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Proceedings of The 19th International Workshop on Neutrinos from Accelerators NUFACT2017 — PoS(NuFact2017) | 2018

Baby MIND: A magnetised spectrometer for the WAGASCI experiment

M. Antonova; A. Kleymenova; P. Benoit; S. Parsa; A. Cervera; Y. Favre; N. Yershov; H.H.J. ten Kate; E. Noah; M Medvedeva; S-P. Hallsjö; G. Vankova-Kirilova; F. Cadoux; R. Asfandiyarov; R. Matev; A. Minamino; H. Pais Da Silva; B. Martinez; O. Mineev; M. Nessi; M. Rayner; M. Khabibullin; L. Nicola; A. Mefodiev; A. Khotyantsev; A. Izmaylov; R. Tsenov; A. Kostin; S. Suvorov; A. Dudarev

The WAGASCI experiment being built at the J-PARC neutrino beam line will measure the ratio of cross sections from neutrinos interacting with a water and scintillator targets, in order to constrain neutrino cross sections, essential for the T2K neutrino oscillation measurements. A prototype Magnetised Iron Neutrino Detector (MIND), called Baby MIND, has been constructed at CERN and will act as a magnetic spectrometer behind the main WAGASCI target. Baby MIND will be installed inside the WAGASCI cavern at J-PARC in the beginning of 2018. Baby MIND will be able to measure the charge and momentum of the outgoing muon from neutrino charged current interactions, to enable full neutrino event reconstruction in WAGASCI. During the summer of 2017, Baby MIND was operated and characterised at the T9 test beam at CERN. Results from this test beam will be presented, including charge identification performance and momentum resolution for charged tracks. These results will be compared to the Monte Carlo simulations. Finally, simulations of charge-current quasi-elastic (CCQE) neutrino interactions in an active scintillator neutrino target, followed by the Baby MIND spectrometer, will be shown to demonstrate the capability of this detector set-up to perform cross-section measurements under different assumptions.


Journal of Instrumentation | 2017

Baby MIND: A magnetized segmented neutrino detector for the WAGASCI experiment

M. Antonova; A. Kleymenova; P. Benoit; S. Parsa; A. Cervera; Y. Favre; N. Yershov; H. Ten Kate; E. Noah; M Medvedeva; S-P. Hallsjö; G. Vankova-Kirilova; F. Cadoux; R. Asfandiyarov; R. Matev; A. Minamino; H. Pais Da Silva; B. Martinez; O. Mineev; M. Nessi; M. Rayner; M. Khabibullin; L. Nicola; A. Mefodiev; A. Khotyantsev; A. Izmaylov; R. Tsenov; A. Kostin; S. Suvorov; A. Dudarev

T2K (Tokai-to-Kamioka) is a long-baseline neutrino experiment in Japan designed to study various parameters of neutrino oscillations. A near detector complex (ND280) is located 280 m downstream of the production target and measures neutrino beam parameters before any oscillations occur. ND280s measurements are used to predict the number and spectra of neutrinos in the Super-Kamiokande detector at the distance of 295 km. The difference in the target material between the far (water) and near (scintillator, hydrocarbon) detectors leads to the main non-cancelling systematic uncertainty for the oscillation analysis. In order to reduce this uncertainty a new WAter-Grid-And-SCintillator detector (WAGASCI) has been developed. A magnetized iron neutrino detector (Baby MIND) will be used to measure momentum and charge identification of the outgoing muons from charged current interactions. The Baby MIND modules are composed of magnetized iron plates and long plastic scintillator bars read out at the both ends with wavelength shifting fibers and silicon photomultipliers. The front-end electronics board has been developed to perform the readout and digitization of the signals from the scintillator bars. Detector elements were tested with cosmic rays and in the PS beam at CERN. The obtained results are presented in this paper.


Journal of Instrumentation | 2018

A fully-active fine-grained detector with three readout views

A. Blondel; F. Cadoux; S. Fedotov; M. Khabibullin; A. Khotjantsev; A. Korzenev; A. Kostin; Y. Kudenko; A. Longhin; A. Mefodiev; P. Mermod; O. Mineev; E. Noah; D. Sgalaberna; A. Smirnov; N. Yershov


Archive | 2017

Baby MIND Experiment Construction Status : arXiv

M. Antonova; A. Kleymenova; P. Benoit; S. Parsa; A. Cervera; Y. Favre; N. Yershov; H.H.J. ten Kate; E. Noah; M Medvedeva; S-P. Hallsjö; G. Vankova-Kirilova; F. Cadoux; R. Asfandiyarov; R. Matev; A. Minamino; H. Pais Da Silva; B. Martinez; O. Mineev; M. Nessi; M. Rayner; M. Khabibullin; L. Nicola; A. Mefodiev; A. Khotyantsev; A. Izmaylov; R. Tsenov; A. Kostin; S. Suvorov; A. Dudarev

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E. Noah

University of Geneva

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A. Kostin

Russian Academy of Sciences

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