# Letter of Interest for a Neutrino Beam from Protvino to KM3NeT/ORCA

**Authors:** A. V. Akindinov, E. G. Anassontzis, G. Anton, M. Ardid, J. Aublin, B., Baret, V. Bertin, S. Bourret, C. Bozza, M. Bruchner, R. Bruijn, J. Brunner,, M. Chabab, N. Chau, A. S. Chepurnov, M. Colomer Molla, P. Coyle, A. Creusot,, G. de Wasseige, A. Domi, C. Donzaud, T. Eberl, A. Enzenh\"ofer, M. Faifman,, M. D. Filipovi\'c, L. Fusco, V. I. Garkusha, T. Gal, S. R. Gozzini, K. Graf,, T. Gr\'egoire, G. Grella, S. Hallmann, A. Heijboer, J. J. Hern\'andez-Rey, J., Hofest\"adt, S. V. Ivanov, C. W. James, M. de Jong, P. de Jong, P., Kalaczy\'nski, I. D. Kakorin, U. F. Katz, N. R. Khan Chowdhury, M. M., Kirsanov, A. Kouchner, V. Kulikovskiy, K. S. Kuzmin, R. Le Breton, O. P., Lebedev, M. Lincetto, E. Litvinovich, D. Lopez-Coto, C. Markou, A. V., Maximov, K. W. Melis, R. Muller, V. A. Naumov, S. Navas, L. Nauta, C., Nielsen, F. N. Novoskoltsev, B. \'O Fearraigh, M. Organokov, G. Papalashvili,, M. Perrin-Terrin, C. Poir\`e, T. Pradier, L. Quinn, D. F. E. Samtleben, M., Sanguineti, J. Seneca, R. Shanidze, E. V. Shirokov, A. Sinopoulou, R. Yu., Sinyukov, M. D. Skorokhvatov, I. Sokalski, A. A. Sokolov, B. Spisso, S. M., Stellacci, B. Strandberg, M. Taiuti, T. Thakore, E. Tzamariudaki, V. Van, Elewyck, E. de Wolf, D. Zaborov, A. M. Zaitsev, J. D. Zornoza, J. Z\'u\~niga

arXiv: 1902.06083 · 2019-09-23

## TL;DR

This paper discusses a proposal to direct a neutrino beam from Protvino to the KM3NeT/ORCA detector, enabling high-sensitivity measurements of neutrino properties, including mass ordering and CP violation, with potential upgrades and additional experiments.

## Contribution

It introduces the P2O experiment concept, detailing its potential sensitivity to neutrino mass ordering and CP violation, and outlines plans for upgrades and supplementary measurements.

## Key findings

- High sensitivity to matter effects with 2595 km baseline.
- Potential to determine neutrino mass ordering within a few years.
- Capability to measure CP violation with increased exposure and detector upgrades.

## Abstract

The Protvino accelerator facility located in the Moscow region, Russia, is in a good position to offer a rich experimental research program in the field of neutrino physics. Of particular interest is the possibility to direct a neutrino beam from Protvino towards the KM3NeT/ORCA detector, which is currently under construction in the Mediterranean Sea 40 km offshore Toulon, France. This proposal is known as P2O. Thanks to its baseline of 2595 km, this experiment would yield an unparalleled sensitivity to matter effects in the Earth, allowing for the determination of the neutrino mass ordering with a high level of certainty after only a few years of running at a modest beam intensity of $\approx$ 90 kW. With a prolonged exposure ($\approx$ 1500 kW*yr), a 2$\sigma$ sensitivity to the leptonic CP-violating Dirac phase can be achieved. A second stage of the experiment, comprising a further intensity upgrade of the accelerator complex and a densified version of the ORCA detector (Super-ORCA), would allow for up to a 6$\sigma$ sensitivity to CP violation and a 10$^\circ$-17$^\circ$ resolution on the CP phase after 10 years of running with a 450 kW beam, competitive with other planned experiments. The initial composition and energy spectrum of the neutrino beam would need to be monitored by a near detector, to be constructed several hundred meters downstream from the proton beam target. The same neutrino beam and near detector set-up would also allow for neutrino-nucleus cross section measurements to be performed. A short-baseline sterile neutrino search experiment would also be possible.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1902.06083/full.md

## Figures

21 figures with captions in the complete paper: https://tomesphere.com/paper/1902.06083/full.md

## References

52 references — full list in the complete paper: https://tomesphere.com/paper/1902.06083/full.md

---
Source: https://tomesphere.com/paper/1902.06083