New methods and simulations for cosmogenic induced spallation removal in Super-Kamiokande-IV

Author:

Locke S.1ORCID,Coffani A.2,Abe K.33,Bronner C.3ORCID,Hayato Y.33ORCID,Ikeda M.3ORCID,Imaizumi S.3,Ito H.3ORCID,Kameda J.33,Kataoka Y.3ORCID,Miura M.33,Moriyama S.33ORCID,Nagao Y.3,Nakahata M.33ORCID,Nakajima Y.33ORCID,Nakayama S.33ORCID,Okada T.3,Okamoto K.3,Orii A.3,Pronost G.3ORCID,Sekiya H.33ORCID,Shiozawa M.33ORCID,Sonoda Y.3,Suzuki Y.3,Takeda A.33,Takemoto Y.3ORCID,Takenaka A.3,Tanaka H.3,Yano T.3ORCID,Hirade K.3,Kanemura Y.3,Miki S.3,Watabe S.3,Han S.3ORCID,Kajita T.33,Okumura K.33ORCID,Tashiro T.3ORCID,Xia J.3ORCID,Wang X.3,Megias G. D.3ORCID,Bravo-Berguño D.4,Labarga L.4ORCID,Marti Ll.4ORCID,Zaldivar B.4,Pointon B. W.56ORCID,Blaszczyk F. d. M.7,Kearns E.73ORCID,Raaf J. L.7,Stone J. L.73,Wan L.7ORCID,Wester T.7ORCID,Bian J.1,Griskevich N. J.1ORCID,Kropp W. R.1,Mine S.1,Smy M. B.13ORCID,Sobel H. W.13ORCID,Takhistov V.13,Weatherly P.1,Yankelevich A.1ORCID,Hill J.8,Kim J. Y.9,Lim I. T.9,Park R. G.9,Bodur B.10ORCID,Scholberg K.103ORCID,Walter C. W.103ORCID,Bernard L.2,Drapier O.2,Hedri S. El2,Giampaolo A.2,Gonin M.2,Mueller Th. A.2ORCID,Paganini P.2ORCID,Quilain B.2,Santos A. D.2,Ishizuka T.11,Nakamura T.12,Jang J. S.13,Learned J. G.14,Anthony L. H. V.15,Sztuc A. A.15,Uchida Y.15,Martin D.15,Scott M.15ORCID,Berardi V.16ORCID,Catanesi M. G.16,Radicioni E.16,Calabria N. F.17ORCID,Machado L. N.17ORCID,De Rosa G.17,Collazuol G.18ORCID,Iacob F.18ORCID,Lamoureux M.18,Ospina N.18ORCID,Mattiazzi M.18ORCID,Ludovici L.19,Nishimura Y.20ORCID,Maewaka Y.20,Cao S.21,Friend M.21,Hasegawa T.21ORCID,Ishida T.21,Kobayashi T.21,Jakkapu M.21,Matsubara T.21ORCID,Nakadaira T.21,Nakamura K.213ORCID,Oyama Y.21ORCID,Sakashita K.21,Sekiguchi T.21,Tsukamoto T.21,Nakano Y.22ORCID,Shiozawa T.22,Suzuki A. T.22,Takeuchi Y.223,Yamamoto S.22,Kotsar Y.22,Ozaki H.22,Ali A.23,Ashida Y.23,Feng J.23,Hirota S.23,Ichikawa A. K.23ORCID,Kikawa T.23,Mori M.23,Nakaya T.233ORCID,Wendell R. A.233ORCID,Yasutome K.23,Fernandez P.24ORCID,McCauley N.24ORCID,Mehta P.24,Tsui K. M.24,Fukuda Y.25ORCID,Itow Y.2626ORCID,Menjo H.26ORCID,Niwa T.26,Sato K.26,Tsukada M.26,Mijakowski P.27,Lagoda J.27,Lakshmi S. M.27,Zalipska J.27,Jung C. K.28,Vilela C.28,Wilking M. J.28,Yanagisawa C.28ORCID,Jiang J.28,Hagiwara K.29,Harada M.29ORCID,Horai T.29,Ishino H.29,Ito S.29,Koshio Y.293ORCID,Ma W.29,Piplani N.29,Sakai S.29ORCID,Kitagawa H.29,Barr G.30,Barrow D.30ORCID,Cook L.303,Goldsack A.303,Samani S.30,Wark D.3031,Nova F.31ORCID,Boschi T.32,Di Lodovico F.32,Taani M.32,Zsoldos S.32ORCID,Gao J.32,Migenda J.32ORCID,Yang J. Y.33ORCID,Jenkins S. J.34ORCID,Malek M.34,McElwee J. M.34,Stone O.34,Thiesse M. D.34ORCID,Thompson L. F.34ORCID,Okazawa H.35,Nakamura K.36,Kim S. B.37,Yu I.37ORCID,Seo J. W.37ORCID,Nishijima K.38ORCID,Koshiba M.39,Iwamoto K.3,Ogawa N.3,Yokoyama M.33ORCID,Martens K.3ORCID,Vagins M. R.31ORCID,Nakagiri K.339,Kuze M.40ORCID,Izumiyama S.40ORCID,Yoshida T.40,Inomoto M.41,Ishitsuka M.41,Matsumoto R.41ORCID,Ohta K.41,Shinoki M.41ORCID,Suganuma T.41,Kinoshita T.41,Martin J. F.42,Tanaka H. A.42,Towstego T.42,Akutsu R.6,Hartz M.6,Konaka A.6,de Perio P.6ORCID,Prouse N. W.6,Chen S.43ORCID,Xu B. D.43ORCID,Zhang Y.43,Posiadala-Zezula M.44,Richards B.45,Jamieson B.46,Walker J.46,Minamino A.47ORCID,Okamoto K.47,Pintaudi G.47,Sasaki R.47

Affiliation:

1. University of California

2. Laboratoire Leprince-Ringuet

3. University of Tokyo

4. University Autonoma Madrid

5. British Columbia Institute of Technology

6. TRIUMF

7. Boston University

8. California State University

9. Chonnam National University

10. Duke University

11. Fukuoka Institute of Technology

12. Gifu University

13. Gwangju Institute of Science and Technology

14. University of Hawaii

15. Imperial College London

16. INFN Sezione di Bari and Università e Politecnico di Bari

17. INFN Sezione di Napoli and Università di Napoli

18. INFN Sezione di Padova and Università di Padova

19. INFN Sezione di Roma and Università di Roma “La Sapienza,”

20. Keio University

21. High Energy Accelerator Research Organization (KEK)

22. Kobe University

23. Kyoto University

24. University of Liverpool

25. Miyagi University of Education

26. Nagoya University

27. National Centre For Nuclear Research

28. State University of New York at Stony Brook

29. Okayama University

30. Oxford University

31. Rutherford Appleton Laboratory

32. King’s College London

33. Seoul National University

34. University of Sheffield

35. Shizuoka University of Welfare

36. Tohoku University

37. Sungkyunkwan University

38. Tokai University

39. The University of Tokyo

40. Tokyo Institute of Technology

41. Tokyo University of Science

42. University of Toronto

43. Tsinghua University

44. University of Warsaw

45. University of Warwick

46. University of Winnipeg

47. Yokohama National University

Abstract

Radioactivity induced by cosmic muon spallation is a dominant source of backgrounds for O(10MeV) neutrino interactions in water Cherenkov detectors. In particular, it is crucial to reduce backgrounds to measure the solar neutrino spectrum and find neutrino interactions from distant supernovae. In this paper we introduce new techniques to locate muon-induced hadronic showers and efficiently reject spallation backgrounds. Applying these techniques to the solar neutrino analysis with an exposure of 2790×22.5kton·day increases the signal efficiency by 12.6%, approximately corresponding to an additional year of detector running. Furthermore, we present the first spallation simulation at Super-Kamiokande, where we model hadronic interactions using . The agreement between the isotope yields and shower pattern in this simulation and in the data gives confidence in the accuracy of this simulation, and thus opens the door to use it to optimize muon spallation removal in new data with gadolinium-enhanced neutron capture detection. Published by the American Physical Society 2024

Funder

Ministry of Education, Culture, Sports, Science and Technology

U.S. Department of Energy

National Science Foundation

National Research Foundation of Korea

Japan Society for the Promotion of Science

National Natural Science Foundation of China

Ministerio de Ciencia e Innovación

Natural Sciences and Engineering Research Council of Canada

Narodowe Centrum Nauki

Science and Technology Facilities Council

European Commission

HORIZON EUROPE Marie Sklodowska-Curie Actions

Compute Canada

Publisher

American Physical Society (APS)

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