56Ni Production in Long-lived Binary Neutron Star Merger Remnants
We investigate the nucleosynthesis and kilonova emission based on numerical-relativity binary neutron star merger simulations that incorporate a two-moment neutrino-transport scheme. Unlike in previous works with simpler neutrino treatments, a massive, fast (up to v = 0.3 c ), proton-rich neutrino-...
Kaydedildi:
| Asıl Yazarlar: | , , , , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2026-01-01
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| Seri Bilgileri: | The Astrophysical Journal Letters |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/2041-8213/ae4104 |
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