Lovelock Thin-Shell Wormholes

Abstract

We construct the asymptotically flat charged thin-shell wormholes of Lovelock gravity in seven dimensions by cut-and-paste technique, and apply the generalized junction conditions in order to calculate the energy-momentum tensor of these wormholes on the shell. We find that for negative second order and positive third order Lovelock coefficients, there are thin-shell wormholes that respect the weak energy condition. In this case, the amount of normal matter decreases as the third order Lovelock coefficient increases. For positive second and third order Lovelock coefficients, the weak energy condition is violated and the amount of exotic matter decreases as the charge increases. Finally, we perform a linear stability analysis against a symmetry preserving perturbation, and find that the wormholes are stable provided the derivative of surface pressure density with respect to surface energy density is negative and the throat radius is chosen suitable.

13 pages, 6 figures

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• Holographic dark energy satisfying the energy conditions in Lovelock gravity
• Thin-shell Wormholes with Ordinary Matter in Pure Gauss-Bonnet Gravity
• Higher Dimensional Particle Model in Third-Order Lovelock Gravity
• Thin-shell wormholes in Einstein and Einstein-Gauss-Bonnet theories of gravity