Observational analysis finds varying scaling laws in astrophysical systems, indicating complex dynamics.
Scaling laws in astrophysical systems that involve energy, geometry, and spatiotemporal evolution provide the theoretical framework for physical models of energy dissipation processes. A leading model is the standard fractal-diffusive self-organized criticality (FD-SOC) model, which is built on four fundamental assumptions: (i) the dimensionality d = 3, (ii) the fractal dimension D V = d − 1/2 = 2.5, (iii) classical diffusion L ∝ T (1/2) , and (iv) the proportionality of the dissipated energy to the fractal volume, E ∝ V . Based on these assumptions, the FD-SOC model predicts a scaling law of T ∝ E k ∝ E (4/5) = E 0.8 . On the observational side, we find only one case (out of the nine analyzed cases) that is consistent with the FD-SOC model, namely, the scaling law of T ∝ E 0.86±0.03 by A. Araujo & A. Valio. The other eight cases have scaling law coefficients clustered around values of k ≈ 0.3−0.4, which possibly can be explained by nonstandard SOC models, i.e., k = 2/( βD V ), in terms of linear expansion β = 2 and/or Euclidean dimension D V = 3. The relatively low values of time duration ranges may also indicate possible truncation biases.
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Aschwanden et al. (2026) studied this question.
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