Impact of molybdenum cross sections on FHR analysis

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  • Kyle M. Ramey
    Georgia Institute of Technology, Atlanta.
  • Marat Margulis
    University of Cambridge
  • Nathaniel Read
    University of Cambridge
  • Eugene Shwageraus
    University of Cambridge
  • Bojan Petrovic
    Georgia Institute of Technology, Atlanta.
A recent benchmarking effort, under the auspices of the Organization for Economic Cooperation and Development (OECD) Nuclear Energy Agency (NEA), has been made to evaluate the current state of modeling and simulation tools available to model fluoride salt-cooled high temperature reactors (FHRs). The FHR benchmarking effort considered in this work consists of several cases evaluating the neutronic parameters of a 2D prismatic FHR fuel assembly model using the participants’ choice of simulation tools. Benchmark participants blindly submitted results for comparison with overall good agreement, except for some which significantly differed on cases utilizing a molybdenum-bearing control rod. Participants utilizing more recently updated explicit isotopic cross sections had consistent results, whereas those using elemental molybdenum cross sections observed reactivity differences on the order of thousands of pcm relative to their peers. Through a series of supporting tests, the authors attribute the differences as being nuclear data driven from using older legacy elemental molybdenum cross sections. Quantitative analysis is conducted on the control rod to identify spectral, reaction rate, and cross section phenomena responsible for the observed differences. Results confirm the observed differences are attributable to the use of elemental cross sections which overestimate the reaction rates in strong resonance channels.

Keywords

  • Molten salt reactor (MSR), Fluoride salt cooled high temperature, reactor (FHR), Molybdenum cross section, Serpent, WIMS
Original languageEnglish
Pages (from-to)817-825
JournalNUCLEAR ENGINEERING AND TECHNOLOGY
Volume54
Issue number3
Early online date23 Sept 2021
DOIs
Publication statusPublished - 1 Mar 2022

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