Mixing neutron star material into the jets in the common envelope jets supernova r-process scenario

I find that the accretion disk around the neutron star (NS) that enters the core of a massive evolved star in the frame of the common-envelope jets supernova (CEJSN) r-process scenario can penetrate the crust of the NS, mix neutron-rich crust material into the disk, and enrich the jets that the disk...

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Bibliographic Details
Main Author: Noam Soker
Format: Article
Language:English
Published: Maynooth Academic Publishing 2025-05-01
Series:The Open Journal of Astrophysics
Online Access:https://doi.org/10.33232/001c.138777
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