We construct globally regular as well as non-abelian black hole solutions of a higher order curvature Einstein-Yang-Mills (EYM) model in d = 5 dimensions. This model consists of the superposition of the first two members of the gravitational hierarchy (Einstein plus first Gauss-Bonnet(GB)) interacting with the superposition of the first two members of the SO(d) Yang-Mills hierarchy.
We study rotating boson stars in five spacetime dimensions. The boson fields consist of a complex doublet scalar field. Considering boson stars rotating in two orthogonal planes with both angular momenta of equal magnitude, a special ansatz for the boson field and the metric allows for solutions with nontrivial dependence on the radial coordinate only. The charge of the scalar field equals the sum of the angular momenta. The rotating boson stars are globally regular and asymptotically flat. For our choice of a sixtic potential the rotating boson star solutions possess a flat spacetime limit. We study the solutions in flat and curved spacetime.
We construct monopole solutions in SU(2) Einstein-Yang-Mills-Higgs theory carrying magnetic charge n. For vanishing and small Higgs self-coupling, these multimonopole solutions are gravitationally bound. Their mass per unit charge is lower than the mass of the n = 1 monopole. For large Higgs self-coupling only a repulsive phase exists.
We study both global as well as local (Nielsen-Olesen) strings in de Sitter
space. While these type of topological defects have been studied in the
background of a de Sitter metric previously, we study here the full set of
coupled equations. We find only ``closed'' solutions. The behaviour of the
metric tensor of these solutions resembles that of ``supermassive'' strings
with a curvature singularity at the cosmological horizon. For global strings
(and the composite defect) we are able to construct solutions which are regular
on the interval from the origin to the cosmological horizon if the global
string core lies completely inside the horizon.Comment: 11 Revtex-pages including 5 ps-figures; v1: typos corrected, note
added; v2: minor changes in conclusion
We study static spherically symmetric gravitating dyon solutions and dyonic black holes in Einstein-Yang-Mills-Higgs theory. The gravitating dyon solutions share many features with the gravitating monopole solutions. In particular, gravitating dyon solutions and dyonic black holes exist only up to a maximal coupling constant, and beside the fundamental dyon solutions there are excited dyon solutions.
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