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.
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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.