Charged rotating black hole formation from thin shell collapse in three dimensions

Resultado de la investigación: Contribución a una revistaArtículo

9 Citas (Scopus)


The thin shell collapse leading to the formation of charged rotating black holes in three dimensions is analyzed in the light of a recently developed Hamiltonian formalism for these systems. It is proposed to demand, as a way to reconcile the properties of an infinitely extended solenoid in flat space with a magnetic black hole in three dimensions, that the magnetic field should vanish just outside the shell. The adoption of this boundary condition results in an exterior solution with a magnetic field different from zero at a finite distance from the shell. The interior solution is also found and assigns another interpretation, in a different context, to the magnetic solution previously obtained by Clément and Hirschmann and Welch.

Idioma originalInglés
Páginas (desde-hasta)2649-2665
Número de páginas17
PublicaciónModern Physics Letters A
EstadoPublicada - 10 nov 2005

Áreas temáticas de ASJC Scopus

  • Física nuclear y de alta energía
  • Astronomía y astrofísica

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