ISOTOPIC ANOMALIES IN SAMARIUM

被引:13
作者
CLAYTON, DD [1 ]
机构
[1] MAX PLANCK INST NUCL PHYS, D-6900 HEIDELBERG, FED REP GER
基金
美国国家航空航天局;
关键词
D O I
10.1016/0012-821X(79)90185-7
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The solar isotopic composition of Sm is decomposed into s, r and p components. The anomaly pattern discovered [1] in EK1-04 Allende inclusion can be presented as a fractionation of the average s-pattern from the average r-pattern. This representation requires a fractionation of 0.029% (amu)-1 and either (1) a 0.42% deficiency of s relative to r and a 0.15% deficiency of p relative to r, or (2) a 0.42% excess of r relative to s and a 0.27% excess of p relative to s. The nature of this anomaly suggests a systematic physical fractionation of r, s and p nuclei from each other in the initial condition leading to EK1-04. A neighboring supernova injection would not be expected to produce this anomaly. © 1979.
引用
收藏
页码:7 / 12
页数:6
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