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Chaplygin traversable wormholes

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arxiv gr-qc/0511003 v2 pith:YZWNLCM3 submitted 2005-11-01 gr-qc astro-phhep-th

Chaplygin traversable wormholes

classification gr-qc astro-phhep-th
keywords chaplyginalphaconstantenergywormholewormholesdarkdensity
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The generalized Chaplygin gas (GCG) is a candidate for the unification of dark energy and dark matter, and is parametrized by an exotic equation of state given by $p_{ch}=-A/\rho_{ch}^{\alpha}$, where $A$ is a positive constant and $0<\alpha \leq 1$. In this paper, exact solutions of spherically symmetric traversable wormholes supported by the GCG are found, possibly arising from a density fluctuation in the GCG cosmological background. To be a solution of a wormhole, the GCG equation of state imposes the following generic restriction $A<(8\pi r_0^2)^{-(1+\alpha)}$, where $r_0$ is the wormhole throat radius, consequently violating the null energy condition. The spatial distribution of the exotic GCG is restricted to the throat neighborhood, and the physical properties and characteristics of these Chaplygin wormholes are further analyzed. Four specific solutions are explored in some detail, namely, that of a constant redshift function, a specific choice for the form function, a constant energy density, and finally, isotropic pressure Chaplygin wormhole geometries.

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Forward citations

Cited by 3 Pith papers

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

  1. Thin-shell wormholes in cosmic voids

    gr-qc 2026-07 unverdicted novelty 5.5

    Symmetric thin-shell wormholes in void-embedded black-hole spacetimes can be stable under a modified cosmic Chaplygin gas but are generically unstable under a generalized cosmic Chaplygin gas.

  2. Thin-shell wormholes in cosmic voids

    gr-qc 2026-07 conditional novelty 5.0

    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.

  3. Rotating traversable wormholes and particle dynamics in $f(R,T)$ gravity

    gr-qc 2026-05 unverdicted novelty 5.0

    Rotating traversable wormholes in f(R,T) gravity are supported by anisotropic fluid satisfying null and strong energy conditions in the slow-rotation approximation, with particle dynamics and gravitational lensing analyzed.