English

Topological parameters in gravity

General Relativity and Quantum Cosmology 2012-01-24 v2 High Energy Physics - Theory

Abstract

We present the Hamiltonian analysis of the theory of gravity based on a Lagrangian density containing Hilbert-Palatini term along with three topological densities, Nieh-Yan, Pontryagin and Euler. The addition of these topological terms modifies the symplectic structure non-trivially. The resulting canonical theory develops a dependence on three parameters which are coefficients of these terms. In the time gauge, we obtain a real SU (2) gauge theoretic description with a set of seven first class constraints corresponding to three SU (2) rotations, three spatial diffeomorphism and one to evolution in a timelike direction. Inverse of the coefficient of Nieh-Yan term, identified as Barbero-Immirzi parameter, acts as the coupling constant of the gauge theory.

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Cite

@article{arxiv.1106.3027,
  title  = {Topological parameters in gravity},
  author = {Romesh K. Kaul and Sandipan Sengupta},
  journal= {arXiv preprint arXiv:1106.3027},
  year   = {2012}
}

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R2 v1 2026-06-21T18:22:56.276Z