Abstract
Relative γ-ray intensities in the decay of 160Tb were precisely measured using two semiconductor detectors. These intensities were used to calculate particle and γ-ray emission probabilities along with their corresponding uncertainties by employing equations derived with standard mathematical error propagating technique (Browne, 1986, 1988).
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Schedule a callMore From: International Journal of Radiation Applications & Instrumentation. Part A, Applied Radiation & Isotopes
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