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

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.

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 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.

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.

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

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.

Quantum entanglement is a key property that allows information to be stored in the correlations between parts of a quantum system, making it difficult to access that information by examining individual parts.