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What does a strongly excited 't Hooft-Polyakov magnetic monopole do?

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arxiv hep-th/0311061 v1 pith:OYBS6S6M submitted 2003-11-07 hep-th gr-qc

classification hep-thgr-qc
keywords magneticmonopoleregionstronglyawaybogomolny-prasad-sommerfieldbreathingbuilt
verification ladder T0 review T1 audit T2 compute T3 formal
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The time evolution of strongly exited SU(2) Bogomolny-Prasad-Sommerfield (BPS) magnetic monopoles in Minkowski spacetime is investigated by means of numerical simulations based on the technique of conformal compactification and on the use of 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 quasi-stable `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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Cited by 2 Pith papers

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    Vortex–antivortex collisions in the deep type-II Abelian-Higgs model show multi-bounce windows embedded in annihilation regions, driven by a Feshbach resonant mode.

  2. Semilinear wave equations in homothetic hyperboloidal coordinates and tail decay

    gr-qc 2026-08 conditional novelty 6.0 of 10

    Homothetic hyperboloidal coordinates give semilinear wave tails the same exponential decay rate at every compactified radius, removing the late-time resolution bottleneck.

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