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Lovelock Uniqueness and Its Hypotheses

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Lovelock’s theorem does not say that general relativity is the only possible theory of gravity. It classifies a sharply delimited set of pure-metric field tensors. In four dimensions, locality, diffeomorphism naturality, symmetry, identically vanishing divergence, smooth dependence, and differential order at most two leave only the Einstein tensor and the metric. Changing the dimension, derivative order, field content, connection, or locality assumption leaves the theorem’s domain.

Required background. We use the Riemann curvature tensor for natural second-order tensors, Hilbert stress–energy for the symmetric source paired with them, and the scope of the equivalence principles to avoid turning local metric physics into a uniqueness premise.

Helpful background. Minkowski geometry supplies the fixed Lorentzian signature, natural tensor operations supply the language of equivariance, and presymplectic potentials clarify why divergence identities arise in variational theories.

Let XX be a smooth four-dimensional manifold and let gg range over nondegenerate pseudo-Riemannian metrics of one fixed signature. Suppose Hμν[g]H_{\mu\nu}[g] satisfies all of the following:

  1. Pure metric and local. At xx, Hg(x)H_g(x) depends only on the metric in an arbitrarily small neighborhood of xx, with no extra fields or fixed background tensors.
  2. Diffeomorphism natural. For every local diffeomorphism φ\varphi, H[φ∗g]=φ∗H[g]H[\varphi^*g]=\varphi^*H[g].
  3. Differential order at most two. The value at xx depends only on the two-jet jx2gj_x^2g: in coordinates, on gαβg_{\alpha\beta} and its first and second derivatives at xx.
  4. Smooth regularity. That dependence on the two-jet is smooth on the bundle of nondegenerate metrics of the chosen signature.
  5. Symmetry. Hμν=HνμH_{\mu\nu}=H_{\nu\mu} for every gg.
  6. Identical divergence freedom. With the Levi-Civita connection of gg, ∇μHμν[g]=0\nabla^\mu H_{\mu\nu}[g]=0 for every metric, without using a field equation.

Then there are real constants aa and bb, independent of position and of the chosen metric, such that

Hμν=aGμν+bgμν.H_{\mu\nu}=aG_{\mu\nu}+b g_{\mu\nu}.

This is the four-dimensional specialization of the smooth natural-tensor classification in Navarro and Navarro 2011, Definition 1.1, printed p. 2, and Theorem 2.6, printed p. 9, Open PDF. Lovelock’s 1971 paper and its 1972 four-dimensional companion are listed below for historical provenance; the proof locators used on this page are the accessible modern treatment.

No action principle, boundary condition, causal condition, or weak-field limit is among these hypotheses. Accordingly, the conclusion classifies the allowed left-hand tensor under the listed assumptions; it does not fix aa, bb, or the matter coupling. Writing

aGμν+bgμν=κTμν,a≠0,aG_{\mu\nu}+b g_{\mu\nu}=\kappa T_{\mu\nu}, \qquad a\ne0,

and dividing by aa, the Newtonian limit fixes the ratio κ/a=8πG\kappa/a=8\pi G, while Λ=b/a\Lambda=b/a. An overall rescaling of both sides is conventional.

Some summaries state a separate assumption that HμνH_{\mu\nu} be linear in the second derivatives of the metric. The smooth-natural version above is more precise about where that property enters. It begins with a smooth two-jet map, not a polynomial ansatz. Symmetry, naturality, and divergence freedom then imply that the map is polynomial in the normal-coordinate second-derivative data, with degree at most

⌊D−12⌋.\left\lfloor\frac{D-1}{2}\right\rfloor.

In D=4D=4 this degree is at most one. Thus linearity in those normal-tensor variables is a conclusion of the Navarro–Navarro formulation, whereas other formulations may impose a linearity or polynomial qualification at the outset. Smoothness still matters: an arbitrary singular or discontinuous rule on metric jets is not covered.

Reall gives the compact four-dimensional corollary Hab=αGab+βgabH_{ab}=\alpha G_{ab}+\beta g_{ab} in Reall 2013, § 6.7, printed p. 65, Eq. (6.34), PDF. That lecture-note passage is a statement of the theorem, not a proof; the proof architecture used here comes from Navarro and Navarro.

The proof has four structural steps.

Reduce jets to an orthogonal-group problem. In normal coordinates at a point, gabg_{ab} is the fixed signature matrix and gab,c=0g_{ab,c}=0. The remaining second derivatives form a vector space NN of normal tensors with specific pair and cyclic symmetries. A second-order natural symmetric tensor is therefore equivalent to a smooth O(p,q)O(p,q)-equivariant map f:N→S2f:N\to S^2. This is developed in Navarro and Navarro 2011, Definitions 1.1–1.2 and Theorem 1.3, printed pp. 2–3, Open PDF.

Differentiate the natural map. The successive derivatives dkfd^kf are themselves equivariant tensors. Divergence freedom forces an additional cyclic index symmetry on them. Definitions 1.1–1.10 establish the natural-bundle, normal-tensor, derivative, and divergence-free framework; Theorem 1.11 then embeds each homogeneous degree-kk possibility into an orthogonal-invariant space (Divk)O(p,q)(\mathrm{Div}^k)^{O(p,q)} Navarro and Navarro 2011, printed pp. 2–6, Open PDF.

Count invariants. Orthogonal invariant theory and the cyclic symmetries show that this invariant space is one-dimensional for k≤⌊(D−1)/2⌋k\le\lfloor(D-1)/2\rfloor and zero above that value. Vanishing sufficiently high derivatives makes ff polynomial rather than merely smooth. These are Navarro and Navarro 2011, Lemma 2.2 and Corollary 2.3, printed pp. 6–7, Open PDF.

Exhibit the basis. Curvature forms and the metric construct Lovelock tensors LkL_k. Each is natural, symmetric, divergence-free, and homogeneous of degree kk. The invariant count shows that no others exist: L0,…,L⌊(D−1)/2⌋L_0,\ldots,L_{\lfloor(D-1)/2\rfloor} form a basis. In four dimensions only L0L_0 and L1L_1 remain; after lowering indices they are proportional to gμνg_{\mu\nu} and GμνG_{\mu\nu}. The construction and basis theorem are Navarro and Navarro 2011, Definition 2.5 and Theorem 2.6, printed p. 9, Open PDF.

This is a proof sketch of the classification’s architecture, not a replacement for the invariant-theory argument.

Higher dimension. For D≥5D\ge5, the Gauss–Bonnet or second Lovelock tensor is generally nonzero:

HμνGB=2(RRμν−2RμαRαν−2RαβRμανβ+RμαβγRναβγ)−12gμνLGB,\begin{aligned} H^{\rm GB}_{\mu\nu}=2\big(&RR_{\mu\nu}-2R_{\mu\alpha}R^\alpha{}_\nu -2R^{\alpha\beta}R_{\mu\alpha\nu\beta}\\ &+R_\mu{}^{\alpha\beta\gamma}R_{\nu\alpha\beta\gamma}\big) -\frac12g_{\mu\nu}\mathcal L_{\rm GB}, \end{aligned}

where LGB=RαβγδRαβγδ−4RαβRαβ+R2\mathcal L_{\rm GB}=R_{\alpha\beta\gamma\delta}R^{\alpha\beta\gamma\delta}-4R_{\alpha\beta}R^{\alpha\beta}+R^2. It satisfies the same second-order, natural, symmetric, divergence-free conditions but is not a combination of GμνG_{\mu\nu} and gμνg_{\mu\nu}. In four dimensions its metric Euler–Lagrange tensor vanishes identically.

Higher differential order. Varying an R2R^2 action gives a divergence-free tensor containing

2RRμν−12gμνR2+2(gμν□−∇μ∇ν)R,2RR_{\mu\nu}-\frac12g_{\mu\nu}R^2 +2(g_{\mu\nu}\Box-\nabla_\mu\nabla_\nu)R,

which generally has fourth derivatives of the metric. It violates the order-two hypothesis.

Extra fields. A scalar–tensor term F(ϕ)RF(\phi)R produces metric terms such as

F(ϕ)Gμν+(gμν□−∇μ∇ν)F(ϕ).F(\phi)G_{\mu\nu} +(g_{\mu\nu}\Box-\nabla_\mu\nabla_\nu)F(\phi).

Their divergence closes together with the scalar equation. This is not a pure-metric natural tensor.

Different connection or locality. Independent torsion or nonmetricity supplies additional tensors not built from the Levi-Civita two-jet. A nonlocal term such as R□−1RR\Box^{-1}R depends on boundary conditions or a Green function rather than only on jx2gj_x^2g. Each is an explicit departure from a stated hypothesis, not a counterexample to the theorem.

Use the degree bound to determine which Lovelock tensors can occur in D=4D=4, D=5D=5, and D=6D=6. What does this show about Gauss–Bonnet dynamics?

Solution

The largest degree is p=⌊(D−1)/2⌋p=\lfloor(D-1)/2\rfloor. For D=4D=4, p=1p=1, so the basis contains only L0L_0 and L1L_1, corresponding to the metric and Einstein tensors. For D=5D=5, p=2p=2, and for D=6D=6, p=2p=2, so L2L_2, the Gauss–Bonnet tensor, is also allowed. Hence its local metric field tensor is identically absent in four dimensions but can contribute nontrivially from five dimensions onward.

  • Lovelock, David. “The Einstein Tensor and Its Generalizations.” Journal of Mathematical Physics 12, no. 3 (1971): 498–501. DOI.
  • Lovelock, David. “The Four-Dimensionality of Space and the Einstein Tensor.” Journal of Mathematical Physics 13, no. 6 (1972): 874–876. DOI.
  • Navarro, Alberto, and José Navarro. “Lovelock’s Theorem Revisited.” Journal of Geometry and Physics 61, no. 10 (2011): 1950–1956. DOI; Open PDF.
  • Reall, Harvey S. General Relativity. Cambridge Part III lecture notes (2013), § 6.7, printed p. 65. PDF.