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Counterexamples to the maximum force conjecture

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arxiv 2102.01831 v2 pith:WWKBBROI submitted 2021-02-03 gr-qc

classification gr-qc
keywords maximumforceconjecturecounter-examplesphysicaltensionwilldimensionless
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abstract

Dimensional analysis shows that the speed of light and Newton's constant of gravitation can be combined to define a quantity $F_* = {c^4\over G_N}$ with the dimensions of force (equivalently, tension). Then in any physical situation we must have $F_{physical} = f \; F_*$, where the quantity $f$ is some dimensionless function of dimensionless parameters. In many physical situations explicit calculation yields $f= O(1)$, and quite often $f \leq {1\over4}$. This has lead multiple authors to suggest a (weak or strong) maximum force/maximum tension conjecture. Working within the framework of standard general relativity, we will instead focus on counter-examples to this conjecture, paying particular attention to the extent to which the counter-examples are physically reasonable. The various counter-examples we shall explore strongly suggest that one should not put too much credence into any universal maximum force/maximum tension conjecture. Specifically, fluid spheres on the verge of gravitational collapse will generically violate the weak (and strong) maximum force conjectures. If one wishes to retain any general notion of "maximum force" then one will have to very carefully specify precisely which forces are to be allowed within the domain of discourse.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Upper bounds on the force function in spatially regular self-gravitating matter configurations

    gr-qc 2026-07 accept novelty 6.0 of 10

    Einstein-matter equations bound the force function F=4πr²p by 2 (generic DEC), 1 (generic T≤0), 1 (isotropic DEC), and 1/2 (isotropic T≤0) in regular spherical spacetimes.

  2. Maximum force conjecture in curved spacetimes of stable self-gravitating matter configurations

    gr-qc 2025-01 conditional novelty 5.0 of 10

    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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