A Closed-Form Surrogate for the Equivalent Diameter of the Kerr Shadow
Arseny Pantsialei

TL;DR
This paper introduces a precise, closed-form approximation for the Kerr black-hole shadow's equivalent diameter, enabling quick size evaluations across a range of spins and inclinations without complex numerical calculations.
Contribution
The authors develop a novel analytical surrogate for the Kerr shadow diameter that combines exact face-on limits with a polynomial correction for inclination dependence.
Findings
Achieves sub-percent accuracy across the parameter space.
Median error of 0.0105% on training data, 0.023% on validation.
Provides fast, analytical size estimates for Kerr shadows.
Abstract
We present a closed-form surrogate for the equivalent diameter of the Kerr black-hole shadow, defined as the diameter of the circle with the same area as the shadow's critical curve. The construction enforces the exact face-on (polar) limit by explicitly separating an analytically computed polar contribution based on the spherical photon-orbit branch where the horizontal impact parameter vanishes. The remaining inclination dependence is captured by a compact 15-parameter polynomial placed inside an exponential correction. The coefficients are determined by ordinary least squares on a deterministic reference grid generated from the Kerr critical-curve area. Over the practical domain of dimensionless spin from 0 to 0.998 and inclination from just above 0 degrees up to 90 degrees (with the exactly polar point treated analytically), the surrogate achieves sub-percent accuracy. On the…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Astrophysics and Cosmic Phenomena
