The Liouville solution in GR with scalar field and exponential potential describes spherically symmetric black hole formation with the horizon expanding at light speed from infinitesimal size at finite time, and mass proportional to time squared.
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Black hole formation by a scalar field
The Liouville solution in GR with scalar field and exponential potential describes spherically symmetric black hole formation with the horizon expanding at light speed from infinitesimal size at finite time, and mass proportional to time squared.