1960
DOI: 10.13182/nse60-a25728
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Thermal Neutron Flux Spectrum in a Medium with a Temperature Discontinuity

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Cited by 28 publications
(6 citation statements)
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“…An important advantage of our numerical approach is that we need make no major simplifying assumptions to facilitate the analysis. For example the early classic analysis of Kottwitz (1960) for this problem, using diffusion theory, assumes no absorption or neutron sources in the moderator. These assumptions are also made by the later transport theory analyses of Williams (1965Williams ( , 1968, Jauho and Virjo (1968) and Gritton and Leonard (1969).…”
Section: Introductionmentioning
confidence: 99%
“…An important advantage of our numerical approach is that we need make no major simplifying assumptions to facilitate the analysis. For example the early classic analysis of Kottwitz (1960) for this problem, using diffusion theory, assumes no absorption or neutron sources in the moderator. These assumptions are also made by the later transport theory analyses of Williams (1965Williams ( , 1968, Jauho and Virjo (1968) and Gritton and Leonard (1969).…”
Section: Introductionmentioning
confidence: 99%
“…In a previous publication (Williams 1965), the author has described a method for computing the neutron flux in a medium with a non-uniform physical temperature. This technique employed the heavy gas model of scattering and the full transport equation; in this way errors arising from diffusion theory in the Kottwitz problem were assessed (Kottwitz 1960) Jauho and Virjo have extended the author's original equation to arbitrary geometry, and in particular to spherical systems, thereby calculating the effect of the radius of curvature of a temperature discontinuity (Jauho and Virjo 1968). The complete flux distribution has also recently been derived for the Kottwitz problem by the application of Case's method of singular eigenfunctions (Gritton and Leonard 1967).…”
Section: Introductionmentioning
confidence: 99%
“…Kottwitz (11) has applied two simple schemes to the problem Figure 9» Deviation of flux spectrum from Maxv;ellian due to absorption only, due to non-uniform temperature only and due to both absorption and non-uniform temperature in an non-absorption medium. Of these, the neutron tem perature approximation which assumes that the thermal energy neutrons have a Haxwellian spectrum at every point in space has been shown to be less satisfactory than the other method due to Selengut (12), Recently, Pearce and Kennedy (21) have worked out the same problem as considered by Kottwitz by applying multigroup technique.…”
Section: Discussionmentioning
confidence: 99%