The authors substitute a polynomial mass function into the Kerr metric to build an interior, then check energy conditions; the result is a standard mass-function Kerr solution, not a new derivation.
A powerful local shear instability in weakly magnetized disks: I
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An Interior Solution for the Kerr Metric: A Novel Approach
The authors substitute a polynomial mass function into the Kerr metric to build an interior, then check energy conditions; the result is a standard mass-function Kerr solution, not a new derivation.