’t Hooft–Polyakov monopoles
Relate the adjoint Higgs boundary map to a smooth magnetic monopole and derive its BPS mass with a canonical gauge-coupling convention.
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The question for today
What you’ll understand
- Specify the monopole’s gauge, Higgs, and finite-energy boundary data.
- Calculate magnetic flux and the canonical BPS mass.
- Distinguish a smooth non-Abelian core from an Abelian gauge-potential singularity.
A pointlike magnetic source in an Abelian theory appears to require a singular core, but a non-Abelian gauge field coupled to an adjoint Higgs field admits a smooth finite-energy alternative. The ’t Hooft–Polyakov monopole stores its structure in a spatially varying Higgs orientation and accompanying gauge field. Its long-distance field looks Abelian, while its core does not. We will specify a canonical SU two normalization, derive the magnetic charge and mass bound, and separate topological existence from the special zero-potential limit that admits first-order equations.
The boundary is a sphere, not a spatial circle
Work in three spatial dimensions with natural units and a real adjoint Higgs field Phi a. Choose field strength F a i j equal to the derivative terms plus g times the antisymmetric gauge-product term; the coupling is inside F and inside the covariant derivative. Canonically normalized static energy contains one half the squared magnetic field and one half the squared Higgs covariant gradient. This differs from conventions placing an overall inverse coupling squared outside the entire action.
At infinity the Higgs magnitude approaches a fixed positive v, leaving an unbroken U one direction. Its normalized orientation defines a map from the spatial sphere at infinity to the sphere of Higgs orientations, SU two modulo U one. Such maps have an integer degree n. Finite energy requires the covariant gradient to decay, so the gauge field compensates the changing orientation. This ties the boundary degree to magnetic flux in the unbroken Abelian field.
The BPS limit isolates a surface term
When lambda vanishes while the asymptotic Higgs magnitude v is kept fixed, the energy can be completed into the square of B minus or plus D Phi. The cross term becomes a surface integral by the non-Abelian Bianchi identity. Evaluating it with the asymptotic Higgs and magnetic field gives a lower mass bound proportional to v times the magnitude of magnetic flux. Saturation requires the corresponding first-order monopole equation.
The positive-charge branch obeys B equal to D Phi, while negative charge uses the opposite sign. These equations have smooth monopole solutions with a massive charged-vector core and a long-range Abelian magnetic tail. At zero scalar potential the Higgs radial fluctuation is massless, so its approach to the vacuum can have a long tail too. Setting lambda to zero does not mean discarding the boundary magnitude that defines the sector and mass scale.
A gauge singularity is not a singular physical core
In a smooth hedgehog gauge, Higgs orientation varies with direction and its magnitude vanishes near the center. The full non-Abelian configuration is regular. Rotating the Higgs to a fixed direction on the sphere leads to an Abelian-looking description that needs gauge patches or a Dirac-string-like potential singularity. That singularity belongs to the chosen potential representation, not to an infinite-energy physical string attached to the smooth monopole.
Electric charge quantization must be checked with the actual representations present. For example, charged gauge bosons and a fundamental probe can carry different units under the surviving U one, so quoting a universal product of electric and magnetic charges without that convention invites a factor-of-two mistake. Classical monopole mass, quantum corrections, scattering moduli, and confinement of magnetic or electric charges are also separate questions. A finite-energy monopole solution provides a controlled nonperturbative object, not an automatic mechanism for every strongly coupled gauge phenomenon.
Work it through
A monopole in canonical units
Use g = 1/2, v = 2 GeV, lambda = 0, and n = 1. Find asymptotic magnetic flux, the saturated monopole mass, charged-vector mass, and its inverse-mass length scale.
The flux is . This is the unbroken-field flux under the specified canonical convention.
The BPS mass is . Lambda = 0 permits saturation when the first-order monopole equation and boundaries are satisfied.
The vector mass is , giving inverse scale . This characterizes a core scale, not a compact support radius; the massless fields retain long-distance tails.
The flux is 8π, BPS mass 16π GeV, and vector inverse-mass scale 1 GeV⁻¹.
The living notebook
Explore the model
Interactive lab · vectors
A direction field requires more than one vector
Use one vector only as a local orientation analogy. Reset, set Angle = 0° and Magnitude = 1, and predict x projection 1. For a fresh run Reset, set Angle = 90° and Magnitude = 1, and predict y projection 1.
- x component
- 1.393
- y component
- 0.975
- Magnitude
- 1.7
Playback traces a fixed vector and its projections. Angle and magnitude set the geometry; the moving marker does not change them. Parameter changes pause playback and recompute the model at the current elapsed time. Reset restores both parameters and returns time to zero. Playback starts paused. Adjust either parameter, then choose Play or Step.
Look forThe instrument has one planar vector. It does not construct a map between spheres, a non-Abelian gauge field, a magnetic flux integral, or a smooth monopole core.
Pause & reason
Check your understanding
Your turn
Try it yourself
Take g = 1, v = 3 GeV, and topological degree n = −2. Find magnetic flux, the classical lower mass bound, and vector mass. Explain what extra condition is needed to replace the bound by equality.
Take a moment to make a prediction or work it out on paper. Open a hint when you need one.
Give me a hint
Keep the flux signed and use absolute degree in the energy bound.
Compare with the solution
The flux is , the mass bound is , and . Equality requires the zero-potential BPS limit and an allowed negative-branch solution with the prescribed boundaries. Degree two in magnitude need not describe one spherically symmetric core; multi-monopole moduli can be relevant.
Keep the idea
Take it with you
- The monopole charge is associated with a Higgs-orientation map on spatial infinity.
- Canonical and overall-inverse-coupling normalizations must not be mixed.
- A smooth non-Abelian monopole, its Abelian gauge patches, and its BPS limit describe different aspects of the same configuration.
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