In this paper we discuss canonical analysis of SO(4,1) constrained BF theory.
The action of this theory contains topological terms appended by a term that
breaks the gauge symmetry down to the Lorentz subgroup SO(3,1). The equations
of motion of this theory turn out to be the vacuum Einstein equations. By
solving the B field equations one finds that the action of this theory contains
not only the standard Einstein-Cartan term, but also the Holst term
proportional to the inverse of the Immirzi parameter, as well as a combination
of topological invariants. We show that the structure of the constraints of a
SO(4,1) constrained BF theory is exactly that of gravity in Holst formulation.
We also briefly discuss quantization of the theory.
Description
[1003.2412] Hamiltonian analysis of SO(4,1) constrained BF theory
%0 Journal Article
%1 durkaKowalski2010
%A Durka, R.
%A Kowalski-Glikman, J.
%D 2010
%K BFthory lorentzian spinfoam
%T Hamiltonian analysis of SO(4,1) constrained BF theory
%U http://arxiv.org/abs/1003.2412
%X In this paper we discuss canonical analysis of SO(4,1) constrained BF theory.
The action of this theory contains topological terms appended by a term that
breaks the gauge symmetry down to the Lorentz subgroup SO(3,1). The equations
of motion of this theory turn out to be the vacuum Einstein equations. By
solving the B field equations one finds that the action of this theory contains
not only the standard Einstein-Cartan term, but also the Holst term
proportional to the inverse of the Immirzi parameter, as well as a combination
of topological invariants. We show that the structure of the constraints of a
SO(4,1) constrained BF theory is exactly that of gravity in Holst formulation.
We also briefly discuss quantization of the theory.
@article{durkaKowalski2010,
abstract = { In this paper we discuss canonical analysis of SO(4,1) constrained BF theory.
The action of this theory contains topological terms appended by a term that
breaks the gauge symmetry down to the Lorentz subgroup SO(3,1). The equations
of motion of this theory turn out to be the vacuum Einstein equations. By
solving the B field equations one finds that the action of this theory contains
not only the standard Einstein-Cartan term, but also the Holst term
proportional to the inverse of the Immirzi parameter, as well as a combination
of topological invariants. We show that the structure of the constraints of a
SO(4,1) constrained BF theory is exactly that of gravity in Holst formulation.
We also briefly discuss quantization of the theory.
},
added-at = {2010-03-13T02:06:18.000+0100},
author = {Durka, R. and Kowalski-Glikman, J.},
biburl = {https://www.bibsonomy.org/bibtex/2d605d5d2e5362d5b0159b26e612732d1/random3f},
description = {[1003.2412] Hamiltonian analysis of SO(4,1) constrained BF theory},
interhash = {087b975c7f5b89cb25947ec84fe5e488},
intrahash = {d605d5d2e5362d5b0159b26e612732d1},
keywords = {BFthory lorentzian spinfoam},
note = {cite arxiv:1003.2412
Comment: 9 pages},
timestamp = {2010-03-13T02:06:19.000+0100},
title = {Hamiltonian analysis of SO(4,1) constrained BF theory},
url = {http://arxiv.org/abs/1003.2412},
year = 2010
}