학술논문

Rejecting cosmic background for exclusive neutrino interaction studies with Liquid Argon TPCs; a case study with the MicroBooNE detector
Document Type
Working Paper
Author
MicroBooNE collaborationAdams, C.Alrashed, M.An, R.Anthony, J.Asaadi, J.Ashkenazi, A.Auger, M.Balasubramanian, S.Baller, B.Barnes, C.Barr, G.Bass, M.Bay, F.Bhat, A.Bhattacharya, K.Bishai, M.Blake, A.Bolton, T.Camilleri, L.Caratelli, D.Terrazas, I. CaroCarr, R.Fernandez, R. CastilloCavanna, F.Cerati, G.Chen, Y.Church, E.Cianci, D.Cohen, E. O.Collin, G. H.Conrad, J. M.Convery, M.Cooper-Troendle, L.Crespo-Anadon, J. I.Del Tutto, M.Devitt, D.Diaz, A.Duffy, K.Dytman, S.Eberly, B.Ereditato, A.Sanchez, L. EscuderoEsquivel, J.Evans, J. J.Fadeeva, A. A.Fitzpatrick, R. S.Fleming, B. T.Franco, D.Furmanski, A. P.Garcia-Gamez, D.Genty, V.Goeldi, D.Gollapinni, S.Goodwin, O.Gramellini, E.Greenlee, H.Grosso, R.Guenette, R.Guzowski, P.Hackenburg, A.Hamilton, P.Hen, O.Hewes, VHill, C.Horton-Smith, G. A.Hourlier, A.Huang, E. -C.James, C.de Vries, J. JanJi, X.Jiang, L.Johnson, R. A.Joshi, J.Jostlein, H.Jwa, Y. -J.Karagiorgi, G.Ketchum, W.Kirby, B.Kirby, M.Kobilarcik, T.Kreslo, I.Lepetic, I.Li, Y.Lister, A.Littlejohn, B. R.Lockwitz, S.Lorca, D.Louis, W. C.Luethi, M.Lundberg, B.Luo, X.Marchionni, A.Marcocci, S.Mariani, C.Marshall, J.Martin-Albo, J.Caicedo, D. A. MartinezMastbaum, A.Meddage, V.Mettler, T.Mistry, K.Mogan, A.Moon, J.Mooney, M.Moore, C. D.Mousseau, J.Murphy, M.Murrells, R.Naples, D.Nienaber, P.Nowak, J.Palamara, O.Pandey, V.Paolone, V.Papadopoulou, A.Papavassiliou, V.Pate, S. F.Pavlovic, Z.Piasetzky, E.Porzio, D.Pulliam, G.Qian, X.Raaf, J. L.Rafique, A.Ren, L.Rochester, L.Ross-Lonergan, M.von Rohr, C. RudolfRussell, B.Scanavini, G.Schmitz, D. W.Schukraft, A.Seligman, W.Shaevitz, M. H.Sharankova, R.Sinclair, J.Smith, A.Snider, E. L.Soderberg, M.Soldner-Rembold, S.Soleti, S. R.Spentzouris, P.Spitz, J.John, J. St.Strauss, T.Sutton, K.Sword-Fehlberg, S.Szelc, A. M.Tagg, N.Tang, W.Terao, K.Thomson, M.Thornton, R. T.Toups, M.Tsai, Y. -T.Tufanli, S.Usher, T.Van De Pontseele, W.Van de Water, R. G.Viren, B.Weber, M.Wei, H.Wickremasinghe, D. A.Wierman, K.Williams, Z.Wolbers, S.Wongjirad, T.Woodruff, K.Yang, T.Yarbrough, G.Yates, L. E.Zeller, G. P.Zennamo, J.Zhang, C.
Source
Subject
Physics - Instrumentation and Detectors
High Energy Physics - Experiment
Nuclear Experiment
Physics - Data Analysis, Statistics and Probability
Language
Abstract
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and cross-section measurements in surface detectors. We present methods for CR rejection in measurements of charged-current quasielastic-like (CCQE-like) neutrino interactions, with a muon and a proton in the final state, measured using liquid argon time projection chambers (LArTPCs). Using a sample of cosmic data collected with the MicroBooNE detector, mixed with simulated neutrino scattering events, a set of event selection criteria is developed that produces an event sample with minimal contribution from CR background. Depending on the selection criteria used a purity between 50% and 80% can be achieved with a signal selection efficiency between 50% and 25%, with higher purity coming at the expense of lower efficiency. While using a specific dataset from the MicroBooNE detector and selection criteria values optimized for CCQE-like events, the concepts presented here are generic and can be adapted for various studies of exclusive {\nu}{\mu} interactions in LArTPCs.
Comment: 12 pages, 10 figures, 1 table