Self-Organized Criticality in Astrophysics

DOI10.1007/978-3-642-15001-2zbMath1211.85001OpenAlexW50218050MaRDI QIDQ3588777

Markus J. Aschwanden

Publication date: 10 September 2010

Full work available at URL: https://doi.org/10.1007/978-3-642-15001-2

zbMATH Keywords

nonlinear dynamicsastrophysicsself-organized criticalityselforganizationpowerlaw distribution

Mathematics Subject Classification ID

Applications of statistics to economics (62P20) Applications of statistics to biology and medical sciences; meta analysis (62P10) Applications of statistics to environmental and related topics (62P12) Applications of statistics to social sciences (62P25) Conformal densities and Hausdorff dimension for holomorphic dynamical systems (37F35) Applications of statistics to physics (62P35) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Astrophysical cosmology (85A40) Statistical astronomy (85A35) Research exposition (monographs, survey articles) pertaining to astronomy and astrophysics (85-02)

Related Items (7)

A Curie-Weiss model of self-organized criticality ⋮ Black swans, extreme risks, and the e-pile model of self-organized criticality ⋮ \textit{Independent approximates} enable closed-form estimation of heavy-tailed distributions ⋮ Path-space moderate deviations for a Curie-Weiss model of self-organized criticality ⋮ Topological field theory of dynamical systems ⋮ Predictability and scaling in a BTW sandpile on a self-similar lattice ⋮ A mixed SOC-turbulence model for nonlocal transport and Lévy-fractional Fokker-Planck equation

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