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Plane symmetric thin-shell wormholes: solutions and stability

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arxiv 0806.4459 v2 pith:37BFT75L submitted 2008-06-27 gr-qc astro-phhep-th

Plane symmetric thin-shell wormholes: solutions and stability

classification gr-qc astro-phhep-th
keywords wormholesplanesymmetricsolutionsstabilitytopologyanalysisconstant
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Using the cut-and-paste procedure, we construct static and dynamic plane symmetric wormholes by surgically grafting together two spacetimes of plane symmetric vacuum solutions with a negative cosmological constant. These plane symmetric wormholes may be viewed as domain walls connecting different universes, having planar topology, and upon compactification of one or two coordinates, cylindrical topology or toroidal topology, respectively. A stability analysis is carried out for the dynamic case by taking into account specific equations of state, and a linearized stability analysis around static solutions is also explored. It is found that thin shell wormholes made of a dark energy fluid or of a cosmological constant fluid are stable, while thin shell wormholes made of phantom energy are unstable.

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  1. Junction Conditions, Radial Stability, Thermodynamics, Optical Geometry and Appearance of Polymer-Quintessence Thin-Shell Wormholes

    gr-qc 2026-07 conditional novelty 5.0

    Keeping the nonareal polymer angular sector in a polymer-quintessence thin-shell wormhole adds a momentum-flux term that reshapes stability, thermodynamics, and cross-throat image branches.