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Prediction of the Average Decay Heat per Fission for MOX Nuclear Fuel
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作者 Amir M. Alramady Hanan M. Barashed Sherif S. Nafee 《Journal of Applied Mathematics and Physics》 2022年第3期887-899,共13页
MIXED Oxide Nuclear fuel (MOX) contains both uranium and plutonium in oxidized form. It is important to calculate the nuclear decay heat due to the single thermal fission (fission due to 0.0235 eV neutron) for all fis... MIXED Oxide Nuclear fuel (MOX) contains both uranium and plutonium in oxidized form. It is important to calculate the nuclear decay heat due to the single thermal fission (fission due to 0.0235 eV neutron) for all fissile nuclei in the MOX fuels (U<sup>235</sup>, Pu<sup>239</sup>, and Pu<sup>241</sup>). These fissile nuclei are the main source of the decay heat in MOX fuel. Decay heat calculation of the weighted fissile material content in MOX fuel is also important. A numerical method was used in this work to calculate the concentrations of all fission products due to the individual thermal fission of the three fissile materials as a function of time N(t). The decay heat calculations for the three fissile materials are directly calculated using the summation method by knowing the different concentrations of fission products over time. The average decay heat of the MOX fuel in induced thermal fission is also concluded. The most influential nuclei in the decay heat were also identified. The method used has been validated by several comparisons before, but the new in this work is using the most recent Evaluated Nuclear Data Library ENDF/B-VIII.0. Calculations of decay heat show very common trends for a period of 10<sup>7</sup> sec after the fission burst of thermal fissions of individual fissile nuclei. Moreover, the code showed high capability in calculating the fission fragments inventories and decay heats due to the decay of fission fragments of 31 fissionable nuclei. 展开更多
关键词 Nuclear Decay Heat fission burst fission Fragments MOX Fuel MATLAB
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Fission Fragment Decay Heat by Using the Most Recent Evaluated Nuclear Data Library ENDF/B-VIII
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作者 Amir M. Alramady Hanan M. Barashed Sherif S. Nafee 《Journal of Applied Mathematics and Physics》 2022年第4期1182-1190,共9页
In this paper, a home-made code was designed to calculate the decay heat emitted by fission fragments as a result of successive radioactive emissions after a fission burst. The nuclear data necessary for the calculati... In this paper, a home-made code was designed to calculate the decay heat emitted by fission fragments as a result of successive radioactive emissions after a fission burst. The nuclear data necessary for the calculations was extracted from the latest version of the Evaluated Nuclear Data Library ENDF/B-VIII.0. The code can calculate the decay heat of thermal and fast neutron-induced fission reactions on the isotopes of Thorium, Protactinium, Uranium, Neptunium, Plutonium, Americium, Curium, California, Einsteinium, and Fermium. A numerical method was used in this work to calculate the decay heat of all fission fragments due to the individual thermal or fast fissions of the isotopes of the previous ten actinides. The most influential nuclei in the decay heat were also identified at different times after the fission event. Moreover, the code showed high capability in calculating the fission fragments inventories and decay heats due to the decay of fission fragments of 31 fissionable nuclei. 展开更多
关键词 Nuclear Decay Heat fission burst fission Fragments MATLAB
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快中子脉冲反应堆厅内空气中裂变产物污染的研究 被引量:1
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作者 黄宪果 苑国琪 +1 位作者 邢世雄 张德鑫 《辐射防护》 CAS CSCD 北大核心 1996年第2期109-113,共5页
本文研究了快中子脉冲反应堆大厅内空气中裂变产物的污染问题。通过对CFBR-Ⅱ快中子脉冲反应堆爆发额定产额脉冲(1.53×1016裂变)后,厅内气溶胶的取样和γ谱分析,确定了裂变产物从黄铜壳内空气中释放到厅内空气中... 本文研究了快中子脉冲反应堆大厅内空气中裂变产物的污染问题。通过对CFBR-Ⅱ快中子脉冲反应堆爆发额定产额脉冲(1.53×1016裂变)后,厅内气溶胶的取样和γ谱分析,确定了裂变产物从黄铜壳内空气中释放到厅内空气中形成气溶胶的释放份额为5×10-3。利用此释放份额计算了厅内空气中不同放射性核素的气溶胶浓度;还计算了该堆爆发额定产额脉冲后不同冷却时间t厅内空气中无分凝混合裂变产物的导出空气浓度DAC(t)值,为该堆辐射安全分析和现场辐射防护提供了依据。 展开更多
关键词 快中子脉冲 反应堆 裂变产物 气溶胶 释放份额
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用于脉冲堆裂变总数测量的闪烁体探测器研制
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作者 高辉 荣茹 +3 位作者 代少丰 李兵 刘晓波 范晓强 《原子能科学技术》 EI CAS CSCD 北大核心 2014年第S1期646-649,共4页
采用波形积分法研制了用于脉冲堆裂变总数测量的闪烁体探测器,采用脉冲峰和脉冲坪信号分路引出的设计,同时测量裂变率相差较大的脉冲峰和脉冲坪。该探测器具有线性电流大、测量范围宽的特点,在测量小产额脉冲时更具优势。该裂变总数测... 采用波形积分法研制了用于脉冲堆裂变总数测量的闪烁体探测器,采用脉冲峰和脉冲坪信号分路引出的设计,同时测量裂变率相差较大的脉冲峰和脉冲坪。该探测器具有线性电流大、测量范围宽的特点,在测量小产额脉冲时更具优势。该裂变总数测量方法与其他方法获得的结果一致。 展开更多
关键词 闪烁体探测器 波形积分法 脉冲堆 裂变总数
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浅超瞬发临界系统中子引发持续裂变链的概率
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作者 刘晓波 杜金峰 范晓强 《原子能科学技术》 EI CAS CSCD 北大核心 2013年第7期1107-1111,共5页
根据中子在核系统中发生不同反应的概率,推导了中子引发持续裂变链概率W(r,E,Ω,t)满足的方程;在定态、浅超瞬发临界前提下,采用二阶近似和微扰方法,得到了引发中子源分布下中子引发概率的表达式。由表达式和Godiva-Ⅱ、Caliban、CFBR-... 根据中子在核系统中发生不同反应的概率,推导了中子引发持续裂变链概率W(r,E,Ω,t)满足的方程;在定态、浅超瞬发临界前提下,采用二阶近似和微扰方法,得到了引发中子源分布下中子引发概率的表达式。由表达式和Godiva-Ⅱ、Caliban、CFBR-Ⅱ脉冲堆的参数得到中子引发脉冲的平均概率分别为0.000 32、0.000 54和0.000 27,采用Godiva-Ⅱ、Caliban自发裂变源引发脉冲实验数据对理论结果进行了比较和分析讨论。 展开更多
关键词 超瞬发临界 持续裂变链 中子引发概率 脉冲堆
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快中子脉冲堆弱源爆发脉冲实验理论研究
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作者 刘建军 施研博 王利民 《核科学与工程》 CAS CSCD 北大核心 2019年第6期1006-1021,共16页
我们在应用Hansen理论研究快中子脉冲堆弱源爆发脉冲实验时发现,理论与实验结果差距非常大。对此,我们分析了原因,然后从求解系统中子数概率分布函数出发,研究和求解了系统有限长裂变链的期望值,给出了有限长裂变链期望值的求解方法和... 我们在应用Hansen理论研究快中子脉冲堆弱源爆发脉冲实验时发现,理论与实验结果差距非常大。对此,我们分析了原因,然后从求解系统中子数概率分布函数出发,研究和求解了系统有限长裂变链的期望值,给出了有限长裂变链期望值的求解方法和基本形式,讨论和定量计算了Godiva-Ⅱ和CFBR-Ⅱ脉冲堆有限长裂变链的期望值。然后研究了有限长裂变链导致缓发中子先驱核增值行为,结果表明,在等待爆发脉冲期间缓发中子数可发生数倍的变化。最后,在两种不同的物理假定下,对Hansen模型给予了改进。改进后的模型可以较理想地模拟Godiva-Ⅱ和CFBR-Ⅱ两个脉冲堆的实验结果,表明结果是可信的。 展开更多
关键词 脉冲堆 中子数概率分布函数 有限长裂变链 缓发中子先驱核 爆发脉冲概率分布函数
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包壳材料与裂变产物的相容性研究
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作者 许咏丽 王家英 李军刚 《高技术通讯》 EI CAS CSCD 1992年第10期24-26,共3页
关键词 燃料元件 包壳管 裂变 反应堆
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World-Universe Model—Alternative to Big Bang Model 被引量:1
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 2020年第1期133-158,共26页
This manuscript provides a comparison of the Hypersphere World-Universe Model (WUM) with the prevailing Big Bang Model (BBM) of the Standard Cosmology. The performed analysis of BBM shows that the Four Pillars of the ... This manuscript provides a comparison of the Hypersphere World-Universe Model (WUM) with the prevailing Big Bang Model (BBM) of the Standard Cosmology. The performed analysis of BBM shows that the Four Pillars of the Standard Cosmology are model-dependent and not strong enough to support the model. The angular momentum problem is one of the most critical problems in BBM. Standard Cosmology cannot explain how Galaxies and Extra Solar systems obtained their substantial orbital and rotational angular momenta, and why the orbital momentum of Jupiter is considerably larger than the rotational momentum of the Sun. WUM is the only cosmological model in existence that is consistent with the Law of Conservation of Angular Momentum. To be consistent with this Fundamental Law, WUM discusses in detail the Beginning of the World. The Model introduces Dark Epoch (spanning from the Beginning of the World for 0.4 billion years) when only Dark Matter Particles (DMPs) existed, and Luminous Epoch (ever since for 13.8 billion years). Big Bang discussed in Standard Cosmology is, in our view, transition from Dark Epoch to Luminous Epoch due to Rotational Fission of Overspinning Dark Matter (DM) Supercluster’s Cores. WUM envisions Matter carried from the Universe into the World from the fourth spatial dimension by DMPs. Ordinary Matter is a byproduct of DM annihilation. WUM solves a number of physical problems in contemporary Cosmology and Astrophysics through DMPs and their interactions: Angular Momentum problem in birth and subsequent evolution of Galaxies and Extrasolar systems—how do they obtain it;Fermi Bubbles—two large structures in gamma-rays and X-rays above and below Galactic center;Diversity of Gravitationally-Rounded Objects in Solar system;some problems in Solar and Geophysics [1]. WUM reveals Inter-Connectivity of Primary Cosmological Parameters and calculates their values, which are in good agreement with the latest results of their measurements. 展开更多
关键词 Big Bang MODEL Four Pillars of Standard Cosmology ANGULAR MOMENTUM Problem Black Holes Hypersphere World-Universe MODEL Multicomponent DARK MATTER Macroobjects Structure Law of Conservation of ANGULAR MOMENTUM Medium of the World Inter-Connectivity of Primary Cosmological Parameters The Beginning of the World DARK EPOCH Rotational fission Luminous EPOCH Macroobject Shell MODEL DARK MATTER Core Gravitational burst Intergalactic Plasma Microwave Background Radiation Far-Infrared Background Radiation Emergent Phenomena CODATA
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瞬发超临界系统内持续裂变链的发展过程
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作者 高辉 谢奇林 +4 位作者 刘晓波 黄坡 宋凌莉 梁文峰 范晓强 《物理学报》 SCIE EI CAS CSCD 北大核心 2013年第22期115-119,共5页
根据基本的概率理论和瞬发临界附近有限裂变链的发展规律,推导了单脉冲源条件下脉冲堆引发持续裂变链过程中的中子数与时间关系式,并得到CFBR-II堆上实验的验证.该关系式进一步发展了Hansen理论模型,除了可以描述裂变链后期的发展趋势,... 根据基本的概率理论和瞬发临界附近有限裂变链的发展规律,推导了单脉冲源条件下脉冲堆引发持续裂变链过程中的中子数与时间关系式,并得到CFBR-II堆上实验的验证.该关系式进一步发展了Hansen理论模型,除了可以描述裂变链后期的发展趋势,还可以描述持续裂变链产生初期中子数的快速增长行为.讨论了引发时间与源强的关系,指出在弱源条件下,引发时间几乎不依赖于源强. 展开更多
关键词 持续裂变链 脉冲堆 引发时间
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