Abstract
Starting from the space of Lorentzian metrics, we examine the full gravitational path
integral in 3 and 4 space-time dimensions. Inspired by recent results obtained in a
regularized, dynamically triangulated formulation of Lorentzian gravity, we gaugefix
to proper-time coordinates and perform a non-perturbative “Wick rotation” on
the physical configuration space. Under certain assumptions about
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