Remarks on evolution of space-times in 3+1 and 4+1 dimensions
Michael T. Anderson (Stony Brook)

TL;DR
This paper constructs a broad class of vacuum space-times in 4+1 dimensions from hyperboloidal initial data, which are complete, smooth, and extend through their horizons, with implications for 3+1 dimensions via dimensional reduction.
Contribution
It introduces a new method to generate large classes of vacuum space-times in higher dimensions without small perturbation assumptions.
Findings
Space-times are future geodesically complete.
They are smooth up to null infinity.
They extend through their Cauchy horizon.
Abstract
A large class of vacuum space-times is constructed in dimension 4+1 from hyperboloidal initial data sets which are not small perturbations of empty space data. These space-times are future geodesically complete, smooth up to their future null infinity, and extend as vacuum space-times through their Cauchy horizon. Dimensional reduction gives non-vacuum space-times with the same properties in 3+1 dimensions.
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