For Kerr-Newman-de Sitter spacetimes, the energy of test fields should be computed with the Killing field ∂t + (a/l^2)∂φ, and with this definition test fields cannot overcharge or overspin extremal black holes.
Toth, Test of the weak cosmic censorship conjecture with a charged scalar field and dyonic KerrNewman black holes , Gen
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Test fields cannot destroy extremal de Sitter black holes
For Kerr-Newman-de Sitter spacetimes, the energy of test fields should be computed with the Killing field ∂t + (a/l^2)∂φ, and with this definition test fields cannot overcharge or overspin extremal black holes.