I'm thinking equivalence principle, possibilities of unbounded space-time curvature, quantum gravity.
Answer
The spit horizon in a Rindler wedge occurs at a distance d = c2/g for the acceleration g. In spatial coordinates this particle horizon occurs at the distance d behind the accelerated frame. Clearly if d = 0 the acceleration is infinite, or better put indefinite or divergent. However, we can think of this as approximating the near horizon frame of an accelerated observer above a black hole. The closest one can get without hitting the horizon is within a Planck unit of length. So the acceleration required for d = ℓp = √Gℏ/c2 is g = c2/ℓp which gives g = 5.6×1053cm/s2. That is absolutely enormous. The general rule is that Unruh radiation has about 1K for each 1021cm/s2 of acceleration. So this accelerated frame would detect an Unruh radiation at ∼ 1031K. This is about an order of magnitude larger than the Hagedorn temperature. We should then use the string length instead of the Planck length 4π√α′ and the maximum acceleration will correspond to the Hagedorn temperature.
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