computo ergo sum

2026-10-01 · chapter Yang–Mills and the mass gapPart 4 Quantisationthe algebra of divergences

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 algebra of divergences — nested subtraction becomes a decomposition in a group, yet still does not leave formal power series

What this chapter shows — Three prescriptions for subtracting nested divergences (BPHZ, Epstein–Glaser, dimensional regularisation). That subtraction becomes a Birkhoff decomposition of a group in the Hopf algebra of Connes–Kreimer (computed in a small model). Costello's families of effective actions, and where all this falls short of the mass gap.

Prerequisite chapters — 4-04 Divergences and renormalisation. Helpful: 1-11 (distributions), 4-03 (Feynman diagrams).

Said first — This is a guide to known results at the level of formal power series, and shows nothing about the existence of Yang–Mills theory or the mass gap. The small model is for seeing the algebraic structure, not a four-dimensional calculation.

Order of this chapter
  1. Nested divergences — seen in a small model: subtracting only the whole leaves the outer scale
  2. The forest formula — BPHZ: subtract from the inside, and count the sets to subtract by forests
  3. Extension in position space — Epstein–Glaser: the freedom is δ and its derivatives
  4. Moving the dimension continuously — dimensional regularisation: divergences become poles 1/ε. The MS scheme
  5. The algebra of diagrams — the Hopf algebra of Connes–Kreimer: the coproduct writes the extraction
  6. Birkhoff decomposition — subtraction becomes a decomposition in a group: counterterms are one factor. Detour: rooted trees and Runge–Kutta methods
  7. Families of effective actions — Costello: a family of actions, one for each scale
  8. Where the algebra reaches and where it does not: the measure and exp(−1/g²) lie outside

01

Nested divergences — seen in a small model

In 4-04 we removed one-loop divergences by subtracting the value at a reference scale μ\mu. What was subtracted was a number independent of the external momenta (a counterterm). From two loops on, a part of a diagram (a subdiagram) diverges on its own (a subdivergence). Two subdivergences are either nested, one containing the other, overlapping, sharing a part without either containing the other, or disjoint.

We use a small model with nesting only (Kreimer's toy model; the definition in §3.2 of Panzer 2012). "One loop" is ∫0∞dy/(y+s)\int_0^\infty dy/(y+s), where s>0s\gt0 is the outer scale and yy the loop variable. Like the four-dimensional bubble it diverges logarithmically, so we regularise by multiplying by y−zy^{-z} (zz is a small positive number, corresponding to the ε\varepsilon of §04), and build nesting by putting the inner value into the outer integrand.

φ(∙)(s)=∫0∞y−z dyy+s=s−zF(z),F(z)=πsin⁡πz=1z+π26z+⋯(1)\varphi(\bullet)(s)=\int_0^\infty\frac{y^{-z}\,dy}{y+s}=s^{-z}F(z),\qquad F(z)=\frac{\pi}{\sin\pi z}=\frac1z+\frac{\pi^2}{6}z+\cdots \tag{1} φ(ℓ2)(s)=∫0∞y−zy+s φ(∙)(y) dy=s−2zF(z) F(2z)(2)\varphi(\ell_2)(s)=\int_0^\infty\frac{y^{-z}}{y+s}\,\varphi(\bullet)(y)\,dy=s^{-2z}F(z)\,F(2z) \tag{2}

Writing the part with negative powers of zz (the pole part) as pole⁡\operatorname{pole}, with L=ln⁡(s/μ)L=\ln(s/\mu) and μ=1\mu=1,

pole⁡φ(∙)=1z,pole⁡φ(ℓ2)=12z2−Lz(3)\operatorname{pole}\varphi(\bullet)=\frac1z,\qquad \operatorname{pole}\varphi(\ell_2)=\frac{1}{2z^2}-\frac{L}{z} \tag{3}

Computed The pole of the double loop contains LL. Subtracting only the pole of the whole, the subtracted quantity contains ln⁡s\ln s and is not a local term that can be added to the action. Example: at z=0.1z=0.1, L=1L=1, φ(ℓ2)=44.49\varphi(\ell_2)=44.49, and its pole part is 50−10=4050-10=40.

02

The forest formula — BPHZ

The cure is to subtract from the inside. In Bogoliubov's prescription, one first adds the term in which the subdivergence is replaced by its counterterm S(∙)=−1/zS(\bullet)=-1/z, and then subtracts the whole.

Rˉ(ℓ2)=φ(ℓ2)+S(∙) φ(∙),pole⁡Rˉ(ℓ2)=−12z2(4)\bar R(\ell_2)=\varphi(\ell_2)+S(\bullet)\,\varphi(\bullet),\qquad \operatorname{pole}\bar R(\ell_2)=-\frac{1}{2z^2} \tag{4}

Computed L/zL/z disappears, and the overall counterterm S(ℓ2)=1/(2z2)S(\ell_2)=1/(2z^2) does not depend on the outer scale (Rˉ\bar R: Bogoliubov's map). For general diagrams the sum is over forests — sets of divergent subdiagrams any two of which are nested or disjoint (including the empty set and the whole diagram). Zimmermann's forest formula is

R Γ=∑F: forests ∏γ∈F(−Tγ) Γ(5)R\,\Gamma=\sum_{\mathcal F:\ \text{forests}}\ \prod_{\gamma\in\mathcal F}\bigl(-T_\gamma\bigr)\,\Gamma \tag{5}

where TγT_\gamma is the operation extracting the divergent part of γ\gamma (in momentum space, the low orders of the Taylor expansion in the external momenta), and the product acts from the inside (a form with details omitted). Example: the forests of ℓ2\ell_2 are ∅,{∙},{ℓ2},{∙,ℓ2}\varnothing,\{\bullet\},\{\ell_2\},\{\bullet,\ell_2\}, and (5) is the expansion (1−Tℓ2)(1−T∙) ℓ2(1-T_{\ell_2})(1-T_\bullet)\,\ell_2. The (1−T∙)(1-T_\bullet) part corresponds to the Rˉ\bar R of (4), and the remaining −Tℓ2-T_{\ell_2} to adding the overall counterterm S(ℓ2)=1/(2z2)S(\ell_2)=1/(2z^2), leaving a value without poles (the φ+\varphi_+ of §05). It is called BPHZ after the initials of Bogoliubov–Parasiuk (1957), Hepp (1966) and Zimmermann (1969), and the gaps in the first proof are said to have been filled by the work of the latter two (§1 of Ebrahimi-Fard–Kreimer 2005). The forest formula with overlaps also follows from the Hopf algebra of rooted trees (§05) (abstract of Kreimer 1999). Known

03

Extension in position space — Epstein–Glaser

This section uses the distributions of 1-11 §04 and §08. We give only the essentials. A test function gg is a function that can be differentiated any number of times and goes to 0 quickly far away, and a distribution tt is a rule assigning linearly a number ⟨t,g⟩\langle t,g\rangle to each test function. ⟨δ,g⟩=g(0)\langle\delta,g\rangle=g(0), and its derivative is defined by ⟨∂αδ,g⟩=(−1)∣α∣∂αg(0)\langle\partial^\alpha\delta,g\rangle=(-1)^{|\alpha|}\partial^\alpha g(0). A sequence of distributions "converges as distributions" if ⟨tn,g⟩\langle t_n,g\rangle converges for every test function gg.

In position space, a divergence is the impossibility of extending a distribution to a singular point. We take examples in Euclidean R4\mathbb R^4. The square of the four-dimensional massless propagator G=1/(4π2∣x∣2)G=1/(4\pi^2|x|^2) (the bubble diagram) behaves as ∣x∣−4|x|^{-4} near the origin, and its integral diverges logarithmically. The method of Epstein–Glaser (1973) was set up in Minkowski space (spacetime with time); it builds time-ordered products (whose expectations are the correlation functions) inductively in the number of vertices (§4 of Brunetti–Fredenhagen 2000), and extends values fixed off the diagonal, where points coincide, onto the diagonal. Renormalisation is exactly the extension of expectations to the diagonal (abstract of the same paper). Since it is formulated as extension, there is no need to write divergent integrals along the way. The extension problem itself has the same form in Euclidean Rd\mathbb R^d, as below. The freedom is measured by the scaling degree ((33) of the same paper; numbering of the arXiv version; convergence as distributions).

sd⁡(t)=inf⁡{ω:λω t(λx)→0 (λ↓0)},sd⁡(∣x∣−a)=a,sd⁡(δ)=d(6)\operatorname{sd}(t)=\inf\bigl\{\omega : \lambda^{\omega}\,t(\lambda x)\to0\ (\lambda\downarrow0)\bigr\},\qquad \operatorname{sd}(|x|^{-a})=a,\quad \operatorname{sd}(\delta)=d \tag{6}

For t0t_0 on Rd∖{0}\mathbb R^d\setminus\{0\} (Theorems 5.2 and 5.3 of the same paper) Known: if sd⁡(t0)<d\operatorname{sd}(t_0)\lt d, the extension preserving the scaling degree is unique. If d≤sd⁡(t0)<∞d\le\operatorname{sd}(t_0)\lt\infty, extensions exist, and the difference of two extensions is supported at the origin, of the form

t−t′=∑∣α∣≤ρcα ∂αδ,ρ=sd⁡(t0)−d(7)t-t'=\sum_{|\alpha|\le\rho}c_\alpha\,\partial^\alpha\delta,\qquad \rho=\operatorname{sd}(t_0)-d \tag{7}

ρ\rho corresponds to the superficial degree of divergence of 4-04, and the constants cαc_\alpha are the freedom of local counterterms. Example: for t0=∣x∣−4t_0=|x|^{-4} (d=4d=4, ρ=0\rho=0), the extension that subtracts g(0)g(0) only inside the ball of radius 1/μ1/\mu,

⟨uμ,g⟩=∫R4g(x)−g(0) 1{∣x∣<1/μ}∣x∣4 d4x(8)\langle u_\mu,g\rangle=\int_{\mathbb R^4}\frac{g(x)-g(0)\,\mathbf 1\{|x|\lt1/\mu\}}{|x|^4}\,d^4x \tag{8}

agrees with t0t_0 for x≠0x\ne0, and converges because the numerator is O(∣x∣)O(|x|). The difference on changing μ\mu is 2π2ln⁡(μ′/μ) g(0)2\pi^2\ln(\mu'/\mu)\,g(0) (2π22\pi^2 is the area of S3S^3), a constant multiple of δ\delta.

Example: for gs=e−∣x∣2/s2g_s=e^{-|x|^2/s^2}, ⟨uμ,gs⟩=2π2(ln⁡(μs)−γ/2)\langle u_\mu,g_s\rangle=2\pi^2(\ln(\mu s)-\gamma/2) (γ\gamma is Euler's constant). At μ=1\mu=1, for s=0.1,1,10s=0.1,1,10 it is −51.148, −5.697, 39.754, and the difference from μ=2\mu=2 is 2π2ln⁡2=13.6822\pi^2\ln2=13.682 in each case. Removing ∣x∣<η|x|\lt\eta without extending gives 85.21, 357.91 at η=10−2,10−8\eta=10^{-2},10^{-8} (s=1s=1), growing. Computed

04

Moving the dimension continuously — dimensional regularisation

We regard momentum integrals as functions of the dimension dd. The bubble of 4-04 (mass mm) converges for d<4d\lt4, giving

I(d)=∫ddk(2π)d 1(k2+m2)2=Γ(2−d/2)(4π)d/2 (m2)d/2−2(9)I(d)=\int\frac{d^dk}{(2\pi)^d}\,\frac{1}{(k^2+m^2)^2}=\frac{\Gamma(2-d/2)}{(4\pi)^{d/2}}\,(m^2)^{d/2-2} \tag{9}

(1/(8πm)1/(8\pi m) at d=3d=3). The right-hand side extends meromorphically to complex dd (as a function complex-differentiable except at isolated points called poles), and has a pole at d=4,6,…d=4,6,\dots. Using this is dimensional regularisation. Here we write d=4−2εd=4-2\varepsilon (half the ϵ\epsilon of the d=4−ϵd=4-\epsilon of 4-04). Then

16π2 I=1ε−γ+ln⁡4π−ln⁡m2+O(ε)(10)16\pi^2\,I=\frac1\varepsilon-\gamma+\ln4\pi-\ln m^2+O(\varepsilon) \tag{10}

and the divergence becomes the pole 1/ε1/\varepsilon. At ε=0.1,0.01,0.001\varepsilon=0.1,0.01,0.001, 16π2I16\pi^2I (m=1m=1) is 12.2535, 101.9814, 1001.9565, and the differences from the approximation (10) are 0.2997, 0.0276, 0.0027. The role of ln⁡kmax⁡2\ln k_{\max}^2 in the ln⁡(kmax⁡2/m2)−1\ln(k_{\max}^2/m^2)-1 cut at ∣k∣<kmax⁡|k|\lt k_{\max} in momentum is played by 1/ε1/\varepsilon. Computed The MS scheme subtracts only 1/ε1/\varepsilon, and the MS‾\overline{\mathrm{MS}} scheme subtracts 1/ε−γ+ln⁡4π1/\varepsilon-\gamma+\ln4\pi. Since a scale μ\mu is introduced (the coupling is multiplied by μ2ε\mu^{2\varepsilon}), −ln⁡(m2/μ2)-\ln(m^2/\mu^2) remains at MS‾\overline{\mathrm{MS}}. The ΛMS‾\Lambda_{\overline{\mathrm{MS}}} of 4-06 is the Λ\Lambda of this scheme.

In 1972 there were papers by Bollini–Giambiagi and by 't Hooft–Veltman (titled "Regularization and renormalization of gauge fields"), and it is said to be used as standard in Yang–Mills perturbation theory as a regularisation that does not break gauge symmetry. The price is that (9) is an analytic continuation diagram by diagram, and gives no measure for non-integer dd. The problem statement too writes that there are few ways to recover the reflection positivity lost by dimensional regularisation and the like (p.11; quoted in 0-03 §03; 4-10).

05

The algebra of diagrams — the Hopf algebra of Connes–Kreimer

Subtraction is the repetition of "extracting a subdiagram γ\gamma" and "the remainder Γ/γ\Gamma/\gamma with γ\gamma collapsed to a point". Before making this an operation, we prepare three words.

Making subtraction an operation is the Hopf algebra of Kreimer (1998) and Connes–Kreimer (1998, 2000): the generators are divergent one-particle irreducible diagrams, the product is setting diagrams side by side, and extraction is the coproduct ((15) of Ebrahimi-Fard–Kreimer 2005). The sum in (11) is over divergent one-particle irreducible proper subdiagrams and their disjoint sets (set side by side as a product). For a set, Γ/γ\Gamma/\gamma is the remainder with all of them collapsed to points. Writing the coproduct as Δ\Delta is a convention of the literature, unrelated to the Δ\Delta of the mass gap.

Δ(Γ)=Γ⊗1+1⊗Γ+∑γ⊊Γγ⊗Γ/γ(11)\Delta(\Gamma)=\Gamma\otimes1+1\otimes\Gamma+\sum_{\gamma\subsetneq\Gamma}\gamma\otimes\Gamma/\gamma \tag{11}

With nesting only, rooted trees suffice in place of diagrams. Vertices are divergent subdiagrams, and children are inner subdivergences. The sum in (11) becomes a sum over admissible cuts (choices of edges that cut every path from the root to a leaf at most once), with the cut-off side going on the left and the root side on the right (Figure 1).

Figure 1 Rooted trees and admissible cuts. The top is the root (the whole diagram), lower is further inside. Coloured lines are cuts; the lower side cut off is the left factor of (12), the root side the right factor. In ℓ₃, ① and ② are on the same path, so they are not cut together
①②ℓ₂: 1 wayb: left, right, bothℓ₃: ① or ②
Δ(ℓ2)=ℓ2⊗1+1⊗ℓ2+∙⊗∙Δ(b)=b⊗1+1⊗b+2 ∙⊗ℓ2+∙∙⊗∙(12)\begin{gathered}\Delta(\ell_2)=\ell_2\otimes1+1\otimes\ell_2+\bullet\otimes\bullet\\ \Delta(b)=b\otimes1+1\otimes b+2\,\bullet\otimes\ell_2+\bullet\bullet\otimes\bullet\end{gathered} \tag{12}

bb is the tree with two children at the root. Regularised values φ\varphi (maps taking values in Laurent series in zz and carrying products to products; characters) form a group under the convolution φ1⋆φ2=m∘(φ1⊗φ2)∘Δ\varphi_1\star\varphi_2=m\circ(\varphi_1\otimes\varphi_2)\circ\Delta (mm is the product of values). The unit is the character that gives 1 to the empty diagram and 0 to other diagrams. Since there are inverses, the problem can be posed as multiplying φ\varphi by a factor SRS_R that cancels its divergences to make SR⋆φ=φ+S_R\star\varphi=\varphi_+ finite. The counterterm SRS_R plays the role of the inverse of φ\varphi (§06). Fixing a scheme RR (for MS the pole part, for MOM the value at s=μs=\mu), the counterterm SRS_R and the renormalised value φ+\varphi_+ are fixed in order of tree size ((21)(25)(26) of Ebrahimi-Fard–Kreimer 2005).

SR(Γ)=−R[Rˉ(Γ)],φ+(Γ)=(1−R)[Rˉ(Γ)]Rˉ(Γ)=φ(Γ)+∑γSR(γ) φ(Γ/γ)(13)\begin{gathered}S_R(\Gamma)=-R\bigl[\bar R(\Gamma)\bigr],\qquad \varphi_+(\Gamma)=(1-R)\bigl[\bar R(\Gamma)\bigr]\\ \bar R(\Gamma)=\varphi(\Gamma)+\sum_{\gamma}S_R(\gamma)\,\varphi(\Gamma/\gamma)\end{gathered} \tag{13}

In the toy model, writing the subtree rooted at vertex vv as tvt_v and the number of vertices as ∣t∣|t|, the values take closed form (Proposition 3.2.2 of Panzer 2012).

φ(t)(s)=s−z∣t∣∏vF(z ∣tv∣)(14)\varphi(t)(s)=s^{-z|t|}\prod_{v}F\bigl(z\,|t_v|\bigr) \tag{14}

Computing (13) for the 8 trees with up to 4 vertices, (i) none of the counterterms contains LL (locality), (ii) the renormalised values are polynomials of degree ∣t∣|t| in LL with top-degree term (−L)∣t∣/t!(-L)^{|t|}/t! (t!=∏v∣tv∣t!=\prod_v|t_v| is the tree factorial), and (iii) the MOM values agreed with Panzer's (3.4.2)–(3.4.5). The difference between MS and MOM is finite. Computed

ComputedTable 1 Renormalisation in the toy model (computed exactly in rationals). The right-hand column is the value of z→0z\to0. Subtracting by MS changes the constants (ℓ2\ell_2 becomes L22+π24\frac{L^2}{2}+\frac{\pi^2}{4}, ℓ3\ell_3 becomes −L36−5π2L12-\frac{L^3}{6}-\frac{5\pi^2L}{12}).

Treet!t!Pole part of the bare valueCounterterm (MS)φ+\varphi_+ (MOM)
∙\bullet11z\frac1z−1z-\frac1z−L-L
ℓ2\ell_2212z2−Lz\frac{1}{2z^2}-\frac Lz12z2\frac{1}{2z^2}L22\frac{L^2}{2}
bb313z3−Lz2+27L2+11π218z\frac{1}{3z^3}-\frac{L}{z^2}+\frac{27L^2+11\pi^2}{18z}−13z3+π218z-\frac{1}{3z^3}+\frac{\pi^2}{18z}−L33−π2L3-\frac{L^3}{3}-\frac{\pi^2L}{3}
ℓ3\ell_3616z3−L2z2+27L2+14π236z\frac{1}{6z^3}-\frac{L}{2z^2}+\frac{27L^2+14\pi^2}{36z}−16z3−π218z-\frac{1}{6z^3}-\frac{\pi^2}{18z}−L36−π2L6-\frac{L^3}{6}-\frac{\pi^2L}{6}
06

Birkhoff decomposition — subtraction becomes a decomposition in a group

The main theorem of Connes–Kreimer (2000) (abstract) is that the dimensionally regularised bare theory gives a loop γ(z)\gamma(z) in the group of characters on a small circle around the integer spacetime dimension DD, and 'the renormalized theory is just the evaluation at z = D of the holomorphic part γ₊ of the Birkhoff decomposition of γ'. z=Dz=D is the integer dimension of spacetime, γ\gamma is the loop given by the regularised theory (the family of characters as the dimension zz moves on the circle), and γ+\gamma_+ is the holomorphic factor of its decomposition. Known Below we write zz as the deviation from DD (the same role as the zz of the toy model, with z=0z=0 the integer dimension).

φ(z)=φ−(z)⋆−1⋆φ+(z)(15)\varphi(z)=\varphi_-(z)^{\star-1}\star\varphi_+(z) \tag{15}

φ−\varphi_- is a polynomial in 1/z1/z (constant term the unit) and is the MS counterterm; φ+\varphi_+ is holomorphic at z=0z=0, and φ+(0)\varphi_+(0) is the renormalised value. As an analogy, it is the multiplicative version of splitting a Laurent series into its pole part and its holomorphic part. Precisely, since the group is not commutative, they are fixed in order of tree size by the induction of (13). That SRS_R and φ+\varphi_+ are again characters is because RR satisfies R2=RR^2=R and the Rota–Baxter identity

R(x) R(y)+R(xy)=R(R(x) y+x R(y))(16)R(x)\,R(y)+R(xy)=R\bigl(R(x)\,y+x\,R(y)\bigr) \tag{16}

((20) of Ebrahimi-Fard–Kreimer 2005). Known Example: for the pole part RR and x=1/z+ax=1/z+a, y=1/z+by=1/z+b, both sides are 2/z2+(a+b)/z2/z^2+(a+b)/z.

Figure 2 is the MOM of the ladder ℓn\ell_n (nn vertices in a row). The sum in (13) becomes Rˉ(ℓn)=φ(ℓn)+∑j<nSR(ℓj) φ(ℓn−j)\bar R(\ell_n)=\varphi(\ell_n)+\sum_{j\lt n}S_R(\ell_j)\,\varphi(\ell_{n-j}); as z→0z\to0 the bare value runs away at the rate z−nz^{-n}, while the subtracted value settles to a polynomial. Computed

Figure 2 Making the knob z smaller, the bare value log⁡10φ(ℓn)\log_{10}\varphi(\ell_n) in the upper panel runs away upwards, and the subtracted value φ+(ℓn)\varphi_+(\ell_n) in the lower panel (solid line) approaches a polynomial in z→0z\to0 (dashed line). The horizontal axis is LL, and n is the number of rungs of the ladder. "Play" lowers z
n = 2, z = 0.100, at L = 1, bare value 44.49, subtracted value −0.0141, limit 0.5000.

ComputedThe numbers in this figure were computed on this machine. The closed forms of (13)(14) are evaluated in the figure and checked against python3.

If JavaScript is disabled: at L=1L=1, the subtracted values at z=0.02, 0.005z=0.02,\ 0.005 are, for n=1n=1: −0.991, −0.998 (limit −1); n=2n=2: 0.394, 0.473 (0.5); n=3n=3: −1.696, −1.776 (−1.812); n=4n=4: 0.655, 1.419 (1.687). The bare values at z=0.02z=0.02 are 49, 1205, 19802, 245195. The difference from the limit shrinks roughly in proportion to zz. Computed

Detour: rooted trees and Runge–Kutta methods

Detour

A subsection you may skip.

Expanding the solution of y′=f(y)y'=f(y) in hh, reading the derivative of order kk as "a vertex with kk children", f, f′f, f′′(f,f), f′f′ff,\ f'f,\ f''(f,f),\ f'f'f becomes ∙, ℓ2, b, ℓ3\bullet,\ \ell_2,\ b,\ \ell_3.

y(h)=y+hf+h22 f′f+h36(f′′(f,f)+f′f′f)+O(h4)(17)y(h)=y+hf+\frac{h^2}{2}\,f'f+\frac{h^3}{6}\bigl(f''(f,f)+f'f'f\bigr)+O(h^4) \tag{17}

The coefficient of h3h^3 is 1/t!1/t! for ℓ3\ell_3, and for bb the reciprocal of the product of 2, from exchanging left and right, and t!=3t!=3; this is the same tree factorial as in Table 1. Runge–Kutta methods are built to reproduce these coefficients up to a given order, and the group handling the expansion is called Butcher's group (Butcher 1972). Brouder (2000), in his abstract, points out the connection between the algebra of rooted trees in renormalisation and Runge–Kutta methods. Known

07

Families of effective actions — Costello

Another route is to regard the family of actions, one for each scale, as the theory (Wilson's renormalisation group; 6-05). Costello (a 2007 paper, a 2011 book) restricts the tt (the square of a length) of the propagator 1/k2=∫0∞e−tk2dt1/k^2=\int_0^\infty e^{-tk^2}dt from ε\varepsilon to TT.

P(ε,T)(k)=∫εTe−tk2 dt=e−εk2−e−Tk2k2(18)P(\varepsilon,T)(k)=\int_\varepsilon^T e^{-tk^2}\,dt=\frac{e^{-\varepsilon k^2}-e^{-Tk^2}}{k^2} \tag{18}

Precisely, the paper is written with the heat kernel on a compact manifold, which on flat space becomes e−tk2e^{-tk^2}. Example: at ε=0.01\varepsilon=0.01, T=100T=100, k2Pk^2P is 0.990, 0.368, 1.2×10−41.2\times10^{-4} at k=1,10,30k=1,10,30. Computed Actions at different scales are linked by the renormalisation group equation (Γ(P,S)\Gamma(P,S) is the sum of diagrams joining vertices of SS by PP).

Seff(T2)=Γ(P(T1,T2), Seff(T1))(19)S_{\mathrm{eff}}(T_2)=\Gamma\bigl(P(T_1,T_2),\,S_{\mathrm{eff}}(T_1)\bigr) \tag{19}

Theorem B of the paper is that, once a scheme is fixed (a choice of which functions of ε\varepsilon to call the singular part), there is a unique counterterm SCT(ε)S^{\mathrm{CT}}(\varepsilon) such that lim⁡ε→0Γ(P(ε,T),S−SCT)\lim_{\varepsilon\to0}\Gamma(P(\varepsilon,T),S-S^{\mathrm{CT}}) exists, and the counterterms are local and independent of TT. The counterterms are power series in ℏ\hbar (the letter counting loops). The effective action at scale TT is the limit as ε→0\varepsilon\to0 after subtracting these counterterms,

ΓR(P(0,T),S)=lim⁡ε→0Γ(P(ε,T), S−SCT(ε))(20)\Gamma^R\bigl(P(0,T),S\bigr)=\lim_{\varepsilon\to0}\Gamma\bigl(P(\varepsilon,T),\,S-S^{\mathrm{CT}}(\varepsilon)\bigr) \tag{20}

and building diagrams with P(0,T)P(0,T) as it is diverges. The effective action too is a formal power series in ℏ\hbar (§08). Theorem C is that, once a scheme is fixed, local actions correspond one-to-one to families of effective actions satisfying (19) and locality as T→0T\to0. Changing the scheme amounts to putting different coordinates on the same family. Known

Gauge symmetry is expressed by the quantum master equation of the Batalin–Vilkovisky (BV) formalism (here only the name; it gathers the condition of keeping gauge symmetry into one equation with auxiliary fields added). The 2007 paper distinguishes renormalisation (constructing counterterms) from quantisation (constructing solutions of the quantum master equation), and gives pure Yang–Mills on compact four-dimensional manifolds as an example of the former, and Chern–Simons theory as a non-trivial example of the latter. The 2011 book is described as containing a proof of the perturbative renormalisability of Yang–Mills by cohomology (an algebraic tool that looks at ker⁡Q/im⁡Q\ker Q/\operatorname{im}Q for maps QQ with Q2=0Q^2=0; here only the name). Renormalisability itself is said to have been established by 't Hooft (1971), 't Hooft–Veltman (1972), Lee–Zinn-Justin (1972), Becchi–Rouet–Stora (1976) and others (6-12 §06). Known

08

Where the algebra reaches and where it does not

All the tools so far work on formal power series in the coupling constant, make each order finite, and confine the freedom to finitely many local terms. Known Three things lie out of reach. (i) The sum of the series: the perturbation series of four-dimensional Yang–Mills is thought to diverge (4-12). Physics (ii) Quantities that are 0 at every order: the one-loop scale (4-07; for pure SU(N)SU(N), β0=11N/3\beta_0=11N/3; conversion between four ways of writing the coefficient in Table 1 of 4-06)

Λ=μ exp⁡ ⁣(−8π2β0 g2)(21)\Lambda=\mu\,\exp\!\Bigl(-\frac{8\pi^2}{\beta_0\,g^2}\Bigr) \tag{21}

(with b0=β0/(16π2)b_0=\beta_0/(16\pi^2), the same formula as (3) of 4-07) has all its Taylor coefficients in gg equal to 0. The mass gap is expected to be proportional to Λ\Lambda Physics, and such quantities cannot be distinguished from 0 within formal power series (6-12 §07). (iii) The measure and positivity: what the problem statement asks for is not a sequence of coefficients but a theory satisfying the axioms (0-03), whose correlation functions should agree at short distances with asymptotic freedom and the predictions of perturbative renormalisation theory (p.6; quoted in 0-03 §07). The algebra of this chapter is on the side of the answers that a construction must reproduce.

An example of the same algebra being used inside a tool outside formal power series is the renormalisation of Hairer's regularity structures. Regularity structures are a framework for solving the equations of stochastic quantisation (6-09; here only the name; a method that solves a time-evolution equation shaken by noise and tries to obtain the measure as its distribution after a long time), and their renormalisation is written with a pair of Hopf algebras and a variant of the Birkhoff decomposition (abstract of Bruned–Hairer–Zambotti 2019). Regularity structures have been used to construct local-in-time solutions (solutions only for a short time) of the stochastic quantisation equation of three-dimensional Yang–Mills–Higgs (abstract of Chandra–Chevyrev–Hairer–Shen 2024). Known What they can handle is subcritical equations (the non-linear term weakens at shorter scales), and four-dimensional Yang–Mills is critical (the strength of the non-linear term does not depend on scale), so it lies outside.


What this chapter can say

Content
What is saidThe five formulations and the theorems quoted (classification of extensions, the main theorem on Birkhoff decomposition, Costello's Theorems B and C) Known. In the toy model: that subtracting only the whole leaves poles containing LL and that Bogoliubov's prescription removes them; that for 8 trees the counterterms are local and the values are polynomials in LL. That the difference of extensions of ∣x∣−4|x|^{-4} is a constant multiple of δ\delta. The pole of the bubble Computed
ConditionalThe toy model has nesting only, and locality is checked within it (in general it rests on the theorems in the literature). The divergence of the perturbation series and Δ∝Λ\Delta\propto\Lambda are expectations Physics
What is not saidMulti-loop calculations in four-dimensional Yang–Mills. The sum of the series. The non-perturbative measure, reflection positivity, the mass gap. The content of the proofs in literature cited by bibliographic data only

Sources and reproduction

ItemKindSource / tools
Read in full textKnownJaffe–Witten, Quantum Yang–Mills Theory (the Clay problem statement) p.6, p.11. Panzer, arXiv:1202.3552 (2012) §3.2–3.4. Ebrahimi-Fard–Kreimer, J. Phys. A 38 (2005) R385 §1–2. Brunetti–Fredenhagen, arXiv:math-ph/9903028 (Commun. Math. Phys. 208 (2000) 623), abstract, §4, §5.1–5.2 (numbering of formulas and theorems from the arXiv version). Costello, arXiv:0706.1533 (2007) §1
Read in abstract onlyKnownKreimer, Adv. Theor. Math. Phys. 2 (1998) 303. Connes–Kreimer, Commun. Math. Phys. 199 (1998) 203; 210 (2000) 249. Kreimer, Commun. Math. Phys. 204 (1999) 669. Brouder, Eur. Phys. J. C 12 (2000) 521. Bruned–Hairer–Zambotti, Invent. Math. 215 (2019) 1039. Chandra–Chevyrev–Hairer–Shen, Invent. Math. 237 (2024) 541 (arXiv:2201.03487)
Bibliographic data onlyKnownBogoliubov–Parasiuk, Acta Math. 97 (1957) 227. Hepp, Commun. Math. Phys. 2 (1966) 301. Zimmermann, ibid. 15 (1969) 208. Epstein–Glaser, Ann. Inst. H. Poincaré A 19 (1973) 211. Bollini–Giambiagi, Nuovo Cim. B 12 (1972) 20. 't Hooft–Veltman, Nucl. Phys. B 44 (1972) 189 (standard use in gauge theories not checked). 't Hooft, ibid. 33 (1971) 173. Lee–Zinn-Justin, Phys. Rev. D 5 (1972) 3121. Becchi–Rouet–Stora, Ann. Phys. 98 (1976) 287. Costello, Renormalization and Effective Field Theory, AMS (2011) (from the publisher's description). Butcher, Math. Comp. 26 (1972) 79
(3)(4), Table 1Computedpython3 (Laurent series in z computed exactly with the standard library's rationals; 8 trees, MS and MOM)
Figure 2, the numbers in §03, §04, §06 and §07Computedpython3 (SciPy numerical integration and the Γ function, closed formulas). The JavaScript of Figure 2 was checked against the python3 values with node

Next chapter to read: 4-06 Asymptotic freedom. Detours: 6-12, 4-12.

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