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Real astrophysical black holes are expected to rotate.
supportedReal astrophysical black holes are expected to rotate. Black-hole spin influences accretion efficiency, jet power, gravitational-wave merger signals, tidal disruption behavior, and the growth history of supermassive black holes.
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Evidence first
Real astrophysical black holes are expected to rotate.
supportedRotating mass drags local inertial frames, an effect called frame dragging.
supportedRelativistic X-ray reflection spectra, continuum fitting, quasi-periodic timing behavior, and horizon-scale observations constrain spin-dependent accretion geometry.