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Thermodynamic Stability of a Schwarzschild Thin-Shell Wormhole

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arxiv 1812.04340 v1 pith:5QTBYYJU submitted 2018-12-11 gr-qc

classification gr-qc
keywords schwarzschildstabilitywormholethin-shellfunctionthermodynamicapplicationsbulk
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The thermodynamic stability of a thin-shell wormhole in a Schwarzschild bulk is considered. From the first law, entropy function is found which satisfies the local intrinsic stability conditions. Heat capacity emerges as a well-defined regular function justifying the stability of a Schwarzschild thin-shell wormhole. The scope of applications of the method is not limited by the Schwarzschild wormhole.

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Cited by 1 Pith paper

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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 of 10

    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.

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