Black hole interior from loop quantum gravity

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.

12 pages, 7 figures. Advances in High Energy Physics Volume 2008 (2008), Article ID 459290

References in corpus (4)

• Black hole evaporation: A paradigm
• Loop Quantum Dynamics of the Schwarzschild Interior
• Loop Quantum Gravity: An Inside View
• Gravitational collapse in loop quantum gravity

Cited by in corpus (1)

• Effective Polymer Dynamics of D-Dimensional Black Hole Interiors