1. Cosmic Ray Background Rejection with Wire-Cell LArTPC Event Reconstruction in the MicroBooNE Detector
- Author
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D. Cianci, A. Hourlier, G. Yarbrough, W. Q. Gu, R. S. Fitzpatrick, T. Kobilarcik, G. Scanavini, M. Del Tutto, P. M. Hamilton, Antonio Ereditato, W. G. Seligman, M. E. Convery, Yichen Li, William Tang, R. Dorrill, B. Eberly, M. Toups, A. Marchionni, K. Mason, M. Bishai, W. C. Louis, M. Kirby, E. Yandel, J. Martín-Albo, E.L. Snider, Xiaohui Qian, H. Y. Wei, G. Karagiorgi, L.S. Rochester, T. L. Usher, Panagiotis Spentzouris, Steven Gardiner, S.R. Soleti, S. Berkman, E. Church, Laura Dominé, B. Viren, R. An, M. Soderberg, L. Ren, J. Mousseau, W. Ketchum, P. Nienaber, L. Escudero Sanchez, A. Mastbaum, E.-C. Huang, J. Anthony, C. Barnes, A. Rafique, Yi Chen, P. Guzowski, E. D. Hall, B. Russell, B. T. Fleming, S. Prince, G. P. Zeller, Afroditi Papadopoulou, T. Wongjirad, H. E. Rogers, J. Moon, J. Zennamo, T. Mettler, John Marshall, J. L. Raaf, D. Devitt, K. E. Duffy, D. Garcia-Gamez, N. Kamp, K. Mistry, M. Rosenberg, O. Benevides Rodrigues, L. Cooper-Troendle, W. Van De Pontseele, P. Abratenko, T. A. Mohayai, R. Castillo Fernandez, G. A. Horton-Smith, S. A. Dytman, D. A. Martinez Caicedo, L. Mora Lepin, N. McConkey, R. Diurba, Ornella Palamara, R. A. Johnson, M. Alrashed, J. Jan de Vries, J. St. John, A. P. Furmanski, D. Marsden, I. Ponce-Pinto, I. Lepetic, M. Ross-Lonergan, C. D. Moore, D. Naples, Kazuhiro Terao, A. Paudel, Chao Zhang, E. Piasetzky, Giuseppe Benedetto Cerati, D. Porzio, G. A. Fiorentini Aguirre, Andrew Smith, Janet Conrad, Andrew Blake, C. Thorpe, L. Jiang, S. Tufanli, Y.-J. Jwa, L. Bathe-Peters, Xiaolu Ji, Avi Ashkenazi, S. Wolbers, L.E. Yates, S. Söldner-Rembold, A. M. Szelc, Veljko Radeka, M. Reggiani-Guzzo, A. Bhanderi, N. Kaneshige, S. F. Pate, S. Sword-Fehlberg, T. A. Bolton, Y. T. Tsai, S. Gollapinni, L. Camilleri, R. LaZur, J. Sinclair, M. H. Shaevitz, J. I. Crespo-Anadón, X. Luo, V. Meddage, I. Kreslo, I. Caro Terrazas, R. Itay, G. Ge, Michael T. Murphy, S. Balasubramanian, Thomas Strauss, M. Wospakrik, John Evans, O. Goodwin, D. W. Schmitz, B. Baller, T. Yang, D. Lorca, R. Guenette, Marc Weber, C. James, V. Basque, V. Papavassiliou, M. Mooney, A. F. Moor, H. W. Yu, V. Paolone, J. Mills, R. Sharankova, K. Li, F. Cavanna, Wei Wu, E. Gramellini, D. Franco, A. Schukraft, J. Asaadi, B. R. Littlejohn, A. Mogan, A. Navrer-Agasson, M. Stancari, Z. Pavlovic, J. Rodriguez Rondon, Kate C. Miller, L. Hagaman, J. Spitz, R. K. Neely, Or Hen, J. A. Nowak, Z. Williams, Patrick Green, M. A. Uchida, N. Foppiani, C. Mariani, H. Greenlee, K. Sutton, B. Kirby, N. Tagg, J. H. Jo, G.D. Barr, D. Caratelli, A. Bhat, and Collaboration, MicroBooNE
- Subjects
Physics ,Physics - Instrumentation and Detectors ,Time projection chamber ,COSMIC cancer database ,Astrophysics::High Energy Astrophysical Phenomena ,Detector ,FOS: Physical sciences ,General Physics and Astronomy ,Flux ,Cosmic ray ,Instrumentation and Detectors (physics.ins-det) ,02 engineering and technology ,021001 nanoscience & nanotechnology ,01 natural sciences ,Visible energy ,High Energy Physics - Experiment ,Nuclear physics ,High Energy Physics - Experiment (hep-ex) ,0103 physical sciences ,High Energy Physics::Experiment ,Neutrino ,010306 general physics ,0210 nano-technology ,Event reconstruction - Abstract
For a large liquid-argon time-projection chamber (LArTPC) operating on or near the Earth's surface to detect neutrino interactions, the rejection of cosmogenic background is a critical and challenging task because of the large cosmic-ray flux and the long drift time of the time-projection chamber. We introduce a superior cosmic background rejection procedure based on the Wire-Cell three-dimensional (3D) event reconstruction for LArTPCs. From an initial 1:20 000 neutrino to cosmic-ray background ratio, we demonstrate these tools on data from the MicroBooNE experiment and create a high-performance generic neutrino event selection with a cosmic contamination of 14.9% (9.7%) for a visible energy region greater than O(200) MeV. The neutrino interaction selection efficiency is 80.4% and 87.6% for inclusive νμ charged-current and νe charged-current interactions, respectively. This significantly improved performance compared with existing reconstruction algorithms marks a major milestone toward reaching the scientific goals of LArTPC neutrino oscillation experiments operating near the Earth's surface.
- Published
- 2021
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