Atmospheric neutrinos in next-generation xenon and argon dark matter experiments

We study the sensitivity of future xenon- and argon-based dark matter neutrino detection experiments to low-energy atmospheric neutrinos. Not accounting for experimental backgrounds, primary obstacle identifying nuclear recoils induced by neutrinos is tail electron recoil distribution due $pp$ solar use NEST code model signals in a xenon detector find that an exposure 700 tonne-years will produce $5\sigma$ explore effect different properties sufficiently long lifetime essential success such measurement.