Cosmic Ray Background Rejection With Wire-Cell Lartpc Event Reconstruction In The Microboone Detector

MicroBooNE collaboration,P. Abratenko,M. Alrashed,R. An,J. Anthony,J. Asaadi,A. Ashkenazi,S. Balasubramanian,B. Baller, C. Barnes, G. Barr, V. Basque, L. Bathe-Peters,O. Benevides Rodrigues,S. Berkman, A. Bhanderi,A. Bhat,M. Bishai,A. Blake,T. Bolton,L. Camilleri,D. Caratelli,I. Caro Terrazas,R. Castillo Fernandez,F. Cavanna, G. Cerati,Y. Chen,E. Church,D. Cianci,J. M. Conrad, M. Convery, L. Cooper-Troendle,J. I. Crespo-Anadon,M. Del Tutto, D. Devitt, R. Diurba,L. Domine,R. Dorrill,K. Duffy,S. Dytman, B. Eberly, A. Ereditato,L. Escudero Sanchez,J. J. Evans,G. A. Fiorentini Aguirre, R. S. Fitzpatrick,B. T. Fleming,N. Foppiani,D. Franco,A. P. Furmanski,D. Garcia-Gamez,S. Gardiner,G. Ge,S. Gollapinni,O. Goodwin, E. Gramellini,P. Green, H. Greenlee,W. Gu, R. Guenette,P. Guzowski, L. Hagaman,E. Hall,P. Hamilton,O. Hen,G. A. Horton-Smith,A. Hourlier,E. C. Huang,R. Itay,C. James,J. Jan de Vries,X. Ji,L. Jiang,J. H. Jo,R. A. Johnson,Y. J. Jwa,N. Kamp, N. Kaneshige,G. Karagiorgi,W. Ketchum,B. Kirby, M. Kirby,T. Kobilarcik,I. Kreslo, R. LaZur, I. Lepetic,K. Li, Y. Li,B. R. Littlejohn,D. Lorca,W. C. Louis,X. Luo,A. Marchionni,C. Mariani,D. Marsden,J. Marshall,J. Martin-Albo,D. A. Martinez Caicedo,K. Mason, A. Mastbaum, N. McConkey,V. Meddage,T. Mettler,K. Miller,J. Mills,K. Mistry,T. Mohayai, A. Mogan,J. Moon,M. Mooney, A. F. Moor,C. D. Moore,L. Mora Lepin,J. Mousseau,M. Murphy,D. Naples, A. Navrer-Agasson, R. K. Neely, P. Nienaber,J. Nowak,O. Palamara, V. Paolone,A. Papadopoulou,V. Papavassiliou,S. F. Pate,A. Paudel, Z. Pavlovic,E. Piasetzky, I. Ponce-Pinto, D. Porzio,S. Prince,X. Qian,J. L. Raaf,V. Radeka,A. Rafique, M. Reggiani-Guzzo,L. Ren, L. Rochester,J. Rodriguez Rondon,H. E. Rogers,M. Rosenberg,M. Ross-Lonergan,B. Russell,G. Scanavini, D. W. Schmitz, A. Schukraft, W. Seligman,M. H. Shaevitz,R. Sharankova, J. Sinclair,A. Smith, E. L. Snider,M. Soderberg, S. Soldner-Rembold,S. R. Soleti, P. Spentzouris,J. Spitz, M. Stancari,J. St. John,T. Strauss,K. Sutton, S. Sword-Fehlberg,A. M. Szelc,N. Tagg,W. Tang,K. Terao,C. Thorpe, M. Toups,Y. -T. Tsai,S. Tufanli,M. A. Uchida, T. Usher,W. Van De Pontseele,B. Viren,M. Weber,H. Wei,Z. Williams,S. Wolbers,T. Wongjirad,M. Wospakrik,W. Wu, E. Yandel,T. Yang, G. Yarbrough, L. E. Yates,H. W. Yu,G. P. Zeller, J. Zennamo,C. Zhang

PHYSICAL REVIEW APPLIED(2021)

引用 23|浏览72
暂无评分
摘要
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 nu(mu) charged-current and nu(e) 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.
更多
查看译文
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要