Signatures of cubic gravity in the strong regime

TL;DR

This paper examines how Einsteinian cubic gravity influences strong gravitational phenomena, revealing modifications to horizon sizes and potential observable effects on light bending and black hole shadows, thus offering avenues for experimental constraints.

Contribution

It provides analytical and numerical solutions for cubic gravity effects on black hole horizons and explores observational signatures like light bending and photon sphere shifts.

Findings

Positive coupling reduces horizon size

Negative coupling increases horizon size

Cubic terms significantly affect black hole shadows

Abstract

We investigate the effects of Einsteinian cubic gravity in the strong gravitational regime. In the first part, we explore analytical solutions for a static, spherically symmetric metric, establishing the existence of maximally symmetric de Sitter solutions, as well as asymptotically de Sitter solutions, with an effective cosmological constant. We also study, analytically and numerically, how the horizon properties are affected by cubic gravity. Our results reveal that a positive coupling constant reduces the horizon size, while a negative one increases it. In the second part, we analyze potential observational signatures of cubic terms, focusing on their effects on the bending of light. Specifically, we investigate the angular difference, related to the deflection angle but valid near the source, along with the behavior of the photon sphere. Our findings show that the strongest effects of the cubic terms occur in the strong gravity regime, and there exists a direct relationship between the value of the coupling constant and the photon sphere position, opening up the possibility to constrain cubic gravity with black hole shadows.