For stable, horizonless, self-gravitating configurations in general relativity, the force function 4πr²p(r) is bounded by c⁴/G, derived from the condition that stable configurations contain no light rings.
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Maximum force conjecture in curved spacetimes of stable self-gravitating matter configurations
For stable, horizonless, self-gravitating configurations in general relativity, the force function 4πr²p(r) is bounded by c⁴/G, derived from the condition that stable configurations contain no light rings.