Speaker
Yoshino Kaminaga
(ICRR, The University of Tokyo)
Description
XENONnT is a direct dark matter search experiment using 8.6 tonnes of Xe. Our observable energy threshold is few keV level, which enables us to search for physics in the low-energy electronic recoils, such as the search for events induced by solar pp neutrinos.
Kr85 is one of the background sources in such low-energy region. To achieve a high significance observation of rare physics events, a precise estimation of Kr85 abundance is required. This poster presents the method and results of the Kr85 background evaluation, and its impact on the sensitivity to solar pp neutrino measurement.
| Collaboration you are representing | XENON |
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Author
Yoshino Kaminaga
(ICRR, The University of Tokyo)
