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dc.contributor.authorMayer, G.
dc.contributor.authorGuba, A.
dc.date.accessioned2022-02-04T22:16:49Z
dc.date.available2022-02-04T22:16:49Z
dc.date.copyright6/3/2020 12:00:00 AM
dc.date.issued2020
dc.identifier.issn2332-8983
dc.identifier.otherners_006_04_041304.pdf
dc.identifier.urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4275249
dc.description.abstractALLEGRO is a helium-cooled fast reactor, which is being developed by the Czech Republic, France, Hungary, Slovakia, and Poland. It will be the demonstrator of the GFR-2400-MWth Generation IV gas-cooled fast reactors. In ALLEGRO, a three-loop safety system is designed to remove decay heat during accident conditions. The nonrotating blower blades may represent a huge pressure loss in the decay heat removal loop (DHR), which hinders natural circulation. The lower the pressure loss coefficient of the DHR blower blades is, the better cooling is available during natural circulation. On the other hand, a large core bypass develops if a DHR valve is opened inadvertently during normal operation. In this case, the higher DHR blower pressure loss is better from core cooling point of view. Consequently, the low pressure loss of the DHR blower is advantageous for core cooling in station blackout (SBO) event but disadvantageous for inadvertent DHR valve opening event. Both the above-mentioned cases may lead to insufficient core cooling in accident conditions, which threatens the integrity of the reactor core. In this study, we present CATHARE thermohydraulic calculations to assess the sensitivity of the DHR blower pressure loss coefficient for the above-mentioned two cases.
dc.publisherThe American Society of Mechanical Engineers (ASME)
dc.titleRole of the Nonrotating Decay Heat Removal Blower Pressure Loss in ALLEGRO Reactor
dc.typeJournal Paper
dc.journal.volume6
dc.journal.issue4
dc.journal.titleJournal of Nuclear Engineering and Radiation Science
dc.identifier.doi10.1115/1.4045805
dc.journal.fristpage041304-1
dc.journal.lastpage041304-6
dc.page6
dc.treeJournal of Nuclear Engineering and Radiation Science:;2020:;volume( 006 ):;issue: 004
dc.contenttypeFulltext


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