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 universe itself may be a hologram, with our interior representation being mirrored at the boundary, similar to a black hole's horizon. The holographic principle is a tool in physics that represents information stored on the surface of a black hole rather than in three dimensions, allowing for predictive and mathematical value.

The information paradox arises because if a particle is created just outside a black hole's event horizon, and one falls in while the other escapes, the one that falls in becomes real and cannot return to the vacuum, leading to a loss of information.

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.

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.

In principle, if one could collect all the Hawking radiation from a black hole, it would contain details about the black hole's interior, suggesting that information is not destroyed.

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.

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.