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dc.contributor.authorSun, Lan
dc.contributor.authorQiu, Liyan
dc.date.accessioned2025-04-21T10:26:08Z
dc.date.available2025-04-21T10:26:08Z
dc.date.copyright12/5/2024 12:00:00 AM
dc.date.issued2024
dc.identifier.issn2332-8983
dc.identifier.otherners_011_02_021901.pdf
dc.identifier.urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4306189
dc.description.abstractIn a deep geological repository (DGR) for the long-term disposal of radioactive waste, gases (e.g., hydrogen (H2), carbon dioxide (CO2) and methane (CH4)) can be generated through a number of processes, such as corrosion of various metals and alloys and degradation of organic materials. If gas induced pressure exceeds the containment capacity of the engineered barrier systems (EBS) or the host rock, the gases could migrate through these barriers and potentially expose people and the environment to radiation. Therefore, a good understanding on the long-term performance of these barriers against gas migration is an important component in DGR design and safety assessment. In the present work, a numerical model has been developed to simulate the diffusion of CO2 (one of the gas species) in the near field of a DGR with the generation from related chemical reactions. The generation of CO2 was investigated to determine if it is a critical factor to impact the DGR safety under Canadian geological formations. A commercial computational fluid dynamics (CFD) code, ANSYS Fluent was used for the calculations. The model considered pH and temperature effects on CO2 migration under Canadian DGR geochemistry conditions.
dc.publisherThe American Society of Mechanical Engineers (ASME)
dc.titleNumerical Analysis of Gas Generation and Migration in a Radioactive Waste Disposal Cell of a Deep Geological Repository
dc.typeJournal Paper
dc.journal.volume11
dc.journal.issue2
dc.journal.titleJournal of Nuclear Engineering and Radiation Science
dc.identifier.doi10.1115/1.4067173
dc.journal.fristpage21901-1
dc.journal.lastpage21901-6
dc.page6
dc.treeJournal of Nuclear Engineering and Radiation Science:;2024:;volume( 011 ):;issue: 002
dc.contenttypeFulltext


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