Extreme event dynamics in the formation of galaxy-sized dark matter structures

DOI10.1016/j.cpc.2008.11.018zbMath1198.85006OpenAlexW2073396856MaRDI QIDQ603358

Haroldo F. Campos Velho, Cesar A. Caretta, Reinaldo R. Rosa, Fernando Manuel Ramos

Publication date: 6 November 2010

Published in: Computer Physics Communications (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.cpc.2008.11.018

zbMATH Keywords

chaotic advectiongalaxies: structure and evolutiongravitational clusteringmethods: statisticalnumerical \(N\)-body simulations

Mathematics Subject Classification ID

Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Uses Software

• ismev

Cites Work

• Computing the probability density function of the stable Paretian distribution
• Fluids of vortices and dark matter
• Multiscaling and nonextensivity of large-scale structures in the Universe
• Critical phenomena in natural sciences. Chaos, fractals, selforganization and disorder: Concepts and tools.
• Evidence of turbulence-like universality in the formation of galaxy-sized dark matter haloes
• The development of chaotic advection
• Analysis of chaotic saddles in high-dimensional dynamical systems: The Kuramoto–Sivashinsky equation
• An introduction to statistical modeling of extreme values

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