# First measurement of neutrino oscillation parameters using neutrinos and   antineutrinos by NOvA

**Authors:** M. A. Acero, P. Adamson, L. Aliaga, T. Alion, V. Allakhverdian, S., Altakarli, N. Anfimov, A. Antoshkin, A. Aurisano, A. Back, C. Backhouse, M., Baird, N. Balashov, P. Baldi, B. A. Bambah, S. Bashar, K. Bays, S. Bending,, R. Bernstein, V. Bhatnagar, B. Bhuyan, J. Bian, T. Blackburn, J. Blair, A. C., Booth, P. Bour, C. Bromberg, N. Buchanan, A. Butkevich, S. Calvez, M., Campbell, T. J. Carroll, E. Catano-Mur, A. Cedeno, S. Childress, B. C., Choudhary, B. Chowdhury, T. E. Coan, M. Colo, J. Cooper, L. Corwin, L., Cremonesi, G. S. Davies, P. F. Derwent, P. Ding, Z. Djurcic, D. Doyle, E. C., Dukes, H. Duyang, S. Edayath, R. Ehrlich, M. Elkins, G. J. Feldman, P. Filip,, W. Flanagan, M. J. Frank, H. R. Gallagher, R. Gandrajula, F. Gao, S. Germani,, A. Giri, R. A. Gomes, M. C. Goodman, V. Grichine, M. Groh, R. Group, B. Guo,, A. Habig, F. Hakl, J. Hartnell, R. Hatcher, A. Hatzikoutelis, K. Heller, V, Hewes, A. Himmel, A. Holin, B. Howard, J. Huang, J. Hylen, F. Jediny, C., Johnson, M. Judah, I. Kakorin, D. Kalra, D. M. Kaplan, R. Keloth, O. Klimov,, L. W. Koerner, L. Kolupaeva, S. Kotelnikov, A. Kreymer, Ch. Kulenberg, A., Kumar, C. D. Kuruppu, V. Kus, T. Lackey, K. Lang, S. Lin, M. Lokajicek, J., Lozier, S. Luchuk, K. Maan, S. Magill, W. A. Mann, M. L. Marshak, M., Martinez-Casales, V. Matveev, D. P. Mendez, M. D. Messier, H. Meyer, T. Miao,, W. H. Miller, S. R. Mishra, A. Mislivec, R. Mohanta, A. Moren, L. Mualem, M., Muether, S. Mufson, K. Mulder, R. Murphy, J. Musser, D. Naples, N. Nayak, J., K. Nelson, R. Nichol, G. Nikseresht, E. Niner, A. Norman, T. Nosek, A., Olshevskiy, T. Olson, J. Paley, R. B. Patterson, G. Pawloski, D. Pershey, O., Petrova, R. Petti, D. D. Phan, R. K. Plunkett, B. Potukuchi, C. Principato,, F. Psihas, A. Radovic, V. Raj, R. A. Rameika, B. Rebel, P. Rojas, V. Ryabov,, O. Samoylov, M. C. Sanchez, S. Sanchez Falero, I. S. Seong, P. Shanahan, A., Sheshukov, P. Singh, V. Singh, E. Smith, J. Smolik, P. Snopok, N. Solomey, E., Song, A. Sousa, K. Soustruznik, M. Strait, L. Suter, A. Sutton, R. L. Talaga,, B. Tapia Oregui, P. Tas, R. B. Thayyullathil, J. Thomas, E. Tiras, D., Torbunov, J. Tripathi, A. Tsaris, Y. Torun, J. Urheim, P. Vahle, J. Vasel, L., Vinton, P. Vokac, T. Vrba, M. Wallbank, B. Wang, T. K. Warburton, M., Wetstein, M. While, D. Whittington, S. G. Wojcicki, J. Wolcott, N. Yadav, A., Yallappa Dombara, K. Yonehara, S. Yu, S. Zadorozhnyy, J. Zalesak, B., Zamorano, R. Zwaska (NOvA Collaboration)

arXiv: 1906.04907 · 2023-02-18

## TL;DR

The NOvA experiment has for the first time measured neutrino oscillation parameters using both neutrinos and antineutrinos, providing new insights into neutrino properties and mass hierarchy.

## Contribution

This paper presents the first combined measurement of neutrino and antineutrino oscillation parameters by NOvA, improving understanding of neutrino mass hierarchy and mixing angles.

## Key findings

- Measured $|	riangle m^2_{32}|$ with high precision
- Favored normal neutrino mass hierarchy by 1.9$\sigma$
- Excluded most $\delta_{CP}$ values near $rac{\pi}{2}$ for inverted hierarchy

## Abstract

The NOvA experiment has made a $4.4\sigma$-significant observation of $\bar\nu_{e}$ appearance in a 2 GeV $\bar\nu_{\mu}$ beam at a distance of 810 km. Using $12.33\times10^{20}$ protons on target delivered to the Fermilab NuMI neutrino beamline, the experiment recorded 27 $\bar\nu_{\mu} \rightarrow \bar\nu_{e}$ candidates with a background of 10.3 and 102 $\bar\nu_{\mu} \rightarrow \bar\nu_{\mu}$ candidates. This new antineutrino data is combined with neutrino data to measure the oscillation parameters $|\Delta m^2_{32}| = 2.48^{+0.11}_{-0.06}\times10^{-3}$ eV$^2/c^4$, $\sin^2 \theta_{23} = 0.56^{+0.04}_{-0.03}$ in the normal neutrino mass hierarchy and upper octant and excludes most values near $\delta_{\rm CP}=\pi/2$ for the inverted mass hierarchy by more than 3$\sigma$. The data favor the normal neutrino mass hierarchy by 1.9$\sigma$ and $\theta_{23}$ values in the upper octant by 1.6$\sigma$.

## Full text

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## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1906.04907/full.md

## References

67 references — full list in the complete paper: https://tomesphere.com/paper/1906.04907/full.md

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Source: https://tomesphere.com/paper/1906.04907