The imaging of Sagittarius A* (Sgr A*) and the supermassive black hole at the center of Messier 87 (M87*) by the Event Horizon Telescope constrains the location and nature of emission from these objects. Coupled with flux limits from the near-infrared through the ultraviolet, the attendant size constraints provide strong evidence for the absence of an accretion-powered photosphere, and therefore for the existence of an event horizon about an astrophysical black hole. Here, we demonstrate that a broad class of naked singularities are also generically excluded, regardless of the nature and unknown physical impact of singularity itself, subject to a single weak assumption about locality. While we restrict our attention to static, spherically symmetric spacetimes, we are nevertheless able to exclude a large number of commonly invoked naked singularity spacetimes in this way.
No takes yet. Share an insight, caveat, or question.
Broderick et al. (2024) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: