Splashback Radius in a Spherical Collapse Model
It was shown several years ago that dark matter halo outskirts are characterized by very steep density profiles in a very small radial range. This feature has been interpreted as a pile-up of different particle orbits at a similar location, namely, splashback material at half an orbit after collapse...
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| Principais autores: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
MDPI AG
2022-09-01
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| coleção: | Universe |
| Assuntos: | |
| Acesso em linha: | https://www.mdpi.com/2218-1997/8/9/462 |
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