Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1878028 | Applied Radiation and Isotopes | 2010 | 6 Pages |
Abstract
The half-life of 124Sb was determined experimentally by following the decay of a source from a radiopure solution with a Centronic IG12 ionisation chamber. Thousands of measurements were performed over a period of 358 days, i.e. about six half-life periods. However, the data analysis was restricted to the first 221 days, in order to limit the dominant uncertainty component associated with the hypothetical possibility of a systematic error on background subtraction. The resulting value for the 124Sb half-life, 60.212 (11) days, is found to be in very good agreement with published values, but carries a lower uncertainty. Major uncertainty contributions pertain to possible systematic errors in background correction, long-term changes in source-detector geometry and medium- and long-term instability of the instrument. Additional measurements were performed with a high-purity germanium detector to confirm the above value.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Radiation
Authors
J. Paepen, T. Altzitzoglou, R. Van Ammel, G. Sibbens, S. Pommé,