English

Non-Local Boundary Conditions in Euclidean Quantum Gravity

General Relativity and Quantum Cosmology 2009-10-31 v2

Abstract

Non-local boundary conditions for Euclidean quantum gravity are proposed, consisting of an integro-differential boundary operator acting on metric perturbations. In this case, the operator P on metric perturbations is of Laplace type, subject to non-local boundary conditions; by contrast, its adjoint is the sum of a Laplacian and of a singular Green operator, subject to local boundary conditions. Self-adjointness of the boundary-value problem is correctly formulated by looking at Dirichlet-type and Neumann-type realizations of the operator P, following recent results in the literature. The set of non-local boundary conditions for perturbative modes of the gravitational field is written in general form on the Euclidean four-ball. For a particular choice of the non-local boundary operator, explicit formulae for the boundary-value problem are obtained in terms of a finite number of unknown functions, but subject to some consistency conditions. Among the related issues, the problem arises of whether non-local symmetries exist in Euclidean quantum gravity.

Keywords

Cite

@article{arxiv.gr-qc/9806057,
  title  = {Non-Local Boundary Conditions in Euclidean Quantum Gravity},
  author = {Giampiero Esposito},
  journal= {arXiv preprint arXiv:gr-qc/9806057},
  year   = {2009}
}

Comments

23 pages, plain Tex. The revised version is much longer, and new original calculations are presented in section 4