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Autori principali: Broderick, Avery E., Salehi, Kiana
Natura: Preprint
Pubblicazione: 2024
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Accesso online:https://arxiv.org/abs/2406.05181
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author Broderick, Avery E.
Salehi, Kiana
author_facet Broderick, Avery E.
Salehi, Kiana
contents 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 exhibit inner turning points for time-like geodesics, and therefore may generically be excluded, regardless of the nature and unknown physical impact of singularity itself, subject to the single weak assumption that the its nongravitational impact is localized to its immediate vicinity. While we restrict our attention to static, spherically symmetric spacetimes, we are nevertheless able to exclude or constrain a large number of commonly invoked naked singularity spacetimes in this way.
format Preprint
id arxiv_https___arxiv_org_abs_2406_05181
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Cosmic Censorship in Sgr A* and M87*: Observationally Excluding Naked Singularities
Broderick, Avery E.
Salehi, Kiana
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
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 exhibit inner turning points for time-like geodesics, and therefore may generically be excluded, regardless of the nature and unknown physical impact of singularity itself, subject to the single weak assumption that the its nongravitational impact is localized to its immediate vicinity. While we restrict our attention to static, spherically symmetric spacetimes, we are nevertheless able to exclude or constrain a large number of commonly invoked naked singularity spacetimes in this way.
title Cosmic Censorship in Sgr A* and M87*: Observationally Excluding Naked Singularities
topic High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2406.05181