de.mpg.escidoc.pubman.appbase.FacesBean
Deutsch
 
Hilfe Wegweiser Impressum Kontakt Einloggen
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT

Freigegeben

Zeitschriftenartikel

The spacetime in the neighborhood of a general isolated black hole

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons20661

Krishnan,  Badri
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Externe Ressourcen
Es sind keine Externen Ressourcen verfügbar
Volltexte (frei zugänglich)

1204.4345
(Preprint), 469KB

CQG_29_20_205006.pdf
(beliebiger Volltext), 361KB

Ergänzendes Material (frei zugänglich)
Es sind keine frei zugänglichen Ergänzenden Materialien verfügbar
Zitation

Krishnan, B. (2012). The spacetime in the neighborhood of a general isolated black hole. Classical and quantum gravity, 29(20): 205006. doi:10.1088/0264-9381/29/20/205006.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-000E-E9AB-8
Zusammenfassung
We construct the spacetime in the vicinity of a general isolated, rotating, charged black hole. The black hole is modeled as a weakly isolated horizon, and we use the characteristic initial value formulation of the Einstein equations with the horizon as an inner boundary. The spacetime metric and other geometric fields are expanded in a power series in a radial coordinate away from the horizon by solving the characteristic field equations in the Newman-Penrose formalism. This is the first in a series of papers which investigate the near horizon geometry and its physical applications using the isolated horizon framework.