Abstract
The main problem of solar neutrino or dark matter searches is to detect low-energy radiation with highest possible quantum efficiency. Due to the rather small cross-sections involved, it means monitoring a large bulk of material for small energy deposits.
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References
A. Drukier and L. Stodolsky: Phys. Rev. D 30, 2295 (1984)
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© 1987 Springer-Verlag Berlin Heidelberg
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Vesztergombi, G. (1987). “Minicylinder” Design for Solar Neutrino Detection (A naive proposal). In: Pretzl, K., Schmitz, N., Stodolsky, L. (eds) Low Temperature Detectors for Neutrinos and Dark Matter. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-72959-1_6
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DOI: https://doi.org/10.1007/978-3-642-72959-1_6
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