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