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Conformal Transformations in d Dimensions

At a continuum RG fixed point, correlation functions of scaling operators become scale covariant. When the stress-tensor criterion of Lesson 13 holds, the spacetime symmetry extends to conformal symmetry: transformations that may stretch lengths by a position-dependent factor, but preserve angles. We assume that extension here and study its kinematic consequences at separated points.

We derive the conformal Killing equation, explain why two dimensions are exceptional, classify the generators in d>2d>2, and construct inversion and special conformal transformations. A connected special-conformal Ward identity then forces scalar-primary two-point functions of unequal dimensions to vanish. Inversion provides an alternative check when it is also a symmetry of the theory. The next page develops three- and four-point functions and the operator product expansion.

Required background. Lesson 13 derives fixed-point scaling and explains the stress-tensor criterion that promotes scale symmetry to conformal symmetry.

Helpful background. Lesson 12 supplies the scaling-dimension and Ising-operator conventions used in the correlator examples.

A differentiable map is conformal when its Jacobian is locally a scale times an orthogonal matrix:

J(x)=Ω(x)R(x),R(x)TR(x)=1.J(x)=\Omega(x)R(x), \qquad R(x)^T R(x)=\mathbf 1.

Equivalently,

J(x)TJ(x)=Ω(x)21,J(x)^T J(x)=\Omega(x)^2\mathbf 1,

or in components,

∂fρ∂xμ∂fρ∂xν=Ω(x)2δμν.{\partial f^\rho\over\partial x^\mu} {\partial f^\rho\over\partial x^\nu} =\Omega(x)^2\delta_{\mu\nu}.

A circle of tangent vectors is therefore mapped to a circle by the derivative. A right angle remains a right angle, while every tangent-vector length is multiplied by Ω(x)\Omega(x). For a nonlinear map this statement describes the infinitesimal limit; a finite circle need not remain a circle. The figure illustrates the derivative itself.

A circle and two tangent vectors are rotated and uniformly enlarged while retaining their angle

The quantitative illustration applies J=1.25R(22∘)J=1.25R(22^\circ) to a tangent circle of radius 0.720.72 and unit vectors u=(1,0)u=(1,0), v=(0.6,0.8)v=(0.6,0.8). Both panels use the same coordinate scale. Every radius and vector length grows by 1.251.25, while the angle between the vectors is unchanged. This is a linear tangent map, not a claim about finite neighborhoods of an arbitrary nonlinear map.

An isometry is the special case Ω=1\Omega=1. A dilation x′=λxx'=\lambda x with λ>0\lambda>0 has Ω=λ\Omega=\lambda. Unit-sphere inversion has a nonconstant scale factor, Ω(x)=1/x2\Omega(x)=1/x^2 away from the origin; its role as geometry must be distinguished from its possible role as a quantum symmetry.

Infinitesimal form: the conformal Killing equation

Section titled “Infinitesimal form: the conformal Killing equation”

Let

x′μ=xμ+ξμ(x).x'^\mu=x^\mu+\xi^\mu(x).

Then

dx′μ=dxμ+∂νξμ dxν,dx'^\mu=dx^\mu+\partial_\nu\xi^\mu\,dx^\nu,

so, to first order in ξ\xi,

ds′2=(δμν+∂μξν+∂νξμ)dxμdxν.ds'^2 =\left(\delta_{\mu\nu}+\partial_\mu\xi_\nu+ \partial_\nu\xi_\mu\right)dx^\mu dx^\nu.

A conformal transformation may only change the metric by a scalar factor. Hence

∂μξν+∂νξμ=2σ(x)δμν.\partial_\mu\xi_\nu+ \partial_\nu\xi_\mu=2\sigma(x)\delta_{\mu\nu}.

Taking the trace gives

σ(x)=1d∂ρξρ,\sigma(x)={1\over d}\partial_\rho\xi^\rho,

and therefore

∂μξν+∂νξμ=2d(∂⋅ξ)δμν.\boxed{ \partial_\mu\xi_\nu+ \partial_\nu\xi_\mu ={2\over d}(\partial\cdot\xi)\delta_{\mu\nu}. }

This is the conformal Killing equation. Ordinary Killing vectors obey the same equation with the right-hand side set to zero. Conformal Killing vectors are allowed to have a trace part; that trace is the infinitesimal local scale transformation.

The elementary solutions are

translations:ξμ=aμ,rotations:ξμ=ωμνxν,ωμν=−ωνμ,dilations:ξμ=αxμ,special conformal:ξμ=2(b⋅x)xμ−bμx2.\begin{aligned} \text{translations:}\qquad &\xi^\mu=a^\mu,\\ \text{rotations:}\qquad &\xi^\mu=\omega^\mu{}_{\nu}x^\nu, \qquad \omega_{\mu\nu}=-\omega_{\nu\mu},\\ \text{dilations:}\qquad &\xi^\mu=\alpha x^\mu,\\ \text{special conformal:}\qquad &\xi^\mu=2(b\cdot x)x^\mu-b^\mu x^2. \end{aligned}

The special conformal vector is worth checking once. Differentiating gives

∂μξν+∂νξμ=4(b⋅x)δμν,∂⋅ξ=2d(b⋅x),\partial_\mu\xi_\nu+\partial_\nu\xi_\mu=4(b\cdot x)\delta_{\mu\nu}, \qquad \partial\cdot\xi=2d(b\cdot x),

so it indeed satisfies the conformal Killing equation.

In two Euclidean dimensions write

z=x1+ix2,ξ(z,zˉ)=ξ1(x1,x2)+iξ2(x1,x2).z=x^1+i x^2, \qquad \xi(z,\bar z)=\xi^1(x^1,x^2)+i\xi^2(x^1,x^2).

For d=2d=2, the conformal Killing equation becomes

∂1ξ1=∂2ξ2,∂1ξ2=−∂2ξ1.\partial_1\xi^1=\partial_2\xi^2, \qquad \partial_1\xi^2=-\partial_2\xi^1.

These are precisely the Cauchy–Riemann equations, so

∂zˉξ(z)=0.\partial_{\bar z}\xi(z)=0.

The antiholomorphic component satisfies

∂zξˉ(zˉ)=0.\partial_z\bar\xi(\bar z)=0.

Thus the local conformal transformations are

z↦f(z),zˉ↦fˉ(zˉ),z\mapsto f(z), \qquad \bar z\mapsto\bar f(\bar z),

with holomorphic and antiholomorphic functions, at least locally where the derivatives do not vanish. For a real orientation-preserving map of the Euclidean plane, the two functions are complex conjugates. In the complexified conformal algebra they are treated as independent left- and right-moving sectors.

The word “local” matters. On the Riemann sphere, the globally nonsingular one-to-one orientation-preserving conformal maps are only the Möbius transformations

z↦az+bcz+d,ad−bc≠0.z\mapsto {az+b\over cz+d}, \qquad ad-bc\ne0.

On a punctured coordinate patch, local holomorphic vector fields have a Laurent basis,

ln=−zn+1∂z,lˉn=−zˉn+1∂zˉ,n∈Z,l_n=-z^{n+1}\partial_z, \qquad \bar l_n=-\bar z^{n+1}\partial_{\bar z}, \qquad n\in\mathbb Z,

which obey

[lm,ln]=(m−n)lm+n,[lˉm,lˉn]=(m−n)lˉm+n,[lm,lˉn]=0.[l_m,l_n]=(m-n)l_{m+n}, \qquad [\bar l_m,\bar l_n]=(m-n)\bar l_{m+n}, \qquad [l_m,\bar l_n]=0.

The quantum version of this algebra, after central extension, will become the Virasoro algebra.

For d>2d>2, the conformal Killing equation is much more rigid. Differentiating and permuting indices gives

∂μ∂νξρ=δμρ∂νσ+δνρ∂μσ−δμν∂ρσ,σ=1d∂⋅ξ.\partial_\mu\partial_\nu\xi_\rho =\delta_{\mu\rho}\partial_\nu\sigma +\delta_{\nu\rho}\partial_\mu\sigma -\delta_{\mu\nu}\partial_\rho\sigma, \qquad \sigma={1\over d}\partial\cdot\xi.

Take ∂ρ\partial^\rho of this identity and use ∂⋅ξ=dσ\partial\cdot\xi=d\sigma. This gives

(d−2)∂μ∂νσ=−δμν□σ.(d-2)\partial_\mu\partial_\nu\sigma =-\delta_{\mu\nu}\Box\sigma.

Its trace gives 2(d−1)□σ=02(d-1)\Box\sigma=0. For d>2d>2 the Hessian of σ\sigma therefore vanishes: σ\sigma is affine, and the displayed second-derivative identity makes ξ\xi at most quadratic on a connected smooth patch. The general solution is

ξμ(x)=aμ+ωμνxν+αxμ+2(b⋅x)xμ−bμx2.\boxed{ \xi^\mu(x)=a^\mu+ \omega^\mu{}_{\nu}x^\nu+ \alpha x^\mu+2(b\cdot x)x^\mu-b^\mu x^2. }

Counting parameters gives

N=d+d(d−1)2+1+d=(d+1)(d+2)2.N=d+{d(d-1)\over2}+1+d ={(d+1)(d+2)\over2}.

For d>2d>2, the Lie algebra of Euclidean conformal transformations is

so(d+1,1).\mathfrak{so}(d+1,1).

Equivalently, the identity component of the conformal group is locally isomorphic to SO0(d+1,1)SO_0(d+1,1). Global statements require the conformal compactification SdS^d and a discrete quotient; inversion lies outside the identity component.

A useful differential-operator basis is

Pμ=∂μ,Mμν=xμ∂ν−xν∂μ,P_\mu=\partial_\mu, \qquad M_{\mu\nu}=x_\mu\partial_\nu-x_\nu\partial_\mu, D=x⋅∂,Kμ=2xμx⋅∂−x2∂μ.D=x\cdot\partial, \qquad K_\mu=2x_\mu x\cdot\partial-x^2\partial_\mu.

With these sign conventions,

[D,Pμ]=−Pμ,[D,Kμ]=Kμ,[Pμ,Kν]=2δμνD−2Mμν.[D,P_\mu]=-P_\mu, \qquad [D,K_\mu]=K_\mu, \qquad [P_\mu,K_\nu]=2\delta_{\mu\nu}D-2M_{\mu\nu}.

The finite-dimensional algebra for d>2d>2 should be compared with the infinite-dimensional local algebra in d=2d=2. That contrast is one of the central structural facts of conformal field theory.

Inversion and special conformal transformations

Section titled “Inversion and special conformal transformations”

Inversion in the unit sphere, on the patch x≠0x\ne0, is

I:x′μ=xμx2.I:\qquad x'^\mu={x^\mu\over x^2}.

Its Jacobian is

∂x′ρ∂xμ=1x2(δρμ−2xρxμx2).{\partial x'^\rho\over\partial x^\mu} ={1\over x^2}\left(\delta^\rho{}_{\mu}-{2x^\rho x_\mu\over x^2}\right).

The matrix in parentheses reflects the radial direction and fixes the transverse directions. Its determinant is −1-1, so inversion is outside the identity component. It is nevertheless a useful geometric construction, whether or not the quantum theory has this additional discrete symmetry. See Rychkov 2016, arXiv v2, §2.2.1, p. 25, and §2.3.3, p. 31, PDF. Orthogonality gives

∂x′ρ∂xμ∂x′ρ∂xν=1(x2)2δμν.{\partial x'^\rho\over\partial x^\mu} {\partial x'^\rho\over\partial x^\nu} ={1\over (x^2)^2}\delta_{\mu\nu}.

Thus inversion has local scale factor

Ω(x)=1x2.\Omega(x)={1\over x^2}.

For two points,

x1′=x1x12,x2′=x2x22,x'_1={x_1\over x_1^2}, \qquad x'_2={x_2\over x_2^2},

we find

∣x1′−x2′∣2=(x1x12−x2x22)2=1x12+1x22−2x1⋅x2x12x22=∣x1−x2∣2x12x22.\begin{aligned} |x'_1-x'_2|^2 &=\left({x_1\over x_1^2}-{x_2\over x_2^2}\right)^2\\ &={1\over x_1^2}+{1\over x_2^2}-{2x_1\cdot x_2\over x_1^2x_2^2}\\ &={|x_1-x_2|^2\over x_1^2x_2^2}. \end{aligned}

Equivalently,

∣x12′∣2=Ω(x1)Ω(x2)∣x12∣2.|x'_{12}|^2=\Omega(x_1)\Omega(x_2)|x_{12}|^2.

The figure checks the endpoint factors on an explicit pair of points.

Two points outside the unit circle map along their rays to inside points with a shorter separation fixed by both endpoint factors

The quantitative unit-sphere inversion uses x1=(2,1)x_1=(2,1) and x2=(2,−1)x_2=(2,-1) in dimensionless coordinates, giving x1′=(0.4,0.2)x'_1=(0.4,0.2) and x2′=(0.4,−0.2)x'_2=(0.4,-0.2). Both panels use the same scale. Each endpoint has Ωi=1/5\Omega_i=1/5, so the separation changes from 22 to 2/52/5 and its square by 1/251/25. This is a geometric identity; no inversion symmetry of a quantum theory is assumed.

A special conformal coordinate map can be constructed by inversion, followed by translation, followed by inversion. With the convention

Kb=I∘T−b∘I,K_b=I\circ T_{-b}\circ I,

one obtains

x′μ=xμ−bμx21−2b⋅x+b2x2.\boxed{ {x'}^\mu={x^\mu-b^\mu x^2\over 1-2b\cdot x+b^2x^2}. }

For b≠0b\ne0, the denominator equals b2∣x−b/b2∣2b^2|x-b/b^2|^2, so the finite Euclidean chart excludes x=b/b2x=b/b^2. The origin has a regular image despite the intermediate inversions. The map belongs to the connected conformal group on the compactification; using two inversions to construct it does not require either inversion to be a quantum symmetry. Expanding to first order in bb gives

x′μ=xμ+2(b⋅x)xμ−bμx2+O(b2),{x'}^\mu=x^\mu+2(b\cdot x)x^\mu-b^\mu x^2+O(b^2),

which is exactly the infinitesimal special conformal vector.

Primary scalar fields and two-point functions

Section titled “Primary scalar fields and two-point functions”

Assume a conformally invariant vacuum and scalar primaries that diagonalize dilations. For connected conformal transformations, a primary of dimension Δ\Delta has the local transformation law

O′(x′)=Ω(x)−ΔO(x).\boxed{ O'(x')=\Omega(x)^{-\Delta}O(x). }

If inversion is also a symmetry and OO is inversion-even without operator mixing, the same law reads

O′(x′)=(x2)ΔO(x).O'(x')=(x^2)^\Delta O(x).

At separated insertions, the corresponding covariance law for connected conformal maps is

⟨O1(x1′)⋯On(xn′)⟩=∏i=1nΩ(xi)−Δi⟨O1(x1)⋯On(xn)⟩.\boxed{ \left\langle O_1(x'_1)\cdots O_n(x'_n)\right\rangle =\prod_{i=1}^n\Omega(x_i)^{-\Delta_i} \left\langle O_1(x_1)\cdots O_n(x_n)\right\rangle. }

For a scalar two-point function of identical primaries,

⟨O(x1)O(x2)⟩=CO∣x1−x2∣2Δ,\langle O(x_1)O(x_2)\rangle={C_O\over |x_1-x_2|^{2\Delta}},

the distance identity gives an algebraic inversion-covariance check:

⟨O(x1′)O(x2′)⟩=CO∣x1′−x2′∣2Δ=CO[Ω(x1)Ω(x2)∣x1−x2∣2]Δ=Ω(x1)−ΔΩ(x2)−ΔCO∣x1−x2∣2Δ.\begin{aligned} \langle O(x'_1)O(x'_2)\rangle &={C_O\over |x'_1-x'_2|^{2\Delta}}\\ &={C_O\over [\Omega(x_1)\Omega(x_2)|x_1-x_2|^2]^\Delta}\\ &=\Omega(x_1)^{-\Delta}\Omega(x_2)^{-\Delta} {C_O\over |x_1-x_2|^{2\Delta}}. \end{aligned}

For spinning primaries one must also rotate the indices by the local orthogonal matrix

Rμν(x)=Ω(x)−1∂x′μ∂xν.R^\mu{}_{\nu}(x)=\Omega(x)^{-1}{\partial x'^\mu\over\partial x^\nu}.

For connected maps this local matrix is a proper rotation. Its representation on tensor or spinor indices is essential for spinning primaries. An extension to reflections requires additional discrete-symmetry data.

Now consider two scalar primaries of dimensions Δi\Delta_i and Δj\Delta_j. Translation, rotation, and scale invariance allow

⟨Oi(x1)Oj(x2)⟩=Cij∣x1−x2∣Δi+Δj.\langle O_i(x_1)O_j(x_2)\rangle ={C_{ij}\over |x_1-x_2|^{\Delta_i+\Delta_j}}.

Connected special-conformal symmetry supplies the stronger constraint. Expanding the covariance law with ξμ=2(b⋅x)xμ−bμx2\xi^\mu=2(b\cdot x)x^\mu-b^\mu x^2 and Ω=1+2b⋅x+O(b2)\Omega=1+2b\cdot x+O(b^2) gives the Ward identity

∑a=12[2xaαxa⋅∂a−xa2∂aα+2Δaxaα]Gij=0.\sum_{a=1}^2 \left[2x_{a\alpha}x_a\cdot\partial_a -x_a^2\partial_{a\alpha}+2\Delta_a x_{a\alpha}\right]G_{ij}=0.

Use translation invariance to set x1=x≠0x_1=x\ne0 and x2=0x_2=0. The second insertion contributes zero. Writing s=Δi+Δjs=\Delta_i+\Delta_j, the radial form gives x⋅∂Gij=−sGijx\cdot\partial G_{ij}=-sG_{ij} and ∂αGij=−sxαGij/x2\partial_\alpha G_{ij}=-s x_\alpha G_{ij}/x^2. Consequently

0=(−2s+s+2Δi)xαGij=(Δi−Δj)xαGij.0=(-2s+s+2\Delta_i)x_\alpha G_{ij} =(\Delta_i-\Delta_j)x_\alpha G_{ij}.

For arbitrary nonzero separation this requires equal dimensions or a vanishing coefficient:

⟨Oi(x1)Oj(x2)⟩=0unless Δi=Δj.\boxed{ \langle O_i(x_1)O_j(x_2)\rangle=0 \qquad \text{unless } \Delta_i=\Delta_j. }

This proof requires no inversion symmetry. An embedding-space derivation and the scalar covariance formulas are given in Rychkov 2016, arXiv v2, §2.2.1, pp. 24–26, PDF. Contact terms at coincident points are outside the argument.

If several scalar primaries share a dimension and compatible internal quantum numbers, their two-point coefficients form a constant matrix. For Hermitian operators in a unitary theory one can diagonalize the positive two-point form after removing null operators. For complex operators the positive form pairs each operator with its adjoint. None of this makes two different equal-dimension operators identical.

In the two-dimensional critical Ising theory, the identity 11, spin field σ\sigma, disorder field μ\mu, and energy field ε\varepsilon can all be represented as scalar conformal fields. Their dimensions are

Δ1=0,Δσ=Δμ=18,Δε=1.\Delta_1=0, \qquad \Delta_\sigma=\Delta_\mu={1\over8}, \qquad \Delta_\varepsilon=1.

These dimensions are developed in Di Francesco, Mathieu and Sénéchal 1997, §§12.2.1–12.2.2, pp. 443–445 and translated to this course’s conventions in Lesson 12. Conformal covariance therefore predicts

⟨σ(x)σ(0)⟩∝1∣x∣1/4,⟨μ(x)μ(0)⟩∝1∣x∣1/4,⟨ε(x)ε(0)⟩∝1∣x∣2.\langle \sigma(x)\sigma(0)\rangle\propto {1\over |x|^{1/4}}, \qquad \langle \mu(x)\mu(0)\rangle\propto {1\over |x|^{1/4}}, \qquad \langle \varepsilon(x)\varepsilon(0)\rangle\propto {1\over |x|^2}.

It also predicts, in a basis adapted to conformal symmetry, that

⟨σ(x)ε(0)⟩=0,\langle \sigma(x)\varepsilon(0)\rangle=0,

because Δσ≠Δε\Delta_\sigma\ne\Delta_\varepsilon. The equality Δσ=Δμ\Delta_\sigma=\Delta_\mu is consistent with Kramers–Wannier duality, but it does not mean that σ\sigma and μ\mu are the same local operator. They are mutually nonlocal: taking an order field around a disorder field detects a branch cut. In the diagonal local Ising CFT, one chooses a mutually local operator algebra rather than treating both lattice realizations as independent local primaries. Conformal invariance fixes powers and tensor structures; the operator algebra still remembers the order–disorder construction.

Conformal symmetry is the symmetry of local angle preservation. Its infinitesimal form is the conformal Killing equation

∂μξν+∂νξμ=2d(∂⋅ξ)δμν.\partial_\mu\xi_\nu+ \partial_\nu\xi_\mu ={2\over d}(\partial\cdot\xi)\delta_{\mu\nu}.

In two dimensions this equation becomes the Cauchy–Riemann equation, producing infinitely many local conformal maps. In d>2d>2 it has only the finite-dimensional solution space generated by translations, rotations, dilations, and special conformal transformations.

Inversion is the key finite transformation. Its distance identity

∣x12′∣2=∣x12∣2x12x22|x'_{12}|^2={|x_{12}|^2\over x_1^2x_2^2}

provides a geometric covariance check. The scalar selection rule follows from a connected special-conformal Ward identity; treating inversion as a quantum symmetry is an additional assumption.

The factor Ω(x)\Omega(x) multiplies lengths, not squared lengths. The metric transforms with Ω(x)2\Omega(x)^2.

The statement that two-dimensional conformal maps are arbitrary holomorphic functions is local. Globally regular maps on the sphere are Möbius transformations.

For a real Euclidean conformal map, the antiholomorphic function is the complex conjugate of the holomorphic one. Treating the two sectors as independent refers to the complexified algebra.

Inversion is singular at the origin and exchanges the origin with infinity. It lies outside the identity component; a conformal theory need not be invariant under it. Algebraic inversion identities are usually cleanest on the conformal compactification.

For d>2d>2, the conformal group is locally related to SO(d+1,1)SO(d+1,1), but the exact global group depends on connected components and a discrete quotient. The Lie-algebra statement conf(Rd)≅so(d+1,1)\mathfrak{conf}(\mathbb R^d)\cong\mathfrak{so}(d+1,1) refers to this finite-dimensional case, not the full local algebra in two dimensions.

Scale invariance alone permits a two-point function proportional to ∣x∣−Δi−Δj|x|^{-\Delta_i-\Delta_j}. The condition Δi=Δj\Delta_i=\Delta_j comes from the larger conformal group.

Exercise 1: Special conformal Killing vector

Section titled “Exercise 1: Special conformal Killing vector”

Verify that

ξμ=2(b⋅x)xμ−bμx2\xi^\mu=2(b\cdot x)x^\mu-b^\mu x^2

satisfies the conformal Killing equation.

Solution

Differentiate:

∂νξμ=2bνxμ+2(b⋅x)δμν−2bμxν.\partial_\nu\xi_\mu =2b_\nu x_\mu+2(b\cdot x)\delta_{\mu\nu}-2b_\mu x_\nu.

Therefore

∂νξμ+∂μξν=4(b⋅x)δμν.\partial_\nu\xi_\mu+\partial_\mu\xi_\nu =4(b\cdot x)\delta_{\mu\nu}.

The divergence is

∂μξμ=2(d+1)(b⋅x)−2(b⋅x)=2d(b⋅x).\partial_\mu\xi^\mu =2(d+1)(b\cdot x)-2(b\cdot x) =2d(b\cdot x).

Thus

2d(∂⋅ξ)δμν=4(b⋅x)δμν,{2\over d}(\partial\cdot\xi)\delta_{\mu\nu} =4(b\cdot x)\delta_{\mu\nu},

which matches the symmetrized derivative.

Show that the two-dimensional conformal Killing equation is equivalent to the Cauchy–Riemann equations for ξ=ξ1+iξ2\xi=\xi^1+i\xi^2.

Solution

For d=2d=2,

∂iξj+∂jξi=(∂kξk)δij.\partial_i\xi_j+\partial_j\xi_i=(\partial_k\xi_k)\delta_{ij}.

The 1111 component gives

2∂1ξ1=∂1ξ1+∂2ξ2,2\partial_1\xi^1=\partial_1\xi^1+\partial_2\xi^2,

so

∂1ξ1=∂2ξ2.\partial_1\xi^1=\partial_2\xi^2.

The 1212 component gives

∂1ξ2+∂2ξ1=0.\partial_1\xi^2+\partial_2\xi^1=0.

These are exactly the Cauchy–Riemann equations, so ∂zˉξ=0\partial_{\bar z}\xi=0.

Derive the inversion distance formula

∣x1′−x2′∣2=∣x1−x2∣2x12x22,xi′=xixi2.|x'_1-x'_2|^2={|x_1-x_2|^2\over x_1^2x_2^2}, \qquad x'_i={x_i\over x_i^2}.
Solution

Compute directly:

∣x1′−x2′∣2=(x1x12−x2x22)2=1x12+1x22−2x1⋅x2x12x22=x12+x22−2x1⋅x2x12x22=∣x1−x2∣2x12x22.\begin{aligned} |x'_1-x'_2|^2 &=\left({x_1\over x_1^2}-{x_2\over x_2^2}\right)^2\\ &={1\over x_1^2}+{1\over x_2^2}-{2x_1\cdot x_2\over x_1^2x_2^2}\\ &={x_1^2+x_2^2-2x_1\cdot x_2\over x_1^2x_2^2}\\ &={|x_1-x_2|^2\over x_1^2x_2^2}. \end{aligned}

Exercise 4: Equal dimensions from inversion covariance

Section titled “Exercise 4: Equal dimensions from inversion covariance”

Assume in addition that inversion preserves the vacuum and that the two scalar primaries are inversion-even with no mixing. Use inversion covariance to recover the equal-dimension condition already derived above from connected symmetry. Take separated points away from the inversion origin.

Solution

Start from the scale-invariant form

⟨Oi(x1)Oj(x2)⟩=Cij∣x1−x2∣Δi+Δj.\langle O_i(x_1)O_j(x_2)\rangle ={C_{ij}\over |x_1-x_2|^{\Delta_i+\Delta_j}}.

At inverted points this becomes

Cij(x12x22)(Δi+Δj)/2∣x1−x2∣Δi+Δj.{C_{ij}(x_1^2x_2^2)^{(\Delta_i+\Delta_j)/2} \over |x_1-x_2|^{\Delta_i+\Delta_j}}.

Primary covariance gives instead

Cij(x12)Δi(x22)Δj∣x1−x2∣Δi+Δj.{C_{ij}(x_1^2)^{\Delta_i}(x_2^2)^{\Delta_j} \over |x_1-x_2|^{\Delta_i+\Delta_j}}.

If Cij≠0C_{ij}\ne0, the powers of x12x_1^2 and x22x_2^2 must match independently, so

Δi+Δj2=ΔiandΔi+Δj2=Δj.{\Delta_i+\Delta_j\over2}=\Delta_i \qquad\text{and}\qquad {\Delta_i+\Delta_j\over2}=\Delta_j.

Thus Δi=Δj\Delta_i=\Delta_j. If the dimensions differ, Cij=0C_{ij}=0.

Exercise 5: Infinitesimal special conformal transformation

Section titled “Exercise 5: Infinitesimal special conformal transformation”

Show that

x′μ=xμ−bμx21−2b⋅x+b2x2{x'}^\mu={x^\mu-b^\mu x^2\over 1-2b\cdot x+b^2x^2}

has infinitesimal form

δxμ=2(b⋅x)xμ−bμx2+O(b2).\delta x^\mu=2(b\cdot x)x^\mu-b^\mu x^2+O(b^2).
Solution

Expand the denominator:

11−2b⋅x+b2x2=1+2b⋅x+O(b2).{1\over 1-2b\cdot x+b^2x^2}=1+2b\cdot x+O(b^2).

Then

x′μ=(xμ−bμx2)(1+2b⋅x)+O(b2),{x'}^\mu=(x^\mu-b^\mu x^2)(1+2b\cdot x)+O(b^2),

so

x′μ=xμ+2(b⋅x)xμ−bμx2+O(b2).{x'}^\mu=x^\mu+2(b\cdot x)x^\mu-b^\mu x^2+O(b^2).

Subtracting xμx^\mu gives the result.

  • Di Francesco, Philippe, Pierre Mathieu, and David Sénéchal. Conformal Field Theory. Springer, 1997. DOI.
  • Rychkov, Slava. EPFL Lectures on Conformal Field Theory in D ≥ 3 Dimensions. arXiv:1601.05000v2 (2016). Versioned PDF. Locators above refer to the preprint’s printed pages.
  • Cardy, John. Scaling and Renormalization in Statistical Physics. Cambridge University Press, 1996. DOI.

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