Numerical Solutions of the Einstein-Yang-Mills System with Cosmological Constant

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dc.creatorMolnar, P.
dc.date1995-03-22
dc.date1995-05-04
dc.date.accessioned2026-07-07T08:59:27Z
dc.date.available2026-07-07T08:59:27Z
dc.descriptionNumerical evidence for a cosmological version of the Bartnik-McKinnon family of particle-like solutions of the Einstein-Yang-Mills system is presented. Our solutions are also static, but space has the topology of a three-sphere. By adjusting the cosmological constant we found numerically a spherically symmetric solution which can be regarded as an excitation of the unique SO(4)-invariant solution. We expect that for each node number there exists such a solution without a cosmological horizon.
dc.description35 pages, latex file
dc.identifierhttps://arxiv.org/abs/gr-qc/9503036
dc.identifierhttp://arxiv.org/abs/gr-qc/9503036
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147718
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNumerical Solutions of the Einstein-Yang-Mills System with Cosmological Constant
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