Revisiting The Gravitational Mirroring In Presence of Compact Objects

TL;DR

This paper introduces the concept of astrophysical mirroring caused by gravitational lensing near dense objects, demonstrating how extreme spacetime curvature can create mirror-like images of sources.

Contribution

It presents a new theoretical framework and numerical analysis for gravitational mirroring effects around compact objects within the Schwarzschild spacetime.

Findings

Dense astrophysical objects can produce extreme gravitational lensing effects.

The gravitational field near such objects can create mirror-like images of distant sources.

The paper discusses potential observational signatures of this phenomenon.

Abstract

We propose a novel concept of astrophysical mirroring in the schwarzschild framework, which emerges as a direct consequence of gravitational lensing effects occurring in the immediate vicinity of extremely dense massive objects within spacetime. Through rigorous theoretical calculations and numerical ray-tracing analysis, we demonstrate that sufficiently compact astrophysical objects possess the capability to induce such extreme curvature in spacetime that the resulting gravitational field can bend light rays to extraordinary degrees, creating what we term a "reflection image" or mirror-like appearance of the source in distant regions of space. We discuss the theoretical framework as well as the observational consequences of this phenomenon.