Abstract

The next generation of neutrino experiments requires measurements of absolute neutrino cross sections at the GeV scale with high precision (∼1%) presently limited by the uncertainties on neutrino flux. Monitoring the lepton production in the decay tunnel of neutrino beams is the most straightforward way to measure the neutrino flux at source. The ENUBET Collaboration develops novel technologies to monitor positrons from K+ → νee+π0 decays on an event by event basis. This technique can achieve a precision in the νe flux below 1% and enable a new generation of cross section and short baseline experiments. In this paper, we present the achievements of the first year of the Project on beamline simulation, rate and dose assessment, detector prototyping and evaluation of the physics reach.

Highlights

  • The ENUBET Collaboration develops novel technologies to monitor positrons from decays on an event by event basis. This technique can achieve a precision in the e flux below 1% and enable a new generation of cross section and short baseline experiments

  • We present the achievements of the first year of the Project on beamline simulation, rate and dose assessment, detector prototyping and evaluation of the physics reach

  • The ENUBET project Neutrinos played a fundamental role in the study of weak interactions and, after the observation of the oscillation phenomenon, they opened a window on physics beyond the standard model

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Summary

IOP Publishing

G Ballerini 1,2, A Berra 1,2 , R Boanta 2,8 , M Bonesini 2, C Brizzolari 1,2, G Brunetti 10, M Calviani 13, S Carturan 20 , M G Catanesi 12 , S Cecchini 3, F Cindolo 3, A Coffani 2,8, G Collazuol 10,11, E Conti 10, F Dal Corso 10, G De Rosa 16,17, A Gola 15, R A Intonti 12 , C Jollet 4, Y Kudenko 18, M Laveder 10,11, A Longhin 10, P F Loverre 6,14 , L Ludovici 6 , L Magaletti 12 , G Mandrioli 3, A Margotti 3, V Mascagna 1,2, N Mauri 3, A Meregaglia 19, M Mezzetto 10, M Nessi 13, A Paoloni 5, M Pari 10,11, G Paternoster 15, L Patrizii 3, C Piemonte 15, M Pozzato 3, M Prest 1,2, F Pupilli 10, E Radicioni 12 , C Riccio 16,17, A C Ruggeri 16, M Soldani 1,2 G Sirri 3, M Tenti 3,7, F Terranova 1,2, E Vallazza 9, M Vesco 20 , L Votano 5 and E Wildner 13

Published under licence by IOP Publishing Ltd
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