| Pagina principale > A high precision narrow-band neutrino beam: The ENUBET project |
| Published Articles | |
| Title | A high precision narrow-band neutrino beam: The ENUBET project |
| Author(s) | Torti, M (INFN, Milan Bicocca ; Milan Bicocca U.) ; Acerbi, F (Fond. Bruno Kessler, Povo ; TIFPA-INFN, Trento ; Trento U.) ; Berra, A (INFN, Milan Bicocca ; Insubria U., Como) ; Bonesini, M (INFN, Milan Bicocca) ; Branca, A (INFN, Padua ; U. Padua, Dept. Phys. Astron.) ; Brizzolari, C (INFN, Milan Bicocca ; Milan Bicocca U.) ; Brunetti, G (INFN, Padua) ; Calviani, M (CERN) ; Capelli, S (INFN, Milan Bicocca ; Insubria U., Como) ; Carturan, S (INFN, Padua ; INFN, Legnaro) ; Catanesi, M G (INFN, Bari) ; Charitonidis, N (CERN) ; Cecchini, S (INFN, Bologna) ; Cindolo, F (INFN, Bologna) ; Collazuol, G (INFN, Padua ; U. Padua, Dept. Phys. Astron.) ; Conti, E (INFN, Padua) ; Dal Corso, F (INFN, Padua) ; Delogu, C (INFN, Padua ; U. Padua, Dept. Phys. Astron.) ; De Rosa, G (INFN, Naples ; U. Naples (main)) ; Falcone, A (INFN, Milan Bicocca ; Milan Bicocca U.) ; Gola, A (Fond. Bruno Kessler, Povo) ; Jollet, C (CENBG, Gradignan) ; Kain, V (CERN) ; Klićek, B (Boskovic Inst., Zagreb) ; Kudenko, Y (Moscow, INR) ; Laveder, M (INFN, Padua ; U. Padua, Dept. Phys. Astron.) ; Longhin, A (INFN, Padua ; U. Padua, Dept. Phys. Astron.) ; Ludovici, L (INFN, Rome) ; Lutsenko, E (INFN, Milan Bicocca ; Insubria U., Como) ; Magaletti, L (INFN, Bari ; Bari U.) ; Mandrioli, G (INFN, Bologna) ; Margotti, A (INFN, Bologna) ; Mascagna, V (INFN, Milan Bicocca ; Insubria U., Como) ; Mauri, N (INFN, Bologna) ; Meazza, L (INFN, Milan Bicocca ; Milan Bicocca U.) ; Meregaglia, A (CENBG, Gradignan) ; Mezzetto, M (INFN, Padua) ; Nessi, M (CERN) ; Paoloni, A (Frascati) ; Pari, M (INFN, Padua ; U. Padua, Dept. Phys. Astron.) ; Parozzi, E G (INFN, Milan Bicocca ; Milan Bicocca U.) ; Pasqualini, L (INFN, Bologna ; U. Bologna, DIFA) ; Paternoster, G (Fond. Bruno Kessler, Povo) ; Patrizii, L (INFN, Bologna) ; Pozzato, M (INFN, Bologna) ; Prest, M (INFN, Milan Bicocca ; Insubria U., Como) ; Pupilli, F (INFN, Padua) ; Radicioni, E (INFN, Bari) ; Riccio, C (INFN, Naples ; U. Naples (main)) ; Ruggeri, A C (INFN, Naples ; U. Naples (main)) ; Scian, C (INFN, Padua ; U. Padua, Dept. Phys. Astron.) ; Sirri, G (INFN, Bologna) ; Stipćevic, M (Boskovic Inst., Zagreb) ; Tenti, M (INFN, Bologna) ; Terranova, F (INFN, Milan Bicocca ; Milan Bicocca U.) ; Vallazza, E (INFN, Milan Bicocca) ; Velotti, F (CERN) ; Vesco, M (INFN, Padua ; U. Padua, Dept. Phys. Astron.) ; Votano, L (Frascati) |
| Publication | 2020 |
| Number of pages | 13 |
| In: | Int. J. Mod. Phys. A 35 (2020) 2044017 |
| In: | 8th International Conference on New Frontiers in Physics (ICNFP 2019), Kolymbari, Crete, Greece, 21 - 29 Aug 2019, pp.2044017 |
| DOI | 10.1142/S0217751X20440170 |
| Subject category | Detectors and Experimental Techniques |
| Abstract | The knowledge of the initial flux, energy and flavor of current neutrino beams is the main limitation for a precise measurement of neutrino cross-sections. The ENUBET ERC project is studying a facility based on a narrow-band neutrino beam capable of constraining the neutrino fluxes normalization through the monitoring of the associated charged leptons in an instrumented decay tunnel. In ENUBET, the identification of large-angle positrons from Ke3 decays at single particle level can potentially reduce the νe flux uncertainty at the level of 1%. This setup would allow for an unprecedented measurement of the νe cross-section at the GeV scale. This input would be highly beneficial to reduce the budget of systematic uncertainties in the next long baseline oscillation projects. Furthermore, in narrow-band beams, the transverse position of the neutrino interaction at the detector can be exploited to determine a priori with significant precision the neutrino energy spectrum without relying on the final state reconstruction. This contribution will present the advances in the design and simulation of the hadronic beam line. Special emphasis will be given to a static focusing system of secondary mesons that can be coupled to a slow extraction proton scheme. The consequent reduction of particle rates and pile-up effects makes the determination of the νμ flux through a direct monitoring of muons after the hadron dump viable, and paves the way to a time-tagged neutrino beam. Time-coincidences among the lepton at the source and the neutrino at the detector would enable an unprecedented purity and the possibility to reconstruct the neutrino kinematics at source on an event-by-event basis. We will also present the performance of positron tagger prototypes tested at CERN beamlines, a full simulation of the positron reconstruction chain and the expected physics reach of ENUBET. |
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