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Black hole interior from loop quantum gravity

Leonardo Modesto
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Abstract

In this paper we calculate modifications to the Schwarzschild solution by using a semiclassical analysis of loop quantum black hole. We obtain a metric inside the event horizon that coincides with the Schwarzschild solution near the horizon but that is substantially different at the Planck scale. In particular we obtain a bounce of the two-sphere for a minimum value of the radius and that it is possible to have another event horizon close to the r=0 point.

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BibTeXRIS

Leonardo Modesto. 2009-05-14. Black hole interior from loop quantum gravity. https://doi.org/10.1155/2008%2F459290

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