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1. Letter of interest for a neutrino beam from Protvino to KM3NeT/ORCA

Author

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. Enzenhöfer, M. Faifman, M. D. Filipović, L. Fusco, V. I. Garkusha, T. Gal, S. R. Gozzini, K. Graf, T. Grégoire, G. Grella, S. Hallmann, A. Heijboer, J. J. Hernández-Rey, J. Hofestädt, S. V. Ivanov, C. W. James, M. de Jong, P. de Jong, P. Kalaczyński, 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. Ó Fearraigh, M. Organokov, G. Papalashvili, M. Perrin-Terrin, C. Poirè, 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, and J. Zúñiga

Subjects
Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

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 $$\approx ~90~\hbox {kW}$$ ≈90kW . With a prolonged exposure ($$\approx 1500\hbox { kW}\,\,\hbox {year}$$ ≈1500kWyear ), a $$2\sigma $$ 2σ 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 $$6\sigma $$ 6σ sensitivity to CP violation and a $$10^\circ {-}17^\circ $$ 10∘-17∘ 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.

Published
2019
Full Text
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2. Letter of interest for a neutrino beam from Protvino to KM3NeT/ORCA

Author

Uli Katz, J. Aublin, A. V. Maximov, R. Bruijn, Alexander Zaitsev, J. Seneca, A. Sinopoulou, A. Domi, R. Yu. Sinyukov, M. Organokov, B. Ó Fearraigh, P. de Jong, O. P. Lebedev, N. R. Khan Chowdhury, Simona Maria Stellacci, E. G. Anassontzis, K. Melis, M. Colomer Molla, M. D. Skorokhvatov, M. Taiuti, C. Donzaud, Massimiliano Lincetto, Miguel Ardid, V. I. Garkusha, R. Le Breton, Vincent Bertin, L. Quinn, Vadim A. Naumov, I. Sokalski, C. Poirè, A. A. Sokolov, V. Kulikovskiy, F. N. Novoskoltsev, J.D. Zornoza, T. Thakore, S. V. Ivanov, D. Zaborov, B. Strandberg, T. Pradier, Mohamed Chabab, S. Sánchez Navas, S. R. Gozzini, E. Litvinovich, L. Nauta, K. S. Kuzmin, A. Creusot, Robert Muller, Matteo Sanguineti, E. Shirokov, Thomas Eberl, A. Kouchner, G. de Wasseige, Christos Markou, K. Graf, M. Kirsanov, C. W. James, A. Heijboer, A. V. Akindinov, D. Lopez-Coto, Miroslav Filipovic, Steffen Hallmann, C. Nielsen, T. Gal, T. Grégoire, G. Grella, A. S. Chepurnov, G. Papalashvili, D. F. E. Samtleben, N. Chau, L.A. Fusco, V. Van Elewyck, J. Hofestädt, J. Brunner, Juan José Hernández-Rey, E. A. De Wolf, S. Bourret, I. D. Kakorin, A. Enzenhöfer, P. Coyle, M. Faifman, Cristiano Bozza, Gisela Anton, E. Tzamariudaki, P. Kalaczynski, M. Perrin-Terrin, B. Baret, M. de Jong, M. Bruchner, B. Spisso, Rezo Shanidze, J. Zúñiga, KM3NeT (IHEF, IoP, FNWI), IHEF (IoP, FNWI), IoP (FNWI), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Ministerio de Ciencia, Innovación y Universidades (España)

Subjects
Sterile neutrino, Physics - Instrumentation and Detectors, Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, beam transport, particle source: design, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nucleon, Scattering, High Energy Physics - Experiment (hep-ex), [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Lepton polarization, neutrino oscillation, neutrino: mass, KM3NeT, Physics, P2O, neutrino: energy spectrum, Detector, phase: CP, near detector: design, Instrumentation and Detectors (physics.ins-det), p: beam, matter: effect, Total cross-section, CP violation, Neutrino, FOS: Physical sciences, lcsh:Astrophysics, neutrino: beam, Nuclear physics, Energy-Range, 0103 physical sciences, lcsh:QB460-466, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, Charged-Current interactions, 14. Life underwater, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Neutrino oscillation, numerical calculations, neutrino nucleon: scattering, Engineering (miscellaneous), Ratio, activity report, 010308 nuclear & particles physics, ORCA, Nu-Mu, neutrino: particle source, Deuterium, sensitivity, FISICA APLICADA, accelerator: upgrade, lcsh:QC770-798, Physics::Accelerator Physics, High Energy Physics::Experiment, Beam (structure)
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., Comment: 27 pages, 15 figures, 2 tables

Published
2019

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