Photon ring structure of rotating regular black holes and no-horizon spacetimes
arXiv:2004.07501 · doi:10.1088/1361-6382/abdd48
Abstract
The Kerr black holes possess a photon region with prograde and retrograde orbits radii, respectively, and , and thereby always cast a closed photon ring or a shadow silhouette for . For , it is a no-horizon spacetime (naked singularity) wherein prograde orbits spiral into the central singularity, and retrograde orbits produce an arc-like shadow with a dark spot at the center. We compare Kerr black holes' photon ring structure with those produced by three rotating regular spacetimes, viz. Bardeen, Hayward, and nonsingular. These are non-Kerr black hole metrics with an additional deviation parameter of related to the nonlinear electrodynamics charge. It turns out that for a given , there exists a critical value of , such that has no zeros for , one double zero at for , respectively, corresponding to a no-horizon regular spacetime and extremal black hole with degenerate horizon. We demonstrate that, unlike the Kerr naked singularity, no-horizon regular spacetimes can possess closed photon ring when , e.g., for , Bardeen (), Hayward () and nonsingular () no-horizon spacetimes have closed photon ring. These results confirm that the mere existence of a closed photon ring does not prove that the compact object is necessarily a black hole. The ring circularity deviation observable for the three no-horizon rotating spacetimes satisfy as per the M87* black hole shadow observations. We have also appended the case of Kerr-Newman no-horizon spacetimes (naked singularities) with similar features.
arXiv comment20 pages, 18 figures and 6 tables. Title modified, references and discussions added. Matches the published version in CQG
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