GR and closeness to a black hole singularity

In summary, a black hole singularity is an infinitely dense and small point in space surrounded by the event horizon, which is the point of no return for anything entering a black hole. General relativity explains that the strong gravitational pull of a black hole warps space-time, causing extreme forces near the singularity. The event horizon, directly related to the singularity, is the boundary where nothing can escape the black hole's gravitational pull. It is highly unlikely that anything could survive a journey through a black hole singularity due to the intense forces, although some theories suggest certain particles may pass through unharmed. Getting too close to a black hole singularity would result in catastrophic consequences, including extreme time dilation and being torn apart by tidal forces
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Randy Subers
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GR and closeness to a black hold singularity
Assume a Schwarzschild black hole. Near the event horizon other than Hawking radiation the behavior of matter and energy are fairly accuratly described by general relativity. How close can one get to the center (the singularity based on GR) before one must switch to a quantum gravity theory to provide accurate predictions?
 
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Nobody knows for sure. According to some theories (firewall, fuzzball, energetic curtain), quantum gravity has dramatic consequences already at the horizon. I have proposed a theory in which there is a quantum gravity core which grows as black hole shrinks due to evaporation: https://arxiv.org/abs/1505.04088
 
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