nLab 3d quantum gravity





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Solving the problem of quantization of systems including gravityquantum gravity – is notoriously hard. It does however simplify drastically in very low dimensions. While the theory in dimension 4 (or higher) is evidently relevant for the phenomenology of the world that we perceive, the Einstein-Hilbert action and its variants that defines the theory of gravity (at least as an effective QFT) makes sense in any dimension.

The case of dimension 3 is noteworthy, because in this case the quantum theory can be and has been fairly completely understood and is nevertheless non-trivial. Informally, this is due to the fact that behaviour of gravity in 3-dimensions is much simpler than in higher dimensions: there cannot be gravitational waves in 3-dimensions, hence no “local excitations”. Accordingly, the theory turns out to have a finite dimensional covariant phase space.

More formally, one finds that in 3-dimensions, the Einstein-Hilbert action, in the first order formulation of gravity (Cartan connection), becomes equivalent to the action functional of a very well studied 3-dimensional field theory, namely Chern-Simons theory for gauge group the Poincaré group Iso(2,1)Iso(2,1) (for vanishing cosmological constant) or the de Sitter group/anti de Sitter group Iso(2,2)Iso(2,2) or Iso(3,1)Iso(3,1) (for non-vanishing cosmological constant). See at de Sitter gravity and at Chern-Simons Gravity.

This means that one can take the quantization of Iso(2,1)Iso(2,1)-Chern-Simons theory as the definition of 3d quantum gravity. This has first been noticed and successfully carried out in (Witten88). One should note here that this means that one allows degenerate vielbein/pseudo-Riemannian metric tensors as field configurations of gravity. In fact, as (Witten88) discusses in detail, this compactification of configuration space can be seen as the source of the reasons why 3d quantum gravity makes exists.

Based on this striking situation in 3-dimensions it is natural to wonder if it makes sense to consider Iso(n,1)Iso(n,1)-higher dimensional Chern-Simons theory, or variants thereof, as theories of quantum gravity in higher dimensions. The for n>2n \gt 2 the corresponding action functionals differ from the Einstein-Hilbert action by higher curvature terms, but in suitable limits of the theory these can be argued to play a negligible role. For more on this see the entry Chern-Simons gravity .


One can add additional terms arriving at what is called massive 3d gravity models . Very relevant for its study is the AdS3/CFT2 correspondence.


  • Nathan Benjamin, Scott Collier, Alexander Maloney, Pure Gravity and Conical Defects, Journal of High Energy Physics 2020 34 (2020) [arXiv:2004.14428, doi:10.1007/JHEP09(2020)034]

  • Mauricio Leston, et al., 3d Quantum Gravity Partition Function at 3 Loops: a brute force computation [arXiv:2307.03830]

3d Gravity and Chern-Simons theory

On 3-dimensional (quantum) gravity (general relativity) with cosmological constant, and its (non-)relation to Chern-Simons theory with non-compact gauge groups:

The original articles on 3d gravity, discussing its formulation as a Chern-Simons theory and discovering its holographic relation to a 2d CFT boundary field theory (well before AdS/CFT was conceived from string theory):

The corresponding non-perturbative quantization of 3-dimensional gravity, via quantization of 3d Chern-Simons theory:

  • Edward Witten, (2+1)-Dimensional Gravity as an Exactly Soluble System Nucl. Phys. B311 (1988) 46. (web)

  • Herman Verlinde, Conformal field theory, two-dimensional quantum gravity and quantization of Teichmüller space, Nuclear Physics B

    Volume 337, Issue 3, 25 June 1990, Pages 652-680 (doi:10.1016/0550-3213(90)90510-K)


Further developments:

See also:

Wilson lines computing holographic entropy in AdS 3/CFT 2AdS_3/CFT_2

Discussion of BTZ black hole entropy and more generally of holographic entanglement entropy in 3d quantum gravity/AdS3/CFT2 via Wilson line observables in Chern-Simons theory:

  • Martin Ammon, Alejandra Castro, Nabil Iqbal, Wilson Lines and Entanglement Entropy in Higher Spin Gravity, JHEP 10 (2013) 110 (arXiv:1306.4338)

  • Jan de Boer, Juan I. Jottar, Entanglement Entropy and Higher Spin Holography in AdS 3AdS_3, JHEP 1404:089, 2014 (arXiv:1306.4347)

  • Alejandra Castro, Stephane Detournay, Nabil Iqbal, Eric Perlmutter, Holographic entanglement entropy and gravitational anomalies, JHEP 07 (2014) 114 (arXiv:1405.2792)

  • Mert Besken, Ashwin Hegde, Eliot Hijano, Per Kraus, Holographic conformal blocks from interacting Wilson lines, JHEP 08 (2016) 099 (arXiv:1603.07317)

  • Andreas Blommaert, Thomas G. Mertens, Henri Verschelde, The Schwarzian Theory - A Wilson Line Perspective, JHEP 1812 (2018) 022 (arXiv:1806.07765)

  • Ashwin Dushyantha Hegde, Role of Wilson Lines in 3D Quantum Gravity, 2019 (spire:1763572)

  • Xing Huang, Chen-Te Ma, Hongfei Shu, Quantum Correction of the Wilson Line and Entanglement Entropy in the AdS 3AdS_3 Chern-Simons Gravity Theory (arXiv:1911.03841)

  • Eric D'Hoker, Per Kraus, Gravitational Wilson lines in AdS 3AdS_3 (arXiv:1912.02750)

  • Marc Henneaux, Wout Merbis, Arash Ranjbar, Asymptotic dynamics of AdS 3AdS_3 gravity with two asymptotic regions (arXiv:1912.09465)

and similarly for 3d flat-space holography:

Discussion for 3d de Sitter spacetime:

  • Alejandra Castro, Philippe Sabella-Garnier, Claire Zukowski, Gravitational Wilson Lines in 3D de Sitter (arXiv:2001.09998)

Last revised on July 11, 2023 at 04:36:34. See the history of this page for a list of all contributions to it.