An improved photo-absorption cross section model for the physics models regime in MCNPX

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Abstract

The photo-nuclear physics model capabilities utilising the CEM2k model implemented in the MCNPX code were improved >100 MeV photon energy by basing the photon transport on experimental photo-absorption cross sections of nuclides rather than on free nucleon cross sections. Below 100 MeV, the photo-nuclear physics model now uses isotope-specific giant dipole resonance (GDR) photo-absorption cross sections that are provided to the code in a parameterised form on a data file. Adjustments of the photo-fission cross sections were implemented to match the BOFOD evaluated data through a CEM2k internal parameter. The physics models with these improvements are better equipped to supplement the tabulated data based photo-nuclear MCNPX capability for isotopes with missing tabulated data evaluations especially in the GDR region, and has improved its predictive power at energies above the GDR resonances.

Original languageEnglish
Pages (from-to)264-269
Number of pages6
JournalRadiation Protection Dosimetry
Volume116
Issue number1-4
DOIs
StatePublished - Dec 20 2005

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