Math 2.0

Relativity and gravitational theory Definition

Horndeski's theory

Builds on Scalar–tensor theoryLorentzian manifoldScalar curvatureEinstein tensorCovariant derivative

Definition

Let gg be a Lorentzian metric on a four-dimensional manifold and ϕ\phi a real scalar field. Write ∇\nabla for the covariant derivative of gg, □ϕ=∇a∇aϕ\square\phi = \nabla^a\nabla_a\phi, X=−12gab∂aϕ ∂bϕX = -\frac12 g^{ab}\partial_a\phi\,\partial_b\phi, RR for the scalar curvature and GabG_{ab} for the Einstein tensor. Let G2,G3,G4,G5G_2, G_3, G_4, G_5 be smooth functions of (ϕ,X)(\phi, X), and write GiX=∂Gi/∂XG_{iX} = \partial G_i/\partial X. Horndeski's theory is the scalar–tensor theory with action S=∫(L2+L3+L4+L5)−g d4x+Sm[g,ψ]S = \int (L_2 + L_3 + L_4 + L_5)\sqrt{-g}\,d^4x + S_m[g, \psi], where

  1. L2=G2(ϕ,X)L_2 = G_2(\phi, X);
  2. L3=−G3(ϕ,X) □ϕL_3 = -G_3(\phi, X)\,\square\phi;
  3. L4=G4(ϕ,X) R+G4X[(□ϕ)2−∇a∇bϕ ∇a∇bϕ]L_4 = G_4(\phi, X)\,R + G_{4X}\left[(\square\phi)^2 - \nabla_a\nabla_b\phi\,\nabla^a\nabla^b\phi\right];
  4. L5=G5(ϕ,X) Gab∇a∇bϕ−16G5X[(□ϕ)3−3 □ϕ ∇a∇bϕ ∇a∇bϕ+2 ∇a∇bϕ ∇b∇cϕ ∇c∇aϕ]L_5 = G_5(\phi, X)\,G_{ab}\nabla^a\nabla^b\phi - \frac{1}{6} G_{5X}\left[(\square\phi)^3 - 3\,\square\phi\,\nabla_a\nabla_b\phi\,\nabla^a\nabla^b\phi + 2\,\nabla_a\nabla^b\phi\,\nabla_b\nabla^c\phi\,\nabla_c\nabla^a\phi\right];

and the matter action SmS_m depends on gg and the matter fields ψ\psi but not on ϕ\phi.

Remarks

This is the form of the Lagrangian found by Kobayashi, Yamaguchi and Yokoyama, which is equivalent to Horndeski's original one. Although the Lagrangian contains second derivatives of ϕ\phi and of gg, the combinations above are chosen so that the field equations contain no derivatives higher than the second. Example: G4=1/(16πG)G_4 = 1/(16\pi G), G2=X−V(ϕ)G_2 = X - V(\phi) and G3=G5=0G_3 = G_5 = 0 give general relativity with a minimally coupled scalar field with potential VV. Example: G4=ϕ/(16π)G_4 = \phi/(16\pi), G2=2ωX/(16πϕ)G_2 = 2\omega X/(16\pi\phi) and G3=G5=0G_3 = G_5 = 0 give Brans–Dicke theory. Non-example: the Lagrangian (□ϕ)2(\square\phi)^2 alone gives a fourth-order equation for ϕ\phi, so it is not in the class. The observed equality of the speeds of gravitational waves and light constrains the theory strongly, essentially forcing G4X≈0G_{4X} \approx 0 and G5G_5 to be nearly constant.

Reading path

To understand this page from the ground up, read these 6 pages in order. The foundations come first.

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  1. Covariant derivative concept
  2. Einstein tensor concept
  3. Lorentzian manifold concept
  4. Scalar curvature concept
  5. Scalar–tensor theory concept
  6. Horndeski's theory definition

Further reading

  1. Web https://en.wikipedia.org/wiki/Horndeski%27s_theory
About this page
TagY23SAQAWAK
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Kinddefinition
WritingW0 stub
MSC83D05
DefinesHorndeski's theory
UsesScalar–tensor theory, Lorentzian manifold, Scalar curvature, Einstein tensor, Covariant derivative
Changed3 November 2026

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