Gaseous Detector with Sub-keV Threshold to Study Neutrino Scattering at Low Recoil Energies

<table>The count rate from CNNS as a function of energy of the recoiled nucleus for different gases. By dashed lines are indicated the count rates from neutrons generated by cosmic rays. The flux of antineutrinos is taken here 10<sup>13</sup> <i>ν</i>/cm<sup>2</sup>/s.</table>

Advances in High Energy Physics

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Figure 2

Figure 2: Gaseous Detector with Sub-keV Threshold to Study Neutrino Scattering at Low Recoil Energies 