Element Formation in Radiation-hydrodynamics Simulations of Kilonovae
Understanding the details of r -process nucleosynthesis in binary neutron star merger (BNSM) ejecta is key to interpreting kilonova observations and identifying the role of BNSMs in the origin of heavy elements. We present a self-consistent, two-dimensional, ray-by-ray radiation-hydrodynamic evoluti...
Gorde:
| Egile Nagusiak: | , , , |
|---|---|
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
IOP Publishing
2024-01-01
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| Saila: | The Astrophysical Journal Letters |
| Gaiak: | |
| Sarrera elektronikoa: | https://doi.org/10.3847/2041-8213/ad74e0 |
| Etiketak: |
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