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Observing Black Holes Spin

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arxiv 1903.11704 v1 pith:BHCDJBFS submitted 2019-03-27 astro-ph.HE astro-ph.GAgr-qc

classification astro-ph.HEastro-ph.GAgr-qc
keywords blackspinholecurrentgravitationalholesmeasurementsradio
verification ladder T0 review T1 audit T2 compute T3 formal
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The spin of a black hole retains the memory of how the black hole grew, and can be a potent source of energy for powering relativistic jets. To understand the diagnostic power and astrophysical significance of black hole spin, however, we must first devise observational methods for measuring spin. Here, I describe the current state of black hole spin measurements, highlighting the progress made by X-ray astronomers, as well as the current excitement of gravitational wave and radio astronomy based techniques. Today's spin measurements are already constraining models for the growth of supermassive black holes and giving new insights into the dynamics of stellar core-collapse, as well as hinting at the physics of relativistic jet production. Future X-ray, radio, and gravitational wave observatories will transform black hole spin into a precision tool for astrophysics and test fundamental theories of gravity.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Geometric properties of slowly rotating black holes embedded in matter environments

    gr-qc 2026-02 conditional novelty 6.0 of 10

    The rotation of a surrounding dark-matter halo shifts the light ring, ISCO, epicyclic frequencies, and resonance locations of a slowly spinning black hole in a way that depends on the halo's angular velocity.

  2. Black hole supercolliders

    gr-qc 2025-06 conditional novelty 5.0 of 10

    Retrograde plunging accretion flows around near-extremal Kerr black holes can collide with free-falling particles at TeV-scale center-of-mass energies.

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