New interpretation of variational principles for gauge theories. I. Cyclic coordinate alternative to ADM split
arXiv:0711.0288 · doi:10.1088/0264-9381/25/17/175011
Abstract
I show how there is an ambiguity in how one treats auxiliary variables in gauge theories including general relativity cast as 3 + 1 geometrodynamics. Auxiliary variables may be treated pre-variationally as multiplier coordinates or as the velocities corresponding to cyclic coordinates. The latter treatment works through the physical meaninglessness of auxiliary variables' values applying also to the end points (or end spatial hypersurfaces) of the variation, so that these are free rather than fixed. [This is also known as variation with natural boundary conditions.] Further principles of dynamics workings such as Routhian reduction and the Dirac procedure are shown to have parallel counterparts for this new formalism. One advantage of the new scheme is that the corresponding actions are more manifestly relational. While the electric potential is usually regarded as a multiplier coordinate and Arnowitt, Deser and Misner have regarded the lapse and shift likewise, this paper's scheme considers new {\it flux}, {\it instant} and {\it grid} variables whose corresponding velocities are, respectively, the abovementioned previously used variables. This paper's way of thinking about gauge theory furthermore admits interesting generalizations, which shall be provided in a second paper.
arXiv comment11 pages
References in corpus (35)
- Quasilocal Energy and Conserved Charges Derived from the Gravitational Action
- The Gravitational Hamiltonian, Action, Entropy, and Surface Terms
- A General Definition of "Conserved Quantities" in General Relativity and Other Theories of Gravity
- Geometrodynamics of Schwarzschild Black Holes
- Numerical Relativity and Compact Binaries
- 3+1 Formalism and Bases of Numerical Relativity
- Binary black holes in circular orbits. II. Numerical methods and first results
- Relativity without relativity
- Binary black holes in circular orbits. I. A global spacetime approach
- The physical gravitational degrees of freedom
- Scale-Invariant Gravity: Particle Dynamics
- Black hole evolution by spectral methods
- The Gravitational Hamiltonian in the Presence of Non-Orthogonal Boundaries
- Proof of the Thin Sandwich Conjecture
- Boundary conditions in linearized harmonic gravity
- Constraint-preserving boundary conditions in numerical relativity
- Scale-Invariant Gravity: Geometrodynamics
- Foundations of Relational Particle Dynamics
- Emergent Semiclassical Time in Quantum Gravity. I. Mechanical Models
- The Hamiltonian boundary term and quasi-local energy flux
- The Generalized Thin-Sandwich Problem and its Local Solvability
- Interacting vector fields in Relativity without Relativity
- On the roots of the Poincare structure of asymptotically flat spacetimes
- Strong-coupled Relativity without Relativity
- Variations on the Seventh Route to Relativity
- Triangleland. I. Classical dynamics with exchange of relative angular momentum
- Relational Particle Models. II. Use as toy models for quantum geometrodynamics
- Relational Particle Models. I. Reconciliation with standard classical and quantum theory
- The geometry of the Barbour-Bertotti theories II. The three body problem
- The geometry of the Barbour-Bertotti theories I. The reduction process
- Does relationalism alone control geometrodynamics with sources?
- Geometrodynamics: Spacetime or Space ?
- Relational particle models as toy models for quantum gravity and quantum cosmology
- Triangleland. II. Quantum Mechanics of Pure Shape
- Classical dynamics on triangleland
Cited by in corpus (28)
- Foundations of Relational Particle Dynamics
- Problem of Time and Background Independence: the Individual Facets
- Triangleland. I. Classical dynamics with exchange of relative angular momentum
- Classical Machian Resolution of the Spacetime Reconstruction Problem
- Does relationalism alone control geometrodynamics with sources?
- Approaching the Problem of Time with a Combined Semiclassical-Records-Histories Scheme
- Machian Time Is To Be Abstracted From What Change?
- On the Semiclassical Approach to Quantum Cosmology
- Relational mechanics of shape and scale
- Shape dynamics and Mach's principles: Gravity from conformal geometrodynamics
- TRiPoD (Temporal Relationalism incorporating Principles of Dynamics)
- A Definition of Background Independence
- Minisuperspace model of Machian Resolution of Problem of Time. I. Isotropic Case
- Spaces of Observables from Solving PDEs. I. Translation-Invariant Theory
- A Local Resolution of the Problem of Time. V. Combining Temporal and Configurational Relationalism for Finite Theories
- On the Conceptual Issues Surrounding the Notion of Relational Bohmian Dynamics
- Relational Motivation for Conformal Operator Ordering in Quantum Cosmology
- Quantum Cosmological Metroland Model
- Scaled Triangleland Model of Quantum Cosmology
- Problem of Time: Facets and Machian Strategy
- A Local Resolution of the Problem of Time. XIV. Grounding on Lie's Mathematics
- Shape Quantities for Relational Quadrilateralland
- Shape Space Methods for Quantum Cosmological Triangleland
- Problem of Time: Temporal Relationalism Compatibility of Other Local Classical Facets Completed
- Where to Apply Relationalism
- Quantum Cosmological Relational Model of Shape and Scale in 1-d
- Relational Quadrilateralland Interpretation of CP^2 and Quotients
- Relational Quadrilateralland. II. The Quantum Theory