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

**Authors:** The NOvA Collaboration: P. Adamson, L. Aliaga, D. Ambrose, N. Anfimov,, A. Antoshkin, E. Arrieta-Diaz, K. Augsten, A. Aurisano, C. Backhouse, M., Baird, B. A. Bambah, K. Bays, B. Behera, S. Bending, R. Bernstein, V., Bhatnagar, B. Bhuyan, J. Bian, T. Blackburn, A. Bolshakova, C. Bromberg, J., Brown, G. Brunetti, N. Buchanan, A. Butkevich, V. Bychkov, M. Campbell, E., Catano-Mur, S. Childress, B. C. Choudhary, B. Chowdhury, T. E. Coan, J. A. B., Coelho, M. Colo, J. Cooper, L. Corwin, L. Cremonesi, D. Cronin-Hennessy, G., S. Davies, J. P. Davies, P. F. Derwent, R. Dharmapalan, P. Ding, Z. Djurcic,, E. C. Dukes, H. Duyang, S. Edayath, R. Ehrlich, G. J. Feldman, M. J. Frank,, M. Gabrielyan, H. R. Gallagher, S. Germani, T. Ghosh, A. Giri, R. A. Gomes,, M. C. Goodman, V. Grichine, R. Group, D. Grover, B. Guo, A. Habig, J., Hartnell, R. Hatcher, A. Hatzikoutelis, K. Heller, A. Himmel, A. Holin, J., Hylen, F. Jediny, M. Judah, G. K. Kafka, D. Kalra, S. M. S. Kasahara, S., Kasetti, R. Keloth, L. Kolupaeva, S. Kotelnikov, I. Kourbanis, A. Kreymer, A., Kumar, S. Kurbanov, K. Lang, W. M. Lee, S. Lin, J. Liu, M. Lokajicek, J., Lozier, S. Luchuk, K. Maan, S. Magill, W. A. Mann, M. L. Marshak, K. Matera,, V. Matveev, D. P. M\'endez, M. D. Messier, H. Meyer, T. Miao, W. H. Miller,, S. R. Mishra, R. Mohanta, A. Moren, L. Mualem, M. Muether, S. Mufson, R., Murphy, J. Musser, J. K. Nelson, R. Nichol, E. Niner, A. Norman, T. Nosek, Y., Oksuzian, A. Olshevskiy, T. Olson, J. Paley, P. Pandey, R. B. Patterson, G., Pawloski, D. Pershey, O. Petrova, R. Petti, S. Phan-Budd, R. K. Plunkett, R., Poling, B. Potukuchi, C. Principato, F. Psihas, A. Radovic, R. A. Rameika, B., Rebel, B. Reed, D. Rocco, P. Rojas, V. Ryabov, K. Sachdev, P. Sail, O., Samoylov, M. C. Sanchez, R. Schroeter, J. Sepulveda-Quiroz, P. Shanahan, A., Sheshukov, J. Singh, J. Singh, P. Singh, V. Singh, J. Smolik, N. Solomey, E., Song, A. Sousa, K. Soustruznik, M. Strait, L. Suter, R. L. Talaga, M. C., Tamsett, P. Tas, R. B. Thayyullathil, J. Thomas, X. Tian, S. C. Tognini, J., Tripathi, A. Tsaris, J. Urheim, P. Vahle, J. Vasel, L. Vinton, A. Vold, T., Vrba, B. Wang, M. Wetstein, D. Whittington, S. G. Wojcicki, J. Wolcott, N., Yadav, S. Yang, J. Zalesak, B. Zamorano, R. Zwaska

arXiv: 1703.03328 · 2017-06-15

## TL;DR

This paper reports an improved measurement of neutrino oscillation parameters using NOvA data, constraining the neutrino mass hierarchy and mixing angles with high confidence.

## Contribution

The study provides new constraints on the neutrino mass hierarchy and mixing angles by combining $
u_e$ appearance and $
u_$ disappearance data with external reactor experiment results.

## Key findings

- Increased $
u_e$ candidate detection with background estimation.
- Disfavoring of inverted hierarchy with lower octant $	heta_{23}$ at >93% C.L.
- Enhanced constraints on $	heta_{13}$ and $	heta_{23}$ parameters.

## 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 $\delta_{CP}$.

## Full text

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## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1703.03328/full.md

## References

41 references — full list in the complete paper: https://tomesphere.com/paper/1703.03328/full.md

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Source: https://tomesphere.com/paper/1703.03328