Black hole and thin-shell wormhole solutions in Einstein-Hoffman-Born-Infeld theory
arXiv:0908.3967 · doi:10.1016/j.physleta.2011.08.036
Abstract
We employ an old field theory model, formulated and discussed by Born, Infeld, Hoffman and Rosen during 1930s. Our method of cutting-gluing of spacetimes resolves the double-valuedness in the displacement vector D(E), pointed out by these authors. A characteristic feature of their model is to contain a logarithmic term, and by bringing forth such a Lagrangian anew, we aim to attract the interest of field theorists to such a Lagrangian. We adopt the Hoffman-Born-Infeld (HBI) Lagrangian in general relativity to construct black holes and investigate the possibility of viable thin-shell wormholes. In particular, the stability of thin-shell wormholes supported by normal matter in 5-dimensional Einstein-HBI-Gauss-Bonnet gravity is highlighted.
17 pages, one figure, some constructive changes has been done
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Cited by in corpus (11)
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- Thin-shell wormholes from the regular Hayward black hole
- Thin-shell wormholes with charge in F(R) gravity
- Stability of generic cylindrical thin shell wormholes
- Stability Analysis of Thin-Shell Wormholes from Charged Black String
- Stable thin-shell wormholes with a Chaplygin gas in Einstein-Maxwell-Gauss-Bonnet gravity
- Geometrothermodynamics of black holes in Lovelock gravity with a nonlinear electrodynamics
- Counterrotational effects on stability of 2+1-dimensional thin-shell wormholes
- Microscopic thin shell wormholes in magnetic Melvin universe
- Born-Infeld Thin-shell Wormholes Supported by Generalized Cosmic Chaplygin Gas
- Thin-shell Wormholes with Ordinary Matter in Pure Gauss-Bonnet Gravity