structural:expansion, quality:corruption
GISR mechanism resolution to the paradox

Since the Hamiltonian of GISR is explicitly Hermitian, the first increasing then decreasing feature feature of the resultant entropy is naturally obtained. What the calculation tells us is that, the intermediate state of an evaporating black hole cannot be considered a semiclassical object with a time-dependent mass. Instead, it should be viewed as a superposition of many different mass ratio combinations of partially radiated black holes and Hawking particles. References designed a Schrödinger cat-type thought experiment to illustrate this fact, where an initial black hole is bind with a group of living cats and each Hawking particle kills one from the group. In a quantum description, because the time and number of hawking particles being radiated cannot be determined definitively, the intermediate state of an evaporating black hole can only be considered a superposition of many cat groups, each with a different ratio of dead members. The most significant flaw in the argument for information loss is the neglect of this superposition.