Abstract
The concept of fixed-area states has proven useful for recent studies of
quantum gravity, especially in connection with gravitational holography. We
explore the Lorentz-signature spacetime geometry intrinsic to such fixed-area
states in this paper. This contrasts with previous treatments which focused
instead on Euclidean-signature saddles for path integrals that prepare such
states. We analyze general features of fixed-area state geometries and
construct explicit examples. The spacetime metrics are real at real times and
have no conical singularities. With enough symmetry the classical metrics are
in fact smooth, though more generally their curvatures feature power-law
divergences along null congruences launched orthogonally from the fixed-area
surface. While we argue that such divergences are not problematic at the
classical level, quantum fields in fixed-area states feature stronger
divergences. At the quantum level we thus expect fixed-area states to be
well-defined only when the fixed-area surface is appropriately smeared.
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