Exploration of LIBS as a novel and rapid elemental mapping technique of nuclear fuels in the form of surrogate TRISO particles

Benjamin T. Manard, Hunter B. Andrews, C. Derrick Quarles, Veronica C. Bradley, Peter Doyle, N. Alex Zirakparvar, Daniel R. Dunlap, Cole R. Hexel

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

Laser-induced breakdown spectroscopy (LIBS) was employed to characterize coatings on surrogate fuel particles. Tri-structural isotropic (TRISO) particles are a proposed nuclear fuel alternative for high temperature reactors. These particles are constructed of a ZrO2 kernel (as a surrogate to uranium), surrounded by an inner pyrolytic carbon layer and are surrounded by an outer carbide layer (ZrC, presented here) to act as a barrier to fission products generated during nuclear reactions. These particles are embedded within a graphite compact and housed within the reactor core. Simply put, due to their robust nature, performing elemental analysis of these particles poses a challenge. Presented here, LIBS is explored as a method for characterizing elemental constituents of these particles, with the focus being on rapid elemental mapping and depth profiling. Different from traditional elemental analysis techniques (e.g., inductively coupled plasma - based methods), LIBS is advantageous because it can directly analyze the sample surface and can detect light elements such as C and O, making it a viable technique for the analysis of small, multilayered particles as spatial elemental information is warranted in the production of these particles. In the work presented here, LIBS was successfully used for discerning small layers (30-50 μm), detecting the location of carbon and oxygen layers, providing fast 2-D mapping (<5 min per particle) and rapid depth profiling (10 s per particle).

Original languageEnglish
Pages (from-to)1412-1420
Number of pages9
JournalJournal of Analytical Atomic Spectrometry
Volume38
Issue number7
DOIs
StatePublished - May 16 2023

Funding

This work was supported by the Laboratory Directed Research and Development Program of Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for the U.S. Department of Energy under contract DE-AC-05-000R22725. The authors would like to acknowledge Adam Malin (ORNL) for the assistance with graphics and Mark Boris (ORNL) for the assistance with optical images presented within this manuscript. Coating development was supported by the DOE Deep Burn Program and coating characterization was supported under NASA's Space Technology Mission Directorate (STMD) through the Space Nuclear Propulsion (SNP) project. This manuscript has been authored in part by UT-Battelle, LLC, under contract DE-AC05-00OR22725 with the US Department of Energy (DOE). The US government retains and the publisher, by accepting the article for publication, acknowledges that the US government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for US government purposes. DOE will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan ( http://energy.gov/downloads/doe-public-access-plan ).

FundersFunder number
Adam Malin
DOE Deep Burn Program
U.S. Department of EnergyDE-AC-05-000R22725
National Aeronautics and Space Administration
Oak Ridge National Laboratory

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