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Free evolution of the hyperboloidal initial value problem in spherical simmetry

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Figure 1.2: Penrose diagram showing the compactification of the Schwarzschild spacetime.
Figure 3.1: Foliations of flat spacetime for different values of the constant trace of the extrinsic curvature K CM C : the leftmost diagram shows maximal slices (Cauchy slices), while the rest show hyperboloidal ones
Figure 3.4: Complete spacetime diagram for the case C CM C = 2, where the slices intersect the white hole horizon.
Figure 3.5: Penrose diagrams showing foliations with M = 1 and critical C CM C for different values of K CM C
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