Volume 61, Number 1, January 2003
|Page(s)||15 - 19|
|Published online||01 January 2003|
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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.