English

Chaplygin traversable wormholes

General Relativity and Quantum Cosmology 2009-11-11 v2 Astrophysics High Energy Physics - Theory

Abstract

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 pch=A/ρchαp_{ch}=-A/\rho_{ch}^{\alpha}, where AA is a positive constant and 0<α10<\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<(8πr02)(1+α)A<(8\pi r_0^2)^{-(1+\alpha)}, where r0r_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.

Keywords

Cite

@article{arxiv.gr-qc/0511003,
  title  = {Chaplygin traversable wormholes},
  author = {Francisco S. N. Lobo},
  journal= {arXiv preprint arXiv:gr-qc/0511003},
  year   = {2009}
}

Comments

9 pages, 2 figures, Revtex4. V2: Considerable comments and references added, now 10 pages