Abstract
A lower limit to the inelastic nuclear photon scattering cross section of ${\mathrm{Rh}}^{103}$ was determined as function of energy. Rhodium foils were exposed to a bremsstrahlung beam and the yield of ${\mathrm{Rh}}^{103}(\ensuremath{\gamma}, {\ensuremath{\gamma}}^{\ensuremath{'}}){\mathrm{Rh}}^{103m}$ was measured as a function of the upper limit of the spectrum. Activities were counted with a windowless $4\ensuremath{\pi}$ proportional counter and ${\mathrm{Ta}}^{181}(\ensuremath{\gamma}, n){\mathrm{Ta}}^{180}$ was used as a monitor above 8 Mev, adopting the improved results of the Sasketchewan group. It was ascertained that the fast neutron contamination of the beam contributed but a small fraction of ${\mathrm{Rh}}^{103m}$ activity. The cross section, obtained from the yield curve by customary methods, is found to go through a peak of the order of 10 mb at about 13 Mev and to be appreciable below the ${\mathrm{Rh}}^{103}(\ensuremath{\gamma}, n){\mathrm{Rh}}^{102}$ threshold (9.35 Mev). The observed location of the peak is considerably lower than would be expected for ${\mathrm{Rh}}^{103}(\ensuremath{\gamma}, n)$ from the empirical $A$-dependence of ($\ensuremath{\gamma}, n$) cross sections, and is also at variance with the observations of Katz and Cameron on ${\mathrm{Au}}^{197}(\ensuremath{\gamma}, {\ensuremath{\gamma}}^{\ensuremath{'}}){\mathrm{Au}}^{197}$, but appears plausible on theoretical grounds as does the magnitude of the cross section.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
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.