Published November 7, 2010 | Version v1
Journal article

A definition of background independence

Creators

  • 1. Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2 L 3G1 (Canada)

Description

We propose a definition for background (in)/dependence in dynamical theories of the evolution of configurations that have a continuous symmetry and test this definition on particle models and on gravity. Our definition draws from Barbour's best matching framework developed for the purpose of implementing spatial and temporal relationalism. Among other interesting theories, general relativity can be derived within this framework in novel ways. We study the detailed canonical structure of a wide range of best matching theories and show that their actions must have a local gauge symmetry. When gauge theory is derived in this way, we obtain at the same time a conceptual framework for distinguishing between background-dependent and -independent theories. Gauge invariant observables satisfying Kuchar's criterion are identified and, in simple cases, explicitly computed. We propose a procedure for inserting a global background time into temporally relational theories. Interestingly, using this procedure in general relativity leads to unimodular gravity.

Availability note (English)

Available from http://dx.doi.org/10.1088/0264-9381/27/21/215018

Additional details

Identifiers

DOI
10.1088/0264-9381/27/21/215018;
PII
S0264-9381(10)50583-5;

Publishing Information

Journal Title
Classical and Quantum Gravity
Journal Volume
27
Journal Issue
21
Journal Page Range
[23 p.]
ISSN
0264-9381
CODEN
CQGRDG

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42033119
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
COSMOLOGY; GAUGE INVARIANCE; GENERAL RELATIVITY THEORY; GRAVITATION; PARTICLE MODELS; SYMMETRY
Descriptors DEC
FIELD THEORIES; INVARIANCE PRINCIPLES; MATHEMATICAL MODELS; RELATIVITY THEORY