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dc.contributor.authorPinem, Surian
dc.contributor.authorHartanto, Donny
dc.contributor.authorLiem, Peng Hong
dc.contributor.authorLuthfi, Wahid
dc.date.accessioned2023-11-29T19:34:51Z
dc.date.available2023-11-29T19:34:51Z
dc.date.copyright2/8/2023 12:00:00 AM
dc.date.issued2/8/2023 12:00:00 AM
dc.date.issued2023-02-08
dc.identifier.issn2332-8983
dc.identifier.otherners_009_03_031502.pdf
dc.identifier.urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4294873
dc.description.abstractThis paper presents the generation and the verification of the few-group homogenized cross section for Batan-FUEL code. This code is routinely used for fuel management in the G. A. Siwabessy Multipurpose Reactor (RSG-GAS). The Monte Carlo code Serpent 2 code, in conjunction with the latest nuclear data library ENDF/B-VIII.0, was used. Calculations using the existing newly generated few-group cross section data were carried out for the 88th core. The calculated core parameters such as excess reactivity and control rod worth are compared to the available experimental data. On the other hand, the fuel burnup fraction and radial power peaking factor (PPF) are compared to the results of Serpent 2. It was shown that the new cross section data have more consistency and a better agreement excess reactivity and control rod worth compared to the experimental data. Similarly, the U-235 burnup fraction and radial power peaking factor by the new cross section data are also shown to concur well with Serpent 2. The newly generated few-group cross section is recommended to replace the existing ones for the fuel management of RSG-GAS.
dc.publisherThe American Society of Mechanical Engineers (ASME)
dc.titleImprovement of Few-Group Homogenized Cross-Sections for RSG-GAS In-Core Fuel Management Code Batan-FUEL
dc.typeJournal Paper
dc.journal.volume9
dc.journal.issue3
dc.journal.titleJournal of Nuclear Engineering and Radiation Science
dc.identifier.doi10.1115/1.4056603
dc.journal.fristpage31502-1
dc.journal.lastpage31502-7
dc.page7
dc.treeJournal of Nuclear Engineering and Radiation Science:;2023:;volume( 009 ):;issue: 003
dc.contenttypeFulltext


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