Testing the nonlinear stability of Kerr-Newman black holes

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The nonlinear stability of Kerr-Newman black holes (KNBHs) is investigated by performing numerical simulations within the full Einstein-Maxwell theory. We take as initial data a KNBH with mass M, angular momentum to mass ratio a and charge Q. Evolutions are performed to scan this parameter space within the intervals 0

Original languageEnglish
Article number124088
JournalPhysical Review D
Volume90
Issue number12
Number of pages8
ISSN1550-7998
DOIs
Publication statusPublished - 30 Dec 2014
Externally publishedYes

    Research areas

  • NUMERICAL RELATIVITY, EVOLUTION, FIELDS

ID: 300081160