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Radiative non-Abelian cosmic strings with negative cosmological constant

R J Slagter1,2,3

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We investigated the SU(2) Einstein–Yang–Mills system with a cosmological constant on a time-dependent non-diagonal cylindrical symmetric spacetime. Only for suitable negative Λ and specific initial values, we find numerically regular wave-like solutions dressed with both electric and magnetic charges. The cosmic string feature is maintained by the finite angle deficit the solutions possess. In general the solution will develop a cosmological horizon; however, it resolves for increasing negative values of the cosmological constant and increasing time. Further, the features of the dyon depend on the angular momentum flux.


PACS

11.27.+d Extended classical solutions; cosmic strings, domain walls, texture

04.20.-q Classical general relativity

98.80.Es Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc)

MSC

83C35 Gravitational waves

83F05 Cosmology

83E30 String and superstring theories (See also 81T30)

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 1 (7 january 2002)

Received 6 September 2001, in final form 31 October 2001

Published 13 December 2001



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