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Energy conditions, traversable wormholes and dust shells

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arxiv gr-qc/0410087 v1 pith:TXZWBEQN submitted 2004-10-18 gr-qc

classification gr-qc
keywords energyconditionswormholejunctionsurfaceaverageddustmatter
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Firstly, we review the pointwise and averaged energy conditions, the quantum inequality and the notion of the ``volume integral quantifier'', which provides a measure of the ``total amount'' of energy condition violating matter. Secondly, we present a specific metric of a spherically symmetric traversable wormhole in the presence of a generic cosmological constant, verifying that the null and the averaged null energy conditions are violated, as was to be expected. Thirdly, a pressureless dust shell is constructed around the interior wormhole spacetime by matching the latter geometry to a unique vacuum exterior solution. In order to further minimize the usage of exotic matter, we then find regions where the surface energy density is positive, thereby satisfying all of the energy conditions at the junction surface. An equation governing the behavior of the radial pressure across the junction surface is also deduced. Lastly, taking advantage of the construction, specific dimensions of the wormhole, namely, the throat radius and the junction interface radius, and estimates of the total traversal time and maximum velocity of an observer journeying through the wormhole, are also found by imposing the traversability conditions.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Linearized stability of T-duality quantum-inspired thin-shell wormholes

    gr-qc 2026-06 unverdicted novelty 6.0 of 10

    Thin-shell wormholes in T-duality quantum-corrected regular spacetimes exhibit an intermediate-radius window of unconditional stability absent in the classical Schwarzschild case.

  2. Thin-shell wormholes in cosmic voids

    gr-qc 2026-07 unverdicted novelty 5.5 of 10

    Thin-shell wormholes can be built inside a cosmic void by gluing two black-hole-in-void spacetimes, and their stability depends sharply on the shell equation of state.

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