MAD accretion flows show higher Higuchi fractal dimensions, lower Hurst indices, and flatter spectral slopes than SANE flows in simulations, with observational data from GRS 1915+105 segregating into matching MAD-like and SANE-like clusters.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Possible fractal nature of accretion flows in MAD and SANE simulations: Implications to GRS 1915+105
MAD accretion flows show higher Higuchi fractal dimensions, lower Hurst indices, and flatter spectral slopes than SANE flows in simulations, with observational data from GRS 1915+105 segregating into matching MAD-like and SANE-like clusters.