“…In addition, the emission rate of the characteristic γ ray of interest from 91m Mo was added artificially into GEANT4 since the simulation physics did not accurately portray the population and decay of the isomeric state. A comparison with recent experimental data (Burbadge et al 2020) suggests that, when a 91 Mo nucleus is detected as a reaction product, there is a 10% probability that a γ ray is created with an energy of 652.9 keV, whose emission we randomize with an exponentially distributed time stamp over a half life of 64.6 s. The probability for the population of the 652.9 keV isomer is consistent with the results of the aforementioned TALYS calculation, which shows that, at 22.75 MeV, 20.7% of the total (p,pn) reactions result in the production of the isomeric state, 91m Mo. Combining this information with the γ intensities found on NNDC (Baglin 2013), we calculate a maximum emission rate of 10.01(21)% of the 652.9(7) keV γ ray in a (p,pn) reaction.…”