Hamiltonian treatment of the gravitational collapse of thin shells

Juan Crisóstomo, Rodrigo Olea

Resultado de la investigación: Contribución a una revistaArtículo

47 Citas (Scopus)

Resumen

A Hamiltonian treatment of the gravitational collapse of thin shells is presented. The direct integration of the canonical constraints reproduces the standard shell dynamics for a number of known cases. The formalism is applied in detail to three-dimensional spacetime and the properties of the [Formula Presented]-dimensional charged black hole collapse are further elucidated. The procedure is also extended to deal with rotating solutions in three dimensions. The general form of the equations providing the shell dynamics implies the stability of black holes, as they cannot be converted into naked singularities by any shell collapse process.

Idioma originalInglés
PublicaciónPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volumen69
N.º10
DOI
EstadoPublicada - 1 ene 2004

Áreas temáticas de ASJC Scopus

  • Física nuclear y de alta energía
  • Física y astronomía (miscelánea)

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