Published on:
2 November 2023
Primary Category:
General Relativity and Quantum Cosmology
Paper Authors:
Kiana Salehi,
Avery Broderick,
Boris Georgiev
Presents a formulation of spinning black hole spacetimes separating event horizon and ergosphere functions
Derives expressions for shadow size and photon rings for a polar observer
Finds measurements independent of ergosphere properties
Generalizes prior characterizations of spherical spacetimes
Provides framework to constrain spinning spacetimes from observations
Probing black hole spacetimes with shadows and photon rings
This paper presents a formulation of spinning black hole spacetimes that separates functions controlling the event horizon and ergosphere. It explores how measurements of the black hole shadow size and photon rings for a polar observer probe these functions. The results generalize prior characterizations for spherical spacetimes. Notably, these measurements do not depend on ergosphere properties. This provides a framework to constrain spinning spacetimes from observations without assumptions about small deviations from Kerr.
Black hole shadow cast by dark matter
Testing for event horizons with rotating surfaces
Key insights on black hole photon spheres and shadows
Black hole shadow and accretion disk images affected by dark fluid equation of state
Analytical description of higher-order photon rings
Quantum effects on a spherical black hole with global monopoles
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