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Thin-shell wormholes: Linearization stability

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arxiv gr-qc/9506083 v1 pith:STKG5QIK submitted 1995-06-30 gr-qc

Eric Poisson , Matt Visser (Washington University) This is my paper · ORCID
classification gr-qc
keywords wormholeslinearizedstabilitythin-shellaroundassumedclasscollection
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The class of spherically-symmetric thin-shell wormholes provides a particularly elegant collection of exemplars for the study of traversable Lorentzian wormholes. In the present paper we consider linearized (spherically symmetric) perturbations around some assumed static solution of the Einstein field equations. This permits us to relate stability issues to the (linearized) equation of state of the exotic matter which is located at the wormhole throat.

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Cited by 7 Pith papers

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

  1. Steering a warp drive without exotic matter

    gr-qc 2026-06 unverdicted novelty 7.0 of 10

    A positive-energy steerable warp drive is constructed by matching the Kinnersley photon rocket to a flat passenger worldtube, with acceleration controlled by Bondi mass loss obeying a closed-form law.

  2. Generalized Unruh temperature for dynamical thin-shell wormholes

    gr-qc 2026-07 accept novelty 6.0 of 10

    For dynamical thin-shell wormholes with asymptotically exponential null-ray maps, the averaged shell acceleration temperature equals the effective particle-creation temperature (generalized Unruh identity).

  3. 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.

  4. Thermodynamics of thin-shell wormholes

    gr-qc 2026-06 unverdicted novelty 5.0 of 10

    The paper derives a generalized first law for thin-shell wormholes showing entropy conservation for isolated transparent shells and flux-dependent entropy change when bulk matter crosses the throat.

  5. Static Dark Fluid Thin Shells in Schwarzschild-de Sitter Spacetimes: Stability and Black Hole Shadows

    gr-qc 2026-02 conditional novelty 5.0 of 10

    Stable static dark-fluid shells separating two Schwarzschild–de Sitter spacetimes exist only for m_+/m_->1 and arise at three scales, imprinting observable black-hole shadow deviations.

  6. Slowly rotating traversable wormholes supported by radially varying string-fluid matter: From regular geometries to photon trajectories

    gr-qc 2026-06 unverdicted novelty 4.0 of 10

    Derives regular, horizon-free, asymptotically flat spacetimes for slowly rotating wormholes supported by radially varying string fluids and analyzes photon trajectories and circular orbits.

  7. Correspondence between quasinormal modes and grey-body factors of spherically symmetric traversable wormholes

    gr-qc 2024-12 conditional novelty 4.0 of 10

    For three families of traversable wormholes, the authors verify that the WKB correspondence between quasinormal modes and grey-body factors, known for black holes, holds to second order beyond the eikonal limit.

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