方法证据记录
NFW Halo Profile
The Navarro-Frenk-White (NFW) profile is a widely-adopted density profile for dark matter halos emerging from cosmological simulations. It provides a simple parametric description of how dark matter density varies with distance from the halo center, essential for modeling galaxy cluster mass distributions, weak lensing, and dark matter annihilation signals.
源记录
引文逐字复制自方法源记录。这些引文不代表任何层级的验证。
Navarro-Frenk-White Dark Matter Profile
分类方法记录 · process-pipeline / particle-physics
- Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997). A universal density profile from hierarchical clustering. The Astrophysical Journal, 490(2), 493. · DOI 10.1086/304888
- Dutton, A. A., & Maccio, A. V. (2014). The abundance of dark matter haloes and the assembly of galaxies. Monthly Notices of the Royal Astronomical Society, 441(4), 3359–3374. · URL
- Diemer, B., & Kravtsov, A. V. (2015). A universal model for halo concentrations. The Astrophysical Journal, 799(2), 108. · DOI 10.1088/0004-637x/799/1/108
精选声明
声明已持久化到证据分类账中，每个声明都有自己的评估。
尚无精选声明
当分类账中没有声明时，此视图不会自行创建声明评估。
相关方法
从方法图中生成，显示为机器建议的关系 — 不推断任何证据声明。