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Higher-dimensional thin-shell wormholes in third-order Lovelock gravity

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arxiv 1506.03427 v2 pith:4O37DYGK submitted 2015-06-10 gr-qc astro-ph.HEhep-th

Higher-dimensional thin-shell wormholes in third-order Lovelock gravity

classification gr-qc astro-ph.HEhep-th
keywords lovelocksolutionsthin-shellthird-orderconditionsenergyorderwormholes
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In this work, we explore asymptotically flat charged thin-shell wormholes of third order Lovelock gravity in higher dimensions, taking into account the cut-and-paste technique. Using the generalized junction conditions, we determine the energy-momentum tensor of these solutions on the shell, and explore the issue of the energy conditions and the amount of normal matter that supports these thin-shell wormholes. Our analysis shows that for negative second order and positive third-order Lovelock coefficients, there are thin-shell wormhole solutions that respect the weak energy condition. In this case, the amount of normal matter increases as the third-order Lovelock coefficient decreases. We also find novel solutions which possess specific regions where the energy conditions are satisfied for the case of a positive second order and negative third-order Lovelock coefficients. Finally, a linear stability analysis in higher dimensions around the static solutions is carried out. Considering a specific cold equation of state, we find a wide range of stability regions.

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Cited by 2 Pith papers

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  1. Linearized stability of T-duality quantum-inspired thin-shell wormholes

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    Thin-shell wormholes in T-duality quantum-corrected regular spacetimes exhibit an intermediate-radius window of unconditional stability absent in the classical Schwarzschild case.

  2. Dyonic Ellis-Bronnikov wormholes from warped extra dimensions

    gr-qc 2026-05 unverdicted novelty 6.0

    Dyonic Ellis-Bronnikov wormholes supported by phantom dilaton, axion, and dyonic gauge fields arise from warped five-dimensional scalar-tensor theories via Kaluza-Klein reduction.