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Linking the ADM formulation to other Hamiltonian formulations of general relativity

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arxiv 2302.12273 v1 pith:5F56LS7Y submitted 2023-02-23 gr-qc hep-thmath-phmath.MP

classification gr-qchep-thmath-phmath.MP
keywords formulationhamiltoniangeneralrelativityarnowitt-deser-misnerformulationsgaugevariables
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abstract

We obtain the Arnowitt-Deser-Misner formulation of general relativity in $n$ dimensions ($n \geq 3$) from its either $SO(n-1,1)$ [$SO(n)$] or $SO(n-1)$ Palatini Hamiltonian formulations and vice versa [we recall that $SO(n-1,1)$ [$SO(n)$] requires no gauge fixing whereas $SO(n-1)$ involves the time gauge]. Similarly, the Hamiltonian formulation of general relativity in terms of Ashtekar-Barbero variables can also be directly obtained from the Arnowitt-Deser-Misner Hamiltonian formulation and vice versa, which is an alternative approach to the way followed by Barbero. We give the relevant maps among the phase-space variables and relate the corresponding symplectic structures and the first-class constraints.

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  1. Generators of Local Lorentz Transformation in ADM-Vielbein Formalism of Gravitational Relativity

    gr-qc 2024-11 conditional novelty 6.0 of 10

    In the tetrad (ADM-vielbein) form of general relativity, the authors build first-class constraints that generate the full local Lorentz group (rotations plus boosts) and verify the Lorentz algebra, but only for N=1, Ni=0.

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