Cited by 247Noncommutative and Quantum Gravity TheoriesRelativity and Gravitational TheoryBlack Holes and Theoretical Physics

Quantum spin dynamics (QSD): II. The kernel of the Wheeler - DeWitt constraint operator

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Thiemann, T·1998·Classical and Quantum Gravity

Abstract

We determine the complete and rigorous kernel of the Wheeler - DeWitt constraint operator for four-dimensional, Lorentzian, non-perturbative, canonical vacuum quantum gravity in the continuum. We do this for the non-symmetric version of the operator constructed previously in this series. We also construct a symmetric, regulated constraint operator. For the regulated Euclidean Wheeler - DeWitt operator as well as for the regulated generator of the Wick transform from the Euclidean to the Lorentzian regime we prove existence of self-adjoint extensions and based on these we propose a method of proof of self-adjoint extensions for the regulated Lorentzian operator. Both constraint operators evaluated at unit lapse as well as the generator of the Wick transform can be shown to have regulator-independent and symmetric duals on the diffeomorphism-invariant Hilbert space. Finally, we comment on the status of the Wick rotation transform in the light of the present results and give an intuitive description of the action of the Hamiltonian constraint.

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Crossref · 10.1088/0264-9381/15/4/012

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  • The Higgs constraint can be analysed more easily in the reduced model because there is only one Higgs vertex.

    “In particular, the Higgs constraint ( [20] and section 2) can be analysed more easily because there is just one Higgs vertex in the reduced model.”

    From Loop quantum cosmology: I. Kinematics (2000) · cites this paper as [20]

  • For LRS models, the possible conjugacy classes of homomorphisms λ: F→G have representatives λ_k: U(1)→SU(2), exp(tτ3) → exp(ktτ3), for k ∈ N0.

    “For LRS models their representatives are given by λ k : U(1) → SU (2), exp(tτ 3 ) → exp(ktτ 3 ) for k ∈ N 0 = {0, 1, . ..} (for a derivation see the example of spherical symmetry in [20] which is in many respects similar to LRS models).”

    From Loop quantum cosmology: I. Kinematics (2000) · cites this paper as [20]

  • The reconstruction of invariant connections from the Higgs field pulls back a spin network function to a function on A_B × U_B; these functions are distributional states of the unreduced theory symmetric under [λ], and all symmetric states arise this way.

    “The basic idea of [20] is to use the reconstruction of invariant connections from the Higgs field to pull back a spin network function, which is a function on the space A of generalized connections on modulo gauge transformations, to a function on the space A B × U B of generalized connections and Higgs fields on the reduced manifold B.”

    From Loop quantum cosmology: I. Kinematics (2000) · cites this paper as [20]

  • The paper uses symmetric distributional states of loop quantum gravity defined in [20], which are exactly symmetric rather than only approximately symmetric at large scales.

    “In the present paper we make use of symmetric, distributional states of loop quantum gravity which have been defined and investigated in [20].Contrary to weaves, they are exactly symmetric, not only approximately at large scales.”

    From Loop quantum cosmology: I. Kinematics (2000) · cites this paper as [20]

  • For a non-compact space manifold, the symmetries can be interpreted as global asymptotic transformations at spatial infinity that are not part of the gauge group.

    “For a non-compact space manifold one can interpret the symmetries as global asymptotic transformations at spatial infinity which are not regarded as elements of the gauge group [23].”

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Research works printed but not linked: 6

  1. Ashtekar A and Lewandowski J 1994 Representation theory of analytic holonomy C algebras Knots and Quantum Gravity ed J Baez (Oxford: Oxford University Press)
  2. Thiemann T 1998 Quantum spin dynamics (QSD): III. Quantum constraint algebra and physical scalar product in quantum general relativity Class. Quantum Grav. 15 in press
  3. Thiemann T The length operator in canonical quantum gravity Harvard University Preprint HUTMP-96/B- 354, gr-qc/9606092 · arXiv
  4. Thiemann T 1998 Quantum spin dynamics (QSD): VI. Quantum Poincaré algebra and a quantum positivity of energy theorem for canonical quantum gravity Class. Quantum Grav. 15 in press
  5. Thiemann T 1998 Quantum spin dynamics (QSD): V. Quantum gravity as the natural regulator of the Hamiltonian constraint of matter quantum field theories Class. Quantum Grav. 15 in press
  6. Thiemann T Complete formula for the matrix elements of the volume operator in canonical quantum gravity Harvard University Preprint HUTMP-96/B-353, gr-qc/9606091 · arXiv

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Authors
Thiemann, T.
Affiliations
Harvard University (US)
Corresponding author
Thiemann, T
Venue
Classical and Quantum Gravity
Published
1998-04-01
Volume
15
Issue
4
Pages
875-905
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2012951907
Cited by
247
References
7
Citations by year
2026: 5 · 2025: 7 · 2024: 10 · 2023: 6 · 2022: 5 · 2021: 12 · 2020: 6 · 2019: 10 · 2018: 12 · 2017: 1 · 2016: 8 · 2015: 11 · 2014: 4 · 2013: 9 · 2012: 8
FWCI
13.10
Type
journal article
Language
en
Open access
Locations
  • Classical and Quantum Gravity (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • Max Planck Institute for Plasma Physics (submittedVersion)
  • Max Planck Digital Library (submittedVersion)
  • MPG.PuRe (Max Planck Society) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • U.S. Department of Energy (DE‐FG02‐)
  • Harvard University
Topics
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
Keywords
Wheeler-DeWitt equation, constraint operators, kernel, quantum spin dynamics, canonical quantum gravity, Lorentzian quantum gravity, Wick rotation, self-adjoint extensions, Hamiltonian constraint, non-perturbative quantum gravity

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