Fast-spinning black holes can bend their disk's own thermal X-rays back onto the disk, and scattering can create a corona-free power-law tail with a distinctive polarization swing.
Astrophysical Black Holes
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
CONDITIONAL 2representative citing papers
Quantizing dust geodesics in a generalized Kerr metric gives a rotating black-hole core that is smaller and equator-elongated relative to the spherical case, with a linear mass/angular-momentum interior profile that avoids Cauchy horizons.
citing papers explorer
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A New Approach for Testing Einstein's Theory of Gravity Close to Rapidly Spinning Black Holes
Fast-spinning black holes can bend their disk's own thermal X-rays back onto the disk, and scattering can create a corona-free power-law tail with a distinctive polarization swing.
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Quantum dust cores of rotating black holes
Quantizing dust geodesics in a generalized Kerr metric gives a rotating black-hole core that is smaller and equator-elongated relative to the spherical case, with a linear mass/angular-momentum interior profile that avoids Cauchy horizons.