EYM equations in the presence of q-stars

Details EYM equations in the presence of q-stars EYM equations in the presence of q-stars

2004-06-10

arxiv.org/abs/hep-th/0406088v1

Phys.Rev. D70 (2004) 045008

Physics

High Energy Physics

High Energy Physics - Theory

11 pages, to appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.70.045008

We study Einstein-Yang-Mills equations in the presence of gravitating non-topological soliton field configurations, of q-ball type. We produce numerical solutions, stable with respect to gravitational collapse and to fission into free particles, and we study the effect of the field strength and the eigen-frequency to the soliton parameters. We also investigate the formation of such soliton stars when the spacetime is asymptotically anti de Sitter.

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