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...
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| Hlavní autor: | |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
IOP Publishing
2025-01-01
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| Edice: | The Astrophysical Journal |
| Témata: | |
| On-line přístup: | https://doi.org/10.3847/1538-4357/ae0625 |
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