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contributor authorHäkkinen, Silja
date accessioned2022-05-08T08:32:38Z
date available2022-05-08T08:32:38Z
date copyright3/15/2022 12:00:00 AM
date issued2022
identifier issn2332-8983
identifier otherners_008_04_041901.pdf
identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4284061
description abstractIn this work, the effect of averaging operating history parameters such as power history, boron concentration and coolant density, and temperature on spent nuclear fuel properties was investigated. The examined properties were assembly activity, decay heat, photon emission rate, spontaneous fission rate, and the concentration of some mobile nuclides and fissile nuclides. Calculations were performed on two similar VVER-440 fuel assemblies irradiated in different positions of the core using Serpent 2. Averaging power history over the entire irradiation history had a significant effect on assembly activity, decay heat, and photon emission rate overestimating these properties approximately 70% right after irradiation. However, the effect quickly died out and after 10 years of cooling, the effect was less than 1%. If the last cycle (third cycle) was modeled accurately and the power density of only the first two cycles was averaged, the differences remained always below 1%. The effect of operating history approximations on spontaneous fission rate and the nuclide concentrations was much smaller remaining mostly below 1.5%. The sensitivity of nuclide concentrations to approximations in individual operating history parameters was dependent on the nuclide in question and no trend applying to all studied nuclides could be observed.
publisherThe American Society of Mechanical Engineers (ASME)
titleImpact of Approximations in Operating History Data on Spent Fuel Properties With Serpent 2
typeJournal Paper
journal volume8
journal issue4
journal titleJournal of Nuclear Engineering and Radiation Science
identifier doi10.1115/1.4051444
journal fristpage41901-1
journal lastpage41901-10
page10
treeJournal of Nuclear Engineering and Radiation Science:;2022:;volume( 008 ):;issue: 004
contenttypeFulltext


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