Weatherall 2016: Newtonian Gravitation vs. Newton-Cartan Theory (Trautman Geometrization and Categorical Equivalence)Research Paper
Motivation
Newtonian gravitation can be written in two ways. In Newtonian gravitation (NG), spacetime has a flat derivative operator and a scalar potential obeying Poisson's equation, and bodies are pushed off the straight lines of by the force . In geometrized Newtonian gravitation (GNG), also called Newton–Cartan theory, the potential is absorbed into a curved derivative operator whose geodesics are the trajectories of freely falling bodies. This is the same geometrization that general relativity performs. Trautman (1965) proved that the two pictures pass into each other.
Weatherall (2016) asks whether NG and GNG are the same theory. He represents each theory by a category of models and calls two theories equivalent when there is an equivalence of categories that preserves empirical content. The answer depends on the arrows chosen for NG:
- NG₁ treats the potential as physical. Its arrows are diffeomorphisms preserving , , and , and NG₁ is not equivalent to GNG.
- NG₂ treats the potential as a gauge quantity, as Newton's Corollary VI suggests. Its arrows are pairs with , and NG₂ is equivalent to GNG (Prop. 6.1).
This is the gravitational twin of the electromagnetic question "potentials vs. field strengths" treated in the companion missions on Weatherall's Understanding Gauge. The other side of the Newton–Cartan story, the classical limit of general relativity, is described under Significance.
Setting
Following Weatherall (p. 3), spacetime is , here in one global chart E = Fin 4 → ℝ with index 0 for time. The classical metrics are (tt) and (hh). Their slices are complete copies of , as Weatherall requires.
A derivative operator is a smooth field of Christoffel symbols Γ x a b c , symmetric in , acting by
It is compatible when and . Curvature uses Malament's sign convention:
Other notation:
- Geometrization: , that is (
geomΓ). - Gauge transformation: (
gaugeΓ). - Curves: a massive body has unit timelike tangent, . Curves are smooth on an open interval.
The objects of the categories are:
- NG (
IsNG Γ φ): compatible, flat and a smooth potential . The mass density is . - GNG (
IsGNG Γ): compatible satisfying, for some smooth ,
The arrows are diffeomorphisms of that preserve and and carry one derivative operator to the other through the transformation law
(IsGNGArrow). NG₁ arrows also preserve (IsNG1Arrow). NG₂ arrows are pairs with , where carries the gauge-transformed pair to (IsNG2Arrow).
Formalization targets
Goal: NG₂ ≃ GNG (ng2_equiv_gng, Weatherall Prop. 6.1)
Geometrization , has these properties:
- It sends NG₂ objects to GNG objects with the same allowed trajectories, and NG₂ arrows to GNG arrows.
- It is full and faithful: every GNG arrow is for a unique .
- It is essentially surjective: every GNG object is isomorphic to a geometrization.
This is exactly the "full, faithful, essentially surjective" route of Weatherall's proof in App. A. These three properties together are equivalent to an equivalence of categories.
Milestones (source order)
geometrization, Prop. 2.1 (Trautman). For flat compatible and Poisson's equation, has these properties:- it is a classical spacetime;
- its timelike geodesics are exactly the curves with ;
- it is the unique derivative operator with that property;
- it satisfies (1)–(3).
recovery, Prop. 2.2 (Trautman). Every classical spacetime satisfying (1)–(3) comes from some flat and potential obeying Poisson's equation.gauge_iff, the non-uniqueness remark after Prop. 2.2. A second pair works iff and . Weatherall states the "if" direction and his proof of Prop. 6.1 uses the "only if" direction. The iff is Malament's Prop. 4.2.5. Note that is allowed: the gauge includes time-dependent uniform accelerations (Corollary VI).geom_naturality, the key computation in App. A. A metric-preserving diffeomorphism carrying to carries to iff it carries to .ng1_not_equiv_gng, the NG₁ row of Table 1 (§6, p. 18). No object map NG₁ → GNG preserves empirical content while inducing bijections of hom-sets. Weatherall states this in prose without a proof. The intended argument is that two NG₁ models related by a nonzero gauge share a geometrization but have no NG₁ arrow between them.
Significance
- Philosophy of physics. This is the standard worked example for categorical criteria of theoretical equivalence: Glymour's criterion versus equivalence of categories. It also shows how "excess structure" (here the potential) is detected by fullness.
- Physics. Newton–Cartan geometry is the non-relativistic limit of general relativity. Fletcher, Manchak, Schneider and Weatherall (2018), Thm 8 restates Malament's (1986) theorem in Künzle's (1976) framework. If a family of Lorentzian metrics has and , and its Einstein tensors converge, then the limit derivative operator satisfies (1) and (2), but not necessarily (3). GR limits therefore land in a slightly larger class than GNG, and condition (3) is exactly what the recovery theorem needs. This makes the present mission the Newtonian half of a planned GR-limit mission.
- Lean. This is a reusable coordinate model of Galilean/Newton–Cartan structures, Christoffel transformation laws and curvature, none of which exist in Mathlib.
Difficulty
- Milestones 1, 3 and 4 are long but elementary tensor computations. The uniqueness clause in 1 needs local existence of solutions of the trajectory ODE (Mathlib's Picard–Lindelöf).
- Milestone 2 is the heart. Compatibility forces to be a rotation field plus an acceleration field . Condition (3) forces to be spatially constant, and condition (2) makes , minus the inertial terms of a rotating frame, a closed form on each slice. The Poincaré lemma, smoothly in the time parameter, then produces . The degree-1 Poincaré lemma on convex sets is in Mathlib, and the companion mission Weatherall 2016: Potentials vs. Field Strengths (continuum) develops the homotopy operator.
- The goal then assembles 2, 3 and 4.
Formalization scope
- Single global chart. Weatherall's spacetime is with arbitrary . Here and are fixed to their standard form in one global chart, a choice of Galilean coordinates; the derivative operators remain arbitrary. Arrows are genuine diffeomorphisms of .
- Normalized curves. Massive bodies have unit tangent , as in Malament (Ch. 4). Without this normalization the geodesic and force laws are not equivalent.
- No category instances. Categories are encoded by their hom-predicates, and "equivalence of categories" by the full / faithful / essentially-surjective data of App. A. Composition laws are not required by any item.
- Out of scope: Weatherall's footnote 32 (spatially compact matter), Glymour's criterion, and the GR limit (planned as a separate mission).
Selected references
- J. O. Weatherall, Are Newtonian Gravitation and Geometrized Newtonian Gravitation Theoretically Equivalent?, Erkenntnis 81 (2016) 1073–1091. Primary source: Props. 2.1, 2.2, 6.1, Table 1, App. A.
- D. B. Malament, Topics in the Foundations of General Relativity and Newtonian Gravitation Theory, University of Chicago Press (2012), Ch. 4 (Props. 4.2.1, 4.2.5). Conventions.
- D. B. Malament, Classical General Relativity, in Handbook of the Philosophy of Physics (2007).
- A. Trautman, Foundations and current problems of general relativity, in Brandeis Summer Institute 1964, Prentice-Hall (1965).
- S. C. Fletcher, J. B. Manchak, M. D. Schneider, J. O. Weatherall, Would Two Dimensions be World Enough for Spacetime?, Stud. Hist. Philos. Mod. Phys. 63 (2018) 100–113. Thm 8 is the Newtonian limit.
- H. P. Künzle, Covariant Newtonian limit of Lorentz space-times, Gen. Rel. Grav. 7 (1976) 445–457.