Strong coupling expansion for general relativity
arXiv:hep-th/0508246 · doi:10.1142/S0218271806009091
Abstract
Strong coupling expansion is computed for the Einstein equations in vacuum in the Arnowitt-Deser-Misner (ADM) formalism. The series is given by the duality principle in perturbation theory as presented in [M.Frasca, Phys. Rev. A 58, 3439 (1998)]. An example of application is also given for a two-dimensional model of gravity expressed through the Liouville equation showing that the expansion is not trivial and consistent with the exact solution, in agreement with the general analysis. Application to the Einstein equations in vacuum in the ADM formalism shows that the spacetime near singularities is driven by space homogeneous equations.
13 pages, no figures. Final version accepted for publication in International Journal of Modern Physics D
References in corpus (2)
Cited by in corpus (16)
- Mapping a Massless Scalar Field Theory on a Yang-Mills Theory: Classical Case
- Green Function Method for Nonlinear Systems
- Green functions and nonlinear systems: Short time expansion
- Mass Gap in Infinite Derivative Non-local Higgs: Dyson-Schwinger Approach
- Proof of triviality of theory
- Dual perturbation expansion for a classical field theory
- Quintessence Dark Energy from strongly-coupled Higgs mass gap: Local and Non-local higher-derivative non-perturbative scenarios
- Infrared analysis of quantum field theories
- Glueball spectrum and hadronic processes in low-energy QCD
- Some exact Green function solutions for non-linear classical field theories
- Dynamical generation of electroweak scale from the conformal sector: A strongly coupled Higgs via the Dyson--Schwinger approach
- Dual Lindstedt series and KAM theorem
- Warping effects in strongly perturbed metrics
- Mass gap in non-perturbative quadratic gravity via Dyson-Schwinger
- Non-perturbative Origin of the Electroweak Scale: RGE in Strongly-coupled Dark Gauge Theories via Dyson-Schwinger
- Non-perturbative Origin of Electroweak Scale via Higgs-portal: Dyson-Schwinger in Conformally Invariant Scalar Sector