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Optical radiation background from \(^{40}\)K decays in undersea neutrino telescopes

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The European Physical Journal C - Particles and Fields Aims and scope Submit manuscript

Abstract.

The photon flux produced by light sources uniformly distributed in an infinite homogeneous medium is calculated on the basis of a known property of light propagation, taking into account the contribution of both absorption and scattering processes. The results are applied to the issue of the decays of \(^{40}\)K content in sea salt and then to the rates detected by photomultipliers deployed in the deep sea. Numerical calculations are in agreement with the recent measurements performed in the Mediterranean Sea by the ANTARES and NEMO Collaborations.

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Received: 29 August 2001 / Revised version: 25 October 2001 / Published online: 14 December 2001

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Massa, F. Optical radiation background from \(^{40}\)K decays in undersea neutrino telescopes. Eur. Phys. J. C 22, 749–756 (2002). https://doi.org/10.1007/s100520100840

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  • DOI: https://doi.org/10.1007/s100520100840

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