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...
में बचाया:
| मुख्य लेखकों: | , |
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| स्वरूप: | Artigo |
| भाषा: | Inglês |
| प्रकाशित: |
MDPI AG
2022-09-01
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| श्रृंखला: | Universe |
| विषय: | |
| ऑनलाइन पहुंच: | https://www.mdpi.com/2218-1997/8/9/462 |
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