Equivalent theories redefine Hamiltonian observables to exhibit change in general relativity

DOI10.1088/1361-6382/AA5CE8zbMath1368.83066arXiv1609.04812OpenAlexW2521432158MaRDI QIDQ5348149

J. Brian Pitts

Publication date: 14 August 2017

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1609.04812

zbMATH Keywords

observablesconversionmassive gravityconstrained Hamiltonian dynamicsproblem of timecanonical quantum theoryDirac-Bergmann

Mathematics Subject Classification ID

Quantum field theory on curved space or space-time backgrounds (81T20) Quantization of the gravitational field (83C45) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40)

Related Items (5)

Reassessing the problem of time of quantum gravity ⋮ Equivalent theories and changing Hamiltonian observables in general relativity ⋮ What are observables in Hamiltonian Einstein-Maxwell theory? ⋮ Change in Hamiltonian general relativity with spinors ⋮ Quantum properties of affine-metric gravity with the cosmological term

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