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          Institute: MPI für Gravitationsphysik     Collection: Geometric Analysis and Gravitation     Display Documents



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ID: 3370.0, MPI für Gravitationsphysik / Geometric Analysis and Gravitation
SU(2) Cosmological Solitons
Authors:Lechner, Christiane; Aichelburg, Peter C.; Husa, S.
Language:English
Date of Publication (YYYY-MM-DD):2000
Title of Journal:Physical Review D
Volume:62
Sequence Number of Article:044047
Review Status:Peer-review
Abstract / Description:We present a class of numerical solutions to the SU(2) nonlinear sigma model coupled to the Einstein equations with a cosmological constant Lambda>=0 in spherical symmetry. These solutions are characterized by the presence of a regular static region which includes a center of symmetry. They are parametrized by a dimensionless "coupling constant" beta, the sign of the cosmological constant, and an integer "excitation number" n. The phenomenology we find is compared to the corresponding solutions found for the Einstein-Yang-Mills (EYM) equations with a positive Lambda (EYMLambda). If we choose Lambda positive and fix n, we find a family of static spacetimes with a Killing horizon for 0<=beta<betamax. As a limiting solution for beta= betamax we find a globally static spacetime with Lambda= 0, the lowest excitation being the Einstein static universe. To interpret the physical significance of the Killing horizon in the cosmological context, we apply the concept of a trapping horizon as formulated by Hayward. For small values of beta an asymptotically de Sitter dynamic region contains the static region within a Killing horizon of cosmological type. For strong coupling the static region contains an "eternal cosmological black hole."
External Publication Status:published
Document Type:Article
Communicated by:Gerhard Huisken
Affiliations:MPI für Gravitationsphysik/Geometric Analysis and Gravitation
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