Year: 2019
Type: article
Abstract: The Event Horizon Telescope has recently provided the first image of the dark shadow around the supermassive black hole M87*. The observation of a highly circular shadow provides strong limits on deviations of M87*'s quadrupole moment from the Kerr value. We show that the absence of such a deviation can be used to constrain the physics of extra dimensions of spacetime. Focusing on the Randall-Sundrum ${\mathrm{AdS}}_{5}$ brane-world scenario, we show that the observation of M87*'s dark shadow sets the limit $\ensuremath{\ell}\ensuremath{\lesssim}170\text{ }\text{ }\mathrm{AU}$, where $\ensuremath{\ell}$ is the ${\mathrm{AdS}}_{5}$ curvature radius. This limit is among the first quantitative constraints on exotic physics obtained from the extraordinary first ever image of the dark shadow of a black hole.
Authors: Sunny Vagnozzi, Luca Visinelli
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Funder: Vetenskapsrådet
Award: G1150067265
OpenAlex ID: W2960227302
