DOI: 10.31274/rtd-180817-524
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Solution of the space-time dependent neutron kinetics equations for a reflected slab reactor

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Cited by 2 publications
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“…As may be seen in Table 1, the fast neutron absorption cross section is taken to be zero and all fissions are assumed to occur in the thermal group with the fission neutrons enter ing the fast group. This model was used previously by Loewe (15) and later by McFadden (10). The original intention was to consider the same perturbations as the latter and compare results along with those obtained from WIGLE-40.…”
Section: Application and Model Usedmentioning
confidence: 99%
See 1 more Smart Citation
“…As may be seen in Table 1, the fast neutron absorption cross section is taken to be zero and all fissions are assumed to occur in the thermal group with the fission neutrons enter ing the fast group. This model was used previously by Loewe (15) and later by McFadden (10). The original intention was to consider the same perturbations as the latter and compare results along with those obtained from WIGLE-40.…”
Section: Application and Model Usedmentioning
confidence: 99%
“…The orthogonality is utilized in the determination of the time coefficients. Another modal approach utilizes Green's function modes (6,7,8,9,10).…”
mentioning
confidence: 99%
“…and later by McFadden(10). The original intention was to consider the same perturbations as the latter and compare results along with those obtained from WIGLE-40.…”
mentioning
confidence: 99%