{"title":"An analytical treatment of time- and space-dependent asymptotic behaviour of slowing down neutron","authors":"Y. Yamamura, Y. Kitazoe, T. Sekiya","doi":"10.1016/0022-3107(73)90003-8","DOIUrl":null,"url":null,"abstract":"<div><p>Asymptotic aspects of space- and time-dependent slowing down of a pulsed neutron is analytically studied, based on the time-dependent diffusion equation. The calculations are mainly concerned with the flux distribution ψ(<em>r, u, t</em>) and the spatially dependent most probable slowing down time <em>t</em><sub>max</sub>(<em>r, u</em>). The analytic solution for ψ(<em>r, u, t</em>) indicates that its spatial dependence is determined only by the time-dependent neutron age τ(<em>u, t</em>), while <em>t</em><sub>max</sub>(<em>r, u</em>) is shown to be dominantly influenced by the stationary neutron age <em>τ</em><sub><em>s</em></sub>(<em>u</em>).</p><p>Through these analyses, the interesting relations are obtained: (a) When <span><math><mtext>t = t</mtext><msub><mi></mi><mn>s</mn></msub><mtext> ≡ «t</mtext><mtext>a</mtext><mtext>̊</mtext><msub><mi></mi><mn>0</mn></msub><mtext>{1 − ξ/(ξ + 4)(ξ + 2)}</mtext></math></span>, τ(<em>u, t</em>), coincides with <em>τ</em><sub><em>s</em></sub>,(<em>u</em>), which implies that the spatial dependence of ψ(<em>r, u, t</em>) at that time is analogous to that of the stationary neutron distribution, where «<em>t</em>å<sub>0</sub> is the first time moment. (b) The most probable slowing down time <em>t</em><sub>max</sub>(<em>r</em>, u) at <span><math><mtext>r = √«r</mtext><msup><mi></mi><mn>2</mn></msup><mtext>a</mtext><mtext>̊</mtext><mtext>)</mtext></math></span> (standard notation) becomes equal to the most probable slowing down time <em>t</em><sub><em>m</em></sub> of the spatially independent distribution ψ(<em>u, t</em>).</p><p>The cross sections employed here are assumed to be constant, but different cross-sections for the source neutrons are allowed.</p></div>","PeriodicalId":100811,"journal":{"name":"Journal of Nuclear Energy","volume":"27 5","pages":"Pages 303-315"},"PeriodicalIF":0.0000,"publicationDate":"1973-05-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0022-3107(73)90003-8","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Nuclear Energy","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/0022310773900038","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
Asymptotic aspects of space- and time-dependent slowing down of a pulsed neutron is analytically studied, based on the time-dependent diffusion equation. The calculations are mainly concerned with the flux distribution ψ(r, u, t) and the spatially dependent most probable slowing down time tmax(r, u). The analytic solution for ψ(r, u, t) indicates that its spatial dependence is determined only by the time-dependent neutron age τ(u, t), while tmax(r, u) is shown to be dominantly influenced by the stationary neutron age τs(u).
Through these analyses, the interesting relations are obtained: (a) When , τ(u, t), coincides with τs,(u), which implies that the spatial dependence of ψ(r, u, t) at that time is analogous to that of the stationary neutron distribution, where «tå0 is the first time moment. (b) The most probable slowing down time tmax(r, u) at (standard notation) becomes equal to the most probable slowing down time tm of the spatially independent distribution ψ(u, t).
The cross sections employed here are assumed to be constant, but different cross-sections for the source neutrons are allowed.