Conventionalism in General Relativity?: Formal Existence Proofs and Reichenbach’s Theorem θ in Context

Weatherall and Manchak (2014) show that, under reasonable assumptions, Reichenbachean universal effects, constrained to a rank-2 tensor field representation in the geodesic equation, always exist in non-relativistic gravity but not so for relativistic spacetimes. Thus, general relativity is less susceptible to underdetermination than its Newtonian predecessor. Dürr and Ben-Menahem (2022) argue that these assumptions are exploitable as loopholes, effectively establishing a (rich) no-go theorem. I disambiguate between two targets of the proof, which have previously been conflated: the existence claim of at least one alternative geometry to a given one and Reichenbach’s (in)famous “theorem theta,” which amounts to a universality claim that any geometry can function as an alternative to any other. I show there is no (rich) no-go theorem to save theorem theta. I illustrate this by explicitly breaking one of the assumptions and generalizing the proof to torsionful spacetimes. Finally, I suggest adopting a programmatic attitude: rather than undermining the proof, one can use it to systematically and rigorously articulate stronger propositions to be proved, thereby systematically exploring the space of alternative spacetime theories.

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Publication Details

Journal
Philosophy of Physics
Published
2026-01-01
DOI
https://doi.org/10.31389/pop.282
Primary Topic
Relativity and Gravitational Theory
Type
article
Field-Weighted Citation Impact
0.00

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article

Conventionalism in General Relativity?: Formal Existence Proofs and Reichenbach’s Theorem θ in Context

Ruward A. Mulder
Philosophy of Physics
Relativity and Gravitational Theory
article

Conventionalism in General Relativity?: Formal Existence Proofs and Reichenbach’s Theorem θ in Context

Ruward A. Mulder
article en

Abstract

Weatherall and Manchak (2014) show that, under reasonable assumptions, Reichenbachean universal effects, constrained to a rank-2 tensor field representation in the geodesic equation, always exist in non-relativistic gravity but not so for relativistic spacetimes. Thus, general relativity is less susceptible to underdetermination than its Newtonian predecessor. Dürr and Ben-Menahem (2022) argue that these assumptions are exploitable as loopholes, effectively establishing a (rich) no-go theorem. I disambiguate between two targets of the proof, which have previously been conflated: the existence claim of at least one alternative geometry to a given one and Reichenbach’s (in)famous “theorem theta,” which amounts to a universality claim that any geometry can function as an alternative to any other. I show there is no (rich) no-go theorem to save theorem theta. I illustrate this by explicitly breaking one of the assumptions and generalizing the proof to torsionful spacetimes. Finally, I suggest adopting a programmatic attitude: rather than undermining the proof, one can use it to systematically and rigorously articulate stronger propositions to be proved, thereby systematically exploring the space of alternative spacetime theories.

Philosophy of PhysicsVol. 4(1)
University of California, Irvine (US), Trinity College (CA)
Trinity College, University of Cambridge
Reduced inequalities
Openalex Percentile: Top 91%
Relativity and Gravitational Theory
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