High School GR and closeness to a black hole singularity

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In the context of a Schwarzschild black hole, general relativity accurately describes the behavior of matter and energy near the event horizon, except for Hawking radiation. The exact proximity to the singularity where quantum gravity theories become necessary remains uncertain. Various theories, including firewall, fuzzball, and energetic curtain concepts, suggest significant quantum gravity effects at the horizon. A proposed theory introduces a quantum gravity core that expands as the black hole undergoes evaporation. This ongoing discussion highlights the complexities of merging general relativity with quantum mechanics in extreme gravitational environments.
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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
 
This is an alert about a claim regarding the standard model, that got a burst of attention in the past two weeks. The original paper came out last year: "The electroweak η_W meson" by Gia Dvali, Archil Kobakhidze, Otari Sakhelashvili (2024) The recent follow-up and other responses are "η_W-meson from topological properties of the electroweak vacuum" by Dvali et al "Hiding in Plain Sight, the electroweak η_W" by Giacomo Cacciapaglia, Francesco Sannino, Jessica Turner "Astrophysical...

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