Image Details
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.
© 2025. The Author(s). Published by the American Astronomical Society.