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What Does a Strongly Excited ’t Hooft–Polyakov Magnetic Monopole Do?

2003/11/07 by Gyula Fodor, István Rácz · 4 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Compactification (mathematics) #Conformal map #Cosmology and Gravitation Theories #Excited state #Geometry #Magnetic monopole #Mathematical physics #Minkowski space #Physics #Pure mathematics #Quantum electrodynamics #Quantum mechanics #Solar and Space Plasma Dynamics #Spacetime #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevlett.92.151801

published as Phys.Rev.Lett. 92 (2004) 151801 · 4 pages, 6 figures

arxiv created 2003/11/07 · openalex publication_date 2004/04/12 · arxiv updated 2016/08/16 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

The time evolution of strongly excited SU(2) Bogomol'nyi-Prasad-Sommerfield magnetic monopoles in Minkowski spacetime is investigated by using numerical simulations based on the technique of conformal compactification and on the use of the hyperboloidal initial value problem. It is found that an initially static monopole does not radiate the entire energy of the exciting pulse toward future null infinity. Rather, a long-lasting quasistable "breathing state" develops in the central region and certain expanding shell structures-built up by very high frequency oscillations-are formed in the far away region.

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