A Supersymmetric Suspicion From Accelerating Black Hole Shadows

TL;DR

This paper investigates whether the observed black hole shadows from EHT data align with predictions from supersymmetric accelerating black hole models, suggesting potential gravitational evidence for supersymmetry.

Contribution

It introduces a novel analysis comparing supersymmetric black hole shadow predictions with EHT observations, proposing a new gravitational perspective on supersymmetry.

Findings

Significant alignment between model predictions and EHT measurements

Evidence supporting supersymmetry characteristics in black hole shadows

Potential gravitational evidence for supersymmetry

Abstract

In light of the Event Horizon Telescope (EHT) images of the supermassive black holes $\textrm{Sgr A}^\star$ and $\textrm{M87}^\star$, we explore a potential supersymmetry suspicion within the observational data. Specifically, we investigate the shadow of a supersymmetric accelerating black hole and compare our findings with observed quantities such as the angular diameter $\mathcal{D}$ and the fractional deviation $\bm{\delta}$. Our analysis reveals a significant alignment between the calculated quantities and the EHT collaboration measurements. This alignment suggests that the features of the black hole shadows observed by the EHT exhibit characteristics consistent with the supersymmetry framework. Our results provide compelling evidence for supersymmetry from a gravitational perspective, which remains absent from the particle physics viewpoint till now.