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.

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 debate continues among quantum physicists about whether the universe could be a simulation, particularly in relation to black holes and information theory, especially since the total amount of information in the universe is finite, meaning all possible universes can be summarized in a calculable number.

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.

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 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 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 relationship between black holes and galaxies is complex, with supermassive black holes likely playing a critical role in the formation and evolution of galaxies, possibly influencing their growth through jets of material they emit.

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