Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
The concentration of dark matter haloes is closely linked to their mass accretion history. We utilize the halo mass accretion histories from large cosmological <i>N</i>-body simulations as inputs for our neural networks, which we train to predict the concentration of individual haloes at a given red...
I tiakina i:
| Ngā kaituhi matua: | , , , |
|---|---|
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
MDPI AG
2025-01-01
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| Rangatū: | Universe |
| Ngā marau: | |
| Urunga tuihono: | https://www.mdpi.com/2218-1997/11/2/37 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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