Action Principle for Isotropic General Relativity

TL;DR

This paper develops a new action principle for isotropic spacetimes in general relativity that fixes physical boundary conditions, leading to a well-posed variational problem and insights into quantum gravity issues.

Contribution

It introduces a boundary condition framework fixing the Schwarzschild-(A)dS metric parameters, ensuring a well-posed variational principle for isotropic spacetimes.

Findings

The action vanishes for stationary isotropic spacetimes.

Each of Schwarzschild black hole and de Sitter space has a unique semiclassical state.

The approach offers new perspectives on quantum gravity problems.

Abstract

We study the generally covariant theory governing an isotropic spacetime region with uniform energy density. Gibbons, Hawking and York showed that fixing the induced boundary metric yields a well-posed variational problem. However, as we demonstrate, fixing the boundary metric violates general covariance and allows the mass of a back hole to vary. This observation has dramatic consequences for path integrals: A sum over spacetimes with fixed boundary metrics is a sum over classically distinct black holes. Instead, we merely demand that coordinates exist such that the metric at the boundary is the Schwarzschild-(A)dS metric of fixed mass M and two-sphere radius R. We derive the action that yields a well-posed variational problem for these physical boundary conditions. The action vanishes for all stationary and isotropic spacetimes. A vanishing action implies that both a Schwarzschild black hole and pure de Sitter space each have one unique semiclassical state. Our results provide a novel and radically conservative approach to several long-standing issues in quantum gravity, such as the wavefunction of the universe, the black hole information paradox, vacuum decay rates and the measure problem of eternal inflation.