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20 April 2024
 
  » arxiv » astro-ph/9701007

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R-Process Freezeout, Nuclear Deformation, and the Rare-Earth Element Peak
R. Surman ; J. Engel ; J.R. Bennett ; B.S. Meyer ;
Date 3 Dec 1996
Subject astro-ph nucl-th
AbstractWe use network calculations of r-process nucleosynthesis to explore the origin of the peak in the solar r-process abundance distribution near nuclear mass number A = 160. The peak is due to a subtle interplay of nuclear deformation and beta decay, and forms not in the steady phase of the r-process, but only just prior to freezeout, as the free neutrons rapidly disappear. Its existence should therefore help constrain the conditions under which the r-process occurs and freezes out.
Source arXiv, astro-ph/9701007
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