The paper sketches a scenario in which evaporating black holes never form a true event horizon, so quasilocal charges can carry information out and prevent information loss.
The energy-momentum tensor of a black hole, or what curves the schwarzschild geometry?Classical and Quantum Gravity, 10(11):2271, 1993
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Dynamical Horizons and Black Hole Soft Hair
The paper sketches a scenario in which evaporating black holes never form a true event horizon, so quasilocal charges can carry information out and prevent information loss.