The Cusp–Halo Relation
Simulations have established that each halo of collisionless dark matter is expected to contain a ρ = Ar ^−1.5 density cusp at its center. This prompt cusp is a relic of the halo’s earliest moments and has a mass comparable to the cutoff scale in the spectrum of initial density perturbations. In t...
Guardado en:
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| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
IOP Publishing
2025-01-01
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| Colección: | The Astrophysical Journal |
| Materias: | |
| Acceso en línea: | https://doi.org/10.3847/1538-4357/ae0625 |
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