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Chiral operators, Ward identities, and vacuum relations

For one chiral field with superpotential W=gX3/3W=gX^3/3, the classical supersymmetric vacuum equation is x2=0x^2=0. As an equation for a complex number, this means x=0x=0. As a relation among operators, it need not mean that the class of XX vanishes. Understanding that difference is our first task.

The preparation is Holomorphy and the quantum effective action. We use flat four-dimensional Lorentzian N=1\mathcal N=1 supersymmetry, with four real supercharges and no gravitational background. The worked theories have gauge-neutral chiral multiplets, canonical positive Kähler metrics, and the component convention LW=WiFi−Wijψiψj/2+h.c.\mathcal L_W=W_iF_i-W_{ij}\psi_i\psi_j/2+\text{h.c.} All explicit polynomial quotients and vacuum potentials below are classical. The operator argument explains what their quantum counterparts must respect; it does not assert that classical relations always survive quantization.

For operators of definite fermion parity, define the graded bracket

[A,B}=AB−(−1)∣A∣∣B∣BA.[A,B\}=AB-(-1)^{|A||B|}BA.

It is a commutator unless both entries are odd, in which case it is an anticommutator. The supercharges are odd. A local operator O\mathcal O is chiral when

[Qˉα˙,O}=0,α˙=1˙,2˙.[\bar Q_{\dot\alpha},\mathcal O\}=0,\qquad \dot\alpha=\dot1,\dot2.

The lowest component of a chiral superfield has this property. We will concentrate on bosonic Lorentz-scalar operators; in a gauge theory they must also be gauge invariant.

An exact change is a sum of barred-supercharge variations,

O ∼ O+∑α˙[Qˉα˙,Yα˙},\mathcal O\ \sim\ \mathcal O+ \sum_{\dot\alpha}[\bar Q_{\dot\alpha},Y^{\dot\alpha}\},

where both representatives are chiral. For bosonic O\mathcal O, the ancestors Yα˙Y^{\dot\alpha} are odd. The equivalence classes form the chiral ring. “Ring” means that we can add classes and multiply them, with an identity class [1][1]; it does not refer to a geometric circle.

Why does multiplication respect the equivalence? Write δˉA=[Qˉ,A}\bar\delta A=[\bar Q,A\} for either barred charge. Its graded product rule is

δˉ(AB)=(δˉA)B+(−1)∣A∣A(δˉB).\bar\delta(AB)=(\bar\delta A)B+(-1)^{|A|}A(\bar\delta B).

If BB is closed and A=YA=Y is odd, then (δˉY)B=δˉ(YB)(\bar\delta Y)B=\bar\delta(YB). Thus multiplying an exact change by a closed operator gives another exact change. The scalar examples below have a commutative ring. Their products are understood as appropriately defined local chiral composites, not as an instruction to multiply arbitrary singular distributions at the same point. Cachazo–Douglas–Seiberg–Witten, §2.1

Recall the site’s normalization,

{Qα,Qˉβ˙}=2σαβ˙μPμ,[Pμ,O]=−i∂μO.\{Q_\alpha,\bar Q_{\dot\beta}\} =2\sigma^\mu_{\alpha\dot\beta}P_\mu,\qquad [P_\mu,\mathcal O]=-i\partial_\mu\mathcal O.

Here σμ=(I,−τi)\sigma^\mu=(I,-\tau_i), σˉμ=(I,+τi)\bar\sigma^\mu=(I,+\tau_i) and η=diag⁡(1,−1,−1,−1)\eta=\operatorname{diag}(1,-1,-1,-1). The τi\tau_i are Pauli matrices. For a bosonic chiral O\mathcal O, the graded Jacobi identity gives

2σαβ˙μ[Pμ,O]={Qα,[Qˉβ˙,O]}+{Qˉβ˙,[Qα,O]}={Qˉβ˙,[Qα,O]}.\begin{aligned} 2\sigma^\mu_{\alpha\dot\beta}[P_\mu,\mathcal O] &=\{Q_\alpha,[\bar Q_{\dot\beta},\mathcal O]\} +\{\bar Q_{\dot\beta},[Q_\alpha,\mathcal O]\}\\ &=\{\bar Q_{\dot\beta},[Q_\alpha,\mathcal O]\}. \end{aligned}

Contract with σˉνβ˙α\bar\sigma^{\nu\dot\beta\alpha}. Since σˉνβ˙ασαβ˙μ=2ηνμ\bar\sigma^{\nu\dot\beta\alpha}\sigma^\mu_{\alpha\dot\beta}=2\eta^{\nu\mu}, we obtain

∂νO=i4σˉνβ˙α{Qˉβ˙,[Qα,O]}.\boxed{\displaystyle \partial^\nu\mathcal O =\frac{i}{4}\bar\sigma^{\nu\dot\beta\alpha} \{\bar Q_{\dot\beta},[Q_\alpha,\mathcal O]\}.}

The ancestor [Qα,O][Q_\alpha,\mathcal O] is odd, which explains the outer anticommutator. The factor i/4i/4 follows from our translation and charge normalization; it must not be copied from a source that suppresses those factors.

Now choose a supersymmetric vacuum ∣Ω⟩|\Omega\rangle, annihilated by QαQ_\alpha and Qˉα˙\bar Q_{\dot\alpha}. Their adjoint relation gives the corresponding annihilation of the bra. Assume the conserved supersymmetry charges and operator products are well defined, with no boundary contribution spoiling the Ward identity.

Let BB be a product of bosonic chiral operators at distinct points. For any odd YY inserted separately,

0=⟨δˉ(YB)⟩Ω=⟨(δˉY)B⟩Ω−⟨Y δˉB⟩Ω=⟨(δˉY)B⟩Ω.0=\langle\bar\delta(YB)\rangle_\Omega =\langle(\bar\delta Y)B\rangle_\Omega -\langle Y\,\bar\delta B\rangle_\Omega =\langle(\bar\delta Y)B\rangle_\Omega.

The first equality follows by moving the charge to the bra or ket. The last uses chirality of every factor in BB. Applying this identity to the boxed ancestor proves

∂x1μ⟨O1(x1)⋯On(xn)⟩Ω=0\partial_{x_1^\mu} \langle\mathcal O_1(x_1)\cdots\mathcal O_n(x_n)\rangle_\Omega=0

away from coincident insertions. This is a Ward identity: a relation between correlation functions implied by a symmetry. It does not say that ∂μO\partial_\mu\mathcal O vanishes as an ordinary local operator in every correlation function. CDSW, (2.1)–(2.2)

If this chosen infinite-volume vacuum also satisfies cluster decomposition, correlations of widely separated groups approach the product of their expectation values. Move the separated chiral insertions arbitrarily far apart. Their correlator is unchanged, so

⟨O1⋯On⟩Ω=∏k=1n⟨Ok⟩Ω.\langle\mathcal O_1\cdots\mathcal O_n\rangle_\Omega =\prod_{k=1}^n\langle\mathcal O_k\rangle_\Omega.

Thus the expectation-value map χΩ([O])=⟨O⟩Ω\chi_\Omega([\mathcal O])=\langle\mathcal O\rangle_\Omega preserves multiplication and sends [1][1] to 11. Such a map to C\mathbb C is called a character of the ring. Factorization uses both the Ward identity and clustering; averaging different vacua can destroy the latter. Nor does this argument establish a normalizable vacuum when none exists. CDSW, (2.3)

From an auxiliary equation to a polynomial quotient

Section titled “From an auxiliary equation to a polynomial quotient”

For neutral chirals with canonical Kähler potential, the classical superfield equation is

−14Dˉ 2Φˉi+Wi(Φ)=0,Dˉ 2=Dˉα˙Dˉα˙.-\frac14\bar{\mathbb D}^{\,2}\bar\Phi_i+W_i(\Phi)=0, \qquad \bar{\mathbb D}^{\,2} =\bar{\mathbb D}_{\dot\alpha}\bar{\mathbb D}^{\dot\alpha}.

The derivatives are those defined in the action lesson. At θ=θˉ=0\theta=\bar\theta=0, Dˉ 2Φˉi=−4Fˉi\bar{\mathbb D}^{\,2}\bar\Phi_i=-4\bar F_i, so the equation gives Fˉi=−Wi\bar F_i=-W_i, checking its sign against the component action.

The barred superspace derivative on this lowest component is a barred supersymmetry variation, up to its fixed normalization. The twice-differentiated expression is therefore exact. Equivalently, the anti-fermion’s barred variation contains Fˉi\bar F_i, and its auxiliary equation identifies that exact component with −Wi-W_i. Consequently,

[Wi]=0[W_i]=0

in the classical chiral ring. This is the content of the F-term relation, not a claim that the polynomial WiW_i is identically zero before passing to equivalence classes. CDSW, §2.2, (2.7)

Restricting to scalar polynomials in these neutral fields gives

Rcl=C[x1,…,xn](W1,…,Wn).\mathcal R_{\rm cl} =\frac{\mathbb C[x_1,\ldots,x_n]}{(W_1,\ldots,W_n)}.

The denominator is an ideal: all sums ∑ifi(x)Wi(x)\sum_i f_i(x)W_i(x) with polynomial coefficients. Two polynomials represent the same class if their difference belongs to this ideal. Writing xix_i for a ring generator is convenient, but it does not yet assign that operator a numerical expectation value.

For our first model,

K=XˉX,W=g3X3,g≠0,K=\bar X X,\qquad W=\frac g3X^3,\qquad g\ne0,

[X]=1[X]=1 and [g]=0[g]=0 in engineering mass dimension. The relation is gx2=0g x^2=0, so

Rcl=C[x]/(x2).\mathcal R_{\rm cl}=\mathbb C[x]/(x^2).

Every polynomial reduces uniquely to a+bxa+bx. Multiplication is

(a+bx)(c+dx)=ac+(ad+bc)xin Rcl.(a+bx)(c+dx)=ac+(ad+bc)x \quad\text{in }\mathcal R_{\rm cl}.

The class [x][x] is nonzero: a degree-one polynomial cannot be a polynomial multiple of x2x^2. Nevertheless [x]2=0[x]^2=0. A nonzero element whose power vanishes is nilpotent.

Compare this with the scalar potential,

V=∣g∣2∣x∣4.V=|g|^2|x|^4.

Its only zero is the point x=0x=0. Every character likewise obeys χ([x])2=0\chi([x])^2=0 in C\mathbb C, hence χ([x])=0\chi([x])=0. Numerical evaluation loses the nonzero nilpotent class. Removing all nilpotents gives the reduced ring, here just C\mathbb C, which is sufficient to describe this point set but contains less information.

An elementary matrix check makes the distinction visible. On the ring’s vector-space basis (1,x)(1,x), multiplication by xx is

Mx=(0010),Mx≠0,Mx2=0.M_x=\begin{pmatrix}0&0\\1&0\end{pmatrix}, \qquad M_x\ne0,\qquad M_x^2=0.

These matrices represent polynomial multiplication; they are not observables on a positive-norm particle Hilbert space. The chiral ring does not include Hermitian conjugation as an internal operation. There is no contradiction with unitarity, and two basis elements do not mean two vacuum points.

Deform the same model by a parameter vv of mass dimension one:

W=g(X33−v2X),v≠0.W=g\left(\frac{X^3}{3}-v^2X\right),\qquad v\ne0.

Now

Rv=C[x]/(x2−v2),V=∣g∣2∣x2−v2∣2.\mathcal R_v=\mathbb C[x]/(x^2-v^2),\qquad V=|g|^2|x^2-v^2|^2.

There are two classical supersymmetric vacua, x=vx=v and x=−vx=-v. Their fluctuation masses are both ∣W′′(±v)∣=2∣gv∣|W''(\pm v)|=2|gv|, for the complex scalar and Weyl fermion.

A class a+bxa+bx is determined by its two values a+bva+bv and a−bva-bv. Conversely,

a=f(v)+f(−v)2,b=f(v)−f(−v)2v.a=\frac{f(v)+f(-v)}2,\qquad b=\frac{f(v)-f(-v)}{2v}.

Thus Rv\mathcal R_v is the ring C⊕C\mathbb C\oplus\mathbb C with componentwise multiplication. The elements

e±=12(1±xv)e_\pm=\frac12\left(1\pm\frac{x}{v}\right)

obey e±2=e±e_\pm^2=e_\pm, e+e−=0e_+e_-=0 and e++e−=1e_++e_-=1. Evaluation in the two vacua sends them to (1,0)(1,0) and (0,1)(0,1).

The multiplication matrix is now

Mx(v)=(0v210).M_x(v)=\begin{pmatrix}0&v^2\\1&0\end{pmatrix}.

For v≠0v\ne0 it has distinct eigenvalues ±v\pm v. At v=0v=0 it becomes the nonzero nilpotent matrix above. The vector-space dimension stays two, but the distinct vacuum points merge. The ring keeps the repeated-root information that the point set discards. This is a classical deformation, not an instanton correction or a new interacting four-dimensional conformal fixed point.

The Ward argument continues to constrain a quantum theory when supersymmetry, its vacuum and the needed operator definitions satisfy the stated assumptions. Determining the actual quantum ring is a further dynamical task.

In particular, a renormalized composite at coincident points is more than a formal product of bare fields. The separated-insertion derivation does not justify ignoring contact terms in every equation containing composite ancestors or integrated action insertions. In a gauge theory, the Konishi anomaly is a concrete warning: a barred-superderivative relation for a matter bilinear acquires a chiral gauge-field-strength operator. Naively multiplying an elementary equation of motion and declaring every resulting classical relation exact can miss that contribution. This is an anomaly of a matter rotation, not permission for an inconsistent gauge anomaly or a statement that supersymmetry itself has failed. Tong, §7.2.3

Quantum dynamics can also deform classical vacuum constraints. Intriligator–Seiberg, §4.2, (4.14)–(4.15) gives a gauge-theory example. Establishing such a deformation requires information beyond the elementary quotient calculated here.

Even classically, gauge theories require gauge-invariant operators and the appropriate D-flatness and gauge-equivalence analysis. A list of polynomial F equations alone is not a universal recipe for counting physical vacua. Likewise, setting g=0g=0 in our neutral model changes the ideal to zero and gives C[x]\mathbb C[x]; one cannot divide by gg, then carry the relation x2=0x^2=0 through that singular change of theory. No superconformal dimension formula is needed for any of these arguments.

Take two neutral canonical chirals with W=λX2YW=\lambda X^2Y, λ≠0\lambda\ne0. Calculate the classical polynomial ring and the vacuum point set. Find a normal form for its elements. Does the class of xx vanish? Check the small-fluctuation masses at a point (x,y)=(0,y0)(x,y)=(0,y_0).

Hint 1

Use both derivatives of WW. Reduce separately monomials containing two factors of xx and those containing both xx and yy.

Hint 2

To show that xx survives, set y=0y=0 in any proposed expression x=Ax2+Bxyx=A x^2+Bxy. For the masses, evaluate the two-by-two matrix WijW_{ij} at the vacuum.

Solution

The equations are WX=2λxyW_X=2\lambda xy and WY=λx2W_Y=\lambda x^2. Therefore

Rcl=C[x,y]/(x2,xy).\mathcal R_{\rm cl}=\mathbb C[x,y]/(x^2,xy).

Every class has the form f(y)+axf(y)+a x, with polynomial ff and constant aa. Its product with g(y)+bxg(y)+b x is

f(y)g(y)+[a g(0)+b f(0)]x.f(y)g(y)+\bigl[a\,g(0)+b\,f(0)\bigr]x.

The class xx is nonzero, because setting y=0y=0 in an ideal-membership equation would make a degree-one polynomial divisible by x2x^2. It squares to zero and is also annihilated by yy.

For numerical vacuum values, x2=0x^2=0 forces x=0x=0, while yy is arbitrary. The reduced ring is C[y]\mathbb C[y]. The full ring contains nilpotent information invisible on that whole vacuum line.

At (0,y0)(0,y_0),

(Wij)=(2λy0000).(W_{ij})=\begin{pmatrix}2\lambda y_0&0\\0&0\end{pmatrix}.

The XX multiplet has mass 2∣λy0∣2|\lambda y_0| and YY is massless. At y0=0y_0=0 both quadratic masses vanish. On a patch where yy is invertible, xy=0xy=0 implies x=0x=0 even as a ring class. The surviving nilpotent is therefore tied to the special point where this extra mass vanishes; it is not an extra numerical vacuum at every point on the line.

2. A supersymmetric mixture that does not cluster

Section titled “2. A supersymmetric mixture that does not cluster”

Assume two supersymmetric clustering vacuum sectors with chiral expectation values vv and −v-v, as in the semiclassical split-root model. Consider their equal statistical mixture. Calculate ⟨x⟩\langle x\rangle, ⟨x2⟩\langle x^2\rangle and the widely separated chiral connected correlator. Does the Ward identity fail? Is this expectation map a character?

Hint 1

In each pure sector separately, the two-point function factorizes to v2v^2, including the sector with expectation value −v-v.

Hint 2

Average correlation functions after evaluating them in each sector. Averaging a product is not generally the same as multiplying averages.

Solution

Linearity of the mixture gives

⟨x⟩mix=0,⟨x2⟩mix=v2,⟨x(z1)x(z2)⟩mix,c=v2\langle x\rangle_{\rm mix}=0,\qquad \langle x^2\rangle_{\rm mix}=v^2,\qquad \langle x(z_1)x(z_2)\rangle_{{\rm mix},c}=v^2

for distinct points, even when their separation becomes arbitrarily large. The connected term subtracts ⟨x⟩mix2=0\langle x\rangle_{\rm mix}^2=0.

Each sector obeys the supersymmetry Ward identity, so their mixture does too. What fails is cluster decomposition. The expectation map is linear and respects the relation x2=v2x^2=v^2, but is not multiplicative: χmix(x2)≠χmix(x)2\chi_{\rm mix}(x^2)\ne\chi_{\rm mix}(x)^2. This example shows exactly which additional assumption turns position independence into a character. A vacuum count should not treat this statistical mixture as a third pure vacuum.

3. Does heavy-field elimination preserve the relations?

Section titled “3. Does heavy-field elimination preserve the relations?”

Return to the neutral model

W=M2H2+y2HX2,M≠0,y≠0.W=\frac M2H^2+\frac y2HX^2,\qquad M\ne0,\quad y\ne0.

Calculate its classical polynomial ring by eliminating hh algebraically. Compare it with the ring from Weff=−y2X4/(8M)W_{\rm eff}=-y^2X^4/(8M). Then set M=0M=0 in the original model and explain why the previous elimination cannot describe the result.

Hint 1

The ideal has two generators, Mh+yx2/2Mh+yx^2/2 and yhxyhx. Substitute the first relation into the second.

Hint 2

Distinguish an exact isomorphism of classical polynomial quotients at nonzero MM from a claim about kinetic terms. At M=0M=0, do not use a formula containing 1/M1/M.

Solution

At nonzero MM, the first relation gives h=−yx2/(2M)h=-yx^2/(2M). The second becomes −y2x3/(2M)=0-y^2x^3/(2M)=0. Hence

C[h,x](Mh+yx2/2,  yhx)≃C[x]/(x3).\frac{\mathbb C[h,x]}{(Mh+yx^2/2,\;yhx)} \simeq\mathbb C[x]/(x^3).

The map sends xx to xx and hh to −yx2/(2M)-yx^2/(2M). Conversely, these substitutions satisfy both original relations, so they define the inverse identification. The quotient has basis 1,x,x21,x,x^2 and one numerical vacuum point.

The effective superpotential gives Weff′=−y2x3/(2M)W_{\rm eff}'=-y^2x^3/(2M) and the same ring. This exact algebraic agreement concerns classical chiral relations. It does not improve the momentum or auxiliary approximation of a truncated effective action.

At M=0M=0, the original ideal is (x2,hx)(x^2,hx), with ring

C[h,x]/(x2,hx).\mathbb C[h,x]/(x^2,hx).

Its point set is the entire line x=0x=0, hh arbitrary. Its elements have normal form f(h)+axf(h)+a x, so it retains a nilpotent at the special point h=0h=0, just as in exercise 1. The field HH must return to the low-energy description. The polynomial ring, the vacuum set and the kinetic effective theory are related pieces of information, but they are not interchangeable.

You can now derive a separated-insertion Ward identity, calculate an F-term quotient, and test whether numerical vacuum values lose information. Classical SQCD applies these questions to a gauge theory: identify its gauge-invariant generators, distinguish classical from quantum relations, and check what makes their expectation values describe actual vacua. Its other preparation is the anomaly lesson.