论文标题
用于应用和基本核物理学的β-赛研究
Beta-decay studies for applied and basic nuclear physics
论文作者
论文摘要
在这篇综述中,我们将使用涵盖应用,核结构和天体物理学感兴趣的主题的总吸收技术介绍最近的β-赛研究结果。所研究的衰减之所以选择衰变,主要是因为它们对a)反应堆中的衰减热量具有很大的影响,这对于当前和将来的反应堆的安全性以及b)反应器电子抗毒剂谱,对粒子/核物理和反应堆监测感兴趣。对于这些研究,选择了总吸收技术,因为这是唯一允许人们从称为pandemonium效应的系统误差中获得β衰减概率的方法。此处提出和讨论的测量主要是在Jyvaskyla大学(芬兰)(芬兰)的Igisol设施进行的,该设施使用Jyfltrap Penning Trap提供的同位素纯梁。示出了例子,以表明我们对选定核的测量结果对反应器的衰减热和抗中性谱的预测产生了很大的影响。其中一些情况涉及β延迟中子发射,因此可以研究中子分离能量以上状态的γ-和中子排放之间的竞争。伽马与中子的发射比可用于约束中子捕获(N,伽马)横截面,以使天体物理学感兴趣的不稳定核。从测量结果中获得的信息也可以用于测试半衰期的核模型预测,以实现天体物理网络计算中感兴趣的衰减。这些比较还为核图表的特定区域的核结构方面提供了见解。
In this review we will present the results of recent beta-decay studies using the total absorption technique that cover topics of interest for applications, nuclear structure and astrophysics. The decays studied were selected primarily because they have a large impact on the prediction of a) the decay heat in reactors, important for the safety of present and future reactors and b) the reactor electron antineutrino spectrum, of interest for particle/nuclear physics and reactor monitoring. For these studies the total absorption technique was chosen, since it is the only method that allows one to obtain beta decay probabilities free from a systematic error called the Pandemonium effect. The measurements presented and discussed here were performed mainly at the IGISOL facility of the University of Jyvaskyla (Finland) using isotopically pure beams provided by the JYFLTRAP Penning trap. Examples are presented to show that the results of our measurements on selected nuclei have had a large impact on predictions of both the decay heat and the anti-neutrino spectrum from reactors. Some of the cases involve beta delayed neutron emission thus one can study the competition between gamma- and neutron-emission from states above the neutron separation energy. The gamma-to-neutron emission ratios can be used to constrain neutron capture (n,gamma)cross sections for unstable nuclei of interest in astrophysics. The information obtained from the measurements can also be used to test nuclear model predictions of half-lives and Pn values for decays of interest in astrophysical network calculations. These comparisons also provide insights into aspects of nuclear structure in particular regions of the nuclear chart.