Constraints on Wormhole Geometries

Physics

Scientific paper

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Scientific paper

A bound on negative energy densities in four-dimensional Minkowski spacetime was recently derived by Roman and Ford from quantum field theory. These quantum inequality restrictions constrain the magnitude and duration of the energy density seen by a timelike geodesic observer. The bound was applied to the stress-energy tensor of static traversable wormhole spacetimes, on a scale in which a local region of spacetime can be considered flat. The results imply that the existence of macroscopic traversable wormholes is very improbable. We analyse and discuss these results.

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