Hamiltonian treatment of the gravitational collapse of thin shells

Juan Crisóstomo, Rodrigo Olea

Resultado de la investigación: Article

40 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 originalEnglish
PublicaciónPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volumen69
N.º10
DOI
EstadoPublished - 1 ene 2004

Huella dactilar

gravitational collapse
naked singularities
formalism

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

Citar esto

@article{deac2a49fe4a409998956a86a557a4e7,
title = "Hamiltonian treatment of the gravitational collapse of thin shells",
abstract = "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.",
author = "Juan Cris{\'o}stomo and Rodrigo Olea",
year = "2004",
month = "1",
day = "1",
doi = "10.1103/PhysRevD.69.104023",
language = "English",
volume = "69",
journal = "Physical Review D - Particles, Fields, Gravitation and Cosmology",
issn = "1550-7998",
number = "10",

}

TY - JOUR

T1 - Hamiltonian treatment of the gravitational collapse of thin shells

AU - Crisóstomo, Juan

AU - Olea, Rodrigo

PY - 2004/1/1

Y1 - 2004/1/1

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=3142590881&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.69.104023

DO - 10.1103/PhysRevD.69.104023

M3 - Article

VL - 69

JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

JF - Physical Review D - Particles, Fields, Gravitation and Cosmology

SN - 1550-7998

IS - 10

ER -