EYM equations in the presence of q-stars
arXiv:hep-th/0406088 · doi:10.1103/PhysRevD.70.045008
Abstract
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.
arXiv comment11 pages, to appear in Phys. Rev. D
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