Barbero's formulation from a BFBF-type action with the Immirzi parameter

preprint2016arXivOpen access

Abstract

Starting from a constrained real BFBF-type action for general relativity that includes both the Immirzi parameter and the cosmological constant, we obtain the Ashtekar-Barbero variables used in the canonical approach to the quantization of the gravitational field. This is accomplished by explicitly solving the second-class constraints resulting from the Hamiltonian analysis of the considered action, and later imposing the time gauge. All throughout this work the tetrad formalism is left aside, obtaining the Ashtekar-Barbero variables entirely in terms of the BB-fields that define the action.

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