Wormholes supported by phantom-like modified Chaplygin gas

Abstract

We have examined the possible construction of a stationary, spherically symmetric and spatially inhomogeneous wormhole spacetime supported by the phantom energy. The later is supposed to be represented by the modified Chaplygin gas equation of state. The solutions so obtained satisfy the flare out and the asymptotic flatness conditions. It is also shown that the averaged null energy condition has to be violated for the existence of the wormhole.

14 pages; 6 figs

References in corpus (6)

• Stability of Chaplygin gas thin-shell wormholes
• Constraints on modified Chaplygin gas from recent observations and a comparison of its status with other models
• Astrophysics of Wormholes
• Conformally symmetric traversable wormholes
• Tolman-Oppenheimer-Volkoff equations in presence of the Chaplygin gas: stars and wormhole-like solutions
• Construction of 3D wormhole supported by phantom energy

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• Charged strange star with Krori-Barua potential in $f(R,T)$ gravity admitting Chaplygin equation of state