Static Cosmological Solutions of the Einstein-Yang-Mills-Higgs Equations

Abstract

Numerical evidence is presented for the existence of a new family of static, globally regular `cosmological' solutions of the spherically symmetric Einstein-Yang-Mills-Higgs equations. These solutions are characterized by two natural numbers ($m\ge 1$, $n\ge 0$), the number of nodes of the Yang-Mills and Higgs field respectively. The corresponding spacetimes are static with spatially compact sections with 3-sphere topology.

7 pages, 5 figures, LaTex

References in corpus (1)

• Some Remarks on Gravitational Global Monopoles

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