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“Minicylinder” Design for Solar Neutrino Detection (A naive proposal)

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Low Temperature Detectors for Neutrinos and Dark Matter
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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

  1. A. Drukier and L. Stodolsky: Phys. Rev. D 30, 2295 (1984)

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  2. K. Pretzl these proceedings

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  3. E. Hartfield and B.J. Thompson: In Handbook of Optics, ed. by Driscoll, Vaughan, (Mc Graw-Hill, New York, 1978) 17–21

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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

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-72961-4

  • Online ISBN: 978-3-642-72959-1

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