論文

査読有り
2000年1月

Fission source convergence of monte carlo criticality calculations in weakly coupled fissile arrays

Journal of Nuclear Science and Technology
  • Toshihiro Yamamoto
  • ,
  • Takemi Nakamura
  • ,
  • Yoshinori Miyoshi

37
1
開始ページ
41
終了ページ
52
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1080/18811248.2000.9714865

Anomalous fission source convergence in a Monte Carlo criticality calculation for a weakly coupled array of two fissile material units are demonstrated. Introducing coupling coefficients among array units, it is quantitatively explained that this anomaly is caused by an insufficient restoring force to the true distribution and its large statistical uncertainty, especially, in a symmetric system. A new approach for estimating the fission source intensity ratio in an array is proposed by obtaining the eigenvector of a coupling coefficient matrix. This method also gives the uncertainty of the ratio as well as the ratio, which is available for evaluating the accuracy of the obtained ratio. The correlation between a calculated keff and the fission source intensity ratio is formulated. It is illustrated theoretically and empirically that there is no significant correlation in a symmetric two-unit array system. In general, care should be taken that a calculated keg may be biased by an incorrect fission source distribution, especially, in a slightly asymmetric system. A regionwise weight adjustment method is developed such that the fission source intensity ratio is forced to converge to a predetermined ratio. Using this method, a satisfactory convergence can be achieved. A larger number of neutrons per generation is recommended for a Monte Carlo criticality calculation of a weakly coupled array of units. © 2000 Taylor & Francis Group, LLC.

リンク情報
DOI
https://doi.org/10.1080/18811248.2000.9714865
CiNii Articles
http://ci.nii.ac.jp/naid/10004308135
Scopus
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=0002656048&origin=inward
Scopus Citedby
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ID情報
  • DOI : 10.1080/18811248.2000.9714865
  • ISSN : 0022-3131
  • CiNii Articles ID : 10004308135
  • SCOPUS ID : 0002656048

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