Vacuum static compactified wormholes in eight - dimensional Lovelock theory
نویسندگان
چکیده
In this paper new exact solutions in eight dimensional Lovelock theory will be presented. These solutions are vacuum static wormhole, black hole and generalized Bertotti-Robinson space-times with nontrivial torsion. All the solutions have a cross product structure of the type M5 × Σ3 where M5 is a five dimensional manifold and Σ3 a compact constant curvature manifold. The wormhole is the first example of a smooth vacuum static Lovelock wormhole which is neither Chern-Simons nor Born-Infeld. It will be also discussed how the presence of torsion affects the ”navigableness” of the wormhole for scalar and spinning particles. It will be shown that the wormhole with torsion may act as ”geometrical filter”: a very large torsion may ”increase the traversability” for scalars while acting as a ”polarizator” on spinning particles. This may have interesting phenomenological consequences. PACS: 04.50.-h, 04.50.Cd, 11.27.+d, 04.20.Jb canfora AT cecs.cl giacomini AT cecs.cl
منابع مشابه
Gravitational solitons and C vacuum metrics in five-dimensional Lovelock gravity
Junction conditions for vacuum solutions in five-dimensional Einstein-Gauss-Bonnet gravity are studied. We focus on those cases where two spherically symmetric regions of space-time are joined in such a way that the induced stress tensor on the junction surface vanishes. So a spherical vacuum shell, containing no matter, arises as a boundary between two regions of the space-time. A general anal...
متن کاملConformal Continuations and Wormhole Instability in Scalar-tensor Gravity
We study the stability of static, spherically symmetric, traversable wormholes existing due to conformal continuations in a class of scalar-tensor theories with zero scalar field potential (so that Fisher’s well-known scalar-vacuum solution holds in the Einstein conformal frame). Specific examples of such wormholes are those with nonminimally (e.g., conformally) coupled scalar fields. All bound...
متن کاملar X iv : h ep - t h / 04 05 05 0 v 1 6 M ay 2 00 4 Five Dimensional Cosmology in Horava - Witten M - Theory
The cosmology in the Hubble expansion era of the Horava-Witten M-theory compactified on a Calabi-Yau threefold is studied in the reduction to five-dimensions where the effects of the Calabi-Yau man-ifold are summarized by the volume modulus, and all perturbative potentials are included. Matter on the branes are treated as first order perturbations of the static vacuum solution, and all equation...
متن کاملar X iv : h ep - t h / 04 05 05 0 v 3 2 D ec 2 00 4 Five Dimensional Cosmology in Horava - Witten M - Theory
The cosmology in the Hubble expansion era of the Horava-Witten M-theory compactified on a Calabi-Yau threefold is studied in the reduction to five-dimensions where the effects of the Calabi-Yau man-ifold are summarized by the volume modulus, and all perturbative potentials are included. Matter on the branes are treated as first order perturbations of the static vacuum solution, and all equation...
متن کاملar X iv : h ep - t h / 04 05 05 0 v 2 2 4 M ay 2 00 4 Five Dimensional Cosmology in Horava - Witten M - Theory
The cosmology in the Hubble expansion era of the Horava-Witten M-theory compactified on a Calabi-Yau threefold is studied in the reduction to five-dimensions where the effects of the Calabi-Yau man-ifold are summarized by the volume modulus, and all perturbative potentials are included. Matter on the branes are treated as first order perturbations of the static vacuum solution, and all equation...
متن کامل