Mur, E.
Childress, S.
Choudhary, B. C.
Chowdhury, B.
Coan, T. E.
Coelho, J. A. B.
Colo, M.
Cooper, J.
Corwin, L.
Cremonesi, L.
Cronin-Hennessy, D.
Davies, G. S.
Davies, J. P.
Derwent, P. F.
Dharmapalan, R.
Ding, P.
Djurcic, Z.
Dukes, E. C.
Duyang, H.
Edayath, S.
Ehrlich, R.
Feldman, G. J.
Frank, M. J.
Gabrielyan, M.
Gallagher, H. R.
Germani, S.
Ghosh, T.
Giri, A.
Gomes, R. A.
Goodman, M. C.
Grichine, V.
Group, R.
Grover, D.
Guo, B.
Habig, A.
Hartnell, J.
Hatcher, R.
Hatzikoutelis, A.
Heller, K.
Himmel, A.
Holin, A.
Hylen, J.
Jediny, F.
Judah, M.
Kafka, G. K.
Kalra, D.
Kasahara, S. M. S.
Kasetti, S.
Keloth, R.
Kolupaeva, L.
Kotelnikov, S.
Kourbanis, I.
Kreymer, A.
Kumar, A.
Kurbanov, S.
Lang, K.
Lee, W. M.
Lin, S.
Liu, J.
Lokajicek, M.
Lozier, J.
Luchuk, S.
Maan, K.
Magill, S.
Mann, W. A.
Marshak, M. L.
Matera, K.
Matveev, V.
Méndez, D. P.
Messier, M. D.
Meyer, H.
Miao, T.
Miller, W. H.
Mishra, S. R.
Mohanta, R.
Moren, A.
Mualem, L.
Muether, M.
Mufson, S.
Murphy, R.
Musser, J.
Nelson, J. K.
Nichol, R.
Niner, E.
Norman, A.
Nosek, T.
Oksuzian, Y.
Olshevskiy, A.
Olson, T.
Paley, J.
Pandey, P.
Patterson, R. B.
Pawloski, G.
Pershey, D.
Petrova, O.
Petti, R.
Phan-Budd, S.
Plunkett, R. K.
Poling, R.
Potukuchi, B.
Principato, C.
Psihas, F.
Radovic, A.
Rameika, R. A.
Rebel, B.
Reed, B.
Rocco, D.
Rojas, P.
Ryabov, V.
Sachdev, K.
Sail, P.
Samoylov, O.
Sanchez, M. C.
Schroeter, R.
Sepulveda-Quiroz, J.
Shanahan, P.
Sheshukov, A.
Singh, J.
Singh, P.
Singh, V.
Smolik, J.
Solomey, N.
Song, E.
Sousa, A.
Soustruznik, K.
Strait, M.
Suter, L.
Talaga, R. L.
Tamsett, M. C.
Tas, P.
Thayyullathil, R. B.
Thomas, J.
Tian, X.
Tognini, S. C.
Tripathi, J.
Tsaris, A.
Urheim, J.
Vahle, P.
Vasel, J.
Vinton, L.
Vold, A.
Vrba, T.
Wang, B.
Wetstein, M.
Whittington, D.
Wojcicki, S. G.
Wolcott, J.
Yadav, N.
Yang, S.
Zalesak, J.
Zamorano, B.
Zwaska, R.
Source :
Phys. Rev. Lett. 118, 231801 (2017)
Publication Year :
2017

Abstract

Results are reported from an improved measurement of $\nu_\mu \rightarrow \nu_e$ transitions by the NOvA experiment. Using an exposure equivalent to $6.05\times10^{20}$ protons-on-target 33 $\nu_e$ candidates were observed with a background of $8.2\pm0.8$ (syst.). Combined with the latest NOvA $\nu_\mu$ disappearance data and external constraints from reactor experiments on $\sin^22\theta_{13}$, the hypothesis of inverted mass hierarchy with $\theta_{23}$ in the lower octant is disfavored at greater than $93\%$ C.L. for all values of $\delta_{CP}$.<br />Comment: 6 pages, 4 figures

Subjects

Subjects :
High Energy Physics - Experiment

Details

Database :
arXiv
Journal :
Phys. Rev. Lett. 118, 231801 (2017)
Publication Type :
Report
Accession number :
edsarx.1703.03328
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevLett.118.231801