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Proceeding Paper

The ENUBET Monitored Neutrino Beam for High Precision Cross-Section Measurements †

by
C.C. Delogu
1,2,*,
F. Acerbi
3,
I. Angelis
4,
L. Bomben
5,6,
M. Bonesini
6,
F. Bramati
6,7,
A. Branca
6,7,
C. Brizzolari
6,7,
G. Brunetti
6,7,
M. Calviani
8,
S. Capelli
5,6,
S. Carturan
9,
M.G. Catanesi
10,
S. Cecchini
11,
N. Charitonidis
8,
F. Cindolo
11,
G. Cogo
2,
G. Collazuol
1,2,
F. Dal Corso
1,
G. De Rosa
12,
A. Falcone
6,7,
B. Goddard
8,
A. Gola
3,
L. Halić
13,
F. Iacob
1,2,
C. Jollet
14,15,
V. Kain
8,
A. Kallitsopoulou
16,
B. Klicek
13,
Y. Kudenko
17,
Ch. Lampoudis
4,
M. Laveder
1,2,
P. Legou
16,
A. Longhin
1,2,
L. Ludovici
18,
E. Lutsenko
5,6,
L. Magaletti
10,
G. Mandrioli
11,
S. Marangoni
6,7,
A. Margotti
11,
V. Mascagna
19,20,
N. Mauri
11,
L. Meazza
6,7,
A. Meregaglia
21,
M. Mezzetto
1,
M. Nessi
8,
A. Paoloni
22,
M. Pari
1,2,
T. Papaevangelou
16,
E.G. Parozzi
6,7,
L. Pasqualini
11,23,
G. Paternoster
3,
L. Patrizii
11,
M. Pozzato
11,
M. Prest
5,6,
F. Pupilli
1,
E. Radicioni
10,
A.C. Ruggeri
12,
D. Sampsonidis
4,
C. Scian
2,
G. Sirri
11,
M. Stipcevic
13,
M. Tenti
11,
F. Terranova
6,7,
M. Torti
6,7,
S.E. Tzamarias
4,
E. Vallazza
6,
F. Velotti
8 and
L. Votano
22
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1
INFN (Istituto Nazionale di Fisica Nucleare)–Sezione di Padova, Via Marzolo 8, 35131 Padova, Italy
2
Physics Department, Università di Padova, Via Marzolo 8, 35131 Padova, Italy
3
Fondazione Bruno Kessler (FBK), INFN (Istituto Nazionale di Fisica Nucleare) and Trento Institute for Fundamental Physics and Applications, 38123 Trento, Italy
4
Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
5
Dipartimento di Scienza e Alta Tecnologia, Università degli studi dell’Insubria, Via Valleggio 11, 22100 Como, Italy
6
INFN (Istituto Nazionale di Fisica Nucleare), Sezione di Milano-Bicocca, Piazza Della Scienza 3, 20126 Milano, Italy
7
Physics Department, Università di Milano-Bicocca, Piazza Della Scienza 3, 20126 Milano, Italy
8
CERN (Conseil Européen pour la Recherche Nucléaire), 1217 Geneva, Switzerland
9
INFN Laboratori Nazionali di Legnaro, Viale dell’Università 2, 35020 Legnaro, Italy
10
INFN (Istituto Nazionale di Fisica Nucleare)–Sezione di Bari, Via Amendola 173, 70126 Bari, Italy
11
INFN (Istituto Nazionale di Fisica Nucleare)–Sezione di Bologna, Viale Berti-Pichat 6/2, 40127 Bologna, Italy
12
INFN (Istituto Nazionale di Fisica Nucleare)–Sezione di Napoli, Via Cinthia, 80126 Napoli, Italy
13
Center of Excellence for Advanced Materials and Sensing Devices, Ruder Boskovic Institute, 10000 Zagreb, Croatia
14
Institut pluridisciplinaire Hubert Curien, Université de Strasbourg, CNRS/IN2P3, 67200 Strasbourg, France
15
Centre de Etudes Nucleaires de Bordeaux Gradignan, 19 Chemin du Solarium, 33170 Bordeaux, France
16
CEA, Centre de Saclay, Irfu/SPP, 91191 Gif-sur-Yvette, France
17
Institute of Nuclear Research, Russian Academy of Science, 119991 Moscow, Russia
18
INFN (Istituto Nazionale di Fisica Nucleare)–Sezione di Roma 1, piazzale A. Moro 2, 00185 Rome, Italy
19
Dipartimento di Ingegneria dell’Informazione, Università Degli Studi di Brescia, Via Branze 38, 25121 Brescia, Italy
20
INFN (Istituto Nazionale di Fisica Nucleare)–Sezione di Pavia, Via Bassi 6, 27100 Pavia, Italy
21
Centre d’Etudes Nucléaires de Bordeaux-Gradignan, Université de Bordeaux, CNRS/IN2P3, 33175 Gradignan, France
22
INFN Laboratori Nazionali di Frascati, Via Fermi 40, 00044 Frascati, Italy
23
Physics Department, Università di Bologna, Viale Berti-Pichat 6/2, 40127 Bologna, Italy
*
Author to whom correspondence should be addressed.
Presented at the 23rd International Workshop on Neutrinos from Accelerators, Salt Lake City, UT, USA, 30–31 July 2022.
Phys. Sci. Forum 2023, 8(1), 8; https://doi.org/10.3390/psf2023008008
Published: 30 June 2023
(This article belongs to the Proceedings of The 23rd International Workshop on Neutrinos from Accelerators)

Abstract

:
The main source of systematic uncertainty on neutrino cross-section measurements at the GeV scale originates from the poor knowledge of the initial flux. The goal of reducing this uncertainty to 1% can be achieved through the monitoring of charged leptons produced in association with neutrinos, by properly instrumenting the decay region of a conventional narrow-band neutrino beam. Large-angle muons and positrons from kaons are measured by a sampling calorimeter on the decay tunnel walls, while muon stations after the hadron dump can be used to monitor the neutrino component from pion decays. Furthermore, the narrow momentum width (<10%) of the beam provides a O (10%) measurement of the neutrino energy on an event-by-event basis, thanks to its correlation with the radial position of the interaction at the neutrino detector. The ENUBET project has been funded by the ERC in 2016 to prove the feasibility of such a monitored neutrino beam and, since 2019, ENUBET is also a CERN neutrino platform experiment (NP06/ENUBET). The breakthrough the project achieved is the design of a horn-less neutrino beamline that would allow for a 1% measurement of ν e and ν μ cross-sections in about 3 years of data taking at CERN-SPS, using ProtoDUNE as far detector.

1. Introduction

The knowledge of the initial flux in conventional neutrino beams is the primary source of systematic error on the neutrino cross-section. ENUBET’s goal is to develop a so-called “monitored neutrino beam”, in which a controlled neutrino flux can be obtained by monitoring the charged leptons from meson decays along an instrumented decay region (the “tagger”) [1]. In June 2016, ENUBET started as an ERC project with the goal of designing a facility for the measurement of large angle positrons from K e 3 decay ( K + e + ν e π 0 ), allowing it to constrain the ν e flux. The project’s primary purpose was then extended, considering the possibility of measuring large-angle muons from the two-body K μ 2 and K μ 3 decays of the kaons ( K + μ + ν μ and K + μ + π 0 ν μ ), as well as the small angle ones from the pion decays ( π + μ + ν μ ) by instrumenting the region after the hadron dump. The physics goal of ENUBET is to use this monitoring technique to reduce below 1% the uncertainty on the ν e and ν μ fluxes and to perform high-precision cross-section measurements, thus boosting the physics potential of next-generation oscillation experiments by reducing their systematic uncertainties.

2. The ENUBET Beamline

The ENUBET beamline is designed as a narrow band secondary beamline relying on normal-conducting magnets. When protons hit a target, they generate secondaries that are sign- and momentum-selected all the way to the instrumented decay tunnel. The transfer line is kept short (about 20 m) to enhance the kaon component, and focuses the mesons with a design momentum of 8.5 G e V / c ± 5 10 % . This is an ideal choice for the e + / π + separation and to span the region of interest for the neutrino energy in DUNE and HyperK. In the most recent design, the transfer line relies on a quadrupole triplet for the initial focusing of the secondaries from the target, followed by a double-bend momentum selection section and additional quadrupoles for constraining the beam envelope: an overview is shown in Figure 1.
The background ν e component at the neutrino detector coming from early kaon decays in the first half of the transfer line is reduced thanks to the bending angle. The facility has been simulated in G4beamline, FLUKA and GEANT4 [2]. According to simulation results, the kaon flux at the tunnel entrance increased in comparison to transfer line designs reported in the past years. Figure 2 shows the most recent simulated fluxes at the entrance of the decay tunnel and the ν spectra at the far detector. The results in terms of neutrino flux would allow us to detect 10 4 ν e C C in about 3 years of data taking, assuming a 500 t, 6 × 6 m 2 LAr detector 50 m away from the end of the beamline.
The latest design has been improved thanks to an extensive optimization campaign that employed a generic optimization framework based on a genetic algorithm. More details on this and on the beamline design features can be found in [3].

3. Tunnel Instrumentation

The ENUBET decay tunnel will be instrumented with a modular sampling calorimeter for positron and muon tagging and e + / μ / π + separation. The tunnel walls are instrumented by three radial layers of LCM (Lateral Compact Modules): sampling calorimeter units of 9 cm 2 transverse area composed by five couples of iron (1.5 cm thick) and plastic scintillator (0.7 cm thick) tiles for a total of 11 cm and 4.3 X 0 in the longitudinal direction. The light is collected using wavelength shifting (WLS) fibers and read out using SiPMs. Rings made of doublets of scintillator tiles (the “t0 layer”) positioned in the inner tunnel surface act as photon veto, allowing for e + / π 0 separation. Figure 3a shows a schematic of the ENUBET event topology.
Prototypes were tested in the CERN East Area to evaluate the physics performance, particularly the separation capabilities for e + / π + and e + / π 0 , as discussed in [4]. The light readout system has been studied in detail and the latest designs were tested on a small prototype of the tagger instrumentation (ENUBINO), in terms of efficiency and uniformity of response. A final demonstrator 1.65 m long and spanning 90° in azimuth (Figure 3b) was built at the INFN-LNL and it has been tested in October 2022 [5].

4. Particle Reconstruction and Assessment of Systematics

The ENUBET facility has been fully simulated using GEANT4, including particle propagation and decay from the transfer line to the detector, hit level detector response, and pile-up effects. Data from the prototype testing at CERN have been used to validate the simulation.
The analysis chain starts with the event builder algorithm, followed by a neural-network-based signal/background separation step [6]. The achieved particle identification performance is:
  • 22% efficiency for K e 3 signal events, with a S/N of 2;
  • 34% efficiency for K μ 2 signal events, with a S/N of 6.
The design of an instrumented hadron dump for the detection of muons from pion decays is under study.
The systematics of neutrino flux are evaluated by employing the relationship between leptons identified in the calorimeter and neutrino flux at the detector. Using the lepton distributions for the observables reported in Figure 4, a signal plus background model that includes a priori hadro-production (HP) and transfer-line-related systematics is constructed. Toy-MC experiments are created and fitted to analyze the systematic uncertainty a posteriori and evaluate the resulting uncertainty reduction. Reweighting the simulation eventually causes the systematic errors to be propagated to the neutrino flux [7]. The main factors contributing to the uncertainty on the neutrino flux include uncertainties in hadro-production (HP), systematics associated with the calorimeter (energy calibration, scintillator aging), and uncertainties in the nominal magnet current. For now, only HP uncertainties have been used for the computation, as they represent the major contribution to the flux uncertainty. The other (minor) components will also be included in the future. Thanks to the ENUBET instrumented tunnel, a successful reduction of the neutrino flux systematics from 10% down to the 1% level has been reached.

Author Contributions

All authors have read and agreed to the published version of the manuscript.

Funding

This project has received funding from the European Research Council (ERC) under the European Unions Horizon 2020 research and innovation programme (grant agreement N. 681647) and by the Italian Ministry of Education and Research—MIUR (Bando “FARE”, progetto NUTECH).

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

Not applicable.

Conflicts of Interest

The authors declare no conflict of interest.

References

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Figure 1. Latest beamline design. Focusing quadrupoles and bending dipoles are shown in gray and orange, respectively. Collimators are made of Iron (blue) or Inermet180 (violet). The decay tunnel (yellow), the hadron dump (light grey) and the proton dump (green) are also shown.
Figure 1. Latest beamline design. Focusing quadrupoles and bending dipoles are shown in gray and orange, respectively. Collimators are made of Iron (blue) or Inermet180 (violet). The decay tunnel (yellow), the hadron dump (light grey) and the proton dump (green) are also shown.
Psf 08 00008 g001
Figure 2. (a) Particle budget at the decay tunnel entrance. The rates obtained for a momentum of 8.5 ± 5% GeV are 4.13 × 10 3 π + / POT and 0.34 × 10 3 K + / POT . (b) Energy spectrum of the ν e C C interactions in the neutrino detector. Colored lines represent the neutrino contribution generated in a specific area of the transfer line, with the neutrinos generated inside the tagger (in red) representing ∼80% of spectrum above 1 GeV. The most relevant component below this threshold is the one coming from the proton dump (in cyan), whose position and shape are still to be fine−tuned.
Figure 2. (a) Particle budget at the decay tunnel entrance. The rates obtained for a momentum of 8.5 ± 5% GeV are 4.13 × 10 3 π + / POT and 0.34 × 10 3 K + / POT . (b) Energy spectrum of the ν e C C interactions in the neutrino detector. Colored lines represent the neutrino contribution generated in a specific area of the transfer line, with the neutrinos generated inside the tagger (in red) representing ∼80% of spectrum above 1 GeV. The most relevant component below this threshold is the one coming from the proton dump (in cyan), whose position and shape are still to be fine−tuned.
Psf 08 00008 g002
Figure 3. (a) Event topology for the ENUBET calorimeter. EM shower from a positron, top; EM shower from a π 0 , middle; hadronic shower from a π + , bottom. The modules involved in a typical e + , π 0 or π + event are marked in red. In the π 0 case, photons coming from its decay do not leave any signal in the t0 doublet. (b) The demonstrator.
Figure 3. (a) Event topology for the ENUBET calorimeter. EM shower from a positron, top; EM shower from a π 0 , middle; hadronic shower from a π + , bottom. The modules involved in a typical e + , π 0 or π + event are marked in red. In the π 0 case, photons coming from its decay do not leave any signal in the t0 doublet. (b) The demonstrator.
Psf 08 00008 g003
Figure 4. Reconstructed events after the application of the neural network. (a) Visible energy of K e 3 positrons. (b) Impact point along calorimeter wall of muons from K μ 2 . In both plots, the background contributions are also reported as in the legend.
Figure 4. Reconstructed events after the application of the neural network. (a) Visible energy of K e 3 positrons. (b) Impact point along calorimeter wall of muons from K μ 2 . In both plots, the background contributions are also reported as in the legend.
Psf 08 00008 g004
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MDPI and ACS Style

Delogu, C.C.; Acerbi, F.; Angelis, I.; Bomben, L.; Bonesini, M.; Bramati, F.; Branca, A.; Brizzolari, C.; Brunetti, G.; Calviani, M.; et al. The ENUBET Monitored Neutrino Beam for High Precision Cross-Section Measurements. Phys. Sci. Forum 2023, 8, 8. https://doi.org/10.3390/psf2023008008

AMA Style

Delogu CC, Acerbi F, Angelis I, Bomben L, Bonesini M, Bramati F, Branca A, Brizzolari C, Brunetti G, Calviani M, et al. The ENUBET Monitored Neutrino Beam for High Precision Cross-Section Measurements. Physical Sciences Forum. 2023; 8(1):8. https://doi.org/10.3390/psf2023008008

Chicago/Turabian Style

Delogu, C.C., F. Acerbi, I. Angelis, L. Bomben, M. Bonesini, F. Bramati, A. Branca, C. Brizzolari, G. Brunetti, M. Calviani, and et al. 2023. "The ENUBET Monitored Neutrino Beam for High Precision Cross-Section Measurements" Physical Sciences Forum 8, no. 1: 8. https://doi.org/10.3390/psf2023008008

APA Style

Delogu, C. C., Acerbi, F., Angelis, I., Bomben, L., Bonesini, M., Bramati, F., Branca, A., Brizzolari, C., Brunetti, G., Calviani, M., Capelli, S., Carturan, S., Catanesi, M. G., Cecchini, S., Charitonidis, N., Cindolo, F., Cogo, G., Collazuol, G., Dal Corso, F., ... Votano, L. (2023). The ENUBET Monitored Neutrino Beam for High Precision Cross-Section Measurements. Physical Sciences Forum, 8(1), 8. https://doi.org/10.3390/psf2023008008

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