Using the Pappas neutron star metric in general relativistic hydrodynamics and electrodynamics simulations shows that near-surface energy and momentum densities differ from Kerr by tens of percent, while electric fields differ by about 10 percent.
Heusler,Black hole uniqueness theorems, transferred to digital print ed., Cambridge lecture notes in physics No
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Hydrodynamic and Electromagnetic Discrepancies between Neutron Star and Black Hole Spacetimes
Using the Pappas neutron star metric in general relativistic hydrodynamics and electrodynamics simulations shows that near-surface energy and momentum densities differ from Kerr by tens of percent, while electric fields differ by about 10 percent.