Bulletin of the American Physical Society
2018 Joint Fall Meeting of the Texas Sections of APS, AAPT and Zone 13 of the SPS
Volume 63, Number 18
Friday–Saturday, October 19–20, 2018; University of Houston, Houston, Texas
Session G01: Poster Session
7:50 PM,
Friday, October 19, 2018
TDECU Football Stadium
Room: Club Suite
Chair: Donna Stokes, University of Houston
Abstract ID: BAPS.2018.TSF.G01.25
Abstract: G01.00025 : Machine Learning Model to Predict Failure Modes of TRISO Particles under High-Temperature Gas-Cooled Reactor Accident Conditions*
Presenter:
Marielle D Gaspar
(Department of Physics and Astronomy, The University of Texas at San Antonio)
Authors:
Marielle D Gaspar
(Department of Physics and Astronomy, The University of Texas at San Antonio)
Seth Pritchard
(Department of Physics and Astronomy, The University of Texas at San Antonio)
Amanda D Fernandez
(Department of Computer Science, The University of Texas at San Antonio)
Elizabeth S Wood
(Department of Physics and Astronomy, The University of Texas at San Antonio)
Tristructured istropic particles, which contain a central kernel of uranium oxycarbide and are surrounded by a multilayered ceramic shell, are the fuel form proposed for high temperature gas-cooled reactors (HTGRs) and very high temperature gas-cooled reactors (VHTRs). These next generation nuclear reactors are proposed for operation at temperatures in excess of 600°C. Though He is the primary fuel coolant, the fuel form could see appreciable amounts of moisture, oxygen, carbon monoxide and carbon dioxide during certain accident scenarios. The exposure to a highly corrosive, mixed gas atmosphere can impact the integrity of the fuel form. The research presented incorporates machine learning approaches using the established thermodynamics of SiC-oxidant reactions and experimental data acquired to enable the prediction of catastrophic reactions, failure atmospheres, and SiC reactions with gas mixtures relevant to certain HTGR and VHTR accident scenarios.
*This work was supported by start-up funds provided by the UTSA College of Science to the Extreme Environmental Materials Laboratory through the Department of Physics and Astronomy. The work is continued from October 1, 2018-September 30, 2021 by funding provided by the Nuclear Energy Universities Program, Grant number 31310018M0046.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.TSF.G01.25
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