A Chimera accretion flow can sustain MAD-level horizon flux and electromagnetic jet power without the standard MAD's eruptive variability, mass-flow geometry, or inner-disk morphology, so MAD-like behavior is multi-diagnostic and history-dependent.
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2 Pith papers cite this work, alongside 37 external citations. Polarity classification is still indexing.
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2026 2representative citing papers
Viscous transonic accretion flow simulations around spinning black holes show that QPO frequency ranges and power-law photon indices correlate with black hole spin.
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The SANE, the MAD, and the Chimera
A Chimera accretion flow can sustain MAD-level horizon flux and electromagnetic jet power without the standard MAD's eruptive variability, mass-flow geometry, or inner-disk morphology, so MAD-like behavior is multi-diagnostic and history-dependent.
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QPOs from the Viscous Transonic Accretion Flow Around a Spinning Black Hole
Viscous transonic accretion flow simulations around spinning black holes show that QPO frequency ranges and power-law photon indices correlate with black hole spin.