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Improved Numerical Generalization of the Bethe-Weizsacker Mass Formula for Prediction the Isotope Nuclear Mass, the Mass Excess Including of Artificial Elements 119 and 120

机译:Bethe-Weizsacker质量公式的改进数值概括,用于预测同位素核质量,包括人工元素119和120的质量过量

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George Gamow's liquid drop model of the nucleus can account for most of the terms in the formula and gives rough estimates for the values of the coefficients. Its semi-numerical equation was first formulated in 1935 by Weizsacker and in 1936 Bethe [1, 2], and although refinements have been made to the coefficients over the years, the structure of the formula remains the same today. Their formula gives a good approximation for atomic masses and several other effects, but does not explain the appearance of magic numbers of protons and neutrons, and the extra binding-energy and measure of stability that are associated with these numbers of nucleons. Mavrodiev and Deliyergiyev [3] formalized the nuclear mass problem in the inverse problem framework. This approach allowed them to infer the underlying model parameters from experimental observation, rather than to predict the observations from the model parameters. They formulated the inverse problem for the numerically generalized semi-empirical mass formula of Bethe and von Weizsacker going step-by-step through the AME2012 [4] nuclear database. The resulting parameterization described the measured nuclear masses of 2564 isotopes with a maximal deviation of less than 2.6 MeV, starting from the number of protons and number of neutrons equal to 1. The unknown functions in the generalized mass formula was discovered in a step-by-step way using the modified procedure realized in the algorithms developed by Aleksandrov [5-7] to solve nonlinear systems of equations via the Gauss-Newton method. In the presented herein article we describe a further development of the obtained by [3] formula by including additional factors,- magic numbers of protons, neutrons and electrons. This inclusion is based the well-known experimental data on the chemically induced polarization of nuclei and the effect of such this polarization on the rate of isotope decay. It allowed taking into account resonant interaction of the spins of nuclei and electron shells. As a result the maximal deviation from the measured nuclear masses of less than 1.9 MeV was reached. This improvement allowed prediction of the nuclear characteristics of the artificial elements 119 and 120.
机译:乔治·加莫(George Gamow)的原子核液滴模型可解释公式中的大多数项,并对系数值进行粗略估计。它的半数值方程式由Weizsacker和1936年的Bethe [1,2]于1935年首次公式化,尽管多年来对系数进行了改进,但该公式的结构至今仍保持不变。他们的公式很好地近似了原子质量和其他一些效应,但没有解释质子和中子的幻数的出现,以及与这些核子数相关的额外结合能和稳定性的度量。 Mavrodiev和Deliyergiyev [3]在反问题框架中形式化了核质量问题。这种方法允许他们从实验观察中推断出基础模型参数,而不是从模型参数中预测观察结果。他们为Bethe和von Weizsacker的数字广义半经验质量公式逐步通过AME2012 [4]核数据库制定了反问题。所得的参数化描述了从质子数和中子数等于1开始的2564个同位素的测量核质量,最大偏差小于2.6 MeV。在逐步发现中,发现了广义质量公式中的未知函数使用Aleksandrov [5-7]开发的算法中实现的改进过程的逐步方法,通过Gauss-Newton方法求解非线性方程组。在本文介绍的文章中,我们描述了通过[3]式获得的进一步发展,包括添加其他因子,质子,中子和电子的幻数。这种包含是基于化学诱导的原子核极化以及这种极化对同位素衰变速率的影响的众所周知的实验数据。它允许考虑核和电子壳自旋的共振相互作用。结果,与测量的核质量的最大偏差小于1.9 MeV。通过这种改进,可以预测人造元素119和120的核特性。

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