Following the general method discussed by us earlier, Liouville gravity and the two-dimensional model of non-Einsteinian gravity L approximately curv^2 + torsion^2+cosm const can be formulated as ISO (1,1) gauge theories. In the first order formalism the models present, besides the Poincare gauge symmetry, additional local symmetries, the K-symmetries. These, related to general coordinate transformations on-shell, have canonical generators Ja satisfying a complicated constraint algebra. One can replace the Ja by means of a simple Dirac procedure, with constraints satisfying an Abelian algebra but still generating the K-symmetry. This can be done without altering the symmetry content and the equations of motion of the models. One then remarkably simplifies the canonical structure, as the constraints now satisfy only the ISO (1, 1) algebra plus an Abelian algebra. Moreover, one shows that the Poincare group can always be used consistently as a gauge group for gravitational theories in two dimensions.

Canonical analysis of Poincare gauge theories for two-dimensional gravity

GRIGNANI, Gianluca;
1993

Abstract

Following the general method discussed by us earlier, Liouville gravity and the two-dimensional model of non-Einsteinian gravity L approximately curv^2 + torsion^2+cosm const can be formulated as ISO (1,1) gauge theories. In the first order formalism the models present, besides the Poincare gauge symmetry, additional local symmetries, the K-symmetries. These, related to general coordinate transformations on-shell, have canonical generators Ja satisfying a complicated constraint algebra. One can replace the Ja by means of a simple Dirac procedure, with constraints satisfying an Abelian algebra but still generating the K-symmetry. This can be done without altering the symmetry content and the equations of motion of the models. One then remarkably simplifies the canonical structure, as the constraints now satisfy only the ISO (1, 1) algebra plus an Abelian algebra. Moreover, one shows that the Poincare group can always be used consistently as a gauge group for gravitational theories in two dimensions.
1993
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11391/109133
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