CI-SM calculations supply new E1 photon strength function predictions for light nuclei that are fed into UHECR propagation simulations for a 40Ca source.
SG acknowledges financial support from F.R.S.- FNRS (Belgium)
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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.