Generating Rotating Spacetime in Ricci-Based Gravity: Naked Singularity as a Black Hole Mimicker

TL;DR

This paper constructs rotating solutions in Ricci-based gravity theories, showing that naked singularities can mimic black hole shadows, with high-energy modifications influencing singularity structure and observational features.

Contribution

It extends known rotating solutions to Eddington-inspired Born-Infeld gravity, revealing how high-energy effects modify singularities and produce black hole-like shadows.

Findings

High-energy modifications suppress but do not eliminate naked singularities.

Naked singularities can cast shadows identical to black holes.

Scalar charge affects shadow shape, resembling Kerr black holes.

Abstract

Motivated by the lack of rotating solutions sourced by matter in General Relativity as well as in modified gravity theories, we extend a recently discovered exact rotating solution of the minimal Einstein-scalar theory to its counterpart in Eddington-inspired Born-Infeld gravity coupled to a Born-Infeld scalar field. This is accomplished with the implementation of a well-developed mapping between solutions of Ricci-Based Palatini theories of gravity and General Relativity. The new solution is parametrized by the scalar charge and the Born-Infeld coupling constant apart from the mass and spin of the compact object. Compared to the spacetime prior to the mapping, we find that the high-energy modifications at the Born-Infeld scale are able to suppress but not remove the curvature divergence of the original naked null singularity. Depending on the sign of the Born-Infeld coupling constant, these modifications may even give rise to an additional timelike singularity exterior to the null one. In spite of that, both of the naked singularities before and after the mapping are capable of casting shadows, and as a consequence of the mapping relation, their shadows turn out to be identical as seen by a distant observer on the equatorial plane. Even though the scalar field induces a certain oblateness to the appearance of the shadow with its left and right endpoints held fixed, the closedness condition for the shadow contour sets a small upper bound on the absolute value of the scalar charge, which leads to observational features of the shadow closely resembling those of a Kerr black hole.