Lagrangian approach to the physical degree of freedom count
arXiv:1406.1156 · doi:10.1063/1.4903183
Abstract
In this paper we present a Lagrangian method that allows the physical degree of freedom count for any Lagrangian system without having to perform neither Dirac nor covariant canonical analyses. The essence of our method is to establish a map between the relevant Lagrangian parameters of the current approach and the Hamiltonian parameters that enter in the formula for the counting of the physical degrees of freedom as is given in Dirac's method. Once the map is obtained, the usual Hamiltonian formula for the counting can be expressed in terms of Lagrangian parameters only and therefore we can remain in the Lagrangian side without having to go to the Hamiltonian one. Using the map it is also possible to count the number of first and second-class constraints within the Lagrangian formalism only. For the sake of completeness, the geometric structure underlying the current approach--developed for systems with a finite number of degrees of freedom--is uncovered with the help of the covariant canonical formalism. Finally, the method is illustrated in several examples, including the relativistic free particle.
LaTeX file, no figures
References in corpus (2)
Cited by in corpus (10)
- The effective field theory approach to the strong coupling issue in gravity
- Lagrangian approach to the physical degree of freedom count
- A Lagrangian constraint analysis of first order classical field theories with an application to gravity
- Spatially covariant gravity with two degrees of freedom: perturbative analysis
- Foundations of ghost stability
- Hamiltonian Gotay-Nester-Hinds analysis of the parametrized unimodular extension of the Holst action
- Constraint characterization and degree of freedom counting in Lagrangian field theory
- Bianchi IX cosmologies in the Einstein-Skyrme system in a sector with non-trivial topological charge
- Gravity: Background Dependence and Propagating Degrees of Freedom
- Combining Symmetries and Helmholtz's Conditions to Construct Lagrangians