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An Inner Product for 4D Quantum Gravity and the Chern-Simons-Kodama State

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arxiv 2212.07446 v2 pith:SQHMKTNM submitted 2022-12-14 hep-th gr-qc

classification hep-thgr-qc
keywords productgravityinnerquantumstatemeasureashtekarcertain
verification ladder T0 review T1 audit T2 compute T3 formal
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We demonstrate that reality conditions for the Ashtekar connection imply a non-trivial measure for the inner product of gravitational states in the polarization where the Ashtekar connection is diagonal, and we express the measure as the determinant of a certain first-order differential operator. This result opens the possibility to perform a non-perturbative analysis of the quantum gravity scalar product. In this polarization, the Chern-Simons-Kodama state, which solves the constraints of quantum gravity for a certain factor ordering, and which has de Sitter space as a semiclassical limit, is perturbatively non-normalizable with respect to the naive ve inner product. Our work reopens the question of whether this state might be normalizable when the correct non-perturbative inner product and choice of integration contour are taken into account. As a first step, we perform a semi-classical treatment of the measure by evaluating it on the round three-sphere, viewed as a closed spatial slice of de Sitter. The result is a simple, albeit divergent, infinite product that might serve as a regulator for a more complete treatment of the problem. Additionally, our results suggest deep connections between the problem of computing the norm of the CSK state in quantum gravity and computing the Chern-Simons partition function for a complex group.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Quantum de Sitter and Analytically Continued Chern Simons Theory

    hep-th 2026-08 conditional novelty 6.0 of 10

    Using complexified integration contours called Lefschetz thimbles, the Kodama state becomes a well-defined wavefunction whose leading form is the Hartle-Hawking Airy function times a Gaussian that suppresses anisotropy.

  2. The Cosmological Constant from a Quantum Gravitational $\theta$-Vacua and the Gravitational Hall Effect

    gr-qc 2025-06 conditional novelty 6.0 of 10

    The cosmological constant is related to the topological theta angle by theta = 12 pi^2 / (Lambda l_Pl^2), suggesting Lambda is topologically protected.

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