Local NLD/PSF parameter uncertainties, not model choice, drive ~0.7 dex p-nuclide abundance spreads in SNIa and CCSN p-process calculations, mainly via nearby (γ,n) rates.
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The impact of nuclear uncertainties on the p-process nucleosynthesis in Supernovae
Local NLD/PSF parameter uncertainties, not model choice, drive ~0.7 dex p-nuclide abundance spreads in SNIa and CCSN p-process calculations, mainly via nearby (γ,n) rates.