Abstract
The relative emission probabilities for the 161-, 303- and 384-keV γ-rays emitted during the decay of 133Xe have been measured by comparing spectra obtained from a sample with spectra from standard 133Ba sources. Corrections were made for random losses, differences in geometry, attenuation due to differing source encapsulation and coincident summing effects. From the corrected rates, the emission probabilities relative to the sum of the 80- and 81-keV γ-rays are 24.2±2.5 × 10 −4, 1.93±0.07 × 10 −4 and 0.90±0.04 × 10 −4 for the 161-, 303- and 384-keV γ-rays respectively. If the sum of the 80- and 81-keV γ-ray emission probabilities is 0.383±0.007, the emission probabilities of the 161-, 303- and 384-keV γ-rays are 9.3±1.0 × 10 −5 and 3.5±0.2 × 10 −5 respectively. All uncertainties quoted here and in the following paper are one standard deviation equivalent unless otherwise stated.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
More From: International Journal of Radiation Applications & Instrumentation. Part A, Applied Radiation & Isotopes
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.