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![3
tion from developing. It can be shown (see Supplemental
Material [51]) that angular momentum is transferred effi-
ciently ...](https://image.slidesharecdn.com/1704-170903203632/75/Primordial-Black-Holes-and-r-Process-Nucleosynthesis-3-2048.jpg?cb=1669302460)
![6
[34] D. Kasen, R. Fernandez, and B. Metzger, Mon. Not. Roy.
Astron. Soc. 450, 1777 (2015), arXiv:1411.3726 [astro-
ph.HE...](https://image.slidesharecdn.com/1704-170903203632/75/Primordial-Black-Holes-and-r-Process-Nucleosynthesis-6-2048.jpg?cb=1669302460)
![8
density profile to follow a polytropic relation [52] with
index n = 1.5 − 3. This range for n subsumes various
NS models,...](https://image.slidesharecdn.com/1704-170903203632/75/Primordial-Black-Holes-and-r-Process-Nucleosynthesis-8-2048.jpg?cb=1669302460)
