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Taming Thiemann’s Hamiltonian constraint in canonical loop quantum gravity: Reversibility, eigenstates, and graph-change analysis

T. L. M. Guedes1,2,*, G. A. Mena Marugán3,†, M. Müller1,2,‡, and F. Vidotto3,4,§

  • *Contact author: t.guedes@fz-juelich.de
  • †Contact author: mena@iem.cfmac.csic.es
  • ‡Contact author: markus.mueller@fz-juelich.de
  • §Contact author: fvidotto@uwo.ca

Phys. Rev. D 112, 026024 – Published 22 July, 2025

DOI: https://doi.org/10.1103/hjdk-kdhk

Abstract

One of the key concepts in loop quantum gravity is the quantization of spacetime geometry, with discrete observables such as the quantum area and volume. The quantum state of the gravitational field is encoded in so-called spin networks, and the conventional quantum-mechanical dynamics is substituted by a description in terms of constrained quantum states, in which several constraints define the physical subspace of the Hilbert space. One of these constraints, commonly called the Hamiltonian constraint, remains an elusive object in loop quantum gravity because its action on spin networks leads to changes in their corresponding graphs. As a result, calculations in loop quantum gravity are often considered unpractical, and neither the eigenstates of the Hamiltonian constraint, which form the physical space of states, nor the concrete effect of this graph-changing character on observables are entirely known. Much worse, there is no reference value to judge whether the commonly adopted graph-preserving approximations lead to results anywhere close to the nonapproximated dynamics. Our work sheds light on several of these issues, by devising a new numerical tool that allows us to implement the action of the Hamiltonian constraint without the need for approximations and to calculate expectation values for the geometric observables. To achieve that, we fill the theoretical gap left in the derivations of the action of the Hamiltonian constraint on spin networks: we provide the first complete derivation of such action for the case of 4-valent spin networks, while updating the corresponding derivation for 3-valent spin networks. Our derivations also include the action of the volume operator. By proposing a new approach to encode spin networks into functions of lists and the derived formulas into functionals, we implement both the Hamiltonian constraint and the volume operator numerically. We are able to transform spin networks with graph-changing dynamics perturbatively and verify that the expectation values for the volume have rather different behavior from the approximated, graph-preserving results. Furthermore, using our tool we find a family of potentially relevant solutions of the Hamiltonian constraint. Our work paves the way to a new generation of calculations in loop quantum gravity, in which graph-changing results and their phenomenology can finally be accounted for and understood.

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References (75)

  1. G. Amelino-Camelia, C. Lämmerzahl, A. Macias, and H. Müller, The search for quantum gravity signals, The-search-for-quantum-gravity-signals, AIP Conf. Proc. 758, 30 (2005).
  2. R. Howl, L. Hackermüller, D. E. Bruschi, and I. Fuentes, Gravity in the quantum lab, Adv. Phys. X 3, 1383184 (2018).
  3. A. Barrau, Testing different approaches to quantum gravity with cosmology: An overview, C.R. Phys. 18, 189 (2017).
  4. M. Bronstein, Republication of: Quantum theory of weak gravitational fields, Gen. Relativ. Gravit. 44, 267 (2012).
  5. P. A. M. Dirac, The theory of gravitation in Hamiltonian form, Proc. R. Soc. A. 246, 333 (1958).
  6. P. A. M. Dirac, Lectures on Quantum Mechanics (Yeshiva University, New York, 2001).
  7. S. W. Hawking, Breakdown of predictability in gravitational collapse, Phys. Rev. D 14, 2460 (1976).
  8. J. A. Wheeler, Superspace and the nature of quantum geometrodynamics, Adv. Ser. Astrophys. Cosmol. 3, 27 (1987).
  9. B. S. DeWitt, Quantum theory of gravity. I. The canonical theory, Phys. Rev. 160, 1113 (1967).
  10. A. Ashtekar, New variables for classical and quantum gravity, Phys. Rev. Lett. 57, 2244 (1986).
  11. J. F. Barbero G., Real ashtekar variables for Lorentzian signature space-times, Phys. Rev. D 51, 5507 (1995).
  12. C. Rovelli and L. Smolin, Knot theory and quantum gravity, Phys. Rev. Lett. 61, 1155 (1988).
  13. T. Thiemann, Anomaly-free formulation of non-perturbative, four-dimensional Lorentzian quantum gravity, Phys. Lett. B 380, 257 (1996).
  14. A. Ashtekar and J. Lewandowski, Background independent quantum gravity: A status report, Classical Quantum Gravity 21, R53 (2004).
  15. R. Koenig, G. Kuperberg, and B. W. Reichardt, Quantum computation with Turaev–Viro codes, Ann. Phys. (Amsterdam) 325, 2707 (2010).
  16. Y.-J. Liu, K. Shtengel, A. Smith, and F. Pollmann, Methods for simulating string-net states and anyons on a digital quantum computer, PRX Quantum 3, 040315 (2022).
  17. S. Trebst, M. Troyer, Z. Wang, and A. W. Ludwig, A short introduction to Fibonacci anyon models, Prog. Theor. Phys. Suppl. 176, 384 (2008).
  18. I. Mäkinen, Introduction to SU(2) recoupling theory and graphical methods for loop quantum gravity, arXiv:1910.06821.
  19. L. H. Kauffman and S. Lins, Temperley-Lieb Recoupling Theory and Invariants of 3-Manifolds (Princeton University Press, Pinceton, NJ, 1994).
  20. D. Brink and G. Satchler, Angular Momentum (Clarendon Press, Oxford, 1968), 2nd ed.
  21. A. Messiah, Quantum Mechanics Vol. II (North Holland Publishing Company, Amsterdam, 1962).
  22. T. L. M. Guedes, G. A. Mena Marugán, F. Vidotto, and M. Müller, Computing the graph-changing dynamics of loop quantum gravity, arXiv:2412.20257.
  23. J. Yang and Y. Ma, Graphical calculus of volume, inverse volume and Hamiltonian operators in loop quantum gravity, Eur. Phys. J. C 77, 1 (2017).
  24. R. Borissov, R. De Pietri, and C. Rovelli, Matrix elements of Thiemann’s Hamiltonian constraint in loop quantum gravity, Classical Quantum Gravity 14, 2793 (1997).
  25. M. Gaul and C. Rovelli, A generalized Hamiltonian constraint operator in loop quantum gravity and its simplest Euclidean matrix elements, Classical Quantum Gravity 18, 1593 (2001).
  26. E. Alesci, T. Thiemann, and A. Zipfel, Linking covariant and canonical loop quantum gravity: New solutions to the Euclidean scalar constraint, Phys. Rev. D 86, 024017 (2012).
  27. H. Sahlmann and W. Sherif, Towards quantum gravity with neural networks: Solving the quantum Hamilton constraint of U(1) BF theory, Classical Quantum Gravity 41, 225014 (2024).
  28. H. Sahlmann and W. Sherif, Towards quantum gravity with neural networks: Solving quantum Hamilton constraints of 3d Euclidean gravity in the weak coupling limit, Classical Quantum Gravity 41, 215006 (2024).
  29. M. Assanioussi, J. Lewandowski, and I. Mäkinen, Time evolution in deparametrized models of loop quantum gravity, Phys. Rev. D 96, 024043 (2017).
  30. In priniciple our focus is on analytic deformations, but see nonetheless the technical subtleties commented in the last paragraph of this section.

  31. C. Rovelli, Quantum Gravity (Cambridge University Press, Cambridge, England, 2004).
  32. A. Ashtekar and P. Singh, Loop quantum cosmology: A status report, Classical Quantum Gravity 28, 213001 (2011).
  33. G. A. Mena Marugán, A brief introduction to loop quantum cosmology, AIP Conf. Proc. 1130, 89 (2009).
  34. T. Thiemann, Quantum spin dynamics (QSD), Classical Quantum Gravity 15, 839 (1998).
  35. T. Thiemann, Quantum spin dynamics (QSD): II. The kernel of the Wheeler-DeWitt constraint operator, Classical Quantum Gravity 15, 875 (1998).
  36. T. Thiemann, Modern Canonical Quantum General Relativity (Cambridge University Press, Cambridge, England, 2007).
  37. A. Ashtekar and J. Lewandowski, Quantum theory of geometry: I. Area operators, Classical Quantum Gravity 14, A55 (1997).
  38. A. Ashtekar and J. Lewandowski, Quantum theory of geometry II: Volume operators, Adv. Theor. Math. Phys. 1, 388 (1998).
  39. T. Thiemann, Closed formula for the matrix elements of the volume operator in canonical quantum gravity, J. Math. Phys. (N.Y.) 39, 3347 (1998).
  40. K. Giesel and T. Thiemann, Consistency check on volume and triad operator quantization in loop quantum gravity: I, Classical Quantum Gravity 23, 5667 (2006).
  41. K. Giesel and T. Thiemann, Consistency check on volume and triad operator quantization in loop quantum gravity: II, Classical Quantum Gravity 23, 5693 (2006).
  42. R. De Pietri and C. Rovelli, Geometry eigenvalues and the scalar product from recoupling theory in loop quantum gravity, Phys. Rev. D 54, 2664 (1996).
  43. J. Yang and Y. Ma, Graphical method in loop quantum gravity: I. Derivation of the closed formula for the matrix element of the volume operator, Eur. Phys. J. C 77, 235 (2017).
  44. C. Rovelli and L. Smolin, Spin networks and quantum gravity, Phys. Rev. D 52, 5743 (1995).
  45. C. Rovelli and L. Smolin, Loop space representation of quantum general relativity, Nucl. Phys. B331, 80 (1990).
  46. D. Horsman, A. G. Fowler, S. Devitt, and R. Van Meter, Surface code quantum computing by lattice surgery, New J. Phys. 14, 123011 (2012).
  47. M. Gutiérrez, M. Müller, and A. Bermúdez, Transversality and lattice surgery: Exploring realistic routes toward coupled logical qubits with trapped-ion quantum processors, Phys. Rev. A 99, 022330 (2019).
  48. K. Giesel and H. Sahlmann, From classical to quantum gravity: Introduction to loop quantum gravity, Proc. Sci. QGQGS2011 (2011) 002 [arXiv:1203.2733].
  49. K. Giesel and T. Thiemann, Algebraic quantum gravity (aqg): I. Conceptual setup, Classical Quantum Gravity 24, 2465 (2007).
  50. C. Charles and E. R. Livine, The Fock space of loopy spin networks for quantum gravity, Gen. Relativ. Gravit. 48, 113 (2016).
  51. I. Mäkinen, Operators of quantum-reduced loop gravity from the perspective of full loop quantum gravity, Phys. Rev. D 102, 106010 (2020).
  52. T. Thiemann, The phoenix project: Master constraint programme for loop quantum gravity, Classical Quantum Gravity 23, 2211 (2006).
  53. Note that the way the grasp is attached to the link along the direction p4 is different when the temporary spin-1/2 link is present. Nonetheless, after applying Eq. (11) when we take the limit in which the spin 1/2 tends to 0, the difference boils down to a braid operation and an arrow flip, giving an overall phase of (−1)1+j4+j4(−1)2j4=−1, which cancels out the minus in the prefactors in Eq. (82). This shows graphically how the volume for 4-valent intertwiners can be obtained from Eq. (82).

  54. J. Brunnemann and D. Rideout, Properties of the volume operator in loop quantum gravity: I. Results, Classical Quantum Gravity 25, 065001 (2008).
  55. Mathematica notebook available in https://github.com/ThiagoLMGuedes/Canonical_LQG.
  56. M. Domagała, K. Giesel, W. Kamiński, and J. Lewandowski, Gravity quantized: Loop quantum gravity with a scalar field, Phys. Rev. D 82, 104038 (2010).
  57. R. Gambini, J. Griego, and J. Pullin, Chern-Simons states in spin-network quantum gravity, Phys. Lett. B 413, 260 (1997).
  58. T. Thiemann and M. Varadarajan, On propagation in loop quantum gravity, Universe 8, 615 (2022).
  59. C. Rovelli and F. Vidotto, Stepping out of homogeneity in loop quantum cosmology, Classical Quantum Gravity 25, 225024 (2008).
  60. M. P. Reisenberger and C. Rovelli, “Sum over surfaces” form of loop quantum gravity, Phys. Rev. D 56, 3490 (1997).
  61. Calculations for such values of the lapse, already close to the unit, might be questionable in a perturbative study. Nonetheless, our results about the relative values of the 2nd-order and 4th-order contributions provide support to their validity, or at least are not in conflict with it.

  62. K. Giesel and T. Thiemann, Scalar material reference systems and loop quantum gravity, Classical Quantum Gravity 32, 135015 (2015).
  63. B. Elizaga Navascués and G. A. Mena Marugán, Hybrid loop quantum cosmology: An overview, Front. Astron. Space Sci. 8, 62482 (2021).
  64. H. M. Haggard and C. Rovelli, Quantum-gravity effects outside the horizon spark black to white hole tunneling, Phys. Rev. D 92, 104020 (2015).
  65. C. Rovelli and F. Vidotto, Small black/white hole stability and dark matter, Universe 4, 127 (2018).
  66. M. Han, C. Rovelli, and F. Soltani, Geometry of the black-to-white hole transition within a single asymptotic region, Phys. Rev. D 107, 064011 (2023).
  67. A. Ashtekar, M. Bojowald, and J. Lewandowski, Mathematical structure of loop quantum cosmology, Adv. Theor. Math. Phys. 7, 233 (2003).
  68. M. Christodoulou and F. d’Ambrosio, Characteristic time scales for the geometry transition of a black hole to a white hole from spinfoams, Classical Quantum Gravity 41, 195030 (2024).
  69. C. Rovelli and F. Vidotto, White-hole dark matter and the origin of past low-entropy, arXiv:1804.04147.
  70. H. Huang, J. Kunz, J. Yang, and C. Zhang, Light ring behind wormhole throat: Geodesics, images, and shadows, Phys. Rev. D 107, 104060 (2023).
  71. It is worth noting that the expression given in Ref. [19] fails to retrieve the correct answer, which is zero, in certain specific cases with violation of triangularity, such as, for example, when the central color [j in Eq. (b2)] alone violates it.

  72. Note that the original expression of the formula in Sec. 8.5 of Ref. [19], also reproduced in Refs. [24, 25, 31], has a typo (a minus sign turned into a plus) relative to the correct derivation presented in Sec. 9.11 of Ref. [19], also reproduced in Refs. [24, 25, 31]. Furthermore, the derivation only holds when the triangularity condition is fulfilled, therefore numerical evaluations using this formula require the additional inclusion of triangularity-based selection rules.

  73. By convention, the attachment of a holonomy is always performed from the right side of an edge. This ordering will be important later, when Eq. (b8) comes into play. If one consistently attaches holonomies from the same side, however, it does not matter which side is chosen as convention.

  74. Note that λca,b=λba,c=λab,c, because (−1)−1=−1.

  75. V. G. Turaev and O. Y. Viro, State sum invariants of 3-manifolds and quantum 6j-symbols, Topology 31, 865 (1992).

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