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Black holes in scale dependent frameworks

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Figure 1.1: The picture shows how the inclusion of scale–dependent couplings extend the classical solution.
Figure 2.1: Radial dependence of the lapse function f (r) for ` 0 = 5, G 0 = 1 and M 0 = 1
Figure 2.2: Apparent black hole horizon r h as a function of M 0 for ` 0 = 5, G 0 = 1 and  = 0.2.
Figure 2.3: Temperature T h as a function of M 0 for ` 0 = 5, G 0 = 1, and  = 0.2. The different curves correspond to the classical case (thin solid red line), the expansion (2.43) for small G/G 0 (dashed green line), the expansion (2.44) for small G/G 0
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