Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes

TL;DR

This paper studies the unique shadow features and energy behavior of Lorentzian-Euclidean black holes, revealing potential observational signatures and differences from traditional black hole models.

Contribution

It introduces analysis of shadows and energy accumulation in Lorentzian-Euclidean black holes, highlighting deviations from Schwarzschild and novel backreaction properties.

Findings

Inner shadow region shows excess intensity indicating new light propagation effects.

Horizon surface accumulates photons and energy with a distinct backreaction response.

Potential observational signatures for horizon-scale modifications of black holes.

Abstract

The Lorentzian-Euclidean black hole has been recently introduced as a geodesically complete spacetime featuring a signature shift at the event horizon where causal geodesics are precluded from reaching the central $r=0$ singularity. In this paper, we investigate the shadows produced by this geometry to identify deviations from the standard Schwarzschild solution. Our analysis reveals an excess intensity in the inner shadow region that points to a potential observational signature of the novel behavior of light rays propagating near the event horizon. This excess could be a probe for horizon-scale modifications of black hole geometries. Furthermore, although the horizon surface of the Lorentzian-Euclidean black hole continuously accumulates photons and energy, we show that its backreaction response differs from that of stable light rings found in various exotic compact objects.