Skip to content

A smooth magnetic monopole exists when an adjoint Higgs field breaks a non-Abelian gauge group so that its direction on the sphere at spatial infinity has nonzero degree. In the SU(2)U(1)SU(2)\to U(1) Georgi–Glashow model, the ’t Hooft–Polyakov monopole has a nonsingular core, magnetic flux 4π/g4\pi/g in the conventions below, and size set by the massive vector and Higgs fields. Electric excitation produces a dyon; a theta term shifts its electric charge by the Witten effect, with a sign fixed by the theta and magnetic-orientation conventions.

Required background. Finite-energy boundary data supplies the sector logic, and local potentials and global gauge configurations distinguishes a smooth bundle configuration from one potential on all space. Helpful background. Theta terms and periodicity fixes the theta convention, while disorder operators explains externally imposed monopole boundary conditions.

Gauge–Higgs theory and finite-energy data

Section titled “Gauge–Higgs theory and finite-energy data”

Use Hermitian SU(2)SU(2) generators Ta=σa/2T^a=\sigma^a/2, so

Dμ=μigAμ,Fμν=μAννAμig[Aμ,Aν].D_\mu=\partial_\mu-igA_\mu, \qquad F_{\mu\nu} =\partial_\mu A_\nu-\partial_\nu A_\mu-ig[A_\mu,A_\nu].

Let Φ=ΦaTa\Phi=\Phi^aT^a be an adjoint scalar with

L=14FμνaFaμν+12(DμΦ)a(DμΦ)aλ4(ΦaΦav2)2.\mathcal L =-\frac14F_{\mu\nu}^aF^{a\mu\nu} +\frac12(D_\mu\Phi)^a(D^\mu\Phi)^a -\frac{\lambda}{4}\left(\Phi^a\Phi^a-v^2\right)^2 .

The vacuum has Φ=v|\Phi|=v and breaks SU(2)SU(2) to the U(1)U(1) generated along the Higgs direction. Finite energy requires

Φv,DiΦ0,Fij0(r).|\Phi|\to v,\qquad D_i\Phi\to0,\qquad F_{ij}\to0 \quad (r\to\infty).

The unit Higgs field Φ^a=Φa/Φ\widehat\Phi^a=\Phi^a/|\Phi| defines

Φ^:S2SU(2)/U(1)S2.\widehat\Phi:S^2_\infty\longrightarrow SU(2)/U(1)\simeq S^2 .

Its degree nmZn_{\mathrm m}\in\mathbb Z labels the magnetic sector. This statement assumes the declared global group and allowed boundary gauge transformations. If all dynamical fields are adjoint, SU(2)SU(2) and SO(3)=SU(2)/Z2SO(3)=SU(2)/\mathbb Z_2 have the same Lie algebra but different line-operator and electric-charge lattices.

For unit magnetic charge, a spherically symmetric ansatz is

Φa=vh(r)r^a,Aia=1k(r)grϵaijr^j,\Phi^a=v\,h(r)\widehat r^{\,a}, \qquad A_i^a =\frac{1-k(r)}{gr}\, \epsilon_{aij}\widehat r^{\,j},

with

h(0)=0,k(0)=1,h()=1,k()=0.h(0)=0,\quad k(0)=1, \qquad h(\infty)=1,\quad k(\infty)=0.

The Higgs magnitude vanishes at the origin, so its direction can unwind there without a singular field. The gauge potential is regular in the hedgehog gauge. The core radii are governed parametrically by

mW=gv,mH=2λv,RgaugemW1,RHiggsmH1.m_W=gv,\qquad m_H=\sqrt{2\lambda}\,v, \qquad R_{\mathrm{gauge}}\sim m_W^{-1}, \quad R_{\mathrm{Higgs}}\sim m_H^{-1}.

The gauge-invariant Abelian field strength selected by the Higgs direction can be written

Fμν=Φ^aFμνa1gϵabcΦ^a(DμΦ^)b(DνΦ^)c.\mathcal F_{\mu\nu} =\widehat\Phi^aF_{\mu\nu}^a -\frac1g\epsilon^{abc}\widehat\Phi^a (D_\mu\widehat\Phi)^b(D_\nu\widehat\Phi)^c .

At large radius it gives

Bnmgr^r2,gmS2BdS=4πnmg.\mathbf B \longrightarrow \frac{n_{\mathrm m}}{g}\frac{\widehat{\mathbf r}}{r^2}, \qquad g_{\mathrm m} \equiv\int_{S^2_\infty}\mathbf B\mathbin{\cdot}\mathrm d\mathbf S =\frac{4\pi n_{\mathrm m}}{g}.

If fundamental probes of electric charge g/2g/2 are allowed, (g/2)gm=2πnm(g/2)g_{\mathrm m}=2\pi n_{\mathrm m} is the Dirac condition. If only adjoint probes occur, the physically distinguishable charge lattice must be stated separately.

The smooth solution was found independently by ’t Hooft 1974, pp. 276–284 and Polyakov 1974, pp. 194–195. Unlike an elementary Dirac monopole potential, the non-Abelian fields and the vanishing Higgs magnitude resolve the core; the asymptotic Abelian field alone does not reveal that resolution.

The Prasad–Sommerfield limit and mass bound

Section titled “The Prasad–Sommerfield limit and mass bound”

In the limit λ0\lambda\to0 with vv fixed, the static energy can be completed as

E=12d3x[(BiaDiΦa)2+2BiaDiΦa]4πvgnm.\begin{aligned} E &=\frac12\int\mathrm d^3x\, \left[ \left(B_i^a-D_i\Phi^a\right)^2 +2B_i^aD_i\Phi^a \right]\\ &\geq \frac{4\pi v}{g}|n_{\mathrm m}|. \end{aligned}

Saturation requires

Bia=DiΦaB_i^a=D_i\Phi^a

for positive magnetic orientation. For nm=1n_{\mathrm m}=1, with ρ=gvr\rho=gvr,

k(ρ)=ρsinhρ,h(ρ)=cothρ1ρ.k(\rho)=\frac{\rho}{\sinh\rho}, \qquad h(\rho)=\coth\rho-\frac1\rho .

These functions obey the required core and asymptotic limits and give

Mmon=4πvg.M_{\mathrm{mon}}=\frac{4\pi v}{g}.

This exact classical solution is Prasad and Sommerfield 1975, pp. 760–762. At λ>0\lambda>0, the topological magnetic sector remains, but the first-order equations and saturated mass formula do not.

A Julia–Zee dyon activates an electric field and, in a convenient gauge, a time component A0A_0 aligned asymptotically with Φ\Phi. Its electric charge is a dynamical or collective datum in addition to nmn_{\mathrm m}; magnetic topology alone does not fix it.

To state the Witten effect, define

F~aμν=12ϵμνρσFρσa,ϵ0123=+1,\widetilde F^{a\mu\nu} =\frac12\epsilon^{\mu\nu\rho\sigma}F^a_{\rho\sigma}, \qquad \epsilon^{0123}=+1,

and add

Lθ=θg232π2FμνaF~aμν.\mathcal L_\theta =\frac{\theta g^2}{32\pi^2} F_{\mu\nu}^a\widetilde F^{a\mu\nu}.

With positive magnetic flux gm=4πnm/gg_{\mathrm m}=4\pi n_{\mathrm m}/g and electric charge measured in units gg appropriate to the adjoint theory, canonical quantization gives the shifted lattice

qeg=ne+θ2πnm,neZ.\frac{q_{\mathrm e}}{g} =n_{\mathrm e} +\frac{\theta}{2\pi}n_{\mathrm m}, \qquad n_{\mathrm e}\in\mathbb Z .

Changing the sign of Lθ\mathcal L_\theta, the definition of F~\widetilde F, or the magnetic orientation changes the sign of the shift. Changing the global gauge group or admitting fundamental probes changes the electric unit and allowed lattice. The invariant statement is the theta-dependent displacement of electric flux for fixed magnetic charge, derived in Witten 1979, pp. 283–287.

The dyon’s classical electric orientation can be a collective coordinate in a controlled BPS regime. Away from that regime it may be lifted, radiate, or mix with nonzero modes. It should not be advertised as an exact protected quantum modulus without the supersymmetry and charge-lattice analysis that supplies such protection.

The shared boundary-family map places the monopole’s S2S^2_\infty Higgs-direction data beside the vortex circle and wall endpoints without treating those domains as interchangeable. The soliton boundary and stability comparison separates magnetic-sector classification from smooth-core existence, BPS minimality, collective phases, and quantum exactness.

For one monopole, translations give three normalizable zero modes and the unbroken electric phase gives another in the BPS theory. For magnetic charge nmn_{\mathrm m}, the smooth SU(2)SU(2) BPS monopole moduli space has dimension 4nm4|n_{\mathrm m}|. The low-velocity approximation and its quantum limitations are treated in Moduli-Space Dynamics and Collective Quantization; exact supersymmetric spectra are a separate subject.

Core regularity. Near r=0r=0, h(r)=O(r)h(r)=O(r) and 1k(r)=O(r2)1-k(r)=O(r^2). Replacing the solution by its 1/r21/r^2 Abelian tail at the origin creates a Dirac singularity that the model was designed to resolve.

Magnetic normalization. Check the flux both from the degree of Φ^\widehat\Phi and from F\mathcal F. Then test it against the smallest allowed electric charge, not merely the Lie algebra.

Mass dimensions. In four spacetime dimensions, [v]=1[v]=1 and gg is dimensionless, so 4πv/g4\pi v/g has the dimension of mass.

Control. The classical solution is reliable when quantum corrections at scale gvgv are small. The BPS equations at λ=0\lambda=0 are a classical statement here; quantum exactness requires additional supersymmetry not assumed on this page.

Identifying a Dirac monopole with a smooth soliton. Their far magnetic fields agree, but a Dirac monopole is specified by singular Abelian boundary data, whereas the ’t Hooft–Polyakov core uses smooth non-Abelian and Higgs fields.

Quoting 4π/g4\pi/g without the global group. The flux unit and its observable distinction depend on the allowed electric probes and line operators.

Writing a convention-free Witten-effect sign. The sign follows from the theta-term sign, dual-tensor convention, and magnetic orientation. State all three before translating a source.

  1. Verify the Dirac pairing for a unit smooth monopole when fundamental SU(2)SU(2) probes of charge g/2g/2 are allowed.
Solution

For nm=1n_{\mathrm m}=1, gm=4π/gg_{\mathrm m}=4\pi/g. The smallest electric charge is qmin=g/2q_{\min}=g/2, hence

qmingm=g24πg=2π.q_{\min}g_{\mathrm m} =\frac g2\frac{4\pi}{g}=2\pi .

The Wilson phase around the Dirac string is therefore unity. If fundamental probes are excluded, this calculation must be replaced by the actual charge lattice.

  1. Check the small- and large-ρ\rho limits of the Prasad–Sommerfield functions.
Solution

Using sinhρ=ρ+ρ3/6+\sinh\rho=\rho+\rho^3/6+\cdots and cothρ=ρ1+ρ/3+\coth\rho=\rho^{-1}+\rho/3+\cdots gives

k(ρ)=1ρ26+,h(ρ)=ρ3+,k(\rho)=1-\frac{\rho^2}{6}+\cdots, \qquad h(\rho)=\frac{\rho}{3}+\cdots,

so the core is regular. At large ρ\rho, k2ρeρk\sim2\rho e^{-\rho} and h=1ρ1+O(e2ρ)h=1-\rho^{-1}+O(e^{-2\rho}), giving a massive non-Abelian tail and the massless Abelian magnetic field.

Bogomolny Bounds and First-Order Equations derives the square completion without assuming supersymmetry. Moduli-Space Dynamics and Collective Quantization explains the low-velocity geodesic approximation.

  • Manton, Nicholas, and Paul Sutcliffe. Topological Solitons. Cambridge Monographs on Mathematical Physics. Cambridge University Press, 2004, ch. 8, pp. 241–348. DOI.
  • Polyakov, Alexander M. “Particle Spectrum in Quantum Field Theory.” JETP Letters 20 (1974): 194–195. Stable article page.
  • Prasad, M. K., and Charles M. Sommerfield. “An Exact Classical Solution for the ’t Hooft Monopole and the Julia–Zee Dyon.” Physical Review Letters 35 (1975): 760–762. DOI.
  • ’t Hooft, Gerard. “Magnetic Monopoles in Unified Gauge Theories.” Nuclear Physics B 79 (1974): 276–284. DOI.
  • Witten, Edward. “Dyons of Charge eθ/2πe\theta/2\pi.” Physics Letters B 86 (1979): 283–287. DOI.