MCNP modelling of scintillation-detector γ-ray spectra from natural radionuclides
γ-ray spectra of natural radionuclides are simulated for a BGO detector in a borehole geometry using the Monte Carlo code MCNP. All γ-ray emissions of the decay of 40K and the series of 232Th and 238U are used to describe the source. A procedure is proposed which excludes the time-consuming electron...
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Veröffentlicht in: | Applied radiation and isotopes 2002-09, Vol.57 (3), p.449-457 |
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Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | γ-ray spectra of natural radionuclides are simulated for a BGO detector in a borehole geometry using the Monte Carlo code MCNP. All
γ-ray emissions of the decay of
40K and the series of
232Th and
238U are used to describe the source. A procedure is proposed which excludes the time-consuming electron tracking in less relevant areas of the geometry. The simulated
γ-ray spectra are benchmarked against laboratory data. |
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ISSN: | 0969-8043 1872-9800 |
DOI: | 10.1016/S0969-8043(02)00118-5 |