Observational Signatures: Shadow cast by the effective metric of photons for black holes with rational non-linear electrodynamics

TL;DR

This paper investigates how non-linear electrodynamics affects black hole spacetime and photon trajectories, revealing expanded horizons and emission profiles, with implications for observational signatures and parameter constraints.

Contribution

It derives the effective metric for photons in non-linear electrodynamics black holes and analyzes their observational signatures, extending understanding of modified black hole spacetimes.

Findings

Increased magnetic charge enlarges the horizon and emission region.

Direct emission dominates over lensing rings.

Non-linear electrodynamics black holes show higher intensity and wider emission regions compared to Schwarzschild black holes.

Abstract

This study explores spherically symmetric non-linear electrodynamics black holes and their effects on light propagation. We derive the governing metric, revealing radial coordinate dynamics within the event horizon. We analyze photon trajectories, finding that increasing magnetic charge expands the horizon and emission range. Furthermore, with the help of the Event Horizon Telescope results, we constrain parameters and emission profiles. Direct emission dominates, while lensing rings play a lesser role. Comparing with Schwarzschild black holes, we observe higher intensity but a wider emission region in non-linear electrodynamics black holes. This work enhances our understanding of modified spacetimes and their impact on black hole properties.