A shell-model variant exploiting the energy-localized Brink-Axel hypothesis computes electric and magnetic radiative strength functions across relevant energies, with benchmarks on 24Mg and new findings for 56Fe on M1 smoothness and incomplete low-energy strength reproduction.
R., Kawano, T., Ullmann, J
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Treating select nuclear isomers as independent states with temperature-dependent rates in r-process networks yields predictions that the 743.3 keV Nb-97m and 555.6 keV Y-91m lines may be detectable at galactic distances by COSI, AMEGO, or LOX.
citing papers explorer
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Radiative strength functions from the energy-localized Brink-Axel hypothesis
A shell-model variant exploiting the energy-localized Brink-Axel hypothesis computes electric and magnetic radiative strength functions across relevant energies, with benchmarks on 24Mg and new findings for 56Fe on M1 smoothness and incomplete low-energy strength reproduction.
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Nuclear Isomers and Their Impact on Gamma-Ray Emission in Binary Neutron Star Mergers
Treating select nuclear isomers as independent states with temperature-dependent rates in r-process networks yields predictions that the 743.3 keV Nb-97m and 555.6 keV Y-91m lines may be detectable at galactic distances by COSI, AMEGO, or LOX.