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Evaluation of neutron tagging efficiency on 0.03% Gd mass concentration in SK-Gd experiment

  • Super-Kamiokande Collaboration
  • Okayama University
  • Institute for Cosmic Ray Research
  • University of Tokyo
  • Department of Physics and Astronomy
  • Long Beach VA and University of California
  • Research Center for Cosmic Neutrinos
  • Facultad de Ciencias
  • Universidad Autónoma de Madrid
  • Department of Physics
  • British Columbia Institute of Technology
  • TRIUMF
  • Boston University

Research output: Contribution to journal › Conference article › peer-review

Abstract

Super-Kamiokande (SK) experiment started the "SK-Gd experiment" by dissolving gadolinium (Gd) sulfate octa-hydrate in ultra-pure water from the tank in July 2020. The neutron tagging efficiency has been improved compared to the pure-water phase by detecting a total energy of 8 MeV gamma rays emitted by thermal neutron capture on Gd. It enables us to improve, for example, the sensitivity of diffuse supernova neutrino background, the accuracy of the reconstruction for the supernova direction, and so on. For these physics targets, accurate evaluation of neutron identification efficiency is essential. In this presentation, I report the calibration results using an Am/Be neutron source to evaluate the efficiency at a Gd mass concentration of 0.03%, starting from June 2022, and the comparison of the estimated neutron detection efficiency with simulation.

Original languageEnglish
Article number1172
JournalProceedings of Science
Volume444
Publication statusPublished - 27 Sept 2024
Event38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan
Duration: 26 Jul 2023 → 3 Aug 2023

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