Fluxes and systematics reduction with decay monitoring

Branca, Antonio; Acerbi, F.; Angelis, I.; Bonesini, M.; Bramati, F.; Brizzolari, C.; Brunetti, G.; Calviani, M.; Capelli, S.; Carturan, S.; Catanesi, M.G.; Cecchini, S.; Charitonidis, N.; Cindolo, F.; Collazuol, G.; Dal Corso, F.; Delogu, C.; De Rosa, G.; Falcone, A.; Goddard, B.; Gola, A.; Iacob, F.; Jollet, C.; Kain, V.; Klicek, B.; Kudenko, Y.G.; Lampoudis, Ch.; Laveder, M.; Longhin, A.; Ludovici, L.; Lutsenko, E.; Magaletti, L.; Mandrioli, G.; Margotti, A.; Mascagna, V.; Mauri, N.; Meazza, L.; Meregaglia, A.; Mezzetto, M.; Nessi, M.; Paoloni, A.; Pari, M.; Parozzi, E.G.; Pasqualini, L.; Paternoster, G.; Patrizii, L.; Pozzato, M.; Prest, M.; Pupilli, Fabio; Radicioni, E.; Riccio, C.; Ruggeri, A.C.; Samponidis, D.; Scian, C.; Sirri, G.; Stipcevic, M.; Tenti, M.; Terranova, F.; Torti, M.; Tzamarias, S.E.; Vallazza, E.; Velotti, F.; Votano, L.

doi:10.22323/1.402.0030

Volume 402 - The 22nd International Workshop on Neutrinos from Accelerators (NuFact2021) - All Sessions

Fluxes and systematics reduction with decay monitoring

A. Branca*, F. Acerbi, I. Angelis, M. Bonesini, F. Bramati, C. Brizzolari, G. Brunetti, M. Calviani, S. Capelli, S. Carturan, M.G. Catanesi, S. Cecchini, N. Charitonidis, F. Cindolo, G. Collazuol, F. Dal Corso, C. Delogu, G. De Rosa, A. Falcone, B. Goddard, A. Gola, F. Iacob, C. Jollet, V. Kain, B. Klicek, Y.G. Kudenko, C. Lampoudis, M. Laveder, A. Longhin, L. Ludovici, E. Lutsenko, L. Magaletti, G. Mandrioli, A. Margotti, V. Mascagna, N. Mauri, L. Meazza, A. Meregaglia, M. Mezzetto, M. Nessi, A. Paoloni, M. Pari, E.G. Parozzi, L. Pasqualini, G. Paternoster, L. Patrizii, M. Pozzato, M. Prest, F. Pupilli, E. Radicioni, C. Riccio, A.C. Ruggeri, D. Samponidis, C. Scian, G. Sirri, M. Stipcevic, M. Tenti, F. Terranova, M. Torti, S.E. Tzamarias, E. Vallazza, F. Velotti and L. Votanoet al. (click to show)

*: corresponding author

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Published on: March 31, 2022

Abstract

The ENUBET collaboration is pursuing an R\&D effort to develop and realize the first monitored neutrino beam. This new technique allows to set a tight constraint on the neutrino flux produced in conventional beams, and thus to measure neutrino cross sections with an unprecedented precision of $\mathcal{O}(1\%)$. In this contribution the method being developed for the assessment of the systematics on the neutrino flux, before and after the constraint, is discussed. First results from a validation test on a toy-model is also presented.

DOI: https://doi.org/10.22323/1.402.0030

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