Turbulent electron-ion coronae around accreting black holes self-regulate into a two-temperature state that generates nonthermal ions and X-ray spectra consistent with observations including an MeV tail.
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3 Pith papers cite this work, alongside 137 external citations. Polarity classification is still indexing.
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Imbalanced turbulence throttles its cascade via the helicity barrier, yielding flat spectra (η<2) that invert minor-ion heating to Q_i ∝ Q_p A_i (A_i/Z_i)^{η-2}, with simulations across β_p0 confirming the (A_i/Z_i)^a trend and strong perpendicular heating at low β.
Radiative cooling in MADs above a transition accretion rate creates thinner denser filaments with increased efficiency, rendering conventional scale height measures misleading and motivating a new definition based on the polar position of the density maximum.
citing papers explorer
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High-energy Emission from Turbulent Electron-ion Coronae of Accreting Black Holes
Turbulent electron-ion coronae around accreting black holes self-regulate into a two-temperature state that generates nonthermal ions and X-ray spectra consistent with observations including an MeV tail.
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Minor Ions as a Diagnostic of Solar Wind Heating: Inverted Mass-to-Charge Scaling in Imbalanced Turbulence
Imbalanced turbulence throttles its cascade via the helicity barrier, yielding flat spectra (η<2) that invert minor-ion heating to Q_i ∝ Q_p A_i (A_i/Z_i)^{η-2}, with simulations across β_p0 confirming the (A_i/Z_i)^a trend and strong perpendicular heating at low β.
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Characterizing the Scale Height and Filamentary Structure of Radiatively Cooled MADs
Radiative cooling in MADs above a transition accretion rate creates thinner denser filaments with increased efficiency, rendering conventional scale height measures misleading and motivating a new definition based on the polar position of the density maximum.