Measured Cosmogenic Background at RENO
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Published on:
August 02, 2019
Abstract
The isotopes of $^{9}$Li and $^{8}$He produced by cosmic-rays are one of main source for backgrounds in reactor neutrino experiments. The isotope decays to a neutron and an electron and mimics an inverse beta decay of an electron antineutrino from reactors. The $^{9}$Li/$^{8}$He background spectrum and rate are measured using the data taken by the RENO, and compared with Monte-Carlo prediction. In this presentation, we report the measured cosmogenic background spectrum and rate at RENO.
DOI: https://doi.org/10.22323/1.340.0880
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.