Surrounding a Fan-Wang regular black hole with a Kiselev-type anisotropic fluid with omega in (-1,-1/3) modestly enlarges the horizon, photon sphere, and shadow, and EHT data constrain the fluid strength a to about 0.09-0.12 for omega=-2/3.
Geometric properties versus particle motion in the Fan-Wang spacetime
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abstract
In this work, we explore general relativistic effects and geometric properties of the Fan-Wang spacetime, one of the simplest regular solutions that can be obtained in nonlinear electrodynamics. In particular, we investigate the motion of test particles, the capture cross-section of neutral massive and massless particles, such as neutrinos and photons, and the gravitational redshift. Additionally, using a perturbative approach, we derive analytical expressions for the perihelion shift and gravitational deflection of massless particles. By identifying the one-parameter corrections to the Schwarzschild spacetime, induced by the magnetic charge contained in the Fan-Wang metric, we show that this spacetime can be falsified, since it modifies classical general relativity predictions even at the local level. Moreover, we argue that these modifications could be experimentally tested with advanced observational instrumentation.
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Effects of matter with anisotropic pressure on the Fan-Wang regular black hole shadows
Surrounding a Fan-Wang regular black hole with a Kiselev-type anisotropic fluid with omega in (-1,-1/3) modestly enlarges the horizon, photon sphere, and shadow, and EHT data constrain the fluid strength a to about 0.09-0.12 for omega=-2/3.