In Finsler-Randers gravity, the Reissner-Nordström and Kerr metrics gain an extra vector field that changes massive particle orbits but leaves photon paths untouched, though the Kerr solution is incomplete.
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Reissner-Nordstr\"om and Kerr-like solutions in Finsler-Randers Gravity
In Finsler-Randers gravity, the Reissner-Nordström and Kerr metrics gain an extra vector field that changes massive particle orbits but leaves photon paths untouched, though the Kerr solution is incomplete.