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Dyson’s equations for quantum gravity in the hartree–fock approximation

Dyson’s equations for quantum gravity in the hartree–fock approximation
Dyson’s equations for quantum gravity in the hartree–fock approximation
Unlike scalar and gauge field theories in four dimensions, gravity is not perturbatively renormalizable and as a result perturbation theory is badly divergent. Often the method of choice for investigating nonperturbative effects has been the lattice formulation, and in the case of gravity the Regge–Wheeler lattice path integral lends itself well for that purpose. Nevertheless, lattice methods ultimately rely on extensive numerical calculations, leaving a desire for alternate methods that can be pursued analytically. In this work, we outline the Hartree–Fock approximation to quantum gravity, along lines which are analogous to what is done for scalar fields and gauge theories. The starting point is Dyson’s equations, a closed set of integral equations which relate various physical amplitudes involving graviton propagators, vertex functions, and proper self-energies. Such equations are in general difficult to solve, and as a result they are not very useful in practice, but nevertheless provide a basis for subsequent approximations. This is where the Hartree–Fock approximation comes in, whereby lowest order diagrams get partially dressed by the use of fully interacting Green’s function and self-energies, which then lead to a set of self-consistent integral equations. The resulting nonlinear equations for the graviton self-energy show some remarkable features that clearly distinguish it from the scalar and gauge theory cases. Specifically, for quantum gravity one finds a nontrivial ultraviolet fixed point in Newton’s constant G for spacetime dimensions greater than two, and nontrivial scaling dimensions between d=2 and d=4, above which one obtains Gaussian exponents. In addition, the Hartree–Fock approximation gives an explicit analytic expression for the renormalization group running of Newton’s constant, suggesting gravitational antiscreening with Newton’s constant slowly increasing on cosmological scales.
2073-8994
Hamber, Herbert W.
e83c2362-977b-44cf-8cee-102c4242befd
Yu, Lu Heng Sunny
ef5bc4e3-409d-455e-a808-f5da5f3d1416
Hamber, Herbert W.
e83c2362-977b-44cf-8cee-102c4242befd
Yu, Lu Heng Sunny
ef5bc4e3-409d-455e-a808-f5da5f3d1416

Hamber, Herbert W. and Yu, Lu Heng Sunny (2021) Dyson’s equations for quantum gravity in the hartree–fock approximation. Symmetry, 13 (1). (doi:10.3390/sym13010120).

Record type: Article

Abstract

Unlike scalar and gauge field theories in four dimensions, gravity is not perturbatively renormalizable and as a result perturbation theory is badly divergent. Often the method of choice for investigating nonperturbative effects has been the lattice formulation, and in the case of gravity the Regge–Wheeler lattice path integral lends itself well for that purpose. Nevertheless, lattice methods ultimately rely on extensive numerical calculations, leaving a desire for alternate methods that can be pursued analytically. In this work, we outline the Hartree–Fock approximation to quantum gravity, along lines which are analogous to what is done for scalar fields and gauge theories. The starting point is Dyson’s equations, a closed set of integral equations which relate various physical amplitudes involving graviton propagators, vertex functions, and proper self-energies. Such equations are in general difficult to solve, and as a result they are not very useful in practice, but nevertheless provide a basis for subsequent approximations. This is where the Hartree–Fock approximation comes in, whereby lowest order diagrams get partially dressed by the use of fully interacting Green’s function and self-energies, which then lead to a set of self-consistent integral equations. The resulting nonlinear equations for the graviton self-energy show some remarkable features that clearly distinguish it from the scalar and gauge theory cases. Specifically, for quantum gravity one finds a nontrivial ultraviolet fixed point in Newton’s constant G for spacetime dimensions greater than two, and nontrivial scaling dimensions between d=2 and d=4, above which one obtains Gaussian exponents. In addition, the Hartree–Fock approximation gives an explicit analytic expression for the renormalization group running of Newton’s constant, suggesting gravitational antiscreening with Newton’s constant slowly increasing on cosmological scales.

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Accepted/In Press date: 29 December 2020
Published date: 12 January 2021

Identifiers

Local EPrints ID: 468391
URI: http://eprints.soton.ac.uk/id/eprint/468391
ISSN: 2073-8994
PURE UUID: a455990f-ba86-4512-a0d8-b96cffc0c058
ORCID for Lu Heng Sunny Yu: ORCID iD orcid.org/0000-0003-2207-4214

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Date deposited: 12 Aug 2022 18:32
Last modified: 17 Mar 2024 04:09

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Author: Herbert W. Hamber

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