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Fig. 2


Dependence of the nucleosynthesis on the electron fraction Ye (from 0.05 upper left to 0.5 lower right), for s0 = 15 kB/baryon, vej = 0.25c and FRDM mass model. Red lines label the resulting abundances, blue symbols refer to the solar system r-process. Beyond hardly any heavy elements beyond the second r-process peak (A = 130) are produced.

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