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Kerr initial data for an isolated rotating black hole is specified
using the ``quasi-isotropic'' coordinates [33]:
The two free parameters are the Kerr mass, ![]() ![]() ![]() ![]() ![]()
The admbase::metric_type parameter can be used to specify
whether the metric should be conformal or not. If the metric is
conformal, then The gauge can be set to the Kerr lapse and shift with the parameters idanalyticbh::initial_lapse = "kerr" idanalyticbh::initial_shift = "kerr"in which case the formulas
where
A set of parameters which initialise an evolution to use the Kerr
intial data with mass ActiveThorns = "... ADMBase StaticConformal IDAnalyticBH ..." admbase::metric_type = "static conformal" admbase::initial_data = "kerr" admbase::initial_lapse = "kerr" admbase::initial_shift = "kerr" idanalyticbh::mass = 1.0 idanalyticbh::a_kerr = 0.3
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