Radiative non-Abelian cosmic strings with negative cosmological constant

Details Radiative non-Abelian cosmic strings with negative cosmological constant Radiative non-Abelian cosmic strings with negative cosmological constant

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cqgra..19..115s&link_type=abstract

Classical and Quantum Gravity, Volume 19, Issue 1, pp. 115-125 (2002).

Mathematics

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Scientific paper

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.

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