We use the formalism of Holographic Space-time (HST) to investigate the claim of  that old black holes contain a firewall, i.e. an in-falling observer encounters highly excited states at a time much shorter than the light crossing time of the Schwarzschild radius. This conclusion is much less dramatic in HST than in the hypothetical models of quantum gravity used in . In HST there is no dramatic change in particle physics inside the horizon until a time of order the Schwarzschild radius.
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