Compară metode
Examinează metodele selectate una lângă alta; rândurile care diferă sunt evidențiate.
| Profilul Haloului NFW× | Ajustarea PDF× | |
|---|---|---|
| Domeniu | Fizica particulelor | Fizica particulelor |
| Familie | Process / pipeline | Process / pipeline |
| Anul apariției≠ | 1997 | 1969 |
| Autorul original≠ | Julio Navarro, Carlos Frenk, Simon White | James Bjorken and collaborators |
| Tip≠ | Halo density model | QCD framework |
| Sursa seminală≠ | 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 ↗ | Bjorken, J. D. (1969). Asymptotic sum rules at infinite momentum. Physical Review, 179(5), 1547. DOI ↗ |
| Denumiri alternative | NFW profile, dark matter density profile, halo model | PDF, structure function, parton model |
| Înrudite | 3 | 3 |
| Rezumat≠ | 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. | Parton Distribution Function (PDF) fitting is the process of determining the probability distributions of quarks and gluons inside hadrons using high-energy collision data. PDFs are fundamental inputs to all hadron collider phenomenology, essential for predicting cross-sections, designing triggers, and interpreting new physics searches at the Large Hadron Collider. |
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