Domenico Fiorenza
Vertex algebras avant Borcherds

Contents

Idea

If you open your favourite book in conformal field theory, within the first 10 pages you will almost surely find an expression like this:

T(z)T(w)D/2(zw) 4+2(zw) 2T(w)+1(zw)T(w)T(z)T(w)\sim \frac{D/2}{(z-w)^4}+\frac{2}{(z-w)^2}T(w)+\frac{1}{(z-w)}\partial T(w)

or equivalently, in the D’Andrea-Kac notation

[T λT]=D12λ 3+2λT+T,[T_\lambda T]= \frac{D}{12}{\lambda^3}+2\lambda T+\partial T,

or even, directly in terms of Laurent coefficients,

[L m,L n]=(mn)L m+n+Dm 3m12δ m,n.[L_m,L_n]= (m-n)L_{m+n}+D\frac{m^3-m}{12}\delta_{m,-n}.

Following Borcherds, expressions like the above are at the basis of the modern axiomatization of vertex algebras. It’s worth recalling how they historically arose from path-integral heuristics.

The basic rules

The players

  • Σ, a Riemann surface
  • , a sheaf on Σ;
  • M=(Σ) (we pretend M to be a differentiable manifold, endowed with a volume form dvol M)
  • ^ ΣΣ, the etale space of
  • ev:M×Σ^ Σ, the map sending a global section X and a point p to the germ X p of X at p
  • C (M×Σ;)ev *{^ Σ}, a set of local fields, i.e., smooth functions on M×Σ whose value at (X,p) only depends on the germ X p.
  • S:M, the action.

Notation: Let V be a (topological) vector space; if f:MV is integrable w.r.t. the measure e Sdvol M, we write

f= Mfe Sdvol M\langle f\rangle =\int_M f\, e^{-S}d vol_M

n-point functions

To a pair (A,X) consisting of a field and a global section, we can associate a distribution A X𝒟(Σ) as follows:

A X:f Σf(p)A(X,p)drmvol ΣA_X\colon f\mapsto \int_\Sigma f(p)A(X,p)d{\rm vol}_\Sigma

Distributions are an algebra (w.r.t. tensor product)

𝒟(Σ m)𝒟(Σ n)𝒟(Σ m+n)\mathcal{D}'(\Sigma^m)\otimes \mathcal{D}'(\Sigma^n)\to \mathcal{ D}'(\Sigma^{m+n})

with

φψ:f Σ m+nφ(p 1)ψ(p 2)f(p 1,p 2)drmvol Σ m+n\varphi\otimes\psi\colon f\mapsto \int_{\Sigma^{m+n}}\varphi(\vec{p}_1)\psi(\vec{p}_2)f(\vec{p}_1,\vec{p}_2)d{\rm vol}_{\Sigma^{m+n}}

so we get a map n×M𝒟(Σ n)

(A 1,,A n;X)A 1,XA n,X(A_1,\dots,A_n;X)\mapsto A_{1,X}\otimes\cdots \otimes A_{n,X}

which we can look at as a map

MrmHom( n,𝒟(Σ n)).M\to{\rm Hom}(\mathcal{F}^{\otimes n},\mathcal{D}'(\Sigma^n)).

Integrating over M we get the n-point function

n: n𝒟(Σ n)\langle\,\rangle_n\colon\mathcal{F}^{\otimes n}\to\mathcal {D}'(\Sigma^n)

Explicitly, for A 1,,A n in , the n-point function A 1A n n is the distribution on Σ n whose density at (p 1,,p n) is

A 1(X,p 1)A n(X,p n) n= MA 1(X,p 1)A n(X,p n)e S(X)dvol M(X)\langle A_1(X,p_1)\cdots A_n(X,p_n)\rangle_n= \int_M A_1(X,p_1)\cdots A_n(X,p_n) e^{-S(X)}d vol_M(X)

We can also look at the map n×M𝒟(Σ n) as to a map nC (M,𝒟(Σ n); we denote denote by A 1A n the image of (A 1,,A n) by this map.

Off-diagonal regularity

Let Δ nΣ n be the big diagonal

Δ n={non-injective maps{1,,n}Σ}}\Delta_n=\bigl\{\text{non-injective maps} \{1,\dots,n\}\to \Sigma\}\bigr\}

Consider the restrictions 𝒟(Σ n)𝒟(Σ nΔ n). We ask the restrictions of the n-point functions to be regular distributions on Σ nΔ n, i.e., for fixed A 1,,A n, the density A 1(p 1)A n(p n) n is a smooth function on on Σ nΔ n. Singularities may appear when p i,p jp for ij. In particular, 1-point functions are smooth.

Regularization

We further assume to have an operator ::,

nC (M×Σ n;)\mathcal{F}^{\otimes n}\to C^\infty(M\times \Sigma^n;\mathbb{C})
A 1A n:A 1A n:A_1\otimes \cdots\otimes A_n\mapsto :A_1\cdots A_n:

such that

A 1A n n=:A 1A n:+singular distribution,\langle A_1\cdots A_n\rangle_n=\langle:A_1\cdots A_n:\rangle+\text{singular distribution},

where the on the right-hand side is integration over M with respect to the measure e Sdrmvol M:

:C (M×Σ n;)C (Σ n;).\langle\,\,\rangle: C^\infty(M\times \Sigma^n;\mathbb{C})\to C^\infty( \Sigma^n;\mathbb{C}).

Via the embedding C (Σ n;)𝒟(Σ n;) induced by a choice of a volume form on Σ, we can look at both A 1A n and :A 1A n: as 𝒟(Σ n;)-valed functions on M. With this identification, the difference A 1A n:A 1A n: is an 𝒟(Σ n;)-valed functions on M whose integral over M is the singular part of A 1A n n. Moreover, we also require :A:=A 1 for 1-point functions. This rules out the trivial regularization given by :A 1A n:=0 for any A 1,,A n. For the 2-point functions regularization gives

AB=:AB:+φ ABA B = : A B: +\,\varphi_{A B}

for a suitable function φ AB:M𝒟(Σ 2;). One the 2-point regularizations have been chosen, we can define higher order regularizations iteratively, as follows:

:A:=A

:AB:=ABφ AB

:ABC:=ABCφ ABCφ BCAφ ACB

:ABCD:=ABCDφ ABCDφ ACBDφ CDAB+φ ABφ CD+φ ACφ BD+φ ADφ BC

and so on. Therefore, in general, if 𝒜=A 1A n, then

:𝒜:=𝒜contractions{:}\mathcal{A}:=\mathcal{A}-\text{contractions}

Remark: If 𝒜=A 1A n and =B 1B m, then

:𝒜:=𝒜allcontractions{:}\mathcal{A}\mathcal{B}:=\mathcal{A}\mathcal{B}-all contractions
:𝒜:=𝒜𝒜contractions{:}\mathcal{A}:=\mathcal{A}-\mathcal{A}contractions
::=contractions{:}\mathcal{B}:=\mathcal{B}-\mathcal{B}contractions

and so

:𝒜:::=:𝒜:+𝒜contractions.{:}\mathcal{A}::\mathcal{B}:=:\mathcal{A}\mathcal {B}:+\mathcal{ A}\mathcal{B}contractions.

Therefore singularities of :𝒜::: come entirely from the 𝒜-contractions of 𝒜.

Example: :A 1A 2::B 1B 2:=φ A 1B 1φ A 2B 2+φ A 1B 2φ A 2B 1+φ A 1B 1:A 2B 2:+φ A 1B 2:A 2B 1:+φ A 2B 1:A 1B 2:+φ A 2B 2:A 1B 1:+:A 1A 2B 1B 2:

Notation: One defines

R AB(z)=:AB:(z,z);R_{A B}(z)=:A B:(z,z);

it is a smooth function on Σ. In physicists’ notation, one writes :A(z)B(w): for :AB:(z,w), and so

R AB(z)=lim wz:A(z)B(w):R_{AB}(z)=\lim_{w\to z}:A(z)B(w):

Moreover, multilinearity of regularization gives

z:A(z)B(w):=: zA(z)B(w):\partial_z:A(z)B(w):=:\partial_zA(z)B(w):

and so

zR AB(z)=R zAB(z)+R A zB(z)\partial_z R_{AB}(z)=R_{\partial_z A\, B}(z)+R_{ A\partial_z B}(z)

The game

The rules of the game

Promote each element A of to an operator A^, its quantization. By this we mean that A^ is an element of some associative algebra. More precisely, consider the free associative algebra

T()= n0 nT(\mathcal{F})=\bigoplus_{n\geq 0}\mathcal{F}^{\otimes n}

generated by , modulo the following relations:

A^ 1A^ n=0iffA 1A nB 1B m m+n Σ m+nΔ m+n n=0\hat{A}_1\cdots \hat{A}_n=0 \qquad iff\qquad \langle A_1\cdots A_n\, B_1\cdots B_m\rangle_{m+n}\biggr\vert_{\Sigma^{m+n}\setminus \Delta^{\ge n}_{m+n}}=0

for any B 1,B m, where

Δ n k={(p 1,,p n)p i=p jforsomeijwithjk}\Delta_n^{\geq k}=\{(p_1,\dots,p_n)\,|\, p_i=p_j for some i\neq j with j\geq k\}

We will adopt the following shorthand notation for the above relations:

𝒜=0.\langle\mathcal{A}\cdots\rangle=0.

Advanced tricks

Lie derivatives

Assume a linear map

i:C 0 (Σ)H 0(M;TM)i\colon C^\infty_0(\Sigma)\to H^0(M;T M)

is given, where TM denotes the tangent bundle of M. Then each 1-form ω on M gives a distribution (ωi) on Σ by

f(ωi f)= M(ωi f)e Sdvol M.f\mapsto\langle (\omega|i_f)\rangle=\int_M(\omega|i_f) e^{-S}d vol_M.

For any vector field v on M, the Lie derivative v satisfies

(dSv)+div(v)= M v(e Sdvol M)=0.\langle (d S|v)\rangle+\langle div(v)\rangle=\int_M \mathcal{L}_v(e^{-S}d vol_M)=0.

Hence, if the vector fields i f are divergence-free, the 1-point function (dSi) is zero. If f is supported away from q 1,,q m, then, for any B 1,,B m,

i f(B 1(X,q 1)B m(X,q m))=0\mathcal{L}_{i_f}(B_1(X,q_1)\cdots B_m(X,q_m))=0

hence

(dSi)=0\langle (d S|i)\cdots\rangle=0

so we recover within this formalism a version of Ehrenfest’s theorem.

Noether’s theorem

Let v be a symmetry of the action, i.e., a vector field such (dSv)=0, and assume furthermore that div(v)=0, so that

div S(v)=0,div_S(v)=0,

where

div S(v)= v(e Sdvol M).div_S(v)=\mathcal {L}_{v}(e^{-S}d vol_M).

Then, for any X in M, the map C (M;) given by

ρdiv S(ρv) X\rho\mapsto div_S(\rho v)_X

is a distribution on Σ which is zero on constant functions. From the exact sequence

0C (Σ)d{Exact1formsonΣ}0,0\to \mathbb{C}\to C^\infty(\Sigma)\stackrel{d}{\to}\{Exact\, 1-forms on \Sigma\}\to 0,

there exist

j v,X:{Exact1formsonΣ}j_{v,X}:\{Exact\, 1-forms on \Sigma\}\to \mathbb{C}

such that

div S(ρv) X=(j v,Xdρ).div_S(\rho v)_X=(j_{v,X}|d\rho).

Assume j v,X extends to a 1-current j v,X:{1formsonΣ}. Then

0= M ρv(e Sdvol M)=(j v,Xdρ)=(j vρ)0=\int_M\mathcal{L}_{\rho v}(e^{-S}d vol_M)= \langle(j_{v,X}|d\rho)\rangle= \langle(\partial j_{v}|\rho)\rangle

Hence j v is the zero distribution and, more in general, j v=0,i.e.j v^=0. Identify j v,X with a 1-form via the canonical pairing of 1-forms on Σ:

(j v,Xω)= Σj v,Xω(j_{v,X}|\omega)=\int_\Sigma j_{v,X} \wedge \omega

Then

dj v=0.\langle d j_{v}\cdots\rangle=0.

Ward identities

Now add a field A. Then

0= M ρvA(p)(e Sdvol M)=(j Xρ)A(p)+ ρvA(p).0=\int_M\mathcal{L}_{\rho v}A(p)(e^{-S}d vol_M)= \langle(\partial j_X|\rho)A(p)\rangle+\langle\mathcal{L}_{\rho v}A(p)\rangle.

If ρ is a bump function at p, then ρvA(p)= vA(p) and so

vA(p)=A(p) Σρdj v=A(p) B pdj v= B pA(p)j v,\langle\mathcal{L}_v A(p)\rangle=\langle A(p)\int_\Sigma \rho d j_{v}\rangle=\langle A(p)\int_{B_p} d j_{v}\rangle =\int_{\partial B_p}\langle A(p) j_{v} \rangle,

where B p denotes a little disk centered at p (the support of the bump function ρ). Let

Q v,p= B pj vQ_{v,p}=\int_{\partial B_p}\langle j_v\cdots \rangle

be the charge of v at p. Then

v p=Q v,p\langle\mathcal{L}_v\cdots\rangle\bigr\vert_p=Q_{v,p}

The holomorphic case

If A(p)j v is holomorphic in B pp, then

B pA(p)j v=Res zpA(p)j v(z)dz\int_{\partial B_p}\langle A(p) j_v \rangle=Res_{z\to p}\langle A(p) j_v(z) \rangle dz

And we obtain

vA(p)=Res zpA(p)j v,\langle\mathcal{L}_v A(p)\rangle=Res_{z\to p}\langle A(p) j_v \rangle,

That is

Q v,p=Res zpj v(z)dz.Q_{v,p}= Res_{z\to p}\langle j_v(z)\cdots\rangle dz.

OPEs

Assume A(z)B(w) is a holomorphic function of z for zw.

We write

(1)A(z)B(w) k1C k(w)1(zw) kA(z)B(w)\sim \sum_{k\geq 1} C_k(w)\frac{1}{(z-w)^k}

to mean

A(z)B(w)= k1C k(w)1(zw) k+:A(z)B(w):\langle A(z)B(w)\cdots \rangle= \sum_{k\geq 1} \langle C_k(w)\cdots \rangle \frac{1}{(z-w)^k}+\langle:A(z)B(w):\cdots \rangle

The expression in equation (1) is called operator product exapansion of A and B (AB OPE for short). Note that :A(z)B(w): is a holomorphic function of z also at z=w.

Since Res wz:A(z)j v(w):dw=0, to compute vA(z) one only needs the Aj v OPE

A(z)j v(w) k1C k(w)1(zw) k.A(z)j_v(w)\sim\sum_{k\geq 1} C_k(w)\frac{1}{(z-w)^k}.

The algebra of currents

Assume two conserved currents j 1 and j 2 are given, and let Q 1,p,Q 2,p be the associated charges at p. Then the commutator [Q 1,p,Q 2,p] acts as

Res zpRes wpj 1(z)j 2(w)Res wpRes zpj 1(z)j 2(w)=Res wpRes zwj 1(z)j 2(w))=Res wp(Res zwj 1(z)j 2(w))).Res_{z\to p}Res_{w\to p}\langle j_1(z)j_2(w)\cdots\rangle-Res_{w\to p}Res_{z\to p}\langle j_1(z)j_2(w)\cdots\rangle= Res_{w\to p}Res_{z\to w}\langle j_1(z)j_2(w))\cdots\rangle =Res_{w\to p}\langle (Res_{z\to w} j_1(z)j_2(w)))\cdots\rangle.

In other words

[j 1,j 2](w)=Res zwj 1(z)j 2(w)[j_1,j_2](w)=Res_{z\to w} j_1(z)j_2(w)

and the Lie bracket is completely determined by the OPE of j 1(z)j 2(w).

Let’s play

Now we specialize the above general setup to conformal field theory on the complex plane. So our Σ will be the complex plane , the sheaf will be the sheaf of smooth fuctions on with values in D, and the action will be the Polyakov action for the standard Euclidean metric both on the source and on the target D, i.e.,

S[X]=12π ΣX μ¯X μS[X]=\frac{1}{2\pi}\int_\Sigma \partial X^\mu\overline{\partial}X_\mu

The tangent space of M=C (; D) at each point X is identified with the subspace C 0 (; D) of compactly supported functions. For any μ=1,,D, a linear map i μ:C 0 (,)H 0(M,TM) is given by i μ,f:X νX ν+δ μ νϵf. Postulating the volume form on M is such that the vector fields i μ,f are divergence-free, we have (dSi μ)=0 for any μ. One then computes (dSi μ)=¯X μ, hence

¯X μ(z)=0\langle \overline{\partial}\partial X^\mu(z)\cdots\rangle=0

by the general argument above. This in particular means that the distribution ¯ z zX μ(z)X ν(w) is supported at z=w, and indeed one computes ¯ z zX μ(z)X ν(w)=πδ μνδ(zw). Since δ(zw)=¯ z zlogzw 2, this is conveniently rewritten as

¯ z z(X μ(z)X μ(w)+12δ μνlogzw 2)=0\overline{\partial}_z\partial_z\langle (X^\mu(z) X_\mu(w)+\frac{1}{2}\delta^{\mu\nu}\log|z-w|^2)\cdots\rangle=0

In particular, X μ(z)X μ(w)+12δ μνlogzw 2 is an harmonic function and so we have the regularization

:X μ(z)X ν(w):=X μ(z)X ν(w)+12δ μνlogzw 2:X^\mu(z)X^\nu(w):=X^\mu(z) X^\nu(w)+\frac{1}{2}\delta^{\mu\nu}\log|z-w|^2

In other words,

φ X μX ν=12δ μνlogzw 2.\varphi_{X^\mu X^\nu}=-\frac{1}{2}\delta^{\mu\nu}\log|z-w|^2.

Similarly,

φ zX μ zX ν=12δ μν1(zw) 2.\varphi_{\partial_z X^\mu\partial_z X^\nu}=-\frac{1}{2}\delta^{\mu\nu}\frac{1}{(z-w)^2}.

The TT OPE

Set

T(z)=R zX μ zX μ(z)=lim zz: zX μ(z) zX μ(z)T(z)=R_{\partial_z X^\mu\partial_z X_\mu}(z)=\lim_{z'\to z}:\partial_z X^\mu(z)\partial_{z'}X_\mu(z')

Then

¯ zT(z)=(R ¯ z zX μ zX μ+R X μ¯ z zX μ)(z)=0,\overline{\partial}_zT(z)=(R_{\overline\partial_z \partial_z X^\mu\partial_z X_\mu}+R_{\partial X^\mu\overline{\partial}_z\partial_z X_\mu})(z)=0,

that is, T(z) is holomorphic! We have

T(z)T(w)=lim (z,w)(z,w): zX μ(z) zX μ(z):: wX ν(w) wX ν(w):=D/2(zw) 4+21(zw) 2: zX μ(z) wX μ(w):+T(z)T(w)=\lim_{(z',w')\to (z,w)}:\partial_zX^\mu(z)\partial_{z'}X_\mu(z'): :\partial_wX^\nu(w)\partial_{w'}X_\nu(w'): = \frac{D/2}{(z-w)^4}+ 2\frac{1}{(z-w)^2}:\partial_zX^\mu(z)\partial_w X_\mu(w):+\cdots
T(z)T(w)=D/2(zw) 4+2(zw) 2T(w)+1(zw) wT(w)+\phantom{T(z)T(w)} =\frac{D/2}{(z-w)^4}+\frac{2}{(z-w)^2}T(w)+\frac{1}{(z-w)}\partial_w T(w)+\cdots

Therefore we have found the TT OPE

T(z)T(w)D/2(zw) 4+2(zw)2T(w)+1(zw) wT(w)+T(z)T(w)\sim \frac{D/2}{(z-w)^4}+\frac{2}{(z-w)2}T(w)+\frac{1}{(z-w)}\partial_w T(w)\phantom{+\cdots}

The Virasoro algebra

Fix w=0. Holomorphic vector fields on 0 act as symmetries of the action. The charge associated with the vector field z n+1z is

j n(z)dz=z n+1T(z)dz.j_n(z)dz=z^{n+1}T(z)dz.

Set

L n=Res z0j n(z)dzL_n=Res_{z\to 0}\langle j_n(z)\cdots\rangle dz

Then

[L m,L n]=Res z0(Res wzj m(w)j n(z)dw)dz=Res z0(Res wzz n+1w m+1T(w)T(z)dw)dz[L_m,L_n]=Res_{z\to 0}\left(Res_{w\to z}\langle j_m(w)j_n(z)\cdots\rangle dw\right)dz=Res_{z\to 0}\left( Res_{w\to z} z^{n+1}w^{m+1}\langle T(w)T(z)\cdots \rangle dw\right)dz

Look at the expression Res wzz n+1w m+1T(w)T(z)dw=z n+1Res wz(z+(wz)) m+1T(w)T(z)dw and use the TT OPE to find

Res wz(z+(wz)) m+1T(w)T(z)dw=Res wz(z+(wz)) m+1(2(wz) 2T(z)+1(wz) zT(z)+D/2(wz) 4)Res_{w\to z}\bigl(z+(w-z)\bigr)^{m+1}\langle T(w)T(z)\cdots\rangle dw= Res_{w\to z}\bigl(z+(w-z)\bigr)^{m+1}( \frac{2}{(w-z)^2}\langle T(z)\cdots\rangle+ \frac{1}{(w-z)} \langle \partial_z T(z)\cdots\rangle+\frac{D/2}{(w-z)^4}\langle\cdots\rangle)
Res wz(z+(wz)) m+1T(w)T(z)dw=D2(m+13)z m2+2(m+11)z mT(z)+z m+1 zT(z)\phantom{Res_{w\to z}\bigl(z+(w-z)\bigr)^{m+1}\langle T(w)T(z)\cdots\rangle dw}= \frac{D}{2}\binom{m+1}{3}z^{m-2} \langle\cdots\rangle+2\binom{m+1}{1}z^m\langle T(z)\cdots\rangle + z^{m+1}\langle \partial_z T(z)\cdots\rangle

Therefore we find

[L m,L n]=Res z0(Dm 3m12z n+m1+2(m+1)z m+n+1T(z)+z n+m+2 zT(z))dz[L_m,L_n]=Res_{z\to 0} \biggl(D \frac{m^3-m}{12}z^{n+m-1}+2(m+1)z^{m+n+1}\langle T(z)\cdots\rangle+ z^{n+m+2}\partial_z \langle T(z)\cdots\rangle\biggr)dz
[L m,L n]=Dm 3m12δ m,n2(m+1)Res z0j n+m(z)dz+Res z0( zz n+m+2)T(z)dz\phantom{[L_m,L_n]}= D\frac{m^3-m}{12}\delta_{m,-n}-2(m+1)Res_{z\to 0}j_{n+m}(z)dz+Res_{z\to 0}(\partial_z z^{n+m+2})\langle{T}(z)\cdots\rangle dz
[L m,L n]=Dm 3m12δ m,n+(mn)Res z0j m+n(z)dz\phantom{[L_m,L_n]}= D\frac{m^3-m}{12}\delta_{m,-n}+(m-n)Res_{z\to 0}j_{m+n}(z)dz
[L m,L n]=(mn)L m+n+Dm 3m12δ m,n.\phantom{[L_m,L_n]}=(m-n)L_{m+n}+D\frac{m^3-m}{12}\delta_{m,-n}.