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We have constructed, numerically, both regular and black hole static solutions to the simplest possible gravitating Yang-Mills–Higgs (YMH) in spacetime dimensions. The YMH systems consist of th power curvature fields without a Higgs potential. The gravitational systems consist of the `Ricci scalar’ of the th power of the Riemann curvature. In 4 spacetime dimensions this is the usual Einstein-YMH (EYMH) studied in \cite{Breitenlohner:1991aa, Breitenlohner:1994di}, whose qualitative results we emulate exactly.

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