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Lovelock's theorem

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Lovelock's theorem of general relativity says that from a local gravitational action which contains only second derivatives of the four-dimensional spacetime metric, then the only possible equations of motion are the Einstein field equations.[1][2][3] The theorem was described by British physicist David Lovelock in 1971.

Statement

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In four dimensional spacetime, any tensor whose components are functions of the metric tensor and its first and second derivatives (but linear in the second derivatives of ), and also symmetric and divergence-free, is necessarily of the form

where and are constant numbers and is the Einstein tensor.[3]

The only possible second-order Euler–Lagrange expression obtainable in a four-dimensional space from a scalar density of the form is[1]

Consequences

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Lovelock's theorem means that if we want to modify the Einstein field equations, then we have five options.[1]

  • Add other fields rather than the metric tensor;
  • Use more or fewer than four spacetime dimensions;
  • Add more than second order derivatives of the metric;
  • Non-locality, e.g. for example the inverse d'Alembertian;
  • Emergence – the idea that the field equations don't come from the action.

See also

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References

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  1. ^ a b c Clifton, Timothy; et al. (March 2012). "Modified Gravity and Cosmology". Physics Reports. 513 (1–3): 1–189. arXiv:1106.2476. Bibcode:2012PhR...513....1C. doi:10.1016/j.physrep.2012.01.001. S2CID 119258154.
  2. ^ Lovelock, D. (1971). "The Einstein Tensor and Its Generalizations". Journal of Mathematical Physics. 12 (3): 498–501. Bibcode:1971JMP....12..498L. doi:10.1063/1.1665613.
  3. ^ a b Lovelock, David (10 January 1972). "The Four-Dimensionality of Space and the Einstein Tensor". Journal of Mathematical Physics. 13 (6): 874–876. Bibcode:1972JMP....13..874L. doi:10.1063/1.1666069.