Gravitational wave emission in binary neutron star early post-merger within a dark environment
Using an effective Lagrangian model inspired by Takami et al. [1] we qualitatively study the early post-merger of a nearly symmetric binary Neutron Star (BNS) merger event with a non-vanishing ambient fraction of dark matter. For this we first mimic the dynamics of two oscillating Neutron Star (NS)...
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| Autors principals: | , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Elsevier
2025-03-01
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| Col·lecció: | Physics Letters B |
| Matèries: | |
| Accés en línia: | http://www.sciencedirect.com/science/article/pii/S0370269325001182 |
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