computo ergo sum

2026-10-01 · chapter Yang–Mills and the mass gapPart 4 Quantisationgauge fixing

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

Gauge fixing and Faddeev–Popov — correct locally, and globally the signs cancel

What this chapter shows — Perturbation theory needs gauge fixing, and its procedure (Faddeev–Popov) produces a determinant and ghosts. After fixing, BRST symmetry remains and formally guarantees independence from the choice of gauge. When an orbit meets the condition surface many times (Gribov copies) the procedure breaks down, and on the lattice the cancellation of signs gives 0/0.

Prerequisite chapters — 4-03 (perturbation theory, propagators) and 3-04 (orbit space, the geometry of Gribov copies, Singer's theorem). Grassmann numbers (§03), BRST cohomology (§04) and the Euler characteristic (§08) are defined on the spot, as far as needed.

Said first — Faddeev–Popov and BRST are tools established at each order of perturbation theory, not a non-perturbative definition. The figures and tables are calculations in a planar model and for constant fields in a box. This chapter shows neither the mass gap nor the construction of the theory.

Order of this chapter
  1. Why fix the gauge — the action is flat along the orbits, and no propagator can be made
  2. A finite-dimensional model — "inserting 1" with rotations of the plane
  3. In field theory — writing the determinant as an integral over anticommuting fields (ghosts) (Detour: in the abelian case the ghosts disappear)
  4. BRST symmetry — the symmetry that remains after fixing, and how physical states are chosen
  5. What happens when there are copies — comparing four ways of counting (Figure 1, Table 1; Detour: counting intersections with signs)
  6. The Gribov region and the fundamental modular region — convex and bounded in every direction
  7. The horizon in a box — the larger the box, the closer the horizon is to the origin (Figure 2, Table 2)
  8. The 0/0 on the lattice — counting with signs gives the Euler characteristic 0
  9. Gauge fixing seen from the mass gap problem — its place in the axioms and in attempts at construction

01

Why fix the gauge — no propagator can be made

Conventions: Euclidean R4\mathbb R^4, ℏ=c=1\hbar=c=1, and we write the Hermitian Aμ=AμaTaA_\mu=A^a_\mu T^a and the coupling gg separately (the style of 3-02; the connection of the geometry chapters is A=−igA\mathcal A=-igA).

(Dμω)a=∂μωa+gfabcAμb ωc,δAμa=1g (Dμλ)a,S=14 ⁣∫ ⁣FμνaFμνa d4x(1)(D_\mu\omega)^a=\partial_\mu\omega^a+g f^{abc}A^b_\mu\,\omega^c,\qquad \delta A^a_\mu=\tfrac1g\,(D_\mu\lambda)^a,\qquad S=\tfrac14\!\int\!F^a_{\mu\nu}F^a_{\mu\nu}\,d^4x \tag{1}

Perturbation theory (4-03) uses the inverse of the quadratic part of the action as the propagator. SS does not change under gauge transformations, so the quadratic part is flat in the direction A=∂λA=\partial\lambda and has no inverse.

S2=12 ⁣∫ ⁣d4k(2π)4 A~μa(−k) Kμν(k) A~νa(k),Kμν=k2δμν−kμkν,Kk=0(2)S_2=\tfrac12\!\int\!\tfrac{d^4k}{(2\pi)^4}\,\tilde A^a_\mu(-k)\,K_{\mu\nu}(k)\,\tilde A^a_\nu(k),\qquad K_{\mu\nu}=k^2\delta_{\mu\nu}-k_\mu k_\nu,\qquad Kk=0 \tag{2}

Example. If k=(0,0,0,κ)k=(0,0,0,\kappa), then K=κ2 diag(1,1,1,0)K=\kappa^2\,\mathrm{diag}(1,1,1,0), and the fourth component does not appear in the action Computed. On Wilson's lattice, where the volume of the orbits (4-02 §07) is finite, no fixing is needed (5-01 §06) Known. It is needed when one expands around A=0A=0 while staying in the continuum.

Let us put into words why there is no inverse. The path integral ∫DA e−S\int\mathcal DA\,e^{-S} (4-02) adds up all fields related by gauge transformations (one orbit). Along the orbit e−Se^{-S} does not change, so the Gaussian integral in that direction does not decay and diverges. Speaking in metaphor, the bottom of the valley is a single trench, flat without end along the trench. Precisely, the kernel KK of the quadratic form (2) has eigenvalue 0 in the direction of kk. So we would like to take the integral along the orbit outside, choose one representative from each orbit and add up the rest. We first see how to take it out in a finite-dimensional model.

02

A finite-dimensional model — Faddeev–Popov with rotations of the plane

The weight e−S(∣x∣)e^{-S(|x|)} on the plane does not change under the rotation RθR_\theta, and the orbits are circles centred at the origin. Here the angle of rotation θ\theta plays the role of "the direction of the orbit". The aim is to bring the integral over θ\theta to the surface without changing the value of ZZ, and for that we put a rewritten 1 into ZZ. We use the rule for the one-variable δ\delta function.

∫dθ δ(G(θ)) ∣G′(θ0)∣=1(G has a single point θ0 where it equals 0 and no other)\int d\theta\,\delta\bigl(G(\theta)\bigr)\,\bigl|G'(\theta_0)\bigr|=1\qquad(G\ \text{has a single point}\ \theta_0\ \text{where it equals}\ 0\ \text{and no other})

If the condition G(x)=0G(x)=0 meets each circle exactly once, θ↦G(Rθx)\theta\mapsto G(R_\theta x) vanishes at a single point only, so the following "insertion of 1" holds.

1=ΔG(x) ⁣∫02π ⁣ ⁣dθ δ(G(Rθx)),ΔG(x)=∣∂∂θG(Rθx)∣G(Rθx)=0(3)1=\Delta_G(x)\!\int_0^{2\pi}\!\!d\theta\,\delta\bigl(G(R_\theta x)\bigr),\qquad \Delta_G(x)=\Bigl|\tfrac{\partial}{\partial\theta}G(R_\theta x)\Bigr|_{G(R_\theta x)=0} \tag{3}

Putting this into Z=∫d2x e−SZ=\int d^2x\,e^{-S} and changing variables x→Rθ−1xx\to R_\theta^{-1}x, since d2xd^2x, SS and ΔG\Delta_G do not change under rotation, the integral over θ\theta leaves the volume of the group 2π2\pi.

Z=2π ⁣∫ ⁣d2x δ(G(x)) ΔG(x) e−S(∣x∣)(4)Z=2\pi\!\int\!d^2x\ \delta\bigl(G(x)\bigr)\,\Delta_G(x)\,e^{-S(|x|)} \tag{4}

This is the whole of the Faddeev–Popov procedure, and the weight ΔG\Delta_G on the surface is the Faddeev–Popov determinant.

Example. Taking the condition to be the positive x1x_1 axis (G=x2G=x_2, x1>0x_1\gt0), ΔG=r\Delta_G=r, and (4) is Z=2π∫0∞r e−SdrZ=2\pi\int_0^\infty r\,e^{-S}dr: the Jacobian of polar coordinates. The determinant measures the size of the orbit (the same role as the Weyl factor in 3-04 §04).

03

In field theory — the determinant and ghosts

We repeat (3)(4) with the group taken to be all pointwise gauge transformations and the condition Ga=∂μAμa−ωaG^a=\partial_\mu A^a_\mu-\omega^a. Since δGa=1g∂μ(Dμλ)a\delta G^a=\frac1g\partial_\mu(D_\mu\lambda)^a, the content of the determinant is the following M\mathcal M. The constant factor 1/g1/g and the sign become an overall constant of the determinant, absorbed into the overall constant of ZZ (which cancels in ratios of expectation values), so we drop them.

M=−∂μDμ,Z=∫DA det⁡M δ(∂μAμ−ω) e−S(5)\mathcal M=-\partial_\mu D_\mu,\qquad Z=\int\mathcal DA\,\det\mathcal M\ \delta(\partial_\mu A_\mu-\omega)\,e^{-S} \tag{5}

Averaging ω\omega with the weight e−∫ω2/2αe^{-\int\omega^2/2\alpha} (many references write the parameter as ξ\xi, but this book uses ξ\xi for the correlation length, so we write α\alpha; the same letter as in 4-03), the δ\delta function turns into a term of the action, and the quadratic form acquires an inverse.

S+12α ⁣∫(∂μAμa)2,Dμνα(k)=1k2(δμν−(1−α)kμkνk2)(6)S+\tfrac1{2\alpha}\!\int(\partial_\mu A^a_\mu)^2,\qquad D^\alpha_{\mu\nu}(k)=\frac1{k^2}\Bigl(\delta_{\mu\nu}-(1-\alpha)\frac{k_\mu k_\nu}{k^2}\Bigr) \tag{6}

α=1\alpha=1 is the Feynman gauge and α→0\alpha\to0 the Landau gauge (the inverse checked numerically Computed). To make det⁡M\det\mathcal M a term of the action as well, we use anticommuting numbers (Grassmann numbers: θiθj=−θjθi\theta_i\theta_j=-\theta_j\theta_i, θi2=0\theta_i^2=0). The rules are ∫dθ 1=0\int d\theta\,1=0 and ∫dθ θ=1\int d\theta\,\theta=1. Since the expansion stops at e−aθˉθ=1+aθθˉe^{-a\bar\theta\theta}=1+a\theta\bar\theta,

∫dθˉ dθ e−aθˉθ=a,∫ ⁣∏idθˉidθi e−θˉMθ=det⁡M(7)\int d\bar\theta\,d\theta\,e^{-a\bar\theta\theta}=a,\qquad \int\!\prod_i d\bar\theta_id\theta_i\,e^{-\bar\theta M\theta}=\det M \tag{7}

Known. The determinant comes out with its sign (the source of the 0/0 of §08). In this way the determinant becomes an integral over anticommuting fields ca,cˉac^a,\bar c^a (ghosts; a different meaning from the "ghost" in 4-10, which refers to the negative-weight states of Pauli–Villars).

det⁡M=∫Dcˉ Dc e−∫cˉa(Mc)a,cˉa(Mc)a≃∂μcˉa∂μca+gfabc(∂μcˉa)Aμbcc(8)\det\mathcal M=\int\mathcal D\bar c\,\mathcal Dc\ e^{-\int\bar c^a(\mathcal Mc)^a},\qquad \bar c^a(\mathcal Mc)^a\simeq\partial_\mu\bar c^a\partial_\mu c^a+g f^{abc}(\partial_\mu\bar c^a)A^b_\mu c^c \tag{8}

(≃\simeq is integration by parts.) A ghost propagator δab/k2\delta^{ab}/k^2 and a vertex proportional to gfabcpμg f^{abc}p_\mu come out Known. Ghosts are not particles that come out, and appear only inside loops (they also enter the β function: 4-06 §03). Example. A real Gaussian integral in nn components gives (det⁡A)−1/2(\det A)^{-1/2} (2-07 §02). In the Feynman gauge (α=1\alpha=1) with g=0g=0 the kernel is k2δμνk^2\delta_{\mu\nu}, so at each momentum the 4 components of the gauge field give (k2)−4/2(k^2)^{-4/2} and the ghosts give (k2)+1(k^2)^{+1} by (7), together (k2)−2/2(k^2)^{-2/2}: only the two transverse polarisations remain (4−2=24-2=2).

Detour: in the abelian case the ghosts disappear

Detour

A subsection you may skip.

For U(1)U(1), fabc=0f^{abc}=0, so M=−∂2\mathcal M=-\partial^2 does not depend on AA, and det⁡M\det\mathcal M cancels in ratios as a constant. No ghosts are needed. In the non-abelian case M\mathcal M depends on AA, so the determinant couples to the field and ghost loops join the diagrams. The abstract of Faddeev–Popov (1967) writes that Feynman and DeWitt showed that in gauge-invariant field theories the rules for closed loops must be changed Known. The change of rules is needed when this M\mathcal M depends on AA.

04

BRST symmetry — the symmetry that remains after fixing

The fixed action still has an anticommuting symmetry ss that mixes the gauge field and the ghosts (with an auxiliary field bab^a added).

sAμa=(Dμc)a,sca=−g2fabccbcc,scˉa=iba,sba=0;S+ ⁣∫ ⁣sΨ,  Ψ=cˉa(∂μAμa−iα2ba)(9)sA^a_\mu=(D_\mu c)^a,\quad sc^a=-\tfrac g2f^{abc}c^bc^c,\quad s\bar c^a=ib^a,\quad sb^a=0;\qquad S+\!\int\!s\Psi,\ \ \Psi=\bar c^a\bigl(\partial_\mu A^a_\mu-\tfrac{i\alpha}2b^a\bigr) \tag{9}

sΨ=ib ∂A+α2b2+cˉ Mcs\Psi=ib\,\partial A+\frac\alpha2b^2+\bar c\,\mathcal Mc, and integrating out bb returns to (6)(8). From sS=0sS=0 and nilpotency s2=0s^2=0 (the Jacobi identity), two things follow formally Known.

"BRST" is said to be the initials of Becchi, Rouet, Stora and Tyutin. Example. Computing s2s^2 symbolically on the part with constant fields, s2Aas^2A^a and s2cas^2c^a had 0 terms for both SU(2) and SU(3). Changing the coefficient −12-\tfrac12 of scsc to −1-1 leaves 2 terms and 25 terms in s2Aas^2A^a Computed.

05

What happens when there are copies — four ways of counting

We build a case in which the "exactly once" of (3) breaks down. Following the Landau gauge (3-04 §05), we take critical points of FF on the circle as representatives, M=∂φ2FM=\partial_\varphi^2F as the determinant, and the set of local minima as the analogue of the Gribov region.

F=−rcos⁡φ−c r2cos⁡3φ:r<r∗=13c gives 2 copies (1 minimum, 1 maximum),r>r∗ gives 6 (3 minima, 3 maxima)(10)F=-r\cos\varphi-c\,r^2\cos3\varphi:\qquad r\lt r_*=\tfrac1{3c}\ \text{gives 2 copies (1 minimum, 1 maximum)},\quad r\gt r_*\ \text{gives 6 (3 minima, 3 maxima)} \tag{10}

For large fields pairs of a local minimum and a local maximum are born, and at those points (0,±r∗)(0,\pm r_*), M=0M=0 (the analogue of the horizon). With the weight e−r2/2e^{-r^2/2} we count r2r^2 (true expectation value 2) in four ways (for the difference between ∣M∣|M| and MM, see the detour of this section): (i) all copies with ∣det⁡∣|\det|, (ii) only the Gribov region (local minima), (iii) only the global minimum of FF (the fundamental modular region), (iv) with signs (the BRST way of counting).

Figure 1 Moving c and r changes the intersections (copies) of the condition surface with the orbit in the plane (left or top) and F(φ) on the circle (right or bottom). ● local minimum (Gribov region), ○ local maximum, green ● global minimum (fundamental modular region), ◇ horizon
c = 0.20, r = 1.20: copies 2, sum of signs 0
⟨r²⟩: true 2.000, |det| 2.924, Gribov region 2.924, global min 2.000, signed 0/0

ComputedThe numbers in this figure were computed on this machine (the closed formulas of formula (10) and Table 1 evaluated on the spot; Table 1 agrees with a brute-force count of critical points to within 0.004).

Table 1 Four ways of counting ⟨r²⟩ (true value 2). Closed formula 4+8e−u(1+u)2+4e−u\frac{4+8e^{-u}(1+u)}{2+4e^{-u}}, u=1/(18c2)u=1/(18c^2)
ccr∗r_*(i) ∣det⁡∣|\det|(ii) Gribov region(iii) Global minimum(iv) With signs
0.084.1672.0058962.00589620/0
0.201.6672.9243252.92432520/0
0.500.6672.2736012.27360120/0

When the number of copies varies from orbit to orbit, (i) is off, and (ii), which leaves copies inside the region, is not fixed either. (iii) is correct, but choosing the global minimum is a global comparison and cannot be written as a local condition. (iv) is 0/0, since local minima and local maxima come in equal numbers.

Example. The error of (i), 4ue−u/(1+2e−u)4ue^{-u}/(1+2e^{-u}) (2×10−82\times10^{-8} at c=0.05c=0.05), is 0 at every order in powers of cc, the same type as e−1/xe^{-1/x} in 4-07 §05 Computed.

Detour: counting intersections with signs

Detour

A subsection you may skip. We look at the difference between ∣M∣|M| and MM in (10) with one variable on a circle.

Take the group to be the circle θ∈[0,2π)\theta\in[0,2\pi), the condition a periodic function f(θ)=0f(\theta)=0, and its zeros θi\theta_i (with f′≠0f'\ne0 there). From the rule for the δ\delta function, ∫δ(f) u dθ=∑iu(θi)/∣f′(θi)∣\int\delta(f)\,u\,d\theta=\sum_iu(\theta_i)/|f'(\theta_i)|,

∫02π ⁣dθ δ(f(θ)) ∣f′(θ)∣=#{θi},∫02π ⁣dθ δ(f(θ)) f′(θ)=∑isign⁡f′(θi)=0(10a)\int_0^{2\pi}\!d\theta\ \delta\bigl(f(\theta)\bigr)\,|f'(\theta)|=\#\{\theta_i\},\qquad \int_0^{2\pi}\!d\theta\ \delta\bigl(f(\theta)\bigr)\,f'(\theta)=\sum_i\operatorname{sign}f'(\theta_i)=0 \tag{10a}

The right-hand side is 0 because a periodic function crosses 0 upwards as many times as it crosses downwards. Example: for f(θ)=sin⁡(θ−θA)f(\theta)=\sin(\theta-\theta_A) there are two intersections; the left-hand side is 2 and the right-hand side 1−1=01-1=0. With absolute values the number of intersections remains; without them, the cancellation of signs. The relation to the obstruction to BRS-invariant gauge fixing done non-perturbatively on the lattice (Neuberger 1987; the abstract writes that it is formally present in the continuum as well) is treated in §08.

06

The Gribov region and the fundamental modular region — convex and bounded in every direction

The abstract of Gribov (1978) writes that in the non-abelian case fixing ∂μAμ\partial_\mu A_\mu does not fix the gauge, and that restricting to the range where the FP determinant is positive seems to be enough Known. Reading the Landau gauge as the stationary points of the norm ∥Ag∥2\|A^g\|^2,

Ω={∂μAμ=0, M(A)>0} (local minima),Λ={A: ∥A∥≤∥Ag∥ ∀g} (global minima),Λ⊂Ωˉ(11)\Omega=\{\partial_\mu A_\mu=0,\ \mathcal M(A)\gt0\}\ (\text{local minima}),\qquad \Lambda=\{A:\ \|A\|\le\|A^g\|\ \forall g\}\ (\text{global minima}),\qquad \Lambda\subset\bar\Omega \tag{11}

Ω\Omega is the Gribov region, its boundary the horizon, and Λ\Lambda the fundamental modular region Known. Ωˉ\bar\Omega is the closure of Ω\Omega (including its boundary). Ω\Omega is an open set given by M>0\mathcal M\gt0, and Λ\Lambda a closed set given by ≤\le; the boundary of Λ\Lambda has points touching the horizon (van Baal, §07), so we write it with the closure.

The solid line in Figure 1 is the analogue of Ω\Omega, and the positive x1x_1 axis the analogue of Λ\Lambda. For the effect on the propagator, see 7-02 §07.

07

The horizon in a box — eigenvalues in a constant background field

Taking a constant SU(2) field Aμa=a δa3δμ1A^a_\mu=a\,\delta^{a3}\delta_{\mu1} in a periodic box of side LL, M\mathcal M is diagonalised by plane waves p=2πn/Lp=2\pi n/L, and splits into colour component 3 (neutral) and ω1±iω2\omega^1\pm i\omega^2 (charged).

λneutral=(2πL)2∣n∣2,λ±=(2πL)2(∣n∣2±s n1),s=gaL2π(12)\lambda_{\text{neutral}}=\bigl(\tfrac{2\pi}L\bigr)^2|n|^2,\qquad \lambda_\pm=\bigl(\tfrac{2\pi}L\bigr)^2\bigl(|n|^2\pm s\,n_1\bigr),\qquad s=\frac{gaL}{2\pi} \tag{12}

The smallest non-trivial eigenvalue (excluding n=0n=0) is 1−s1-s at n=(±1,0,0,0)n=(\pm1,0,0,0), and the horizon is at

g ah=2π/L ⟶ 0(L→∞)(13)g\,a_{\rm h}=2\pi/L\ \longrightarrow\ 0\quad(L\to\infty) \tag{13}

van Baal (the section "Gauge fields on the three-torus" of 1997) does the same calculation in the Coulomb gauge on the three-torus with C=gaLC=gaL, and shows that the Gribov region is the cube ∣Ck∣≤2π|C_k|\le2\pi and that copies of A=0A=0 under twisted (antiperiodic) gauge transformations lie on the horizon Known. The fundamental modular region is ∣Ck∣≤π|C_k|\le\pi (s≤12s\le\frac12) when antiperiodic transformations are also identified (pure Yang–Mills). When there are fields in the fundamental representation (quarks) and only periodic transformations are allowed, it is ∣Ck∣≤2π|C_k|\le2\pi (s≤1s\le1), and its boundary touches the horizon Known.

Figure 2 Moving s (the size of the background) moves the eigenvalues of the FP operator (in units of (2π/L)², with transverse n equal to 0). Grey is neutral, blue and orange charged, red negative. The "boundary of Λ (s = 0.5)" in the readout is the value when antiperiodic transformations are also identified (s = 1 with periodic transformations only)
s = 0.30: smallest non-trivial eigenvalue 0.70 ×(2π/L)²

ComputedThe numbers in this figure were computed on this machine (formula (12) evaluated on the spot). At s=0s=0, 0.5, 1 and 2 the smallest non-trivial eigenvalue is 1, 0.5, 0 and −1 (in order: A=0A=0, the boundary of the fundamental modular region [when antiperiodic transformations are also identified], the horizon, and the copy of A=0A=0 under a periodic transformation).

We also checked on the lattice. On an L4L^4 lattice, setting the links in direction 1 to eiθσ3/2e^{i\theta\sigma_3/2} and diagonalising the second derivative of the Landau gauge functional ∑(1−12Re tr gxUx,μgx+μ†)\sum(1-\tfrac12\mathrm{Re\,tr}\,g_xU_{x,\mu}g^\dagger_{x+\mu}) momentum by momentum, the charged eigenvalues agreed with 12[cos⁡θ2−cos⁡(p1±θ2)]+12∑ν≠1(1−cos⁡pν)\tfrac12[\cos\tfrac\theta2-\cos(p_1\pm\tfrac\theta2)]+\tfrac12\sum_{\nu\ne1}(1-\cos p_\nu) (with lattice spacing 1, θ=ga\theta=ga).

Table 2 The horizon of the lattice FP matrix (bisection)
LL481632
θhL/2π\theta_{\rm h}L/2\pi1.0000001.0000001.0000001.000000

Computedpython3, NumPy. The difference from the closed formula is at most 3×10−163\times10^{-16}.

The larger the box, the closer to the origin the horizon is in long-wavelength directions, and the abstract of Gribov writes that this restriction cancels the infrared singularity and leads to a linear interaction at long distances Physics. It has not become a theorem about the four-dimensional measure.

08

The 0/0 on the lattice — it vanishes when counted with signs

The ghosts gave det⁡M\det\mathcal M without absolute value (formula (7)). So the integral of BRST-symmetric gauge fixing counts the copies on an orbit with sign⁡det⁡M\operatorname{sign}\det\mathcal M.

ZGF[U]=∫∏xdgx δ(G(Ug))det⁡M(Ug)=∑copiessign⁡det⁡M=χ(G)N=0(14)Z_{\rm GF}[U]=\int\prod_x dg_x\ \delta\bigl(G(U^g)\bigr)\det\mathcal M(U^g)=\sum_{\text{copies}}\operatorname{sign}\det\mathcal M=\chi(G)^N=0 \tag{14}

We define the words used here. The Euler characteristic χ\chi: the sum over the critical points (those whose matrix of second derivatives is non-degenerate) of a smooth function on a compact manifold without boundary (1-05), each counted with the sign of the determinant of that matrix (+1+1 if the number of negative eigenvalues is even, −1-1 if odd). This number does not depend on the choice of function (the Poincaré–Hopf theorem). On a circle a minimum counts +1+1 and a maximum −1-1, giving χ(S1)=0\chi(S^1)=0; on the sphere χ(S2)=2\chi(S^2)=2. For a compact connected Lie group GG of positive dimension χ(G)=0\chi(G)=0, and for product spaces χ(GN)=χ(G)N\chi(G^N)=\chi(G)^N Known. Morse theory is the name of the theory that reads the shape of a manifold by counting critical points in this way.

The last two equalities read the sum of signs as the Euler characteristic of GNG^N (NN is the number of lattice points) (Schaden 1999's interpretation via Morse theory, formula (2) of Mehta et al. 2014; on orbits whose critical points are non-degenerate), and χ(G)=0\chi(G)=0 Known (6-11 §05). Expectation values of gauge-invariant quantities are 0/0. Mehta et al. call this "Neuberger's 0/0 problem" and cite Neuberger's papers of 1986 and 1987, and the abstract of the 1987 paper says that this obstruction met non-perturbatively is formally present in the continuum formulation as well Known.

Example. The "sum of signs 0" in Figure 1 is its smallest version (χ(S1)=0\chi(S^1)=0). The same abstract also argues that at every order of the perturbative expansion the BRS invariance of the lattice does the job of local gauge invariance. This is because the cancellation of signs does not show up at any order of perturbation theory, the same type as e−1/(18c2)e^{-1/(18c^2)} in the example of §05. The ways around it change the way of counting Known.

For a comparison with the algebra of divergences, see 6-12.

09

Gauge fixing seen from the mass gap problem

What the problem statement asks for are correlations of gauge-invariant local fields (such as tr FμνFρσ\mathrm{tr}\,F_{\mu\nu}F_{\rho\sigma}) and the gap of the reconstructed Hamiltonian (0-03). Gauge fixing is an indispensable tool in perturbation theory (§04). Elsewhere it has the following place Known.

What Singer's theorem forbids is only continuous global slices, and the 0/0 too is a phenomenon of fixing a covariant gauge BRST-symmetrically over the whole lattice. The remaining question is still "does the measure of gauge-invariant correlations exist in the four-dimensional continuum limit, and does the spectrum have a gap".


What this chapter can say

Content
What is saidThe formal derivation of (3) to (9) Known. Table 1, Table 2, the numbers in the figures, the symbolic calculation of s2s^2 Computed. (10a) in the detour Paper (elementary)
ConditionalThe Slavnov identities to all orders of perturbation theory in massive linear gauges; unitarity and gauge independence in the perturbative sense in the Higgs–Kibble model. The unitarity of Kugo–Ojima within a framework that assumes the theory exists Physics. The properties of the Gribov region checked at the level of abstracts. (14) on non-degenerate orbits. The effect on the infrared Physics
What is not saidThe arrangement of copies in the four-dimensional continuum theory, the measure on the fundamental modular region, the identification of the BRST and OS spaces. Neuberger's argument only as far as the abstract. This site shows neither the mass gap nor the construction of the continuum theory

Sources and reproduction

ItemKindSource / tools
The procedure, Gribov copiesKnownL. D. Faddeev, V. N. Popov, Phys. Lett. B 25 (1967) 29; V. N. Gribov, Nucl. Phys. B 139 (1978) 1 (abstracts)
BRST, unitarityKnownC. Becchi, A. Rouet, R. Stora, Commun. Math. Phys. 42 (1975) 127 (the abelian Higgs–Kibble model; bibliographic data only); Ann. Phys. 98 (1976) 287 (abstract); T. Kugo, I. Ojima, Prog. Theor. Phys. Suppl. 66 (1979) 1 (abstract). I. V. Tyutin, arXiv:0812.0580 (bibliographic data only)
The Gribov regionKnownD. Zwanziger, Nucl. Phys. B 209 (1982) 336; G. Dell'Antonio, D. Zwanziger, Commun. Math. Phys. 138 (1991) 291; D. Zwanziger, Phys. Rev. D 69 (2004) 016002 (abstracts); P. van Baal, hep-th/9711070 (text of the sections "Complete gauge fixing" and "Gauge fields on the three-torus")
The 0/0 on the lattice and ways around itKnownH. Neuberger, Phys. Lett. B 175 (1986) 69 (bibliographic data only); Phys. Lett. B 183 (1987) 337 (abstract only); D. Mehta, N. S. Daleo, J. D. Hauenstein, C. Seaton, Phys. Rev. D 90 (2014) 054504, arXiv:1406.6678 (abstract, text §I, §II); M. Schaden, Phys. Rev. D 59 (1999) 014508 (bibliographic data only); L. von Smekal et al. arXiv:0710.2410 (abstract); M. Ghiotti et al. hep-th/0611058 (abstract)
Quotations in §09KnownA. Jaffe, E. Witten, "Quantum Yang–Mills Theory" (Clay) §6.5; I. Chevyrev, H. Shen, arXiv:2302.12160 (abstract); J. Magnen, V. Rivasseau, R. Sénéor, Commun. Math. Phys. 155 (1993) 325 (via the quotation in 4-10 §09)
Tables, figures, the numbers in §01, §03, §04Computedpython3, NumPy (toy_fp, box_horizon, lattice_formula_check, brst_nilpotent, propagator_check). The figures evaluate formulas (10)(12) in JavaScript

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