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The study of geodesic motion in curved spacetime provides critical insights into the stability and causal structure of gravitational solutions. In this paper, we analyze the conditions under which test particles can escape the gravitational pull of exotic compact objects. By applying the effective potential method to modified gravity backgrounds, we determine the critical energy thresholds required for escape trajectories. Our results suggest that modifications to the Einstein-Hilbert action significantly alter the capture radius of black holes.
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We all have those dates that stick with us—the moments when everything finally "clicks." For me, that date was . It was the day I stopped just "getting through" my to-do list and started actually mastering my time. The "Escape Now" Mindset
The endless pinging of collaboration apps. By applying the effective potential method to modified
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