{"title":"慢化中子随时间和空间渐近行为的解析处理","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":"{\"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}","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
摘要
基于时变扩散方程,分析研究了脉冲中子的时空慢化的渐近性质。计算主要涉及通量分布ψ(r, u, t)和空间相关的最可能慢化时间tmax(r, u)。ψ(r, u, t)的解析解表明,其空间相关性仅由随时间变化的中子年龄τ(u, t)决定,而tmax(r, u)主要受静止中子年龄τs(u)的影响。通过这些分析,得到了有趣的关系:(a)当t = ts≡«tamat0{1−ξ/(ξ + 4)(ξ + 2)}时,τ(u, t)与τs,(u)重合,这意味着此时ψ(r, u, t)的空间依赖性类似于平稳中子分布的空间依赖性,其中«tamat0是第一时刻矩。(b)最可能的慢化时间tmax(r, u)在r =√«r2)(标准符号)变成等于空间独立分布ψ(u, t)的最可能的慢化时间tm。这里采用的截面假定是恒定的,但是源中子的不同截面是允许的。
An analytical treatment of time- and space-dependent asymptotic behaviour of slowing down neutron
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.