Black Hole Interior from Loop Quantum Gravity

Figure 4

Plot of 𝑌²(𝑡) for 𝑚=10 and 𝛾𝛿∼1 (in the horizontal axis, we have the temporal coordinate 𝑡; in the vertical axis, we have 𝑌²(𝑡)). The red trajectory corresponds to the classical Schwarzschild solution, and the green trajectory corresponds to the semiclassical solution.