Lower bound on the time-to-mass ratio of circular trajectories in spherically symmetric curved spacetimes

It is proved that the Einstein-matter field equations supplemented by the weak (positive) energy condition yield the dimensionless lower bound T∞/M(r)≥63π on the orbital-time-to-mass ratio of closed circular motions in curved spacetimes, where {r,T∞,M(r)} are respectively the radius of the circular...

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Bibliographic Details
Main Author: Shahar Hod
Format: Article
Language:English
Published: Elsevier 2025-05-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269325001911
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