The information that falls into a black hole is stored on its horizon in a way that cannot be easily reconstructed, resembling a hologram rather than a photograph.

The holographic principle suggests that the information falling into a black hole can be thought of as both falling in and being stored on its horizon.

The resolution to the information paradox may involve allowing non-local connections between particles through wormholes while preserving quantum mechanics, suggesting that gravity emerges from a quantum description and isn't fundamental but rather a result of deeper quantum mechanics.

The event horizon of a black hole is a boundary beyond which nothing can escape, not even light. It's a point in spacetime that separates events that can affect an outside observer from those that cannot.

Inside the event horizon, the nature of space and time changes dramatically. As an object falls into a black hole, it experiences time differently, with their future leading them inevitably to the singularity, which is a point in time rather than space from their perspective.

The black hole's interior might be quantum entangled with Hawking radiation outside, allowing for information retrieval without physically moving it from inside to outside.

When observing Hawking radiation, one can notice entanglement between the radiation and the interior of a black hole, indicating that information is not lost.

Almost all the information in the universe is in the form of black holes; they contain significantly more information than anything else.

To reconstruct the information from a black hole's horizon, one would need to shine the right kind of light on it, similar to how a hologram works, but this process is not straightforward and requires advanced technology.