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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2 Pith papers cite this work. Polarity classification is still indexing.
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A new observable signature from frame-dragging processes near spinning black holes enables testing Einstein gravity and spin measurement via X-ray polarimetry.
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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A New Method for Testing Einstein's Theory of Gravity Close to Rapidly Spinning Black Holes
A new observable signature from frame-dragging processes near spinning black holes enables testing Einstein gravity and spin measurement via X-ray polarimetry.