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arXiv:2605.05239

Quantizing gravitational fields with an entropy-corrected action principle

Jianhao M. Yang

quant-phgr-qcSubmitted May 3, 2026• Announced May 5, 2026
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Abstract

A variational framework for the quantization of gravitational fields is developed based on an extension of the stationary action principle. Within this framework, the Wheeler-DeWitt equation for the gravitational wave functional is recovered without assuming operator promotion of the canonical momentum, thus avoiding the ambiguity of operator ordering in canonical quantization. The derivation is based on three main ingredients. First, motivated by information-theoretic considerations, the classical stationary action principle is generalized by incorporating a correction term constructed from the relative entropy associated with field fluctuations. Second, an ensemble formulation on superspace is enhanced to incorporate this entropy correction. Third, the formalism is further refined to provide a unified treatment of quantization and constraints, thereby addressing the long-standing ambiguity concerning the ordering of quantization and constraint reduction. The framework is then applied to gravitational fields coupled to a massless scalar field. Using an emergent time parameter defined via the rate equation of the gravitational fields, a Schrodinger equation for the scalar-field wave functional is recovered, supplemented by an additional quantum correction term suppressed at order $G\hbar^2$. Finally, we comment on possible connections between the notion of relative entropy employed here and holographic dualities in quantum gravity.

AI Summary

The paper asks whether canonical gravitational quantization can be formulated through an information-corrected variational principle rather than postulated momentum operators. It extends an ensemble-on-configuration-space framework to ADM gravity, assuming intrinsic local random field fluctuations and a minimum observable action scale of $\hbar/2$. The proposed action is $A_t=\langle A_c\rangle+(\hbar/2)I_f$, with $I_f$ constructed from classical Kullback–Leibler divergences. Extremizing the action over an infinitesimal foliation step gives a formal Gaussian fluctuation distribution. Its covariance is then used to turn the accumulated relative entropy into a Fisher-information-type functional. Varying the resulting ensemble action, with diffeomorphism constraints incorporated through Lagrange multipliers, yields continuity and quantum Hamilton–Jacobi equations. Combining them using $\Psi=\sqrt{\rho}e^{iS/\hbar}$ recovers a Wheeler–DeWitt equation with divergence-form kinetic ordering, placing $G_{ijkl}/\sqrt h$ between functional derivatives. Replacing KL divergence by Tsallis divergence of order $\alpha$ rescales the information correction by $\alpha$. For gravity coupled to a massless scalar, a factorization of the wave functional and assumptions of weaker gravitational dependence in the matter factor allow gravitational trajectories to define an emergent clock. The resulting matter Schrödinger equation contains nonlinear classical and quantum gravitational corrections, described as order $G\hbar^2$. Stated limitations include the absence of a microscopic model for the fluctuations and reliance on a classical trajectory-based clock rather than a fully quantum clock. Renormalization, ultraviolet behavior, spacetime emergence, and black-hole information are not resolved. Connections to holographic relative entropy remain speculative.

Little sign of AI-generated textOverclaimsUnclear noveltyStrong assumptionsPossible error

Central claim may not hold: The indefinite DeWitt supermetric makes the proposed gravitational fluctuation Gaussian nonnormalizable and its asserted covariance nonpositive, invalidating the probability identity underlying the entropy correction; its kernel also contradicts the claimed independence from the background metric. The claimed elimination of operator-ordering ambiguity is stronger than established because the derivation fixes a measure and uniform-reference entropy prescription without showing that changing the measure preserves that prescription. The emergent-time derivation discards a mixed quantum-potential contribution without controlling it relative to the corrections retained after the background equation cancels. The classical gravitational correction is proportional to G times squared derivatives of S₁, and its wave-functional rewriting does not establish the claimed ℏ² suppression. The final wave-functional correction formulas have a sign error in Γ_cl and incorrectly replace √ρ₁ by (Ψ₁Ψ₁*)^{1/4} in Γ_q.

Written by gpt-6.1-sol from the paper's full text. Automated: it can be wrong.

Journal reference
Int. J. Theor. Phys. 65 (2026)
DOI
10.1007/s10773-026-06518-8
Comments
22 pages. This paper is related to arXIv:2302.14619, arXiv:2310.02274, arXiv:2503.02362, and arXiv:2509.22747

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A variational framework for the quantization of gravitational fields is developed based on an extension of the stationary action principle. Within this framework, the Wheeler-DeWitt equation for the gravitational wave functional is recovered without assuming operator promotion of the canonical momentum, thus avoiding the ambiguity of operator ordering in canonical quantization. The derivation is based on three main ingredients. First, motivated by information-theoretic considerations, the classical stationary action principle is generalized by incorporating a correction term constructed from the relative entropy associated with field fluctuations. Second, an ensemble formulation on superspace is enhanced to incorporate this entropy correction. Third, the formalism is further refined to provide a unified treatment of quantization and constraints, thereby addressing the long-standing ambiguity concerning the ordering of quantization and constraint reduction. The framework is then applied to gravitational fields coupled to a massless scalar field. Using an emergent time parameter defined via the rate equation of the gravitational fields, a Schrodinger equation for the scalar-field wave functional is recovered, supplemented by an additional quantum correction term suppressed at order Gℏ2G\hbar^2Gℏ2. Finally, we comment on possible connections between the notion of relative entropy employed here and holographic dualities in quantum gravity.
The paper asks whether canonical gravitational quantization can be formulated through an information-corrected variational principle rather than postulated momentum operators. It extends an ensemble-on-configuration-space framework to ADM gravity, assuming intrinsic local random field fluctuations and a minimum observable action scale of ℏ/2\hbar/2ℏ/2. The proposed action is At=⟨Ac⟩+(ℏ/2)IfA_t=\langle A_c\rangle+(\hbar/2)I_fAt​=⟨Ac​⟩+(ℏ/2)If​, with IfI_fIf​ constructed from classical Kullback–Leibler divergences.
Extremizing the action over an infinitesimal foliation step gives a formal Gaussian fluctuation distribution. Its covariance is then used to turn the accumulated relative entropy into a Fisher-information-type functional. Varying the resulting ensemble action, with diffeomorphism constraints incorporated through Lagrange multipliers, yields continuity and quantum Hamilton–Jacobi equations. Combining them using Ψ=ρeiS/ℏ\Psi=\sqrt{\rho}e^{iS/\hbar}Ψ=ρ​eiS/ℏ recovers a Wheeler–DeWitt equation with divergence-form kinetic ordering, placing Gijkl/hG_{ijkl}/\sqrt hGijkl​/h​ between functional derivatives. Replacing KL divergence by Tsallis divergence of order α\alphaα rescales the information correction by α\alphaα.
For gravity coupled to a massless scalar, a factorization of the wave functional and assumptions of weaker gravitational dependence in the matter factor allow gravitational trajectories to define an emergent clock. The resulting matter Schrödinger equation contains nonlinear classical and quantum gravitational corrections, described as order Gℏ2G\hbar^2Gℏ2.
Stated limitations include the absence of a microscopic model for the fluctuations and reliance on a classical trajectory-based clock rather than a fully quantum clock. Renormalization, ultraviolet behavior, spacetime emergence, and black-hole information are not resolved. Connections to holographic relative entropy remain speculative.
Abstract Recently it is shown that the non-relativistic quantum formulations can be derived from an extended least action principle Yang (2023). In this paper, we apply the principle to massive scalar fields, and derive the Schrödinger equation of the wave functional for the scalar fields. The principle extends the least action principle in classical field theory by factoring in two assumptions. First, the Planck constant defines the minimal amount of action a field needs to exhibit in order to be observable. Second, there are constant random field fluctuations. A novel method is introduced to define the information metrics to measure additional observable information due to the field fluctuations, which is then converted to the additional action through the first assumption. Applying the variation principle to minimize the total actions allows us to elegantly derive the transition probability of field fluctuations, the uncertainty relation, and the Schrödinger equation of the wave functional. Furthermore, by defining the information metrics for field fluctuations using general definitions of relative entropy, we obtain a generalized Schrödinger equation of the wave functional that depends on the order of relative entropy. Our results demonstrate that the extended least action principle can be applied to derive both non-relativistic quantum mechanics and relativistic quantum scalar field theory. We expect it can be further used to obtain quantum theory for non-scalar fields.
We present a novel framework for quantizing constrained quantum systems in which the processes of quantization and constraint enforcement are performed simultaneously. The approach is based on an extension of the stationary action principle, incorporating an information-theoretic term arising from vacuum fluctuations. Constraints are included directly in the Lagrangian via Lagrange multipliers, allowing the subsequent variational procedure to yield the quantum dynamics without ambiguity regarding the order of quantization and reduction. We demonstrate the method through two examples: (i) a one-dimensional system with vanishing local momentum, where the simultaneous approach produces the time-independent Schrödinger equation while conventional reduced and Dirac quantization yield only trivial states, and (ii) a bipartite system with global translational invariance, where all three methods agree. These results show that the proposed framework generalizes standard quantization schemes and provides a consistent treatment of systems with constraints that cannot be expressed as linear operators acting on the wave function. In addition to a unified variational principle for constrained quantum systems, the formalism also offers an information-theoretic perspective on quantum effects arising from vacuum fluctuations.
Abstract Tensor networks are used to describe the ground state wavefunction of the quantum many-body system. Recently, it has been shown that a tensor network can generate the anti-de Sitter (AdS) geometry by using the entanglement renormalization approach, which provides a new way to realize bulk reconstruction in the AdS/conformal field theory correspondence. However, whether the dynamical connections can be found between the tensor network and gravity is an important unsolved problem. In this paper, we give a novel proposal to integrate ideas from tensor networks, entanglement entropy, canonical quantization of quantum gravity and the holographic principle and argue that the gravitational dynamics can be generated from a tensor network if the wave function of the latter satisfies the Wheeler–DeWitt equation.
Abstract We show that the formulations of non-relativistic quantum mechanics can be derived from an extended least action principle. The principle can be considered as an extension of the least action principle from classical mechanics by factoring in two assumptions. First, the Planck constant defines the minimal amount of action a physical system needs to exhibit during its dynamics in order to be observable. Second, there is constant vacuum fluctuation along a classical trajectory. A novel method is introduced to define the information metrics to measure additional observability due to vacuum fluctuations, which is then converted to an additional action through the first assumption. Applying the variational principle to minimize the total actions allows us to recover the basic quantum formulations including the uncertainty relation and the Schrödinger equation in the position representation. In the momentum representation, the same method can be applied to obtain the Schrödinger equation for a free particle while further investigation is still needed for a particle with an external potential. Furthermore, the principle brings in new results on two fronts. At the conceptual level, we find that the information metrics for vacuum fluctuations are responsible for the origin of the Bohm quantum potential. Even though the Bohm potential for a bipartite system is inseparable, the underlying vacuum fluctuations are local. Thus, inseparability of the Bohm potential does not justify a non-local causal relation between the two subsystems. At the mathematical level, quantifying the information metrics for vacuum fluctuations using more general definitions of relative entropy results in a generalized Schrödinger equation that depends on the order of relative entropy. The extended least action principle is a new mathematical tool. It can be applied to derive other quantum formalisms such as quantum scalar field theory.
Tensor networks are powerful techniques that widely used in condensed matter physics. In this language, the wave function of a quantum manybody system is described by a network of tensors with specific entanglement structures. Recently, it is shown that tensor network can generate the anti-de Sitter (AdS) geometry by using the entanglement renormalization approach. However, whether the dynamical connections can be found between the tensor network and the gravity is an important unsolved problem. In this paper, we give a novel proposal to integrate ideas from tensor networks, entanglement entropy, canonical quantization of quantum gravity and the holographic principle and argue that the gravitational dynamics can be generated from a tensor network if the wave function of the latter satisfies the Wheeler-DeWitt equation.
Key aspects of the manifestly-covariant theory of quantum gravity (Cremaschini and Tessarotto 2015–2017) are investigated. These refer, first, to the establishment of the four-scalar, manifestly-covariant evolution quantum wave equation, denoted as covariant quantum gravity (CQG) wave equation, which advances the quantum state ψ associated with a prescribed background space-time. In this paper, the CQG-wave equation is proved to follow at once by means of a Hamilton–Jacobi quantization of the classical variational tensor field g ≡ g μ ν and its conjugate momentum, referred to as (canonical) g-quantization. The same equation is also shown to be variational and to follow from a synchronous variational principle identified here with the quantum Hamilton variational principle. The corresponding quantum hydrodynamic equations are then obtained upon introducing the Madelung representation for ψ , which provides an equivalent statistical interpretation of the CQG-wave equation. Finally, the quantum state ψ is proven to fulfill generalized Heisenberg inequalities, relating the statistical measurement errors of quantum observables. These are shown to be represented in terms of the standard deviations of the metric tensor g ≡ g μ ν and its quantum conjugate momentum operator.