The Hamiltonian constraint in the teleparallel equivalent of general relativity

DOI10.1007/BF02109526zbMath0867.58033OpenAlexW2003099295MaRDI QIDQ674855

José W. Maluf

Publication date: 6 March 1997

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf02109526

zbMATH Keywords

Schrödinger equationquantizationgeneral relativityHamiltonian constraintspherically symmetric geometry

Mathematics Subject Classification ID

Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other equations of quantum mechanics (81Q05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Geometric quantization (53D50)

Related Items (8)

Self-dual teleparallel formulation of general relativity and the positive energy theorem ⋮ Noether symmetries and quantum cosmology in extended teleparallel gravity ⋮ A geometric view on local Lorentz transformations in teleparallel gravity ⋮ Anisotropic stellar solutions in torsion-trace gravity under Karmarkar condition ⋮ ADM-like Hamiltonian formulation of gravity in the teleparallel geometry ⋮ The gravitation energy–momentum pseudotensor: The cases of F(R) and F(T) gravity ⋮ General regular charged space-times in teleparallel equivalent of general relativity ⋮ Sparling two-forms, the conformal factor and the gravitational energy density of the teleparallel equivalent of general relativity

Cites Work

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• A BRST-like operator for space with zero curvature but non-zero torsion tensor
• Role of surface integrals in the Hamiltonian formulation of general relativity
• Ashtekar's complex variables in general relativity and its teleparallelism equivalent
• Spherically symmetric gravity as a completely integrable system.
• The energy problem in Einstein's theory of gravitation (Dedicated to the memory of V. A. Fock)
• Canonical approach to quantum gravity
• Hamiltonian formulation of the teleparallel description of general relativity

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