computo ergo sum

2026-10-01 · chapter Yang–Mills and the mass gapPart 4 Quantisationcanonical quantisation, the Gauss constraint

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

Canonical quantisation and the Hamiltonian — Gauss's law becomes a condition on states

What this chapter shows — The procedure of imposing commutation relations and building the Hamiltonian (canonical quantisation).
That A0A_0 has no momentum, and Gauss's law becomes a condition on states: "unchanged by small gauge transformations".
That this condition removes the flat motion in gauge directions, and on a circle fixes the levels by the Casimir.

Prerequisite chapters — 2-05 (spectrum, gap), 3-03 (action, Gauss's law). For oscillators, 2-06.

Said first — In the four-dimensional continuum theory, the Hamiltonian of this chapter is a formula in form only and has not been constructed as an operator (what is rigorous is the lattice, 5-03, and low-dimensional models). It shows nothing about the mass gap.

Order of this chapter
  1. The procedure of canonical quantisation
  2. A0A_0 has no momentum — a constraint
  3. Quantising in the temporal gauge — wave functionals
  4. Gauss's law is a condition on states — charges and large gauge transformations
  5. Seen in the free field — removing the flat directions (Figure 1, Table 1)
  6. Yang–Mills on a circle — class functions and the Casimir (Figure 2, Table 2, Table 3)
  7. Detour: small boxes, and arguments from wave functionals
  8. The route of solving Gauss's law outright — Gribov
  9. What is formal

01

The procedure of canonical quantisation — making coordinates and momenta into operators

The problem statement defines the mass gap by the spectrum of the Hamiltonian HH (the vacuum is HΩ=0H\Omega=0): “A quantum field theory has a mass gap Δ\Delta if HH has no spectrum in the interval (0,Δ)(0,\Delta) for some Δ>0\Delta\gt0.” (Jaffe–Witten §4) Known. One route to writing down that HH from the classical field is canonical quantisation (the other is 4-02).

With finitely many degrees of freedom there are three steps (2-05). (i) Make the momenta pi=∂L/∂q˙ip_i=\partial L/\partial\dot q_i. (ii) Write H=∑ipiq˙i−LH=\sum_ip_i\dot q_i-L in terms of q,pq,p. (iii) Replace q,pq,p by operators on a Hilbert space and impose the following.

[qi,pj]=i δij(ℏ=1)(1)[q_i,p_j]=i\,\delta_{ij}\qquad(\hbar=1) \tag{1}

On wave functions, pj=−i ∂/∂qjp_j=-i\,\partial/\partial q_j. For fields the index becomes a point x\mathbf x, and δij\delta_{ij} becomes δ3(x−y)\delta^3(\mathbf x-\mathbf y). Example. A scalar field of mass mm splits into an oscillator for each wave number, and the gap was mm (2-06 §08). In Yang–Mills, at step (i) a variable appears for which no momentum can be made.

02

A0A_0 has no momentum — Gauss's law appears as a constraint

The conventions are the same as in 3-03 §01 (ℏ=c=1\hbar=c=1, Dμ=∂μ−igAμD_\mu=\partial_\mu-igA_\mu, (DiX)a=∂iXa+gfabcAibXc(D_iX)^a=\partial_iX^a+gf^{abc}A^b_iX^c on adjoint fields). The colour electric field is

Eia=Fi0a=−∂tAia+(DiA0)a(2)E^a_i=F^a_{i0}=-\partial_tA^a_i+(D_iA_0)^a \tag{2}

and L=12∫∑a(∣Ea∣2−∣Ba∣2) d3xL=\tfrac12\int\sum_a(|\mathbf E^a|^2-|\mathbf B^a|^2)\,d^3x (the magnetic field contains no time derivative). The momentum of AiaA^a_i is Πia=−Eia\Pi^a_i=-E^a_i, but LL does not contain ∂tA0\partial_tA_0, so the momentum of A0A_0 is identically 0.

We write step (ii). What corresponds to ∑ipiq˙i\sum_ip_i\dot q_i is ∫Πia ∂tAia d3x\int\Pi^a_i\,\partial_tA^a_i\,d^3x. Reading (2) as ∂tAi=−Ei+DiA0\partial_tA_i=-E_i+D_iA_0 and substituting,

∫Πia ∂tAia d3x=∫(∣E∣2−E⋅DA0)d3x\int\Pi^a_i\,\partial_tA^a_i\,d^3x=\int\bigl(|\mathbf E|^2-\mathbf E\cdot\mathbf DA_0\bigr)d^3x

follows. Subtracting LL from this leaves 12(∣E∣2+∣B∣2)\tfrac12(|\mathbf E|^2+|\mathbf B|^2) and −∫E⋅DA0-\int\mathbf E\cdot\mathbf DA_0. In the last term, integration by parts moves DD onto E\mathbf E (we take the fields to be 0 far away). The derivative part ∂i\partial_i changes sign by ordinary integration by parts. For the gfabcAibgf^{abc}A^b_i part, fabcf^{abc} changes sign under exchange of indices (it is antisymmetric), so relabelling the indices likewise changes the sign once. So −∫E⋅DA0 d3x=∫A0a(D⋅E)a d3x-\int\mathbf E\cdot\mathbf DA_0\,d^3x=\int A^a_0(\mathbf D\cdot\mathbf E)^a\,d^3x, and

H=∫[12(∣E∣2+∣B∣2)+A0a (D⋅E)a]d3x(3)H=\int\Bigl[\tfrac12\bigl(|\mathbf E|^2+|\mathbf B|^2\bigr)+A^a_0\,(\mathbf D\cdot\mathbf E)^a\Bigr]d^3x \tag{3}

follows (∣E∣2=∑a∣Ea∣2|\mathbf E|^2=\sum_a|\mathbf E^a|^2) Known. A0A_0 is an undetermined multiplier that appears only linearly (the λ\lambda of the toy in 2-01 §08), and its equation (D⋅E)a=0(\mathbf D\cdot\mathbf E)^a=0 is Gauss's law ((3) of 3-03). Such a condition is called a constraint, and its general treatment is said to begin with Dirac (1950).

03

Quantising in the temporal gauge — wave functionals and the electric field operator

We set A0=0A_0=0 by a gauge transformation (the temporal gauge; it is enough to solve ∂tΩ=−ig ΩA0\partial_t\Omega=-ig\,\Omega A_0 at each point). The remaining freedom is time-independent gauge transformations. The coordinates are Aia(x)A^a_i(\mathbf x) and the momenta are the Πia=−Eia\Pi^a_i=-E^a_i of §02. Since Π=−E\Pi=-E, the field version of (1), [A,Π]=iδ[A,\Pi]=i\delta, is

[Aia(x),Ejb(y)]=−i δabδij δ3(x−y)(4)[A^a_i(\mathbf x),E^b_j(\mathbf y)]=-i\,\delta^{ab}\delta_{ij}\,\delta^3(\mathbf x-\mathbf y) \tag{4}

(the sign is negative because E=−ΠE=-\Pi). We represent states by functions of configurations (wave functionals) ψ[A]\psi[A]. For small ϵ\epsilon and a function hia(x)h^a_i(\mathbf x),

ψ[A+ϵh]−ψ[A]≈ϵ∫hia(x) δψδAia(x) d3x\psi[A+\epsilon h]-\psi[A]\approx\epsilon\int h^a_i(\mathbf x)\,\frac{\delta\psi}{\delta A^a_i(\mathbf x)}\,d^3x

the function δψ/δAia(x)\delta\psi/\delta A^a_i(\mathbf x) for which this holds is called the functional derivative. It is the finite-dimensional ψ(q+ϵh)−ψ(q)≈ϵ∑ihi ∂ψ/∂qi\psi(q+\epsilon h)-\psi(q)\approx\epsilon\sum_ih_i\,\partial\psi/\partial q_i with the index ii replaced by the point x\mathbf x and the sum by an integral. Following the p=−i ∂/∂qp=-i\,\partial/\partial q of (1), Πia(x)=−i δ/δAia(x)\Pi^a_i(\mathbf x)=-i\,\delta/\delta A^a_i(\mathbf x), so it acts as Eia(x)=i δ/δAia(x)E^a_i(\mathbf x)=i\,\delta/\delta A^a_i(\mathbf x), and (3) is formally

H=∫[−12δ2δAia(x)2+12BiaBia]d3x(5)H=\int\Bigl[-\tfrac12\frac{\delta^2}{\delta A^a_i(\mathbf x)^2}+\tfrac12B^a_iB^a_i\Bigr]d^3x \tag{5}

(δ2/δAia(x)2\delta^2/\delta A^a_i(\mathbf x)^2 is summed over aa and ii) Known. It can be read as a particle with infinitely many coordinates moving in the potential energy 12∫∣B∣2\tfrac12\int|\mathbf B|^2. Strictly, (5) is form only (§09). Rescaling as A^=gA\hat A=gA,

H=∫[−g22 δ2δA^2+12g2 ∣B^∣2]d3x(6)H=\int\Bigl[-\frac{g^2}{2}\,\frac{\delta^2}{\delta\hat A^2}+\frac{1}{2g^2}\,|\hat{\mathbf B}|^2\Bigr]d^3x \tag{6}

and when gg is large the electric term wins, when small the magnetic term. The coefficients g2/2ag^2/2a and 2N/g2a2N/g^2a in (16) of 5-03 are the lattice version of these two terms. Example. Of the 3(N2−1)3(N^2-1) components AiaA^a_i at each point, the condition of the next section removes N2−1N^2-1 gauge directions, leaving 2(N2−1)2(N^2-1) (the same number as in 3-03 §03). The one component that the classical theory removed with two things, the constraint and the remaining gauge transformations, is removed at once by (10) in the quantum theory.

04

Gauss's law is a condition on states — unchanged by small gauge transformations

Since A0A_0 has been removed, Gauss's law is no longer among the equations of motion. The Gauss operator

Ga(x)=(D⋅E)a=∂iEia+gfabcAibEic(7)G^a(\mathbf x)=(\mathbf D\cdot\mathbf E)^a=\partial_iE^a_i+gf^{abc}A^b_iE^c_i \tag{7}

has three properties Known. (a) It generates gauge transformations. Setting G(α)=∫αaGa d3xG(\alpha)=\int\alpha^aG^a\,d^3x, integration by parts and (4) give

G(α) ψ[A]=−i ddϵ ψ[A+ϵ Dα]∣ϵ=0(8)G(\alpha)\,\psi[A]=-i\,\frac{d}{d\epsilon}\,\psi[A+\epsilon\,D\alpha]\Big|_{\epsilon=0} \tag{8}

(A↦A+ϵDαA\mapsto A+\epsilon D\alpha is (4) of 3-02 with α\alpha taken as gϵαg\epsilon\alpha, that is, an infinitesimal gauge transformation). (b) It commutes with HH. The two terms of (5) are gauge invariant, so [H,Ga(x)]=0[H,G^a(\mathbf x)]=0. (c) It forms a closed algebra.

[Ga(x),Gb(y)]=−ig fabc Gc(x) δ3(x−y)(9)[G^a(\mathbf x),G^b(\mathbf y)]=-ig\,f^{abc}\,G^c(\mathbf x)\,\delta^3(\mathbf x-\mathbf y) \tag{9}

Ga=0G^a=0 cannot be made an operator identity, because the commutator of G(α)G(\alpha) and AjA_j is −i Djα≠0-i\,D_j\alpha\ne0. Instead it is imposed on states.

Ga(x) ψ=0  ⟺  ψ[AΩ]=ψ[A](10)G^a(\mathbf x)\,\psi=0\iff\psi[A^\Omega]=\psi[A] \tag{10}

The Ω\Omega on the right are those continuously connected to the identity transformation. States satisfying (10) are the physical states. By (b) time evolution preserves this subspace, and by (c) the conditions do not contradict one another. Observables are restricted to gauge-invariant ones, and the mass gap is the gap of HH on the physical states (4-11 §09).

Example. For a uniform field of SU(2)SU(2) (a real matrix AiaA^a_i of 3×33\times3; uniform fields are in 3-02 §07), Ga=ig εabcAib ∂/∂Aic=−gLaG^a=ig\,\varepsilon^{abc}A^b_i\,\partial/\partial A^c_i=-gL^a. La=−iεabcAib ∂/∂AicL^a=-i\varepsilon^{abc}A^b_i\,\partial/\partial A^c_i is the angular momentum that turns the colour index, and satisfies [La,Lb]=iεabcLc[L^a,L^b]=i\varepsilon^{abc}L^c. This is the same commutation relation as that of the generators [Ta,Tb]=ifabcTc[T^a,T^b]=if^{abc}T^c (3-02 §02), so G=−gLG=-gL gives the −ig-ig of (9). Gauge-invariant functions are functions of ATAA^{\mathsf T}A and of the sign of det⁡A\det A. With differences we checked that GaG^a annihilates 12∣B∣2\tfrac12|\mathbf B|^2 and det⁡A\det A to within 2×10−102\times10^{-10} but does not annihilate A11A^1_1, and that (9) holds to relative 2×10−112\times10^{-11} Computed.

Charges, and large gauge transformations

If there are static colour charges, the condition is Gaψ=ρaψG^a\psi=\rho^a\psi. The abstract of Kogut–Susskind (1975) describes the gauge-invariant configurations on the lattice as “a collection of strings with quarks at their ends. The strings are lines of non-Abelian electric flux.” Known (Table 3). Also, what (8) generates is only transformations connected to the identity. A transformation TT that approaches 1 far away and has winding number 1 from R3∪{∞}=S3\mathbb R^3\cup\{\infty\}=S^3 to SU(2)SU(2) (3-05 §07) is not connected to the identity. So ψ[AT]=e−iθψ[A]\psi[A^T]=e^{-i\theta}\psi[A] does not contradict (10) (with the convention (Tψ)[A]=ψ[AT](T\psi)[A]=\psi[A^T] it has the same direction as (12) of 3-05; with the opposite convention, e+iθe^{+i\theta}). This is the θ\theta of θ vacua Physics.

05

Seen in the free field — Gauss's law removes the flat directions

With g=0g=0, split the component of wave number k\mathbf k into the longitudinal part aLa_L parallel to k\mathbf k and the transverse part aTa_T perpendicular to it. The magnetic field contains only the transverse part, so writing just one transverse direction,

Hk=12(pT2+pL2)+12∣k∣2aT2(11)H_{\mathbf k}=\tfrac12\bigl(p_T^2+p_L^2\bigr)+\tfrac12|\mathbf k|^2a_T^2 \tag{11}

and Gk∝k⋅Ek∝pLG_{\mathbf k}\propto\mathbf k\cdot\mathbf E_{\mathbf k}\propto p_L. The longitudinal direction is the direction of the gauge transformation A↦A+∇χ\mathbf A\mapsto\mathbf A+\nabla\chi and has no restoring force, so in the whole HH the energy of longitudinal motion piles up continuously on top of each level. Gauss's law pLψ=0p_L\psi=0 removes this continuum, and the Fock space of the transverse oscillators (photons; 2-06 §07) remains Known. Figure 1 closes the longitudinal direction into a circle of length 2R2R (∣k∣=1|\mathbf k|=1) and shows how, of the levels E(n,m)=n+12(πm/R)2E(n,m)=n+\tfrac12(\pi m/R)^2 (m∈Zm\in\mathbb Z), m=0m=0 remain.

Figure 1 Changing the length RR of the longitudinal direction with the knob changes the levels on the left and the gap on the right. Thick lines are states constant along the longitudinal direction (m=0m=0), thin lines states that move along it. On the right the solid line is the gap of the whole space, the dashed line the gap of the states satisfying Gauss's law
R = 4.00: total gap 0.3084, physical 1, levels with E ≤ 3: 16, physical 4

ComputedThe numbers in this figure were computed on this machine (closed formulas computed on the spot; agreeing with Table 1).

ComputedTable 1 The longitudinal length RR and the gap (∣k∣=1|\mathbf k|=1). The number of levels is E≤3E\le3 (always 4 for physical ones)
RTotal gapPhysical gapNumber of levels (total)
21.0000018
40.30843116
320.004821120

The total gap min⁡(1,π2/2R2)\min(1,\pi^2/2R^2) is 0 for R→∞R\to\infty: the gap of HH itself in the temporal gauge is filled by motion in gauge directions. The physical gap ∣k∣|\mathbf k| also tends to 0 as the box is enlarged, and the free field has no mass gap (for a field of mass mm the gap was mm; 2-06 §08).

06

Yang–Mills on a circle — states are class functions of the holonomy

When space is a circle of length LL (1+11+1 dimension) there is no magnetic field, and H=12∫0LEaEa dxH=\tfrac12\int_0^LE^aE^a\,dx. Gauss's law says that EE is carried by parallel transport (1-07), and parallel transport in the adjoint preserves length, so H=L2EaEa(0)H=\tfrac L2E^aE^a(0). All that remains for gauge-invariant functions is the conjugacy class of the holonomy round the circle, U=Pexp⁡(ig∮A1dx)U=P\exp(ig\oint A_1dx). A function unchanged by conjugation U↦gUg−1U\mapsto gUg^{-1} is called a class function, and the trace of a representation matrix a character (1-02). Witten (1992) §4 writes “Ψ must be a class function of U, invariant under conjugation, and so must have an expansion in characters”, and expresses HH by the Casimir operator Known. Ea(0)E^a(0) acts as gg times the derivative that turns UU in the direction TaT^a, and

H χr(U)=g2L2 C2(r) χr(U)(12)H\,\chi_r(U)=\frac{g^2L}{2}\,C_2(r)\,\chi_r(U) \tag{12}

follows (χr\chi_r is the character of the irreducible representation rr, and C2C_2 the value of ∑aTaTa\sum_aT^aT^a; 1-04). The eigenvalues were found exactly by Rajeev (1988), and the route from the transfer matrix is 6-02 §07. Example. For SU(2)SU(2), writing the eigenvalues of UU as e±iθe^{\pm i\theta}, χj=sin⁡((2j+1)θ)/sin⁡θ\chi_j=\sin((2j+1)\theta)/\sin\theta, and the levels are g2L/2g^2L/2 times j(j+1)j(j+1). The gap 38g2L\tfrac38g^2L can be read as the energy of a loop of electric flux running once round the circle (tension 38g2\tfrac38g^2).

The volume of the orbit fixes the levels

The inner product of class functions is taken with Haar measure 2πsin⁡2θ dθ\tfrac2\pi\sin^2\theta\,d\theta. Taking the density 2π1−a02 da0\tfrac2\pi\sqrt{1-a_0^2}\,da_0 (a semicircle) of a0a_0 in 1-08 §03 and setting a0=cos⁡θa_0=\cos\theta gives this form. sin⁡2θ\sin^2\theta is the area of the conjugacy class (a sphere in S3S^3), that is, the volume of the gauge orbit (4-02 §07). Writing (12) with θ\theta,

H=g2L2(−14sin⁡2θddθsin⁡2θddθ)(13)H=\frac{g^2L}{2}\Bigl(-\frac{1}{4\sin^2\theta}\frac{d}{d\theta}\sin^2\theta\frac{d}{d\theta}\Bigr) \tag{13}

and on u=sin⁡θ fu=\sin\theta\,f, g2L8(−u′′−u)\frac{g^2L}{8}(-u''-u), that is, a particle in a box on the interval [0,π][0,\pi] (u=sin⁡nθu=\sin n\theta, n=2j+1n=2j+1) minus 1. If the measure is forgotten and the flat Laplacian is used, the levels change to k2/4k^2/4 (Table 2). In the three-dimensional Coulomb gauge this volume factor appears as the Faddeev–Popov determinant (§08).

Figure 2 A circle of SU(2)SU(2) (g=1g=1). Choose 2j2j and LL and press "Play" to advance time (1 second on screen is time 1); the density (solid line) of θ\theta for the state that superposes χ0\chi_0 and χj\chi_j half and half oscillates with angular frequency Δ=Ej−E0\Delta=E_j-E_0. Making 2j2j or LL larger makes the oscillation faster. The dashed line is the Haar weight; on the right, the levels (12)
2j = 1, L = 2.0: Δ = 0.750, period 2π/Δ = 8.38, phase Δt = 0.00π

ComputedThe numbers in this figure were computed on this machine (characters and the closed formula of (12) computed on the spot; agreeing with Table 2).

ComputedTable 2 Eigenvalues of (13) (in units of g2L/2g^2L/2; differences with 4000 Haar-weighted points), and the k=2jk=2j-th from the bottom of −14d2/dθ2-\tfrac14d^2/d\theta^2 with the measure forgotten (slope 0 at both ends of [0,π][0,\pi]; a periodic function symmetric under θ↦−θ\theta\mapsto-\theta)
2jj(j+1)Differences (Haar)k²/4 with the measure forgotten
000.0000000
10.750.7500000.25
222.0000001
33.753.7499982.25

Counting on the lattice — states that violate Gauss's law

Cut the circle into NN links (a=L/Na=L/N) and set H=g2a2∑ℓEℓ2H=\frac{g^2a}{2}\sum_\ell E_\ell^2 (the two-dimensional version of 5-03 §07; there are no plaquettes). As a metaphor, one link is a top spinning on SU(2)SU(2) (5-03 §06), with (2j+1)×(2j+1)(2j+1)\times(2j+1) states of angular momentum jj for left and right rotations. Precisely, this is the Peter–Weyl theorem, which splits the state space L2(SU(2))L^2(SU(2)) of a link by representation Known. So the energy is g2a2∑ℓjℓ(jℓ+1)\frac{g^2a}{2}\sum_\ell j_\ell(j_\ell+1) and the multiplicity ∏ℓ(2jℓ+1)2\prod_\ell(2j_\ell+1)^2. At a vertex the ends of two links meet, and Gauss's law requires that the combination of their two representations be unchanged by rotation (be a scalar). 00 appears in the coupling of angular momenta j⊗j′=∣j−j′∣⊕⋯⊕(j+j′)j\otimes j'=|j-j'|\oplus\cdots\oplus(j+j') only when j=j′j=j', and then exactly once (Schur's lemma) Known. So neighbouring jj are equal, there is one physical state for each jj, and the levels are (12) regardless of NN.

ComputedTable 3 A lattice circle of SU(2)SU(2) (in units of g2L/2g^2L/2). The lowest physical excitation is always 0.75, and there are 3 physical states with E≤2E\le2
NLowest excitation (total)Number of states with E≤2E\le2 (total)
10.7514
40.1875115,504
160.0468752.44×10²²

The lowest excitation of the whole space is a single link with j=12j=\tfrac12, that is, a state with a pair of charges at its two ends (§04), and its energy 38g2a\tfrac38g^2a is the tension times the distance aa. It tends to 0 as a→0a\to0, so 38g2L\tfrac38g^2L remains only once we restrict to physical states.

07

Detour: small boxes, and arguments from wave functionals

Detour

A section you may skip.

In a three-dimensional periodic box (side ℓ\ell) the uniform components Aia=ciaA^a_i=c^a_i are special. Restricting (5) to these components gives H0=−12ℓ3∂c2+ℓ32∣B(c)∣2H_0=-\frac{1}{2\ell^3}\partial_c^2+\frac{\ell^3}{2}|\mathbf B(c)|^2 (the magnetic field is only the commutator term g c2g\,c^2; 3-02 §07), and rescaling as c=g−1/3ℓ−1yc=g^{-1/3}\ell^{-1}y,

H0=g2/3ℓ[−12∂2∂y2+12∣B1(y)∣2](14)H_0=\frac{g^{2/3}}{\ell}\Bigl[-\tfrac12\frac{\partial^2}{\partial y^2}+\tfrac12|\mathbf B_1(y)|^2\Bigr] \tag{14}

(B1\mathbf B_1 is the magnetic field of g=1g=1). The levels are proportional to g2/3/ℓg^{2/3}/\ell, and if gg is small they lie below the 2π/ℓ2\pi/\ell of the non-uniform components. The abstract of Lüscher (1983) writes “When non-abelian gauge fields are enclosed in a box with periodic boundary conditions, the spectrum of the hamiltonian becomes discrete”, and expands the levels in powers of g2/3g^{2/3} Known. Keeping only two components inside the bracket gives the x2y2x^2y^2 well of 2-05. The small box (the side where gg is small, by asymptotic freedom) is the opposite end from the four-dimensional question, which asks about infinite volume. Lüscher's gg is the renormalised coupling measured at the size of the box, not the classical gg of (14) itself.

Feynman (1981), in 2+12+1 dimensions, after cautioning in the abstract that “Only qualitative or suggestive discussions are made.”, argues that the gauge invariance of the wave functional leads to “a finite energy for any excitation (“glueball”) above the ground state” Physics.

08

The route of solving Gauss's law outright — the Coulomb gauge and Gribov

There is also the route of fixing the gauge further and solving the constraint first. Splitting as E=ET−∇ϕ\mathbf E=\mathbf E_T-\nabla\phi (∇⋅ET=0\nabla\cdot\mathbf E_T=0) in the Coulomb gauge ∇⋅A=0\nabla\cdot\mathbf A=0, Gauss's law is a linear equation for ϕ\phi.

Mϕ=−ρ,M=−∇⋅D(15)M\phi=-\rho,\qquad M=-\nabla\cdot\mathbf D \tag{15}

ρa=gfabcAibET,ic\rho^a=gf^{abc}A^b_iE^c_{T,i} is the colour charge carried by the transverse field itself. If MM can be inverted, then with K=M−1(−∇2)M−1K=M^{-1}(-\nabla^2)M^{-1},

H=12 ⁣∫ ⁣(∣ET∣2+∣B∣2)+12 ⁣∫ ⁣ρ Kρ(16)H=\tfrac12\!\int\!\bigl(|\mathbf E_T|^2+|\mathbf B|^2\bigr)+\tfrac12\!\int\!\rho\,K\rho \tag{16}

(the integral is d3xd^3x) Known. The abstract of Christ–Lee (1980) writes that the change of variables from the temporal gauge produces “an unconventional operator ordering”, and that “new nonlocal interactions, even in the familiar Coulomb gauge” appear Known. The volume factor of the orbit corresponding to the sin⁡2θ\sin^2\theta of §06 is det⁡M\det M Known. This is the Jacobian of changing variables to the gauge condition (coordinates on the slice ∇⋅A=0\nabla\cdot\mathbf A=0), and is called the Faddeev–Popov determinant (details in 4-08). The difficulty is that when AA is large, MM has zero eigenvalues. The abstract of Gribov (1978) writes “the fixing of the divergence of the potential in non-Abelian theories does not fix its gauge” Known. That a slice cannot be chosen globally is Singer's theorem in 3-04. The (10) of the temporal gauge avoids this difficulty.

09

What is formal — the problem of defining the Hamiltonian

In four dimensions (5) lacks meaning in three respects. (i) Eia(x)Eia(x)E^a_i(\mathbf x)E^a_i(\mathbf x) is a product of distributions at the same point (1-11 §09, 1-09 §09). (ii) The sum of zero-point energies 12∣k∣\tfrac12|\mathbf k| diverges (2-06 §09), and with interactions this is paired with renormalisation (4-04). (iii) In the inner product ∫∣ψ∣2DA\int|\psi|^2\mathcal DA, the absence of Lebesgue measure in infinite dimensions (1-09 §02) overlaps with the divergence of the orbit volume (the fact that an interacting HH cannot be placed on the Fock space of the free field, that is, Haag's theorem, is also involved; 4-09).

On the lattice the state space is fixed, and Gauss's law can be imposed exactly at each vertex (Table 3). What remains is whether the gap stays positive in the limit where the lattice spacing goes to 0 and the box to infinity. The problem statement writes “Establishing a quantum mechanical Hilbert space is part of the solution to this Millennium problem.” (§6.5) Known. §6.1 states that the Osterwalder–Schrader construction links the route of Hilbert spaces and the route of functional integrals. §6.5 writes that much of the mathematical progress so far has come from understanding functional integration (“Much of the mathematical progress reviewed above results from understanding functional integration”). On this route HH is reconstructed from the measure in imaginary time (4-02 §08, 4-10 §09). This chapter shows nothing about four-dimensional Yang–Mills.


What this chapter can say

MatterWhat is saidWhat is not said
(1)–(10)Formal derivation Known. Check on uniform fields ComputedMeaning as operators for fields in four dimensions. θ is at the level of physics
(11)–(13), figures, tablesThe free-field model and the levels on a circle Known, differences and counting ComputedThe case of space of two or more dimensions
(14)–(16), detourCounting of scales and classical rewriting KnownTerms from quantum ordering (text not checked). Feynman's argument is qualitative Physics
The mass gap—HH has not been constructed in four dimensions. Nothing is shown

Sources and reproduction

ItemKindSource / tools
The problem statement (§4, §6.1, §6.5)TextA. Jaffe, E. Witten, Quantum Yang–Mills Theory, Clay Math. Inst. (2000)
Class functions and the Casimir on a circleText §4, §4.2E. Witten, J. Geom. Phys. 9 (1992) 303–368, arXiv:hep-th/9204083
The ordering terms of §08 and det⁡M\det MAbstract (text bibliographic data only; the det⁡M\det M term not checked)N. H. Christ, T. D. Lee, Phys. Rev. D 22 (1980) 939
Quotations in §04 and §06–§08AbstractJ. Kogut, L. Susskind, Phys. Rev. D 11 (1975) 395 / S. G. Rajeev, Phys. Lett. B 212 (1988) 203 / M. Lüscher, Nucl. Phys. B 219 (1983) 233 / R. P. Feynman, Nucl. Phys. B 188 (1981) 479 / V. N. Gribov, Nucl. Phys. B 139 (1978) 1
General theory of constraintsBibliographic data onlyP. A. M. Dirac, Can. J. Math. 2 (1950) 129–148 (attribution not checked)
(2)–(10), (15)(16)KnownStandard derivation. Signs recomputed in the conventions of 3-03
The check in §04, Tables 1–3, figuresComputedPython 3.12, NumPy, SciPy (gauss_uniform.py, flat_mode.py, holonomy.py, ring_counts.py). The figures are plain JavaScript

Next chapter to read: 4-02 The path integral and Euclideanisation. The lattice Hamiltonian is in 5-03, gauge fixing in 4-08.

← 3-07 Yang–Mills inside the Standard ModelContents4-02 The path integral and Euclideanisation →

Revised 2026-10-01: first version.