Abstract
The search for neutrino signals from gravitational core collapses in the Milky Way is one of the main lines of research at the Baksan Underground Scintillation Telescope (BUST). Neutrons generated by cosmic-ray muons produce a considerable background in such experiments. The contribution from the elastic scattering of fast neutrons off protons to the overall single-event background rate measured in the inner detector planes is estimated via neutron activation analysis. The resulting value of the fast-neutron flux agrees with one based on the results from FLUKA modeling for the depth of the BUST detector. The same technique can be used to estimate the neutron background in similar experiments focused on rare events.
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ACKNOWLEDGMENTS
This work was performed on the Baksan Underground Scintillation Telescope at the shared resource center of the Baksan Neutrino Observatory, Institute for Nuclear Research, Russian Academy of Sciences.
Funding
This work was supported by the basic research program “Physics of Fundamental Interactions and Nuclear Technology” of the Presidium of the Russian Academy of Sciences.
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Translated by D. Safin
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Kochkarov, M.M., Boliev, M.M., Dzaparova, I.M. et al. Fast-Neutron Background at the Baksan Underground Scintillation Telescope. Bull. Russ. Acad. Sci. Phys. 83, 927–929 (2019). https://doi.org/10.3103/S1062873819080227
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DOI: https://doi.org/10.3103/S1062873819080227