SU(3) monopoles and their fields
arXiv:hep-th/9704153 · doi:10.1103/PhysRevD.56.5200
Abstract
Some aspects of the fields of charge two SU(3) monopoles with minimal symmetry breaking are discussed. A certain class of solutions look like SU(2) monopoles embedded in SU(3) with a transition region or ``cloud'' surrounding the monopoles. For large cloud size the relative moduli space metric splits as a direct product AH\times R^4 where AH is the Atiyah-Hitchin metric for SU(2) monopoles and R^4 has the flat metric. Thus the cloud is parametrised by R^4 which corresponds to its radius and SO(3) orientation. We solve for the long-range fields in this region, and examine the energy density and rotational moments of inertia. The moduli space metric for these monopoles, given by Dancer, is also expressed in a more explicit form.
17 pages, 3 figures, latex, version appearing in Phys. Rev. D
Cited by in corpus (16)
- Magnetic Monopole Dynamics, Supersymmetry, and Duality
- Low Energy Dynamics for 1/4 BPS Dyons
- Quantisation of Monopoles with Non-abelian Magnetic Charge
- Explicit Multimonopole Solutions in SU(N) Gauge Theory
- Multicloud solutions with massless and massive monopoles
- Two Massive and One Massless Sp(4) Monopoles
- Magnetic monopole bibliography
- Two-Monopole Systems and the Formation of Non-Abelian Clouds
- Scattering of massless and massive monopoles in an SU(N) theory
- Nahm Data and the Mass of 1/4-BPS States
- Properties of non-BPS SU(3) monopoles
- Magnetic Charge Lattices, Moduli Spaces and Fusion Rules
- G2 monopoles
- Interactions of massless monopole clouds
- Massless monopole clouds and electric-magnetic duality
- Multimagnetic Monopoles