双β和β衰变准粒子随机相位近似方法的等标量配对相互作用

IF 3.2 2区 物理与天体物理 Q2 PHYSICS, NUCLEAR
J. Terasaki, Y. Iwata
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引用次数: 4

摘要

我们在以前的一系列论文中提出了一种确定有效轴矢量电流耦合和等标量质子-中子配对相互作用强度的方法,用于用准粒子随机相位近似计算无中子双衰变的核矩阵元素。这两个参数的组合在这种方法中有不确定性,但现在这种不确定性被消除了。本文将该方法应用于$^{136}$Xe和$^{130}$Te的无中子双β衰变,并预测了核矩阵元素和缩短的半衰期。我们的计算首先通过使用双中微子双-$\beta$衰变的自检方法进行了测试,该测试确保了我们的方法在$^{136}$Xe上的应用。然而,事实证明,我们的方法在$^{130}$Te中并不成功。对我们计算的$^{138}$Xe的$\beta$衰变作了进一步的验证,得到了令人满意的结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Isoscalar pairing interaction for the quasiparticle random-phase approximation approach to double- β and β decays
We have proposed in a series of previous papers a method to determine the effective axial-vector current coupling and the strength of the isoscalar proton-neutron pairing interaction for calculating the nuclear matrix elements of the neutrinoless double-$\beta$ decay by the quasiparticle random-phase approximation. The combination of these two parameters have had an uncertainty in this approach, but now this uncertainty is removed. In this paper, we apply our method to the neutrinoless double-$\beta$ decays of $^{136}$Xe and $^{130}$Te and predict the nuclear matrix elements and reduced half-lives. Our calculation is tested first by a self-check method using the two-neutrino double-$\beta$ decay, and this test ensures the application of our method to $^{136}$Xe. It turns out, however, that our method is not successful in $^{130}$Te. Further test is made for our calculation of the $\beta$ decay of $^{138}$Xe, and a satisfactory result is obtained.
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来源期刊
Physical Review C
Physical Review C PHYSICS, NUCLEAR-
CiteScore
5.80
自引率
35.50%
发文量
863
期刊介绍: Physical Review C (PRC) is a leading journal in theoretical and experimental nuclear physics, publishing more than two-thirds of the research literature in the field. PRC covers experimental and theoretical results in all aspects of nuclear physics, including: Nucleon-nucleon interaction, few-body systems Nuclear structure Nuclear reactions Relativistic nuclear collisions Hadronic physics and QCD Electroweak interaction, symmetries Nuclear astrophysics
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