𝑅-Process Nucleosynthesis in MHD Jet Explosions of Core-Collapse Supernovae

Figure 7

Nucleosynthesis calculation results using ETFSI (a) and FRDM (b). The third peak is reproduced for both mass formula. However, the slope of the abundance pattern of FRDM is too steep around 𝐴≃200 to compare with the solar pattern. The last peak of 𝐴>200 cannot be reproduced in both cases.

(a)

(b)