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Testing the Universality of Self-organized Criticality in Galactic, Extragalactic, and Black Hole Systems
by
Aschwanden, Markus J
, Göǧüş, Ersin
in
Astrophysics
/ Black holes
/ Cosmic rays
/ Criteria
/ Data analysis
/ Datasets
/ Fluxes
/ Gamma rays
/ Observatories
/ Power law
/ Scaling laws
/ Solar physics
/ Spacecraft
/ Statistical distributions
/ Statistical tests
/ Textbooks
/ X-rays
2025
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Testing the Universality of Self-organized Criticality in Galactic, Extragalactic, and Black Hole Systems
by
Aschwanden, Markus J
, Göǧüş, Ersin
in
Astrophysics
/ Black holes
/ Cosmic rays
/ Criteria
/ Data analysis
/ Datasets
/ Fluxes
/ Gamma rays
/ Observatories
/ Power law
/ Scaling laws
/ Solar physics
/ Spacecraft
/ Statistical distributions
/ Statistical tests
/ Textbooks
/ X-rays
2025
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While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
Testing the Universality of Self-organized Criticality in Galactic, Extragalactic, and Black Hole Systems
by
Aschwanden, Markus J
, Göǧüş, Ersin
in
Astrophysics
/ Black holes
/ Cosmic rays
/ Criteria
/ Data analysis
/ Datasets
/ Fluxes
/ Gamma rays
/ Observatories
/ Power law
/ Scaling laws
/ Solar physics
/ Spacecraft
/ Statistical distributions
/ Statistical tests
/ Textbooks
/ X-rays
2025
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Testing the Universality of Self-organized Criticality in Galactic, Extragalactic, and Black Hole Systems
Journal Article
Testing the Universality of Self-organized Criticality in Galactic, Extragalactic, and Black Hole Systems
2025
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Overview
In this study, we test whether the power law slopes (α F ) for fluxes (F), and (α E ) for energies (E) are universal in their size distributions, N(F)∝F−αF and N(E)∝E−αE , in astrophysical observations of galactic, extragalactic, and black hole systems. This is a test of fundamental importance for self-organized criticality (SOC) systems. The test decides whether (i) power laws are a natural consequence of the scale-freeness and inherent universality of SOC systems, or (ii) if they depend on more complex physical scaling laws. The former criterion allows quantitative predictions of the power-law-like size distributions, while the latter criterion requires individual physical modeling for each SOC variable and data set. Our statistical test, carried out with 61 published data sets, is consistent with the former option, which implies that observed power laws can simply be derived from the scale-freeness and do not require specific physical models to understand their statistical distributions. The observations show a mean and standard deviation of α F = 1.78 ± 0.29 for SOC fluxes and α E = 1.66 ± 0.22 for SOC fluences, and thus are consistent with the prediction of the fractal-diffusive SOC model, with α F = 1.80 and α E = 1.67.
Publisher
IOP Publishing
Subject
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