Locke, S. orcid.org/0000-0001-9400-5977, Coffani, A., Abe, K. et al. (217 more authors) (2024) New methods and simulations for cosmogenic induced spallation removal in Super-Kamiokande-IV. Physical Review D, 110. 032003. ISSN 2470-0010
Abstract
<jats:p>Radioactivity induced by cosmic muon spallation is a dominant source of backgrounds for <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mi mathvariant="script">O</a:mi><a:mo stretchy="false">(</a:mo><a:mn>10</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:mi>MeV</a:mi><a:mo stretchy="false">)</a:mo></a:mrow></a:math> 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 <f:math xmlns:f="http://www.w3.org/1998/Math/MathML" display="inline"><f:mn>2790</f:mn><f:mo>×</f:mo><f:mn>22.5</f:mn><f:mtext> </f:mtext><f:mtext> </f:mtext><f:mi>kton</f:mi><f:mo>·</f:mo><f:mi>day</f:mi></f:math> 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.</jats:p> <jats:sec> <jats:title/> <jats:supplementary-material> <jats:permissions> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2024</jats:copyright-year> </jats:permissions> </jats:supplementary-material> </jats:sec>
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2024 The Authors. This is an Open Access article distributed under the terms of the Creative Commons Attribution Licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. |
Keywords: | 5106 Nuclear and Plasma Physics; 5107 Particle and High Energy Physics; 51 Physical Sciences |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematical and Physical Sciences |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 15 Oct 2024 15:12 |
Last Modified: | 15 Oct 2024 15:12 |
Published Version: | http://dx.doi.org/10.1103/physrevd.110.032003 |
Status: | Published |
Publisher: | American Physical Society (APS) |
Refereed: | Yes |
Identification Number: | 10.1103/physrevd.110.032003 |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:218458 |