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2026-10-01 · chapter Yang–Mills and the mass gapPart 3 Yang–Mills theory (classical)the gauge principle

The whole book Contents and reading orders
  1. Part 0 Entrance — how to read this book
  2. 0-01 How to read this book
  3. 0-02 One picture
  4. 0-03 Reading the problem statement word by word
  5. 0-04 Four dimensions in mathematics and four dimensions in physics
  6. Part 1 Mathematical preparation
  7. 1-01 Vector spaces and linear maps
  8. 1-02 What a group is
  9. 1-03 Lie groups and Lie algebras
  10. 1-04 SU(2) and SU(3)
  11. 1-05 Manifolds and tangent spaces
  12. 1-06 Differential forms and the exterior derivative
  13. 1-07 Vector bundles and connections
  14. 1-08 Probability and measure
  15. 1-09 Probability in infinite dimensions
  16. 1-10 Hilbert spaces and self-adjoint operators
  17. 1-11 Fourier analysis and distributions
  18. 1-12 Detour: what happens only in four dimensions
  19. Part 2 Physical preparation
  20. 2-01 Lagrangians and the action
  21. 2-02 The idea of a field
  22. 2-03 Electromagnetism is a gauge theory
  23. 2-04 Special relativity and spacetime
  24. 2-05 The bones of quantum mechanics
  25. 2-06 The harmonic oscillator and creation and annihilation
  26. 2-07 The idea of the path integral
  27. 2-08 Statistical mechanics and phase transitions
  28. 2-09 Detour: the gap and the correlation length in the Ising model
  29. 2-10 The relaxation time and the dynamical exponent z
  30. Part 3 Yang–Mills theory (classical)
  31. 3-01 The gauge principle
  32. 3-02 Non-abelian gauge fields
  33. 3-03 The action and the equations
  34. 3-04 Gauge theory as geometry
  35. 3-05 Instantons and topology
  36. 3-06 Detour: Donaldson and exotic R⁴
  37. 3-07 Yang–Mills inside the Standard Model
  38. Part 4 Quantisation
  39. 4-01 Canonical quantisation and the Hamiltonian
  40. 4-02 The path integral and Euclideanisation
  41. 4-03 Perturbation theory and Feynman diagrams
  42. 4-04 Divergences and renormalisation
  43. 4-05 The algebra of divergences
  44. 4-06 Asymptotic freedom
  45. 4-07 Dimensional transmutation and Λ
  46. 4-08 Gauge fixing and Faddeev–Popov
  47. 4-09 The axioms of quantum field theory
  48. 4-10 The Osterwalder–Schrader axioms and reconstruction
  49. 4-11 The definition of the mass gap
  50. 4-12 Detour: the perturbation series diverges
  51. Part 5 Lattice gauge theory
  52. 5-01 Wilson's lattice
  53. 5-02 The strong-coupling expansion
  54. 5-03 Reflection positivity and the transfer matrix
  55. 5-04 The infinite-volume limit and the cluster expansion
  56. 5-05 Weak coupling and the continuum limit
  57. 5-06 How U(1) differs from the non-abelian case
  58. 5-07 The Monte Carlo method
  59. 5-08 Measuring glueballs and the string tension
  60. 5-09 What to hold fixed when taking the limit
  61. 5-10 Lattice gauge theory with finite groups
  62. 5-11 Detour: Bakry–Émery and one-link integration
  63. Part 6 Constructive field theory
  64. 6-01 What constructive field theory is
  65. 6-02 Solvability in two dimensions and the Yang–Mills measure
  66. 6-03 Constructing scalar fields
  67. 6-04 The cluster expansion
  68. 6-05 The sequence of renormalisation group steps
  69. 6-06 Ultraviolet stability of three-dimensional Yang–Mills
  70. 6-07 Four dimensions
  71. 6-08 Triviality of φ⁴ in four dimensions
  72. 6-09 Stochastic quantisation and regularity structures
  73. 6-10 Where four dimensions stops
  74. 6-11 Obstacles other than divergence
  75. 6-12 Detour: "if 1/0 is given a symbol"
  76. Part 7 From the side of physics
  77. 7-01 How physics sees it
  78. 7-02 Mechanisms of confinement
  79. 7-03 The string picture
  80. 7-04 Large N
  81. 7-05 String theory and extra dimensions
  82. 7-06 How extra dimensions become invisible
  83. 7-07 Where gauge fields come from
  84. 7-08 Holography
  85. 7-09 The mass gap becomes geometry
  86. 7-10 Back to four dimensions
  87. 7-11 Supersymmetry and Seiberg–Witten
  88. 7-12 The sentence that plays the role of an equivalence principle
  89. 7-13 Where the way physics digs parts from mathematics
  90. Part 8 A dictionary of two languages — the physical and the mathematical view
  91. 8-01 How to read the dictionary
  92. 8-02 Dictionary A
  93. 8-03 Dictionary B
  94. 8-04 Dictionary C
  95. 8-05 The physical counterparts of our assumptions
  96. Part 9 Where things stand, and open tasks
  97. 9-01 How far the world has come
  98. 9-02 Where the two ways of digging part
  99. 9-03 Candidates for new concepts
  100. 9-04 The list of open tasks
  101. 9-05 Common misconceptions
  102. Part 10 Towards a proof of the mass gap — building the first step of the staircase
  103. 10-00 Entrance — the staircase, and the random walk, the ruler and the clock
  104. 10-01 The line of construction and Assumption H
  105. 10-02 Roads tried on the four-dimensional lattice, and walls
  106. 10-03 The four steps of the staircase — why we start from 0+1 dimensions
  107. 10-04 The path measure of the double well, and kinks
  108. 10-05 The statement of the first step — four conditions and Proposition 4.5
  109. 10-06 (H1) Local Poincaré within a phase
  110. 10-07 The map of (H2) — seven routes and the seam of the ring
  111. 10-08 What computer-assisted means — the conditions on the chain inside the window
  112. 10-09 The sector framework and the three strands of route 5
  113. 10-10 The list of detour plans — types of breakage
  114. 10-11 (H3)(H4) and the constant of the core
  115. 10-12 The integrated table and the dependency graph
  116. 10-13 Lean statements and the limits of machine checking
  117. 10-14 Reconciliation — the numbers of the record and the known numbers
  118. 10-15 What remains and its cost — the distance to a theorem
  119. 10-16 What is not claimed
  120. 10-17 Insights and small questions
  121. Part 11 Further considerations — beyond Assumption H, and other views
  122. 11-00 Further considerations — entrance
  123. 11-01 One form that obstructs H — a nearly conserved global quantity
  124. 11-02 Choosing the ruler and the coordinates again — the length at which conservation breaks
  125. 11-03 Two ways to repair H — the sector H and the local H
  126. 11-04 Which H the one-sided bridge needs
  127. 11-05 Making time continuous — the Hamiltonian lattice and the vacuum measure
  128. 11-06 Paying with rarity instead of convexity — renormalisation on groups and log-Sobolev
  129. 11-07 Because it is four dimensions — the dimensionless coupling and topology
  130. 11-08 Questions, and what is not claimed
  131. 11-A1 Table of notation for Part 11
  132. Appendices
  133. A-01 Table of notation
  134. A-02 Glossary
  135. A-03 Guide to the literature
  136. A-04 Lean and machine checking
  137. A-05 How this book was made
  138. A-06 Index of assumptions

The gauge principle — demanding a local symmetry requires a tool for comparison, and that tool carries the force

What this chapter shows — That demanding a (local) symmetry that turns the phase point by point breaks the derivative, and that a tool for comparing neighbouring points (a connection) repairs it. That this tool becomes a field, couples to the conserved charge, and carries a force. That for SU(2) the gauge field itself is also turned.

Prerequisite chapters — 2-03 (gauge transformations, phase factors) and 1-04 (SU(2), the adjoint representation). Beyond these we use only Noether's theorem from 2-01 and the indices of 2-04 §07. We take ℏ=c=1\hbar=c=1, ε0=1\varepsilon_0=1 (Heaviside–Lorentz units).

Said first — The gauge principle is a guide for choosing the form of a theory, not a theorem (section 07). The non-abelian field strength and self-interaction are left to 3-02. Only classical fields are treated, and this chapter shows nothing about the mass gap of Yang–Mills.

Order of this chapter
  1. Global symmetry — charge is conserved
  2. Turning locally — the derivative breaks
  3. A tool for comparison — the connection and the covariant derivative (Figure 1, Table 1)
  4. Making A a dynamical field — the field strength, and the mass term that cannot be written
  5. A force appears — coupling to the conserved charge (Figure 2)
  6. The same demand for SU(2) — a field that is itself turned, and the problem of mass
  7. What the principle decides, and what it does not (Table 2)
  8. Detour: "gauge" was originally a measuring rod
  9. Where this book is going

01

Global symmetry — turning everything by the same amount

In 2-03 the potentials A\mathbf A came first, and the replacement of phase (G') was found afterwards. This chapter goes the other way: it derives the electromagnetic field by demanding that "the theory does not change even if the phase is turned arbitrarily point by point". This procedure is the gauge principle.

The starting point is a field ψ(t,x)\psi(t,\mathbf x) with complex values, the simplest model of a charged particle. Take the Lagrangian density (2-01, 2-02) to be

L0=∣∂tψ∣2−∣∇ψ∣2−V(∣ψ∣2)(1)\mathcal L_0=|\partial_t\psi|^2-|\nabla\psi|^2-V(|\psi|^2) \tag{1}

(for example V=M2∣ψ∣2V=M^2|\psi|^2, where MM is the mass of the particle). Turning by a constant α\alpha as ψ↦eiαψ\psi\mapsto e^{i\alpha}\psi leaves L0\mathcal L_0 invariant (a global U(1) symmetry; U(1) is the group of complex numbers of absolute value 1, 1-02). Noether's theorem (2-01) gives a conservation law, written with a constant qq multiplied in.

ρ=iq(ψ∗∂tψ−ψ ∂tψ∗),J=−iq(ψ∗∇ψ−ψ∇ψ∗),∂tρ+∇⋅J=0(2)\rho=iq\bigl(\psi^*\partial_t\psi-\psi\,\partial_t\psi^*\bigr),\qquad \mathbf J=-iq\bigl(\psi^*\nabla\psi-\psi\nabla\psi^*\bigr),\qquad \partial_t\rho+\nabla\cdot\mathbf J=0 \tag{2}

Example. For a plane wave ψ=ei(k⋅x−ωt)\psi=e^{i(\mathbf k\cdot\mathbf x-\omega t)} (ω>0\omega\gt0), ρ=2qω\rho=2q\omega, J=2qk\mathbf J=2q\mathbf k. qq becomes the charge in section 05. A global symmetry says that "nothing changes if the reference of phase at every point is shifted all at once".

02

Turning locally breaks the derivative

Let the angle of turning change from point to point, ψ↦eiα(t,x)ψ\psi\mapsto e^{i\alpha(t,\mathbf x)}\psi (a local transformation). ∣ψ∣2|\psi|^2 does not change, but the derivative acquires an extra term (∂μ\partial_\mu are the components of ∂t\partial_t and ∇\nabla, μ=0,1,2,3\mu=0,1,2,3).

∂μ(eiαψ)=eiα(∂μψ+i(∂μα) ψ)\partial_\mu\bigl(e^{i\alpha}\psi\bigr)=e^{i\alpha}\bigl(\partial_\mu\psi+i(\partial_\mu\alpha)\,\psi\bigr)

Example. The gradient energy ∣∇ψ∣2|\nabla\psi|^2 of a constant field ψ=1\psi=1 is 0, but turning by α=kx\alpha=kx gives ψ=eikx\psi=e^{ikx}, ∣∇ψ∣2=k2|\nabla\psi|^2=k^2. Only the reference was changed, yet (1) counts it as a different state.

The derivative is the limit of the difference ψ(x+εn)−ψ(x)\psi(x+\varepsilon n)-\psi(x) of two neighbouring points divided by ε\varepsilon (nn is the unit vector of the direction). If the two values are turned by different angles, the difference mixes "the change in the field" with "the change in the reference". Values at different points cannot be subtracted as they stand.

Why demand local transformations? The abstract of Yang and Mills (1954) says that the usual invariance under isospin rotations (section 06) is not consistent with the idea of localised fields (the content of the abstract is in 3-02 §01) Known. This is a demand (a principle), not a theorem, and whether nature follows it is decided by experiment (section 07).

03

A tool for comparison — the connection and the covariant derivative

To compare values at different points, we need a correspondence: "which reference of phase at the point yy corresponds to the reference at the point xx". We call this the comparator U(y,x)∈U(1)U(y,x)\in U(1), write U(y,x)ψ(x)U(y,x)\psi(x) for ψ(x)\psi(x) carried to yy, and stipulate that under transformations

U(y,x)↦eiα(y) U(y,x) e−iα(x)(3)U(y,x)\mapsto e^{i\alpha(y)}\,U(y,x)\,e^{-i\alpha(x)} \tag{3}

Carrying in the opposite direction is the inverse element, U(x,y)=U(y,x)−1U(x,y)=U(y,x)^{-1}. Then the difference ψ(y)−U(y,x)ψ(x)\psi(y)-U(y,x)\psi(x) is merely multiplied by eiα(y)e^{i\alpha(y)}. Carry before comparing: that is the point.

For two nearby points the comparator is close to 1, and we name the rate of its deviation the field AμA_\mu: U(x+εn,x)=exp⁡(iqε nμAμ(x))+O(ε2)U(x+\varepsilon n,x)=\exp\bigl(iq\varepsilon\,n^\mu A_\mu(x)\bigr)+O(\varepsilon^2). The opposite direction is its inverse, so U(x,x+εn)=exp⁡(−iqε nμAμ(x))+O(ε2)U(x,x+\varepsilon n)=\exp\bigl(-iq\varepsilon\,n^\mu A_\mu(x)\bigr)+O(\varepsilon^2). Carrying the value at x+εnx+\varepsilon n to xx with this before subtracting, and taking the limit of the difference quotient with nn in the direction μ\mu,

Dμψ=lim⁡ε→0U(x,x+εn) ψ(x+εn)−ψ(x)ε=(∂μ−iqAμ)ψ(4)D_\mu\psi=\lim_{\varepsilon\to0}\frac{U(x,x+\varepsilon n)\,\psi(x+\varepsilon n)-\psi(x)}{\varepsilon}=\bigl(\partial_\mu-iqA_\mu\bigr)\psi \tag{4}

This is the covariant derivative. Expanding (3) in y=x+εny=x+\varepsilon n determines how AμA_\mu changes.

ψ↦eiαψ,Aμ↦Aμ+1q ∂μα,Dμψ↦eiαDμψ(5)\psi\mapsto e^{i\alpha}\psi,\qquad A_\mu\mapsto A_\mu+\frac1q\,\partial_\mu\alpha,\qquad D_\mu\psi\mapsto e^{i\alpha}D_\mu\psi \tag{5}

Example. Putting A0=−ϕA_0=-\phi, (A1,A2,A3)=A(A_1,A_2,A_3)=\mathbf A (the notation of 2-04), α=qχ\alpha=q\chi, (5) becomes A↦A+∇χ\mathbf A\mapsto\mathbf A+\nabla\chi, ϕ↦ϕ−∂tχ\phi\mapsto\phi-\partial_t\chi, ψ↦eiqχψ\psi\mapsto e^{iq\chi}\psi. These are (G)(G') of 2-03. From the demand we have arrived at the electromagnetic potentials and their gauge transformations. Multiplying comparators along a path gives the phase factor of 2-03 §05, in geometric language parallel transport (1-07 §03).

Seen on a chain

If space is cut into a sequence of points j=0,1,2,…j=0,1,2,\dots, the comparator becomes a Uj=U(j+1,j)=eiθjU_j=U(j{+}1,j)=e^{i\theta_j} on each edge (2-03 §08, the link variables of 5-01), and instead of the derivative we use the re-compared difference. (3) becomes θj↦θj+αj+1−αj\theta_j\mapsto\theta_j+\alpha_{j+1}-\alpha_j, and

e−iθj′ψj+1′−ψj′=eiαj(e−iθjψj+1−ψj)e^{-i\theta_j'}\psi_{j+1}'-\psi_j'=e^{i\alpha_j}\bigl(e^{-i\theta_j}\psi_{j+1}-\psi_j\bigr)

The sum of squared absolute values does not change, while the sum of naive differences ψj+1−ψj\psi_{j+1}-\psi_j does.

Figure 1 Changing s turns the phase at each point (large circles). With "Connection: on" the comparators on the edges (small circles) also turn by (3), and the sum of re-compared differences does not change. With "Connection: off" it changes
Figure 1
s = 0.00, sum of naive differences = 1.317, sum of re-compared differences = 1.317

ComputedThe numbers in the figure are computed on the spot. Point by point with the connection on, moving ss from 0 to 1 in steps of 0.25, the sum of naive differences is 1.317, 8.070, 19.536, 22.541, 17.700, while the sum of re-compared differences stays 1.317 (with the connection off both are the former; turning everything by the same amount, both are 1.317).

ComputedTable 1 A ring of 12 points (random field and comparators) before and after transformation. WW is the product of the comparators once round (SU(2) is in section 06), and W′W' is the value after the transformation. "Max. entry of W′−WW'-W" is the maximum absolute value of the entries of the difference matrix.

GroupTurningSum of naive differences before → afterSum of re-compared differences before → afterMax. entry of W′−WW'-W∣tr W′−tr W∣\lvert\mathrm{tr}\,W'-\mathrm{tr}\,W\rvert
U(1)point by point65.474 → 50.85683.239 → 83.23900
SU(2)same everywhere82.514 → 82.51475.704 → 75.7041.399×10−169\times10^{-16}
SU(2)point by point82.514 → 85.31075.704 → 75.7040.2391×10−151\times10^{-15}

The change in the sum of re-compared differences is within 3×10−143\times10^{-14} in every case (rounding error). Turning U(1) by the same amount everywhere, no column changes.

04

Making A a dynamical field — the field strength, and the term that cannot be written

To make AμA_\mu a field obeying its own equation, we add to the action a term containing derivatives of AA that does not change under (5). The material is the comparator of a closed path, in which, by (3), all the α\alpha cancel. Going from xx in the direction μ\mu, then in the direction ν\nu, once round a square of side ε\varepsilon, and back to xx,

U□=exp⁡(iqε2Fμν)+O(ε3),Fμν=∂μAν−∂νAμ(6)U_\square=\exp\bigl(iq\varepsilon^2F_{\mu\nu}\bigr)+O(\varepsilon^3),\qquad F_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu \tag{6}

The same quantity also appears in [Dμ,Dν]ψ=−iqFμνψ[D_\mu,D_\nu]\psi=-iqF_{\mu\nu}\psi. The comparator carries from start to end, like the parallel transport of 1-07, and rewriting in the geometric notation Ageom=−iqAA_{\text{geom}}=-iqA, Fgeom=−iqFF_{\text{geom}}=-iqF, (6) becomes exp⁡(−ε2Fgeom)\exp(-\varepsilon^2F_{\text{geom}}), agreeing with (10) of 1-07 and Up≈exp⁡(−a2Fμν)U_p\approx\exp(-a^2F_{\mu\nu}) down to the sign (in 5-01, which reads the lattice links in the opposite direction, the sign of the exponent is reversed). Example. The components are F0i=−EiF_{0i}=-E_i, Fij=εijkBkF_{ij}=\varepsilon_{ijk}B_k (2-04), and FF is the electric and magnetic fields themselves. The electric and magnetic fields were the curvature of the comparator (the deviation after going round a small loop, 1-07 §05). Listing the invariant terms with the lowest order of derivatives,

L=∣Dtψ∣2−∣Dψ∣2−V(∣ψ∣2)+12(∣E∣2−∣B∣2),Dt=∂t+iqϕ,  D=∇−iqA(7)\mathcal L=|D_t\psi|^2-|\mathbf D\psi|^2-V(|\psi|^2)+\tfrac12\bigl(|\mathbf E|^2-|\mathbf B|^2\bigr),\qquad D_t=\partial_t+iq\phi,\ \ \mathbf D=\nabla-iq\mathbf A \tag{7}

The last term is −14FμνFμν-\tfrac14F_{\mu\nu}F^{\mu\nu} ((8) of 2-04). The way of coupling that merely replaces the ∂\partial of (1) by DD is called minimal coupling.

The term that cannot be written. The term −12m2AμAμ=12m2(ϕ2−∣A∣2)-\tfrac12m^2A_\mu A^\mu=\tfrac12m^2(\phi^2-|\mathbf A|^2) that would give AA a mass changes under (5) by terms in −m2q(ϕ ∂tα+A⋅∇α)-\tfrac{m^2}{q}\bigl(\phi\,\partial_t\alpha+\mathbf A\cdot\nabla\alpha\bigr) and the second order of α\alpha. A mass term cannot be written for a field that comes from the gauge principle (as in 2-03 §04) Known. This affects the distance a force reaches in section 05, and becomes a difficulty in section 06.

05

A force appears — coupling to the conserved charge

Expanding (7) in qq, the quantities of section 01 appear as they are.

L=L0−ϕ ρ+A⋅J+q2(ϕ2−∣A∣2)∣ψ∣2+12(∣E∣2−∣B∣2)(8)\mathcal L=\mathcal L_0-\phi\,\rho+\mathbf A\cdot\mathbf J+q^2\bigl(\phi^2-|\mathbf A|^2\bigr)|\psi|^2+\tfrac12\bigl(|\mathbf E|^2-|\mathbf B|^2\bigr) \tag{8}

The gauge field couples to the conserved quantity (2) of the global symmetry, with the same qq that appeared in the transformation. This is exactly the form of (L) of 2-03.

Varying (8) with respect to ϕ\phi gives Gauss's law.

∇⋅E=ρ−2q2ϕ ∣ψ∣2=iq(ψ∗Dtψ−ψ (Dtψ)∗)\nabla\cdot\mathbf E=\rho-2q^2\phi\,|\psi|^2=iq\bigl(\psi^*D_t\psi-\psi\,(D_t\psi)^*\bigr)

The right side is not the ρ\rho of (2) itself but that with its ∂t\partial_t replaced by DtD_t (terms containing ϕ\phi are added). For a point charge QQ at rest at the origin, we put this right side equal to Q δ3(x)Q\,\delta^3(\mathbf x). In the static case E=−∇ϕ\mathbf E=-\nabla\phi, and from −∇2ϕ=Q δ3(x)-\nabla^2\phi=Q\,\delta^3(\mathbf x), ϕ=Q G0(r)\phi=Q\,G_0(r). The energy of a charge Q′Q' at distance rr is

U(r)=QQ′ Gm(r),G0(r)=14πr,Gm(r)=e−mr4πr  (with a mass term added provisionally)(9)\mathcal U(r)=QQ'\,G_m(r),\qquad G_0(r)=\frac{1}{4\pi r},\qquad G_m(r)=\frac{e^{-mr}}{4\pi r}\ \ (\text{with a mass term added provisionally}) \tag{9}

Example. For m=0m=0, charges of the same sign repel, and the force reaches far away like 1/r21/r^2. Merely demanding a local symmetry has produced a force between distant charges. In the theory (7) (when the minimum of VV is at ψ=0\psi=0), adding the forbidden mass term provisionally would give (−∇2+m2)ϕ=ρ(-\nabla^2+m^2)\phi=\rho, and GmG_m (Yukawa type) does not reach much further than about 1/m1/m. Without it, the force is of Coulomb type and reaches far.

However, gauge invariance does not guarantee that a force reaches far. Even classically, with a Higgs field the distance reached becomes finite while gauge invariance is kept (3-07) Known. In terms of (8), when the minimum of VV is at ∣ψ∣2=v2>0|\psi|^2=v^2\gt0 and ∣ψ∣2|\psi|^2 stays there, the term q2(ϕ2−∣A∣2)∣ψ∣2q^2(\phi^2-|\mathbf A|^2)|\psi|^2 has the same form as the mass term 12m2(ϕ2−∣A∣2)\tfrac12m^2(\phi^2-|\mathbf A|^2) of m2=2q2v2m^2=2q^2v^2 ((9) of 3-07 puts the minimum of the size of the field at v/2v/\sqrt2, so the same mass is written m=qvm=qv).

Figure 2 is (−Δlat+m2)Gm=δ(-\Delta_{\mathrm{lat}}+m^2)G_m=\delta found numerically on a cubic lattice (spacing 1) (Δlatf\Delta_{\mathrm{lat}}f is the sum of the values at the six neighbours minus 6f6f).

Figure 2 Changing m changes 4πr·G_m(r) (1 for Coulomb). The solid line is the continuous e^(−mr), the dots the cubic lattice. m > 0 is the case with a mass term added by hand (not gauge invariant)
Figure 2
m = 0.00, rough reach 1/m = ∞, r = 4: lattice 1.020, continuum 1.000

ComputedThe dots are computations on this machine, the solid line is computed on the spot. Static values: for r=1, 4, 12r=1,\,4,\,12 the lattice 4πr G04\pi r\,G_0 is 1.082, 1.020, 1.002, approaching Coulomb further than a few lattice spacings away. 4πr G0.54\pi r\,G_{0.5} is 0.670, 0.147, 0.0027 (the continuous e−0.5re^{-0.5r} is 0.607, 0.135, 0.0025), and the rate of decay along the lattice axis is μ=0.4949\mu=0.4949, from cosh⁡μ=1+m2/2\cosh\mu=1+m^2/2.

06

The same demand for SU(2)

The proton and the neutron have almost equal masses and feel the nuclear force in almost the same way. The isospin view gathers the two into a two-component field ψ=(ψ1,ψ2)\psi=(\psi_1,\psi_2), and the theory of the form (1) does not change under the mixing rotations ψ↦Ωψ\psi\mapsto\Omega\psi (Ω∈SU(2)\Omega\in SU(2), 1-04; to distinguish it from the VV of (1), the matrix is written Ω\Omega, as in 3-02). Yang–Mills (1954) imposed the demand of section 02 on this symmetry.

Making the comparator an SU(2) matrix with U(y,x)↦Ω(y) U(y,x) Ω(x)−1U(y,x)\mapsto\Omega(y)\,U(y,x)\,\Omega(x)^{-1}, and for two nearby points U(x+εn,x)=exp⁡(igε nμAμ)+O(ε2)U(x+\varepsilon n,x)=\exp(ig\varepsilon\,n^\mu A_\mu)+O(\varepsilon^2), Aμ=AμaTaA_\mu=A^a_\mu T^a (Ta=σa/2T^a=\sigma^a/2; relative to the geometric notation of 1-07, Ageom=−igA=−iA^A_{\text{geom}}=-igA=-i\hat A; A^=gA\hat A=gA is the "coupling absorbed" notation of 3-02 §02),

Dμ=∂μ−igAμ,Aμ↦ΩAμΩ−1−ig (∂μΩ)Ω−1,Dμψ↦Ω Dμψ(10)D_\mu=\partial_\mu-igA_\mu,\qquad A_\mu\mapsto\Omega A_\mu\Omega^{-1}-\frac ig\,(\partial_\mu\Omega)\Omega^{-1},\qquad D_\mu\psi\mapsto\Omega\,D_\mu\psi \tag{10}

Example. For Ω=eiα\Omega=e^{i\alpha} (1×11\times1) we return to (5) (gg playing the role of qq), and in geometric notation this is the A↦ΩAΩ−1−(dΩ)Ω−1A\mapsto\Omega A\Omega^{-1}-(d\Omega)\Omega^{-1} of 1-07 §07 (1-07 writes the transformation matrix as gg, but here gg is the coupling constant). There are three differences from U(1).

  1. The number of fields. As many as the dimension of the Lie algebra are needed: 1 for U(1) (the photon), 3 for SU(2) (A1,A2,A3A^1,A^2,A^3), 8 for SU(3) (gluons), N2−1N^2-1 for SU(N).
  2. The gauge field itself is turned. The ΩAΩ−1\Omega A\Omega^{-1} of (10) turns AA even when Ω\Omega is constant (the adjoint representation, 1-04 §06). Unlike the photon, it carries itself the "charge" it couples to. This is why in Table 1 the WW of SU(2) changes as Ω0WΩ0−1\Omega_0W\Omega_0^{-1} even under a global rotation, and only tr W\mathrm{tr}\,W remains; self-interaction comes from here (3-02).
  3. There is one coupling constant. For U(1) a different qq can be put freely for each field. For a simple non-abelian group (1-03 §08) there is only one coupling constant gg, and the strength of the coupling to each matter field is determined by gg and the generators TaT^a of that field's representation (σa/2\sigma^a/2 for a two-component field, (Ta)bc=−iεabc(T^a)_{bc}=-i\varepsilon_{abc} for a three-component field in the adjoint representation) Known. The outline of the reason is that the non-linear term of the field strength −ig[Aμ,Aν]-ig[A_\mu,A_\nu] (section 09, 3-02) ties the normalisation of AA to gg and fixes it, and that if the group is simple the invariant form of the kinetic term is unique up to a constant multiple (2-04 §07, 1-03).

The problem of mass. For SU(2) too, no mass term can be written for the gauge field. In Yang's recollection, at a seminar in Princeton in late February 1954, Pauli asked "what is the mass of this field?" (the story is in the detour of 3-02). The nuclear force is short-range, which does not fit the Coulomb-type reach of section 05. §1 of the Jaffe–Witten problem statement also writes that the absence of mass in the classical waves was a serious obstacle Known, and says it was overcome for the weak force by adding a Higgs field (3-07), and for the strong force by a property of the quantum theory itself (asymptotic freedom, 4-06) Physics. Showing as mathematics the mass gap expected in the latter (4-11) is the task of the problem statement.

07

What the principle decides, and what it does not

The gauge principle is a strong constraint, but it does not determine the theory uniquely (Table 2).

What it decidesWhat it does not decide
That a connection AA is needed, and its transformation laws (5)(10)Which group (choosing U(1), SU(2), SU(3) is up to experiment)
That derivatives can enter only through DD, and that the current coupled to is conservedThe ratios of charges for U(1) (if the group is a circle, the nn of the representation eiα↦einαe^{i\alpha}\mapsto e^{in\alpha} is an integer and charges are in integer ratios; whether it is a circle or the line R\mathbb R lies outside the principle)
That no mass term can be written for the gauge fieldThat the kinetic term is F2F^2 (F4F^4 is also invariant; the reason only low-dimension terms are kept is in 4-04)
That configurations carried into each other by gauge transformations represent the same physicsChoosing minimal coupling (merely replacing ∂\partial by DD). The principle does not forbid non-minimal ways of coupling (∣ψ∣2FμνFμν|\psi|^2F_{\mu\nu}F^{\mu\nu} is also invariant)

An example for the second row of the table. If the group is a circle, the charge of every field is an integer multiple of a single unit. If the group is the line R\mathbb R, the ratios of charges can be any real numbers, and the principle alone gives no reason for charges to line up as integer multiples of one unit. An example for the third row. A term like F4F^4 is of higher order in the fields than F2F^2, and in four dimensions its coefficient has the dimension of length to the fourth power, so it is thought to have less effect the longer the distance (2-04 §08, 4-04 §06) Physics.

A local "symmetry" differs from an ordinary symmetry in producing a constraint (Gauss's law) and a redundancy of description (2-01 §08). How to divide out the redundancy is the subject of 3-04 and 4-08.

There is one more difference from an ordinary symmetry. A symmetry is spontaneously broken when the action (in statistical mechanics, the energy) is symmetric but the equilibrium state (the expectation values) is not. An example is the spontaneous magnetisation of 2-08 §04. Elitzur (1975) argued that in lattice gauge theory without gauge fixing a local symmetry is not spontaneously broken (the expectation values of quantities that are not gauge invariant are 0), and showed it concretely in simple systems on abelian lattices Known.

08

Detour: "gauge" was originally a measuring rod

Detour

A section you may skip.

The words "gauge transformation" and "gauge invariance" first appear in physics in Weyl's 1918 paper attempting to derive gravity and electromagnetism from a single geometry, where they meant changing the standard of length (calibration; the German Eich-, the verb eichen) (O'Raifeartaigh–Straumann §I) Known. Weyl voiced his dissatisfaction with Riemannian geometry, in which the magnitudes of vectors at two distant points can be compared directly (English translation, ibid. §II).

A true infinitesimal geometry should, however, recognize only a principle for transferring the magnitude of a vector to an infinitesimally close point …

(A truly infinitesimal geometry should recognise only a principle for transferring the magnitude of a vector to an infinitely near point.) This is the same idea as the comparator of section 03, except that what is carried is length, not phase. Weyl's theory has a real-valued field wμw_\mu expressing at what rate the standard of length changes from point to point, and carrying a vector along a path γ\gamma from a point pp to a point qq changes its length ℓ\ell as

ℓ(q)=exp⁡(−∫γwμ dxμ) ℓ(p)\ell(q)=\exp\Bigl(-\int_\gamma w_\mu\,dx^\mu\Bigr)\,\ell(p)

((2.2) of O'Raifeartaigh–Straumann; the sign depends on conventions). Going once round a closed path and back, the length is multiplied by a real factor exp⁡(−∮wμ dxμ)\exp\bigl(-\oint w_\mu\,dx^\mu\bigr). As with (6), in a region without holes this factor is 1 for every loop when ∂μwν−∂νwμ=0\partial_\mu w_\nu-\partial_\nu w_\mu=0, and Weyl regarded wμw_\mu as the electromagnetic potential (ibid. §II).

Einstein objected at once: the frequency of an atomic clock would change with the path it had followed, contradicting the stability of atomic spectra Known.

When quantum mechanics appeared, London (1927) realised that making the exponent imaginary turns it into a change of the phase of the wave function (that invariance had been found by Fock (1926)). In his 1928 book and 1929 paper Weyl raised this as "the principle of gauge invariance", and wrote that the electromagnetic field necessarily accompanies the wave field of matter (Jackson–Okun §III.B) Known. The name stayed, derived as it was from the calibration of length. As a metaphor it is "a theory in which the measuring rod can be chosen freely at each point", but precisely, what can be chosen at each point is not a scale of length but a complex phase (in general, a group element). The first non-abelian model was Klein (1938), but it was forgotten, and today's line is held to start from Yang–Mills (1954) (ibid. §V).

09

Where this book is going

In 3-02 the square of (6) is turned with SU(N). Because comparators depend on the order of multiplication, a commutator is added to the field strength, and self-interaction appears.

Fμν=∂μAν−∂νAμ−ig[Aμ,Aν]F_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu-ig[A_\mu,A_\nu]

Imposing Gauss's law in the quantum theory is 4-01. On the lattice of 5-01 the comparators UjU_j are the variables, and the action is built from the products around the squares of (6) (plaquettes). That gg becomes dimensionless in four dimensions is in 2-04 §08 and the four-dimensions article.

To sum up: the demand for a local symmetry calls in a gauge field, that field couples to the conserved charge and carries a force, and classically its mass term cannot be written by hand (adding a Higgs field changes matters; 3-07). The problem statement asks to show that, in the four-dimensional non-abelian case, a mass gap nevertheless arises in the quantum theory (0-03).


What this chapter can say

ItemWhat is saidWhat is not said
Sections 01–05: the covariant derivative (4), the transformation law (5), the field strength (6), that the mass term is not invariant, coupling to the conserved current, the two forms of (9)Standard derivation for classical fields Known. The numbers in Table 1 and Figures 1 and 2 ComputedThe lattice values are for spacing 1; the continuum limit is not taken
The distance a force reachesIn the theory (7) (minimum of VV at ψ=0\psi=0), that without a mass term the force is of Coulomb type and reaches far KnownThat the force reaches far does not follow from gauge invariance alone. The content of the Higgs mechanism is in 3-07
Section 06: the SU(2) transformation law (10), the number of fields, being turned in the adjoint, that there is one coupling constant(10), the number of fields, the turning in the adjoint Known. Only an outline of why there is one coupling constant (2-04 §07, 1-03)The formula for self-interaction (3-02)
The problem of massThat no mass term can be written by hand for the classical gauge field Known. How it was overcome for the strong force is PhysicsThe mass gap of the quantum theory (unsolved; this chapter shows nothing)
Section 07: the standing of the principle, Elitzur's resultThat the principle is a guide for choosing the form of a theory. Elitzur's result at the level of the abstract (argued, and shown in simple systems on abelian lattices)Deriving the principle as a theorem. The content of Elitzur's argument for general groups (the text has not been checked)
The history in section 08What is written in the two reviews KnownThe texts of the original papers (bibliographic data only)

Sources and reproduction

ItemKindSource / tools
Table 1, Figure 1Computedpython3, NumPy (covariant_diff.py). The figure is computed on the spot
The dots of Figure 2, the values in section 05Computedpython3, SciPy (lattice_green.py: Gm(r)=∫0∞e−(m2+6)tIr(2t)I0(2t)2dtG_m(r)=\int_0^\infty e^{-(m^2+6)t}I_r(2t)I_0(2t)^2dt, modified Bessel functions; reproduces the identity G0(0)−G0(1)=1/6G_0(0)-G_0(1)=1/6 to 10 digits). Cross-check by FFT, check_fft.py
Motivation, Pauli's questionKnownC. N. Yang, R. L. Mills, Phys. Rev. 96 (1954) 191 (abstract checked). C. N. Yang, Selected Papers 1945–1980 with Commentary (1983) p. 525 (bibliographic data only; checked through the quotation in O'Raifeartaigh–Straumann §VII)
The obstacle of massless classical waves, and overcoming it by the Higgs field and asymptotic freedomKnownA. Jaffe, E. Witten, Quantum Yang–Mills Theory (the Clay problem statement) §1 (text checked)
Local symmetries are not spontaneously broken (Elitzur)KnownS. Elitzur, Phys. Rev. D 12 (1975) 3978 (abstract checked)
The history in section 08KnownJ. D. Jackson, L. B. Okun, Rev. Mod. Phys. 73 (2001) 663, arXiv:hep-ph/0012061 (§III.B and §V checked). L. O'Raifeartaigh, N. Straumann, Rev. Mod. Phys. 72 (2000) 1, arXiv:hep-ph/9810524 (§I, §II, §V and §VII of the arXiv version checked). Original papers bibliographic data only (from the reference lists of the two reviews): H. Weyl, Sitzungsber. Akad. Wiss. Berlin (1918) 465 / V. Fock, Z. Phys. 39 (1926) 226 / F. London, Z. Phys. 42 (1927) 375 / H. Weyl, Gruppentheorie und Quantenmechanik (Hirzel, Leipzig, 1928) / H. Weyl, Z. Phys. 56 (1929) 330 / O. Klein, in New Theories in Physics (conference in Warsaw, 1938)

Next chapter: 3-02 Non-abelian gauge fields.

← 2-10 The relaxation time and the dynamical exponent zContents3-02 Non-abelian gauge fields →

Revised 2026-10-01: first version.