Image Details
Caption: Figure 3.
The behavior of the black-hole shadow radius (solid red line) in HSW void spacetimes with a quintessential field. In the left panel, δc is varied while keeping γ = 0.1 and ρs = 0.1 fixed. The middle panel illustrates the effect of changing γ with δc = 0.1 and ρs = 0.1, and the right panel shows how variations in ρs influence f(r) with δc = 0.1 and γ = 0.1. The orange and gray regions correspond to the EHT horizon-scale images of Sgr A∗ and M87∗ at 1σ, while the light blue and light green regions represent consistency at 2σ, respectively.
© 2025. The Author(s). Published by the American Astronomical Society.