The advent of high-resolution black hole imaging—most notably by the Event Horizon Telescope(EHT)—has propelled black hole physics into a new observational regime[1].However,most theoretical interpretations remain a...The advent of high-resolution black hole imaging—most notably by the Event Horizon Telescope(EHT)—has propelled black hole physics into a new observational regime[1].However,most theoretical interpretations remain anchored in stationary,time-averaged general relativistic magnetohydrodynamic(GRMHD)simulations within the Kerr paradigm,often neglecting dynamic accretion structures and potential deviations from general relativity[2].展开更多
文摘The advent of high-resolution black hole imaging—most notably by the Event Horizon Telescope(EHT)—has propelled black hole physics into a new observational regime[1].However,most theoretical interpretations remain anchored in stationary,time-averaged general relativistic magnetohydrodynamic(GRMHD)simulations within the Kerr paradigm,often neglecting dynamic accretion structures and potential deviations from general relativity[2].
