Abstract
We review the covariant canonical formalism initiated by D'Adda, Nelson and Regge in 1985, and extend it to include a definition of form-Poisson brackets (FPB) for geometric theories coupled to $p$-forms, gauging free differential algebras. The form-Legendre transformation and the form-Hamilton equations are derived from a $d$-form Lagrangian with $p$-form dynamical fields $\phi$. Momenta are defined as derivatives of the Lagrangian with respect to the "velocities" $d\phi$ and no preferred time direction is used. Action invariance under infinitesimal form-canonical transformations can be studied in this framework, and a generalized Noether theorem is derived, both for global and local symmetries. We apply the formalism to vielbein gravity in $d=3$ and $d=4$. In the $d=3$ theory we can define form-Dirac brackets, and use an algorithmic procedure to construct the canonical generators for local Lorentz rotations and diffeomorphisms. In $d=4$ the canonical analysis is carried out using FPB, since the definition of form-Dirac brackets is problematic. Lorentz generators are constructed, while diffeomorphisms are generated by the Lie derivative. A "doubly covariant" hamiltonian formalism is presented, allowing to maintain manifest Lorentz covariance at every stage of the Legendre transformation. The idea is to take curvatures as "velocities" in the definition of momenta.
Highlights
Geometric theories like gravity or supergravity are conveniently formulated in the language of differential forms
We review the covariant canonical formalism initiated by D’Adda, Nelson, and Regge in 1985, and extend it to include a definition of form-Poisson brackets (FPBs) for geometric theories coupled to p-forms
In the d 1⁄4 3 theory we can define form-Dirac brackets, and use an algorithmic procedure to construct the canonical generators for local Lorentz rotations and diffeomorphisms
Summary
Geometric theories like gravity or supergravity are conveniently formulated in the language of differential forms. Because the Lagrangian of a d-dimensional theory is written as a d-form, it is invariant by construction under diffeomorphisms (up to a total derivative) This framework is well suited to the case of p-form fields coupled to (super)gravity, and a group-geometric approach has been developed since the late 1970s based on free differential algebras [1,2,3,4,5,6,7,8] The essential ideas appeared in papers by De Donder and Weyl more than 70 years ago [15,16] Some of these approaches are quite similar in spirit to the one we discuss here, but to our knowledge the first proposal of a d-form Hamiltonian, together with its application to gravity, can be found in Ref. Momenta are defined as the derivatives of L with respect to R, and all formulas (e.g., the Hamilton equations of motion) become automatically Lorentz covariant, with derivatives being replaced throughout by covariant derivatives
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