Limits on Sensitivity of Large Silicon Bolometers for Solar Neutrino Detection
C. J. MARTOFF 1
1 Department of Physics, Stanford University, Stanford, CA 94305.
Estimates are given for ultimate limits on background in proposed direct-counting measurements of neutrino scattering from large silicon crystals. Methods of background reduction are discussed. In the best case, the limiting backgrounds due to activities from cosmic-ray spallation of silicon would be less than the expected true event rate for reactor neutrino measurements of coherent neutral-current scattering from silicon nuclei. Considerable reduction of the estimated high-energy backgrounds would be required for a good signal-to-noise ratio in solar neutrino detection.
Submitted on December 29, 1986
Accepted on May 26, 1987