Abstract
The impact of nuclear mass uncertainties on the r -process abundances has been systematically studied with the classical r -process model by varying the mass of every individual nucleus in the range of ±0.1 to ±3.0 MeV based on six different mass models. A new quantitative relation between the uncertainties of r -process abundances and those of the nuclear masses is extracted, i.e., a mass uncertainty of ±0.5 MeV would lead to an abundance uncertainty of a factor around 2.5. It is found that this conclusion holds true for various mass models.
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CITATION STYLE
Jiang 姜, X. F. 晓飞, Wu 吴, X. H. 鑫辉, & Zhao 赵, P. W. 鹏巍. (2021). Sensitivity Study of r-process Abundances to Nuclear Masses. The Astrophysical Journal, 915(1), 29. https://doi.org/10.3847/1538-4357/ac042f
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