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000020168 0247_ $$2DOI$$a10.3938/jkps.59.791
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000020168 041__ $$aeng
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000020168 084__ $$2WoS$$aPhysics, Multidisciplinary
000020168 1001_ $$0P:(DE-HGF)0$$aLeray, S.$$b0
000020168 245__ $$aResults from the IAEA Benchmark of Spallation Models
000020168 260__ $$aSeoul$$bKorean Physical Society$$c2011
000020168 300__ $$a791 - 796
000020168 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article
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000020168 440_0 $$014823$$aJournal of the Korean Physical Society$$v59$$x0374-4884$$y2
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000020168 520__ $$aSpallation reactions play an important role in a wide domain of applications. In the simulation codes used in this field, the nuclear interaction cross-sections and characteristics are computed by spoliation models. The International Atomic Energy Agency (IAEA) has recently organised a benchmark of the spoliation models used or that could be used in the future into high-energy transport codes. The objectives were, first, to assess the prediction capabilities of the different spoliation models for the different mass and energy regions and the different exit channels and, second, to understand the reason for the success or deficiency of the models. Results of the benchmark concerning both the analysis of the prediction capabilities of the models and the first conclusions on the physics of spoliation models are presented.
000020168 536__ $$0G:(DE-Juel1)FUEK413$$2G:(DE-HGF)$$aPhysik der Hadronen und Kerne$$cP53$$x0
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000020168 650_7 $$2WoSType$$aJ
000020168 65320 $$2Author$$aSpallation
000020168 65320 $$2Author$$aNeutron sources
000020168 65320 $$2Author$$aIntra-nuclear cascade models
000020168 65320 $$2Author$$aEvaporation-fission models
000020168 7001_ $$0P:(DE-HGF)0$$aDavid, J. C.$$b1
000020168 7001_ $$0P:(DE-HGF)0$$aKhandaker, M.$$b2
000020168 7001_ $$0P:(DE-HGF)0$$aMank, G.$$b3
000020168 7001_ $$0P:(DE-HGF)0$$aMengoni, A.$$b4
000020168 7001_ $$0P:(DE-HGF)0$$aOtsuka, N.$$b5
000020168 7001_ $$0P:(DE-Juel1)VDB384$$aFilges, D.$$b6$$uFZJ
000020168 7001_ $$0P:(DE-HGF)0$$aGallmeier, F.$$b7
000020168 7001_ $$0P:(DE-HGF)0$$aKonobeyev, A.$$b8
000020168 7001_ $$0P:(DE-HGF)0$$aMichel, R.$$b9
000020168 773__ $$0PERI:(DE-600)2046361-3$$a10.3938/jkps.59.791$$gVol. 59, p. 791 - 796$$p791 - 796$$q59<791 - 796$$tJournal of the Korean Physical Society$$v59$$x0374-4884$$y2011
000020168 8567_ $$uhttp://dx.doi.org/10.3938/jkps.59.791
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000020168 9131_ $$0G:(DE-Juel1)FUEK413$$bStruktur der Materie$$kP53$$lPhysik der Hadronen und Kerne$$vPhysik der Hadronen und Kerne$$x0
000020168 9132_ $$0G:(DE-HGF)POF3-612$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vCosmic Matter in the Laboratory$$x0
000020168 9141_ $$y2011
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