Precision analysis of 198Au beta spectral shape

T. Nagarajan, M. Ravindranath, K. V. Reddy
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引用次数: 3

Abstract

The investigation of the 965 keV transitions of 198Au shows that the same data analysed with the Fermi function taken from NBS tables and that from Dzhelepov and Zyrianova (corrected for finite size) differ by 3% in slope. With a shape factor C(W)=k(1+aW) the coefficient a has been determined to be -0.022+or-0.011 using Bhalla and Rose tables with Buhring's screening correction and the correct end point determined from the proper physical behaviour of the shape factor in the neighbourhood of the end point energy. The use of this coefficient through the PBS method gives alpha 412K=(301+or-3)10-4 in agreement with theory as well as the recent very accurate IEC methods. This means that the disagreement of the PBS method with theory and other accurate methods arises mainly through the occurrence of a shape factor in the electron energy spectrum and the use of the correct shape factor in the PBS method gives good agreement.
198Au β光谱形状的精度分析
对198Au的965 keV跃迁的研究表明,用NBS表中的费米函数分析的相同数据与Dzhelepov和Zyrianova(修正有限尺寸)的数据在斜率上有3%的差异。形状因子C(W)=k(1+aW),系数a已被确定为-0.022+或0.011使用Bhalla和Rose表与布林的筛选校正和正确的端点由形状因子在端点能量附近的适当物理行为确定。通过PBS方法使用该系数得到alpha 412K=(301+or-3)10-4,与理论以及最近非常精确的IEC方法一致。这意味着PBS方法与理论和其他精确方法的不一致主要是由于电子能谱中出现了形状因子,而在PBS方法中使用正确的形状因子得到了很好的一致性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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