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Profil NFW (Navarro-Frenk-White)×Metoda maticového prvku×
OborČásticová fyzikaČásticová fyzika
RodinaProcess / pipelineProcess / pipeline
Rok vzniku19971988
TvůrceJulio Navarro, Carlos Frenk, Simon WhiteK. Kondo
TypHalo density modelProbability calculation framework
Původní zdrojNavarro, J. F., Frenk, C. S., & White, S. D. M. (1997). A universal density profile from hierarchical clustering. The Astrophysical Journal, 490(2), 493. DOI ↗Kondo, K. (1988). Dynamical likelihood method for reconstruction of events produced by the top-quark pair in the lepton + jets channel at hadron colliders. Journal of the Physical Society of Japan, 57(12), 4126–4140. link ↗
Další názvyNFW profile, dark matter density profile, halo modelMEM, matrix element calculation, amplitude evaluation
Příbuzné33
ShrnutíThe 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.The Matrix Element Method (MEM) is a powerful analysis technique that leverages quantum field theory amplitudes to extract maximum physics information from individual events. By comparing observed detector signatures to predictions from matrix elements, MEM provides unbiased, model-independent measurements with excellent theoretical precision and sensitivity to new physics.
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ScholarGatePorovnat metody: NFW Halo Profile · Matrix Element Method. Získáno 2026-06-18 z https://scholargate.app/cs/compare