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The Conformal Constraint in Canonical Quantum Gravity

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arxiv 1011.0061 v1 pith:D6CFURA5 submitted 2010-10-30 gr-qc hep-th

classification gr-qchep-th
keywords quantummattershouldbackgroundbetacanonicalconformalconstraint
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Perturbative canonical quantum gravity is considered, when coupled to a renormalizable model for matter fields. It is proposed that the functional integral over the dilaton field should be disentangled from the other integrations over the metric fields. This should generate a conformally invariant theory as an intermediate result, where the conformal anomalies must be constrained to cancel out. When the residual metric is treated as a background, and if this background is taken to be flat, this leads to a novel constraint: in combination with the dilaton contributions, the matter lagrangian should have a vanishing beta function. The zeros of this beta function are isolated points in the landscape of quantum field theories, and so we arrive at a denumerable, or perhaps even finite, set of quantum theories for matter, where not only the coupling constants, but also the masses and the cosmological constant are all fixed, and computable, in terms of the Planck units.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 40 citations worldwide. Full citation record

  1. Microscopic entropy of de Sitter spacetime and entropic solution to the old cosmological constant problem

    hep-th 2026-06 unverdicted novelty 5.0 of 10

    Requiring the RG flow of the de Sitter entropy parameter α to increase monotonically toward the infrared yields a cosmological constant matching the observed value.

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