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.
Sieja, Phys
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CI-SM calculations supply new E1 photon strength function predictions for light nuclei that are fed into UHECR propagation simulations for a 40Ca source.
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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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Modeling Ultra-High-Energy Cosmic Rays propagation using the input from Configuration Interaction Shell Model
CI-SM calculations supply new E1 photon strength function predictions for light nuclei that are fed into UHECR propagation simulations for a 40Ca source.