We calculate modifications to the Schwarzschild solution by using a semiclassicalanalysis of loop quantum black hole. We obtain a metric inside the event horizon that coincideswith the Schwarzschild solution near the horizon but that is substantially different at the Planckscale. In particular, we obtain a bounce of theS2sphere for a minimum value of the radius andthat it is possible to have another event horizon close to ther=0point.
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