Abstract

Discrete γ‐ray spectra have been measured for nuclei populated in 191Ir(n,xnγ) reactions, with x ⩽ 11, as a function of incident neutron energy using neutrons from the “white” neutron source at the Los Alamos Neutron Science Center’s WNR facility. The energy of the neutrons was determined using the time‐of‐flight technique. The data were taken using the GEANIE spectrometer. The cross sections for emission of 202 γ rays of 181–191Ir were determined for neutron energies 0.2 MeV < En < 300 MeV. Comparison with model calculations, using the GNASH reaction model, and with GEANIE results from the similar 193Ir(n,xnγ) reactions is made.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

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.