Hamiltonian approach to GR - Part 2: covariant theory of quantum gravity
Claudio Cremaschini, Massimo Tessarotto

TL;DR
This paper develops a non-perturbative, covariant quantum gravity theory based on Hamiltonian structures, deriving a quantum wave equation, and exploring its implications for graviton mass and the cosmological constant.
Contribution
It introduces a novel covariant quantum gravity framework using Hamiltonian and Hamilton-Jacobi formalisms, with a new quantum wave equation and perturbative approximation scheme.
Findings
Derivation of a covariant quantum wave equation for gravity.
Identification of conditions for a discrete energy spectrum.
Estimation of graviton mass and quantum origin of the cosmological constant.
Abstract
A non-perturbative quantum field theory of General Relativity is presented which leads to a new realization of the theory of Covariant Quantum-Gravity (CQG-theory). The treatment is founded on the recently-identified Hamiltonian structure associated with the classical space-time, i.e., the corresponding manifestly-covariant Hamilton equations and the related Hamilton-Jacobi theory. The quantum Hamiltonian operator and the CQG-wave equation for the corresponding CQG-state and wave-function are realized in scalar form. The new quantum wave equation is shown to be equivalent to a set of quantum hydrodynamic equations which warrant the consistency with the classical GR Hamilton-Jacobi equation in the semiclassical limit. A perturbative approximation scheme is developed, which permits the adoption of the harmonic oscillator approximation for the treatment of the Hamiltonian potential.…
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