Wormholes threaded by chiral fields
E. G. CharalampidisDepartment of Mathematics, Physics and Computational Sciences, Faculty of Engineering, Aristotle University of Thessaloniki, Thessaloniki 54124, GreeceTheodora IoannidouDepartment of Mathematics, Physics and Computational Sciences, Faculty of Engineering, Aristotle University of Thessaloniki, Thessaloniki 54124, GreeceBurkhard KleihausDepartment of Mathematics, Physics and Computational Sciences, Faculty of Engineering, Aristotle University of Thessaloniki, Thessaloniki 54124, GreeceJutta KunzDepartment of Mathematics, Physics and Computational Sciences, Faculty of Engineering, Aristotle University of Thessaloniki, Thessaloniki 54124, Greece
2013en
ABI
Аннотация
We consider Lorentzian wormholes with a phantom field and chiral matter fields. The chiral fields are described by the nonlinear sigma model with or without a Skyrme term. When the gravitational coupling of the chiral fields is increased, the wormhole geometry changes. The single throat is replaced by a double throat with a belly in between. For a maximal value of the coupling, the radii of both throats reach zero. Then the interior part pinches off, leaving a closed universe and two (asymptotically) flat spaces. A stability analysis shows that all wormholes threaded by chiral fields inherit the instability of the Ellis wormhole.
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Идентификаторлар
Иқтибослар ва манбалар
2 та иқтибос0 та фойдаланилган манба