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

OriginalsprogEngelsk
Artikelnummer124088
TidsskriftPhysical Review D
Vol/bind90
Udgave nummer12
Antal sider8
ISSN1550-7998
DOI
StatusUdgivet - 30 dec. 2014
Eksternt udgivetJa

ID: 300081160