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- W2028046670 abstract "The interaction of hadronic and purely muonic secondary cosmic rays is demonstrated by comparison of Ge-background spectra with a coverage of 1 and 15 meter water equivalent (m.w.e.), respectively. A compilation is given of cosmic-induced background lines, including processes like nuclear and atomic de-excitation and activation. Effects of muonic electron photon showers are investigated using different materials for the inner shield at 15 mw.e. The observed background spectra mainly consist of a bremsstrahlungs-continuum from muonic shower electrons induced in the inner shield and annihilation photons by the same source and partly from stopped positive muons. In general, low activity lead is most effective in background reduction, at least above 90 keV, since it absorbs shower bremsstrahlung best and has the lowest γ-yield for inelastic neutron scattering." @default.
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- W2028046670 date "1993-10-01" @default.
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- W2028046670 title "Cosmic ray-induced background in Ge-spectrometry" @default.
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- W2028046670 doi "https://doi.org/10.1016/0168-583x(93)95931-t" @default.
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