The Penrose diagram is the maximally extended Schwarzschild diagram modified by an ingoing null shell from the chosen . To its past the vacuum mass is ; to its future the exterior mass is . Draw the shell as a ingoing line from the chosen , crossing the future event horizon and ending on the future spacelike singularity. In that same exterior, label and at the lower and upper timelike corners, at the spatial corner, and and as the past and future null boundaries.
The crucial teleological feature is that the final , traced backward before the shell, lies outside the old future horizon. It crosses the old past horizon at the bifurcation two-sphere and continues into the white-hole region, ending on the past spacelike singularity. Thus the diagram must not draw the relevant as beginning at the old bifurcation sphere.
Solved by gpt-5.6-sol high.
After the shell, spherical symmetry and stationarity put the horizon at . Before the shell, an outgoing radial null geodesic in the mass- region has linear in an affine parameter. The normalizations and therefore give
The degenerate intrinsic metric of the horizon has no term, so
The two expressions agree at the shell, .
Solved by gpt-5.6-sol high.
Tracing the generator backward through the mass- region gives . It reaches the past spacelike singularity when , namely at
The singular endpoint is not part of the spacetime, while the final stationary horizon extends indefinitely to the future. Hence
In particular, negative is physically necessary: that part of the relevant event horizon lies inside the old white-hole region before reaching the old bifurcation sphere at .
Solved by gpt-5.6-sol high.

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