Pairing square-root-area-weighted vacuum perturbations with full-area-weighted resonant fields produces a coupling matrix whose singular values and reconstructed real-space patterns are invariant to coordinate choice.
and Scepi, Nicolas and Dexter, Jason, year = 2022, month = apr
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Simulations of accreting black holes in standard and complex spacetimes indicate that magnetic geometry, quantum corrections, and binary dynamics influence flares, precession, photon rings, and multi-wavelength variability, with potential EHT constraints.
Radio precedes X-ray Compton luminosity by ~3 days in the rising hard state but lags by ~8 days in the decaying hard state of GX 339-4, with inner magnetic field strength estimated from accretion rate and truncation radius accounting for both.
citing papers explorer
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Coordinate-invariant flux-surface Fourier analysis in tokamaks
Pairing square-root-area-weighted vacuum perturbations with full-area-weighted resonant fields produces a coupling matrix whose singular values and reconstructed real-space patterns are invariant to coordinate choice.
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GRMHD and GRRT Simulations of Black Hole Accretion: Flares, Precession, and Complex Spacetimes
Simulations of accreting black holes in standard and complex spacetimes indicate that magnetic geometry, quantum corrections, and binary dynamics influence flares, precession, photon rings, and multi-wavelength variability, with potential EHT constraints.
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Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion
Radio precedes X-ray Compton luminosity by ~3 days in the rising hard state but lags by ~8 days in the decaying hard state of GX 339-4, with inner magnetic field strength estimated from accretion rate and truncation radius accounting for both.