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Non-Abelian gravitating solitons with negative cosmological constant

Peter Breitenlohner1, Dieter Maison1 and George Lavrelashvili2

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Static, spherically symmetric solutions with regular origin are investigated of the Einstein–Yang–Mills theory with a negative cosmological constant Λ. A combination of numerical and analytical methods leads to a clear picture of the 'moduli space' of the solutions. Some issues discussed in the existing literature on the subject are reconsidered and clarified. In particular the stability of the asymptotically AdS solutions is studied. Like for the Bartnik–McKinnon (BK) solutions obtained for Λ = 0 there are two different types of instabilities—'topological' and 'gravitational'. Regions with any number of these instabilities are identified in the moduli space. While for BK solutions there is always a non-vanishing equal number of instabilities of both types, this degeneracy is lifted and there exist stable solutions, genuine sphalerons with exactly one unstable mode and so on. The boundaries of these regions are determined.


PACS

05.45.Yv Solitons

11.15.-q Gauge field theories

04.20.-q Classical general relativity

11.10.Lm Nonlinear or nonlocal theories and models

MSC

37K40 Soliton theory, asymptotic behavior of solutions

83Cxx General relativity

81T13 Yang-Mills and other gauge theories (See also 53C07, 58E15)

Subjects

Gravitation and cosmology

Particle physics and field theory

Statistical physics and nonlinear systems

Dates

Issue 6 (21 March 2004)

Received 21 October 2003

Published 2 March 2004



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