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Black-hole Shadows and Null Geodesics in Hamaus–Sutter–Wandelt Void Spacetimes with a Quintessential Field: Observational Signatures from EHT Data of M87 and Sgr A

  • Authors: A. Errehymy, S. Hansraj, C. Hansraj

A. Errehymy et al 2025 The Astrophysical Journal 995 .

  • Provider: AAS Journals

Caption: Figure 6.

The energy-emission rate is analyzed for different parameter choices 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 highlights the impact of varying γ with δc = 0.1 and ρs = 0.1, while the right panel illustrates the influence of ρs on f(r) with δc = 0.1 and γ = 0.1.

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