Constraints on Oscillation Parameters from ν_{e} Appearance and ν_{μ} Disappearance in NOvA.

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, Null Null

PHYSICAL REVIEW LETTERS(2017)

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摘要
Results are reported from an improved measurement of nu(mu) -> nu(e) transitions by the NOvA experiment. Using an exposure equivalent to 6.05 x 10(20) protons on target, 33 nu(e) candidates are observed with a background of 8.2 +/- 0.8 (syst.). Combined with the latest NOvA nu(mu) disappearance data and external constraints from reactor experiments on sin(2) 2 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).
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