Origin and Full Characterization of the Secondary (Assembly) Halo Bias
The clustering of dark matter halos depends not only on their mass, the so-called primary bias, but also on their internal properties, the so-called secondary bias. While the former effect is well understood within the Press–Schechter and excursion set models of structure formation, the latter is no...
में बचाया:
| मुख्य लेखकों: | , , |
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| स्वरूप: | Artigo |
| भाषा: | Inglês |
| प्रकाशित: |
IOP Publishing
2024-01-01
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| श्रृंखला: | The Astrophysical Journal |
| विषय: | |
| ऑनलाइन पहुंच: | https://doi.org/10.3847/1538-4357/ad84f1 |
| टैग: |
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