An effective Hamiltonian for 2D-black-hole physics
Departamento de Física, Universidade Federal
do Paraná c.p. 19091, cep 81531.990, Curitiba-PR, Brazil
Corresponding author: email@example.com
Accepted: 17 October 2002
In another application of the methods of Henneaux, Teitelboim and Vergara developed for diffeomorphisms invariant models, the CGHS theory of 2D black holes is focused in order to obtain the true degrees of freedom, the simplectic structure and the effective Hamiltonian that rules the dynamics in reduced phase-space.
PACS: 04.20.-q – Classical general relativity / 04.60.Kz – Lower dimensional models; minisuperspace models
© EDP Sciences, 2003