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Thin-shell wormholes with a generalized Chaplygin gas in Einstein-Born-Infeld theory

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arxiv 1205.2685 v2 pith:7TYPWITQ submitted 2012-05-11 gr-qc

classification gr-qc
keywords born-infeldparameterchaplyginelectrodynamicsgeneralizedmaxwellstabilitytheory
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We construct spherically symmetric thin-shell wormholes supported by a generalized Chaplygin gas in Born-Infeld electrodynamics coupled to Einstein gravity, and we analyze their stability under radial perturbations. For different values of the Born-Infeld parameter and the charge, we compare the results with those obtained in a previous work for Maxwell electrodynamics. The stability region in the parameter space reduces and then disappears as the value of the Born-Infeld parameter is modified in the sense of a larger departure from Maxwell theory.

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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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