来自加速黑洞阴影的超对称迹象
A Supersymmetric Suspicion From Accelerating Black Hole Shadows
AI总结：
本文通过对比超对称加速黑洞阴影与EHT对Sgr A*和M87*的观测数据，发现角直径和分数偏差显著一致，从而从引力角度为超对称提供了迄今粒子物理未能给出的证据。
摘要：
鉴于事件视界望远镜（EHT）对超大质量黑洞 $\textrm{Sgr A}^\star$ 和 $\textrm{M87}^\star$ 的成像结果，我们在观测数据中探索了一种可能的超对称迹象。具体而言，我们研究了超对称加速黑洞的阴影，并将计算结果与观测量（如角直径 $\mathcal{D}$ 和分数偏差 $\bmδ$）进行比较。分析表明，计算量与 EHT 合作组的测量值之间存在显著一致性。这种一致性表明，EHT 观测到的黑洞阴影特征与超对称框架所预期的特性相符。我们的结果从引力视角为超对称提供了有力证据，而迄今为止，粒子物理学视角仍未提供这样的证据。
英文摘要：
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 $\bmδ$. 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.
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