A key challenge for black‑hole computing is extracting results when the event horizon prevents direct readout. In 1974, Stephen Hawking showed that quantum effects cause black holes to emit a faint glow now known as Hawking radiation. This radiation...

second law of thermodynamics strongly disfavors a spontaneous split, as it would represent a decrease in total entropy. Stephen Hawking’s classical area theorem reinforces this, positing that the area of an event horizon cannot decrease over time under...