computo ergo sum

2026-10-01 · chapter Yang–Mills and the mass gapPart 1 Mathematical preparationHilbert spaces and spectra

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

Hilbert spaces and self-adjoint operators — measuring "the lowest" and "the next" in infinite dimensions

What this chapter shows — Spaces in which functions are treated as vectors whose length can be measured, and unbounded operators such as differentiation. That the spectrum is wider than the set of eigenvalues, and that boundary conditions are part of the operator. That the variational principle measuring the lowest value and the gap is the same thing as the best constant of the Poincaré inequality.

Prerequisite chapters — 1-01 (inner products, Hermitian matrices, diagonalisation). Sections 02, 05, 08 and 09 touch on 1-08 and 1-09 (sets of length 0, Brownian motion, Gaussian distributions).

Said first — We introduce the entrance to functional analysis, and omit the details of domains and the proofs of theorems. The Hamiltonians of quantum field theory are much harder to handle (4-09), and this chapter shows nothing about the Yang–Mills mass gap.

Order of this chapter
  1. Why infinite dimensions — the lower eigenvalues stay, the upper ones run away (Figure 1, Table 1)
  2. Hilbert spaces — limits stay inside the space
  3. Operators and self-adjointness — boundary conditions are part of the operator
  4. The spectrum — some values have no eigenvalue
  5. The spectral theorem — the gap decides the rate of decay
  6. The variational principle — upper bounds are easy, lower bounds need other information (Table 2, box "The asymmetry of upper and lower bounds")
  7. The Poincaré inequality — the best constant is the inverse of the gap
  8. The weighted Poincaré inequality — 1/κ if convex, large if there are two valleys (Figure 2, Table 3)
  9. With many variables — products, Gaussians, the free field, and two gaps
  10. Detour: counting eigenvalues — Weyl's law and the shape of a drum

01

Why infinite dimensions — the lower eigenvalues stay, the upper ones run away

In finite dimensions the smallest eigenvalue and the gap to the next can always be computed (1-01). What is asked is whether the gap stays positive in the limit of more and more degrees of freedom. As an example, discretise on a lattice of NN equal parts the rule assigning −u′′-u'' to a function uu on [0,1][0,1] vanishing at both ends (the same form as the Hessian matrix of 2-01 §05).

(ANu)j=N2 (−uj−1+2uj−uj+1),u0=uN=0;λk(N)=4N2sin⁡2kπ2N(1≤k≤N−1)(1)(A_Nu)_j=N^2\,(-u_{j-1}+2u_j-u_{j+1}),\quad u_0=u_N=0;\qquad \lambda_k(N)=4N^2\sin^2\frac{k\pi}{2N}\quad(1\le k\le N-1) \tag{1}

The eigenvectors are uj=sin⁡(kπj/N)u_j=\sin(k\pi j/N) (this can be checked by substitution). Fixing kk and letting N→∞N\to\infty gives λk(N)→k2π2\lambda_k(N)\to k^2\pi^2. This is an eigenvalue of −u′′=λu, u(0)=u(1)=0-u''=\lambda u,\ u(0)=u(1)=0. The top eigenvalue grows to near 4N24N^2 and has no limit.

ComputedTable 1 Eigenvalues of the matrix of (1) (the difference between a tridiagonal eigenvalue computation and (1) is at most 10−1510^{-15} relative).

Nλ₁λ₂top
109.7887038.19660390.2
409.8645339.397316390.1
1609.8692939.47334102390.1
continuumπ² = 9.869604π² = 39.47842(none)
Figure 1 Left: the ratios of eigenvalues of (1) λ_k(N)/k²π² (dots, k = 1 … N − 1) plotted against t = k/N. The dots lie on the curve (sin(πt/2)/(πt/2))² (dashed) regardless of N, and increasing N brings the dot for number k (circle) towards the ratio 1. The ratio 4/π² at the right end means that the top end levels off at 4N². Right: the k-th eigenvector (dots) and sin kπx (dashed)
N = 12, k = 3, λ_k(N) = 84.35, k²π² = 88.83, ratio = 0.9496

ComputedThe numbers in the figure are computed on the spot from (1) (checked against Table 1).

The ratio is fixed by t=k/Nt=k/N alone: λk(N)/k2π2=(sin⁡(πt/2)/(πt/2))2\lambda_k(N)/k^2\pi^2=\bigl(\sin(\pi t/2)/(\pi t/2)\bigr)^2 (the dashed line on the left of Figure 1). At k=N/2k=N/2, 8/π2≈0.818/\pi^2\approx0.81; at the right end t→1t\to1, 4/π2≈0.414/\pi^2\approx0.41. Fixing kk and increasing NN gives t→0t\to0, and the ratio approaches 1. An eigenvector with kk near NN is, at the lattice points, exactly the values of sin⁡kπx\sin k\pi x, but its oscillation is as fine as the spacing of the points, so joining the points makes it look like a different shape. In fact sin⁡(kπj/N)=−(−1)jsin⁡((N−k)πj/N)\sin(k\pi j/N)=-(-1)^j\sin((N-k)\pi j/N): a slow oscillation multiplied by a sign that alternates point by point (visible on the right of Figure 1 by bringing kk near N−1N-1). What remains in the limit is the lower eigenvalues and the gap, and the limiting object is an operator unbounded above. In the continuum limit of lattice gauge theory (5-05) too, what is read from the lattice is the lower end of the spectrum (the lightest state) Physics. That this limit exists in four dimensions has not been proved (6-10).

02

Hilbert spaces — limits stay inside

To treat functions as "vectors with infinitely many components" we need an inner product (1-01 §05) and completeness. Complete means that sequences whose terms come arbitrarily close to one another (Cauchy sequences) have limits inside the space. A complex vector space with these two is called a Hilbert space.

ℓ2={(c1,c2,… ):∑k∣ck∣2<∞},L2(0,1)={f:∫01∣f∣2dx<∞},⟨f,g⟩=∫01f‾ g dx(2)\ell^2=\Bigl\{(c_1,c_2,\dots):\sum_k|c_k|^2\lt\infty\Bigr\},\qquad L^2(0,1)=\Bigl\{f:\int_0^1|f|^2dx\lt\infty\Bigr\},\qquad \langle f,g\rangle=\int_0^1\overline{f}\,g\,dx \tag{2}

In L2L^2, functions that differ only on a set of length 0 are regarded as the same (1-08). Continuous functions alone are not complete: tanh⁡(n(x−12))\tanh(n(x-\frac12)) come close to one another, yet their destination is a step function. To take the destination of "a sequence making the ratio smaller and smaller" in section 06, the complete L2L^2 is needed Known.

ek=2sin⁡kπx (k≥1)e_k=\sqrt2\sin k\pi x\ (k\ge1) is an orthonormal basis of L2(0,1)L^2(0,1), and for ck=⟨ek,f⟩c_k=\langle e_k,f\rangle, ∥f∥2=∑k∣ck∣2\lVert f\rVert^2=\sum_k|c_k|^2 (Parseval's identity) Known (1-11). Example. For f=x(1−x)f=x(1-x), ck=42/(kπ)3c_k=4\sqrt2/(k\pi)^3 for odd kk and 0 for even. ∑k odd32/(kπ)6=1/30\sum_{k\,\text{odd}}32/(k\pi)^6=1/30 agrees with ∫01x2(1−x)2dx=1/30\int_0^1x^2(1-x)^2dx=1/30. The ℓ2\ell^2 of 1-09 connects to spaces of functions in this way.

03

Operators and self-adjointness — domains and boundary conditions

An operator whose supremum of stretching factors ∥A∥=sup⁡ψ≠0∥Aψ∥/∥ψ∥\lVert A\rVert=\sup_{\psi\ne0}\lVert A\psi\rVert/\lVert\psi\rVert is finite is called bounded. −d2/dx2-d^2/dx^2 multiplies eke_k by k2π2k^2\pi^2, so it is not bounded, and there are functions whose second derivatives are not in L2L^2. So the subspace of functions it may be applied to, the domain D(A)D(A), is specified as part of the operator. If ⟨ϕ,Aψ⟩=⟨Aϕ,ψ⟩\langle\phi,A\psi\rangle=\langle A\phi,\psi\rangle on D(A)D(A), it is symmetric. Self-adjointness is one step stronger: it says that the partners ϕ\phi of this identity do not increase even when sought outside D(A)D(A). To be exact, the set of ϕ\phi for which there is a η\eta with ⟨ϕ,Aψ⟩=⟨η,ψ⟩\langle\phi,A\psi\rangle=\langle\eta,\psi\rangle for all ψ∈D(A)\psi\in D(A) is taken as the domain D(A†)D(A^\dagger) of the adjoint A†A^\dagger, and A†ϕ=ηA^\dagger\phi=\eta is defined. If symmetric, D(A)⊂D(A†)D(A)\subset D(A^\dagger), and when D(A†)=D(A)D(A^\dagger)=D(A) it is self-adjoint. The spectral theorem and time evolution e−itAe^{-itA} (2-05) presuppose self-adjointness Known. For the momentum P=−i d/dxP=-i\,d/dx, integration by parts gives the following.

⟨ϕ,Pψ⟩−⟨Pϕ,ψ⟩=−i [ ϕ‾ ψ ]01(3)\langle\phi,P\psi\rangle-\langle P\phi,\psi\rangle=-i\,\bigl[\,\overline{\phi}\,\psi\,\bigr]_0^1 \tag{3}

(a) If D={ψ(0)=ψ(1)=0}D=\{\psi(0)=\psi(1)=0\}, it is symmetric, but the partner ϕ\phi needs no condition, and P†eizx=zeizxP^\dagger e^{izx}=ze^{izx} for every complex number zz, so it is not self-adjoint. (b) If Dθ={ψ(1)=eiθψ(0)}D_\theta=\{\psi(1)=e^{i\theta}\psi(0)\}, the partner satisfies the same condition and it is self-adjoint, with eigenvalues 2πn+θ (n∈Z)2\pi n+\theta\ (n\in\mathbb Z). The phase difference qΦ/ℏq\Phi/\hbar from a magnetic flux Φ\Phi threading the ring plays the role of θ\theta (the Aharonov–Bohm effect of 2-03). For −d2/dx2-d^2/dx^2 too, with u=0u=0 at the ends (Dirichlet) the spectrum is {k2π2}k≥1\{k^2\pi^2\}_{k\ge1}, and with u′=0u'=0 (Neumann) it is {k2π2}k≥0\{k^2\pi^2\}_{k\ge0}. Boundary conditions are part of the operator, and change the lowest value.

04

The spectrum — values for which no inverse can be made

In infinite dimensions there are cases where a map is one-to-one but its inverse is not bounded. So the spectrum is defined as follows.

σ(A)={λ∈C: (A−λ)−1 does not exist as a bounded operator},∥(A−λ)−1∥=1dist⁡(λ,σ(A))(4)\sigma(A)=\bigl\{\lambda\in\mathbb C:\ (A-\lambda)^{-1}\ \text{does not exist as a bounded operator}\bigr\},\qquad \bigl\lVert(A-\lambda)^{-1}\bigr\rVert=\frac1{\operatorname{dist}(\lambda,\sigma(A))} \tag{4}

The identity on the right holds when AA is self-adjoint and λ∉σ(A)\lambda\notin\sigma(A), and then σ(A)\sigma(A) is a closed subset of the real line Known. Example. The operator MM multiplying by xx on L2(0,1)L^2(0,1) has no eigenvalues, since xf=λfxf=\lambda f implies f=0f=0. Even so, for λ∈[0,1]\lambda\in[0,1], 1/(x−λ)1/(x-\lambda) is not bounded, and σ(M)=[0,1]\sigma(M)=[0,1]. A function of length 1 that is constant only on [λ,λ+ε][\lambda,\lambda+\varepsilon] has ∥(M−λ)f∥≤ε\lVert(M-\lambda)f\rVert\le\varepsilon: there are things arbitrarily close to eigenvectors (Weyl's criterion of 2-05 §03). Discretising makes the eigenvalues lattice points, which fill up [0,1][0,1] (the lower eigenvalues of section 01 stay apart).

Isolated eigenvalues of finite multiplicity are called the discrete spectrum, and the rest the essential spectrum. The mass gap is the claim that the vacuum eigenvalue 0 is isolated and the rest of the spectrum lies at Δ>0\Delta\gt0 or above (4-11).

05

The spectral theorem — the gap decides the rate of decay

A self-adjoint operator can be carried by a suitable unitary to "an operator multiplying by a real-valued function", like MM (the spectral theorem) Known. It is the infinite-dimensional version of the diagonalisation of matrices (1-01), and to be exact it includes parts that cannot be written with eigenvalues alone. Functions gg can be substituted, and if there is a basis of eigenvectors it takes the following form.

g(A) ψ=∑kg(λk) ⟨ek,ψ⟩ ek,∥e−tAψ−⟨e0,ψ⟩e0∥≤e−Δt ∥ψ−⟨e0,ψ⟩e0∥(5)g(A)\,\psi=\sum_kg(\lambda_k)\,\langle e_k,\psi\rangle\,e_k,\qquad \bigl\lVert e^{-tA}\psi-\langle e_0,\psi\rangle e_0\bigr\rVert\le e^{-\Delta t}\,\bigl\lVert\psi-\langle e_0,\psi\rangle e_0\bigr\rVert \tag{5}

The right-hand side is for the case A≥0A\ge0, with the eigenspace of 0 spanned by e0e_0 of length 1 and the rest of the spectrum in [Δ,∞)[\Delta,\infty); it follows by using e−tλ≤e−Δte^{-t\lambda}\le e^{-\Delta t} on each component. The gap is the slowest rate at which the components other than the lowest disappear (for the reading in imaginary time see 2-05 §05). Example 1. For the heat equation ∂tu=∂x2u\partial_tu=\partial_x^2u on a rod insulated at both ends, AA is the Neumann −d2/dx2-d^2/dx^2, Δ=π2\Delta=\pi^2, and the deviation of the temperature from its mean is at most e−π2/2≈0.0072e^{-\pi^2/2}\approx0.0072 times at t=0.5t=0.5. Example 2. The inverse of the Dirichlet −d2/dx2-d^2/dx^2 is (Gf)(x)=∫01G(x,y)f(y) dy(Gf)(x)=\int_0^1G(x,y)f(y)\,dy, G(x,y)=min⁡(x,y)−xyG(x,y)=\min(x,y)-xy (−(Gf)′′=f-(Gf)''=f and the zeros at both ends can be checked). Making X(t)=B(t)−tB(1)X(t)=B(t)-tB(1) from the Brownian motion BB of 1-09 gives zeros at both ends (the Brownian bridge), and its covariance E[X(s)X(t)]E[X(s)X(t)] is exactly G(s,t)G(s,t). The eigenvalues of GG are (kπ)−2(k\pi)^{-2}, and the finiteness of the sum ∑k(kπ)−2=1/6\sum_k(k\pi)^{-2}=1/6 is the condition of 1-09 (4) for samples of the Brownian bridge to lie in L2L^2.

06

The variational principle — easy from above, hard from below

The lower end of the spectrum of a self-adjoint operator bounded below is the infimum of the Rayleigh quotient. The nn-th too can be written in the form "take the maximum over a nn-dimensional subspace, and the minimum over subspaces" (the min-max principle; for the eigenvalues below the essential spectrum, in increasing order counted with multiplicity) Known.

inf⁡σ(A)=inf⁡0≠ψ∈D(A)⟨ψ,Aψ⟩⟨ψ,ψ⟩,λn=min⁡dim⁡V=n max⁡0≠ψ∈V⟨ψ,Aψ⟩⟨ψ,ψ⟩(6)\inf\sigma(A)=\inf_{0\ne\psi\in D(A)}\frac{\langle\psi,A\psi\rangle}{\langle\psi,\psi\rangle},\qquad \lambda_n=\min_{\dim V=n}\ \max_{0\ne\psi\in V}\frac{\langle\psi,A\psi\rangle}{\langle\psi,\psi\rangle} \tag{6}

Expanded in eigenvectors, the Rayleigh quotient is a weighted average of eigenvalues ∑λk∣ck∣2/∑∣ck∣2\sum\lambda_k|c_k|^2/\sum|c_k|^2, and does not fall below λ1\lambda_1. The eigenvalues of the matrix restricted to a subspace VV are upper bounds for λ1,λ2,…\lambda_1,\lambda_2,\dots, and decrease as VV is enlarged (the Rayleigh–Ritz method). Example. Putting x(1−x)x(1-x) into the Dirichlet −d2/dx2-d^2/dx^2 gives the quotient (1/3)/(1/30)=10≥π2(1/3)/(1/30)=10\ge\pi^2. For estimates from below there is Temple's inequality. If RR is the Rayleigh quotient of ψ∈D(A)\psi\in D(A), and we know a lower bound μ\mu for the next eigenvalue (R<μ≤λ2R\lt\mu\le\lambda_2), the following holds Known.

λ1 ≥ R−∥Aψ∥2/∥ψ∥2−R2μ−R(7)\lambda_1\ \ge\ R-\frac{\lVert A\psi\rVert^2/\lVert\psi\rVert^2-R^2}{\mu-R} \tag{7}

If ψ=x(1−x)\psi=x(1-x), then Aψ=2A\psi=2, ∥Aψ∥2/∥ψ∥2=120\lVert A\psi\rVert^2/\lVert\psi\rVert^2=120. Here λ2=4π2\lambda_2=4\pi^2 is known exactly (section 03), so we can put μ=39\mu=39, giving λ1≥10−20/29=9.310\lambda_1\ge10-20/29=9.310. The Ritz value for 39.50…39.50\dots appearing below Table 2 is an upper bound for λ2\lambda_2, and is no basis for μ\mu. The variational principle alone gives only upper bounds; holding it down from below needs other information. In Temple's inequality it is the lower bound μ\mu for the next level (the convexity V′′≥κV''\ge\kappa of section 08 is another example). This is, with finitely many degrees of freedom, the shape of why the proof of the mass gap is hard (2-05 §04, 4-11).

ComputedTable 2 Rayleigh–Ritz values on Vn={x(1−x)p(x): p of degree at most n−1 }V_n=\{x(1-x)p(x):\ p\ \text{of degree at most}\ n-1\ \text{}\} and the lower bound from (7) (μ=39\mu=39). The matrices were built exactly with fractions.

nUpper bound for λ₁Lower bound for λ₁ (7)Upper bound for λ₃
110.0000000009.310344828—
39.8697496219.866602308102.1303
59.8696044359.86960252489.1736
exact9.86960440188.82644

The antisymmetric functions added for even nn improve only λ2\lambda_2, and the upper bound comes down to 42, 39.50155, 39.4784742,\ 39.50155,\ 39.47847 (4π2=39.478424\pi^2=39.47842). At n=5n=5, π2\pi^2 is caught in an interval of width 2×10−62\times10^{-6} (the lower end depends on μ=39≤4π2\mu=39\le4\pi^2).

The asymmetry of upper and lower bounds — one from above, all from below

To hold a gap or the lowest eigenvalue from above, it is enough to exhibit one trial vector. Every value of the quotient (6) is an upper bound as it stands. To hold it from below, one must show that the quotient does not fall below it for every vector, and information outside the variational principle is needed (the μ\mu of Temple's inequality, the convexity of section 08, the decomposition of the whole by the spectral theorem) Known. The Poincaré constant CPC_P (section 07) is the inverse of the gap, so the directions swap: one trial function gives a lower bound for CPC_P, and an upper bound needs every function.

The mass gap Δ>0\Delta\gt0 is a lower bound on the energy of states orthogonal to the vacuum (4-11 §01). This book puts it in one sentence: a proof of the mass gap is a proof of a lower bound. Trial states and measurements of finitely many correlations give upper bounds for Δ\Delta, and say nothing about the gap being positive (4-11 §02, 8-01 §08). As a metaphor: looking for the lowest valley in the mountains, finding one valley lets you say "at most this low", but "there is no valley lower than this" needs the whole range to be examined. To be exact: evaluating the infimum of (6) with one ψ\psi gives an upper bound, and holding the infimum itself from below needs every ψ\psi.

07

The Poincaré inequality — the best constant is the inverse of the gap

The Poincaré inequality is "a function with small slope does not stray far from its mean" put in numbers. On the interval [0,1][0,1] it takes the following form, and the constant 1/π21/\pi^2 cannot be made smaller Known.

∫01∣f−fˉ∣2dx ≤ 1π2∫01∣f′∣2dx,fˉ=∫01f dx(8)\int_0^1\bigl|f-\bar f\bigr|^2dx\ \le\ \frac1{\pi^2}\int_0^1|f'|^2dx,\qquad \bar f=\int_0^1f\,dx \tag{8}

Proof. Writing f−fˉ=∑k≥1ak2cos⁡kπxf-\bar f=\sum_{k\ge1}a_k\sqrt2\cos k\pi x with the Neumann eigenfunctions 1, 2cos⁡kπx1,\ \sqrt2\cos k\pi x, the left-hand side is ∑∣ak∣2\sum|a_k|^2 and the integral on the right is ∑k2π2∣ak∣2≥π2∑∣ak∣2\sum k^2\pi^2|a_k|^2\ge\pi^2\sum|a_k|^2. Equality holds only when f=a+bcos⁡πxf=a+b\cos\pi x. On an interval of length LL the constant is (L/π)2(L/\pi)^2, proportional to the square of the size (the version on a circle is (4) of 7-06).

This is the variational principle of section 06 used for "the next after 0" of the Neumann operator. In general, if for a self-adjoint A≥0A\ge0 only constants satisfy Af=0Af=0 and the gap is Δ\Delta, then the best constant of Var⁡(f)≤CP⟨f,Af⟩\operatorname{Var}(f)\le C_P\langle f,Af\rangle is CP=1/ΔC_P=1/\Delta, and by (5) the smoothing motion settles at rate 1/CP1/C_P. The Dirichlet version ∫∣f∣2≤π−2∫∣f′∣2\int|f|^2\le\pi^{-2}\int|f'|^2 (f(0)=f(1)=0f(0)=f(1)=0) has the same number, but equality is at sin⁡πx\sin\pi x, and the content is different. Example. For f=xf=x the left-hand side is 1/121/12 and the right-hand side 1/π21/\pi^2, with ratio 0.82.

08

The weighted Poincaré inequality — 1/κ if convex, large if there are two valleys

What field theory needs is the form for a probability measure μ(dx)=e−V(x)dx/Z\mu(dx)=e^{-V(x)}dx/Z (ZZ is the constant making the total 1). Write the inner product as ⟨f,g⟩μ=∫f‾ g dμ\langle f,g\rangle_\mu=\int\overline f\,g\,d\mu, the space of functions of finite length in this inner product as L2(μ)L^2(\mu), and the variance as Var⁡μ(f)=∫∣f−∫f dμ∣2dμ\operatorname{Var}_\mu(f)=\int\bigl|f-\textstyle\int f\,d\mu\bigr|^2d\mu.

Var⁡μ(f)≤CP∫∣f′∣2 dμ;Var⁡μ(x) ≤ CP ≤ 1κ(V′′≥κ>0)(9)\operatorname{Var}_\mu(f)\le C_P\int|f'|^2\,d\mu;\qquad \operatorname{Var}_\mu(x)\ \le\ C_P\ \le\ \frac1\kappa\quad(V''\ge\kappa\gt0) \tag{9}

The best CPC_P is the inverse of the gap of Lf=−f′′+V′f′Lf=-f''+V'f' after 0. LL is self-adjoint on L2(μ)L^2(\mu), integration by parts gives ⟨f,Lf⟩μ=∫∣f′∣2dμ\langle f,Lf\rangle_\mu=\int|f'|^2d\mu, and only constants satisfy Lf=0Lf=0 (the same form as section 07; from the side of the ground state, 2-05 §08). The inequality on the left follows by putting in f=xf=x. The one on the right is said to be a corollary of the variance inequality of Brascamp–Lieb (1976), and also follows from the logarithmic Sobolev inequality of Bakry–Émery (1985) (an inequality stronger than the Poincaré inequality) Known. In one dimension the following line suffices. Differentiating Lf=λfLf=\lambda f, g=f′g=f' gives Lg+V′′g=λgLg+V''g=\lambda g; the inner product with gg gives ∫∣g′∣2dμ+∫V′′g2dμ=λ∫g2dμ\int|g'|^2d\mu+\int V''g^2d\mu=\lambda\int g^2d\mu, hence λ≥κ\lambda\ge\kappa (assuming there is an eigenfunction and the boundary terms vanish). For the normal distribution V=x2/(2σ2)V=x^2/(2\sigma^2) all three are σ2\sigma^2 (Chernoff 1981).

Figure 2 Moving c (from −2 to 4) splits the weight exp(−V_c) (shaded) into two peaks, and the f giving equality (solid line) changes from the straight line x/√Var(x) (dashed) to a step
c = 2.0, barrier c²/4 = 1.00, Var(x) = 1.6655 ≤ C_P = 2.6714 (there is no κ > 0, so there is no upper bound on the right)

ComputedThe numbers in the figure were computed on this machine (the best ff and CPC_P were found with python3 and embedded; the weight e−Vce^{-V_c} is computed on the spot).

ComputedTable 3 CPC_P for Vc=x4/4−cx2/2V_c=x^4/4-cx^2/2 (found by turning LL into an operator of Schrödinger type and using three-point differences; the method is in the table of sources; halving the step agrees to 4 digits). At c<0c\lt0, κ=−c\kappa=-c.

c1/κVar(x)C_P
−20.5000.34510.3503
0—0.67600.7307
1—1.04181.2625
2—1.66552.6714
3—2.58537.6577
4—3.670733.580

With two valleys (c>0c\gt0, height of the hill between the valleys c2/4c^2/4), CPC_P grows much faster than Var⁡(x)\operatorname{Var}(x), and at c=4c=4 it is 9 times as large. The best ff becomes a step close to −1-1 in the left valley and +1+1 in the right, and its slope matters only on the hill, where there is almost no weight. A narrowing of the weight makes CPC_P large.

09

With many variables — products, Gaussians, the free field, and two gaps

When there are many variables x=(x1,…,xn)x=(x_1,\dots,x_n), replace the ∣f′∣2|f'|^2 of (9) by the squared length of the gradient ∣∇f∣2=∑j∣∂jf∣2|\nabla f|^2=\sum_j|\partial_jf|^2. The basics are the following two Known.

(i) The CPC_P of a product measure of independent variables is the maximum of the CPC_P of the factors, and does not depend on the number of variables. LL becomes the sum of the LL for each variable, the eigenfunctions are products f1(x1)⋯fn(xn)f_1(x_1)\cdots f_n(x_n) and the eigenvalues sums, so the value after 0 is the minimum of the gaps of the factors (assuming a basis of eigenfunctions).

(ii) The CPC_P of the Gaussian measure with mean 0 and covariance matrix CC is the largest eigenvalue of CC. Taking the eigenvectors of CC as orthogonal coordinates, the measure splits into a product of independent one-dimensional Gaussians whose variances are the eigenvalues of CC (1-08), and ∣∇f∣2|\nabla f|^2 does not change under a change of orthogonal coordinates. The rest uses (i) and the one-dimensional CP=σ2C_P=\sigma^2 (section 08).

For the free field on the ring of 1-08 (10), C=(−Δlat+m2)−1C=(-\Delta_{\mathrm{lat}}+m^2)^{-1}. The eigenvalues of −Δlat-\Delta_{\mathrm{lat}} are at least 0, and 0 is the constant direction (the direction shifting every xjx_j by the same amount), so the smallest eigenvalue of C−1C^{-1} is m2m^2, hence CP=1/m2C_P=1/m^2. Combined with the correlation length ξ≈1/m\xi\approx1/m (1-08 (11)) this gives CP≈ξ2C_P\approx\xi^2 (this CPC_P is measured with the gradient in the field variables xjx_j. In lattice gauge theory, taking the angles of the links as variables changes the constant factor, so we always state which is used. 10-01).

Here we distinguish two gaps. For the free field, the inverse m2m^2 of CPC_P is the gap of LL (the rate at which e−tLe^{-tL} removes the deviation from the mean in (5)). On the other hand, the gap of the Hamiltonian when 1-08 (10) is read as an imaginary-time path integral is 1/ξ1/\xi in units of the lattice spacing (1-08 (11); ≈m\approx m when mm is small). The squared relation CP≈ξ2C_P\approx\xi^2 is a free-field computation; whether it holds in general in interacting theories is the question of 10-01, and has not been proved (the same form on a group is in 5-11).

10

Detour: counting eigenvalues — Weyl's law and the shape of a drum

Detour

A section you may skip. Kac (1966) relates that at the end of October 1910, Lorentz, invited to give the Wolfskehl lectures in Göttingen, posed at the end of his fourth lecture the problem that "the number of high-frequency standing waves in a cavity should be proportional to its volume regardless of its shape", and Weyl, who was in the audience, proved it in less than two years. For the Dirichlet −Δ-\Delta on a planar region Ω\Omega it takes the following form Known.

N(λ)=#{k: λk≤λ} ∼ ∣Ω∣4π λ(λ→∞);d dimensions give N(λ)∝∣Ω∣ λd/2(10)N(\lambda)=\#\{k:\ \lambda_k\le\lambda\}\ \sim\ \frac{|\Omega|}{4\pi}\,\lambda\quad(\lambda\to\infty);\qquad d\ \text{dimensions give}\ N(\lambda)\propto|\Omega|\,\lambda^{d/2} \tag{10}

ComputedFor the unit square (eigenvalues π2(j2+k2)\pi^2(j^2+k^2)), N=79269N=79269 at λ=106\lambda=10^6. Adding to the leading term 79577.579577.5 the correction −λ/π-\sqrt\lambda/\pi for the perimeter 4 gives 79259.279259.2. Kac discussed that the area and the perimeter can be "heard" from the sequence of eigenvalues (to be exact, are determined by the sequence of eigenvalues alone), and asked about the shape itself. The answer is no: Gordon, Webb and Wolpert (1992) constructed planar regions of different shapes with the same sequence of eigenvalues. Reading λ\lambda as the squared momentum Λ2\Lambda^2, the number of modes up to Λ\Lambda is proportional to Λ4\Lambda^4 in four dimensions. This abundance of short-distance degrees of freedom is one of the starting points for thinking about divergences (4-04, 1-12).


What this chapter can say

ContentStatus
The eigenvalues of (1), the convergence of the lower eigenvalues and the divergence of the top endSaid Known (Table 1, Figure 1 Computed)
Reading the lower end of the spectrum from the lattice in the continuum limit (end of section 01)At the level of Physics. That this limit exists in four dimensions has not been proved (6-10)
Hilbert spaces, self-adjointness, the spectrum, the spectral theorem, Weyl's law (10)Definitions and examples given, theorems cited Known
The variational principle (6), Temple's lower bound (7), Table 2Said Known, Computed. μ=39\mu=39 is a value we could put because we know λ2=4π2\lambda_2=4\pi^2
The Poincaré inequality (8), CP=1/ΔC_P=1/\Delta, (9), the CPC_P of products and of Gaussian measures, the CP=1/m2C_P=1/m^2 of the free fieldSaid Known. The one-dimensional line for (9) and the line for (i) of section 09 assume the existence of eigenfunctions. Table 3 and Figure 2 are Computed
The relation between CPC_P and the correlation length in interacting theoriesNot treated (10-01; not proved). CP≈ξ2C_P\approx\xi^2 is a free-field computation
The spectrum of the Hamiltonian of quantum field theory, the Yang–Mills mass gapNot treated (4-09, 4-11). Nothing is shown

Sources and reproduction

ItemKindSource / tools
Tables 1–3, Figures 1–2, the numbers of section 10Computedpython3 on this machine (NumPy 1.26, SciPy 1.11). Table 3 was found by putting f=ψeV/2f=\psi e^{V/2}, turning LL into −d2/dx2+V′2/4−V′′/2-d^2/dx^2+V'^2/4-V''/2 (the ψ=fϕ0\psi=f\phi_0 of 2-05 §08 with ϕ0=e−V/2\phi_0=e^{-V/2}), and using three-point differences on [−7,7][-7,7]. The figures are plain JavaScript, with the readouts checked against the tables with node
(4)–(7), the spectral theorem, Weyl's criterionKnownG. Temple, Proc. R. Soc. Lond. A 119 (1928) 276–293 / W. Ritz, J. reine angew. Math. 135 (1909) 1–61 / J. von Neumann, Math. Ann. 102 (1930) 49–131 (regarded as a representative paper on the spectral theorem in infinite dimensions) / M. Reed, B. Simon, Methods of Modern Mathematical Physics I (Academic Press, 1972). All bibliographic data only
(9), the CPC_P of products and of Gaussian measures in section 09KnownH. J. Brascamp, E. H. Lieb, J. Funct. Anal. 22 (1976) 366–389 (bibliographic data only; that the inequality on the right of (9) follows as its corollary is not checked) / D. Bakry, M. Émery, Sém. Probab. XIX (1985) 177–206 (the summary at the start checked) / H. Chernoff, Ann. Probab. 9 (1981) 533–535 (abstract checked) / D. Bakry, I. Gentil, M. Ledoux, Analysis and Geometry of Markov Diffusion Operators (Springer, 2014; bibliographic data only)
Weyl's law, Lorentz's problem, drumsKnownH. Weyl, Math. Ann. 71 (1912) 441–479 (title checked, bibliographic data only) / M. Kac, Amer. Math. Monthly 73 (1966) no. 4, part II, 1–23 (text checked) / C. Gordon, D. L. Webb, S. Wolpert, Bull. AMS 27 (1992) 134–138, arXiv:math/9207215 (abstract checked)

Next chapter: 1-11 Fourier analysis and distributions. For use in quantum mechanics, see 2-05.

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Revised 2026-10-01: first version.