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Holomorphic Decoupling, Integrating In and Out, and Scale Matching

Holomorphic decoupling compares exact Wilsonian descriptions across a supersymmetric mass threshold. Matching the complex gauge coupling fixes the relation between holomorphic scales; solving the heavy field’s F-term then transports exact superpotentials and their coefficients. The procedure is branch-sensitive and scheme-sensitive, but within one declared convention it provides a stringent consistency test.

Required background. Holomorphic and canonical couplings fixes the gauge-coupling scheme. Nonperturbative superpotentials supplies the exact term to be matched.

Helpful background. Decoupling theorems and threshold corrections supplies the general EFT logic behind integrating out a massive field.

Let a high-energy theory have one-loop holomorphic coefficient bHb_H and scale

ΛHbH=μbHe2πiτH(μ).\Lambda_H^{b_H}=\mu^{b_H}e^{2\pi i\tau_H(\mu)}.

Suppose a massive chiral sector has a supersymmetric holomorphic mass source mm, and the low-energy theory has coefficient bL>bHb_L>b_H. Choose one finite holomorphic subtraction convention above and below the threshold, with unit finite matching constant. Comparing the analytic gauge-kinetic coefficients gives

ΛLbL=mbL−bHΛHbH.\Lambda_L^{b_L} =m^{b_L-b_H}\Lambda_H^{b_H}.

This equation includes phases: mm is complex, and an anomalous rotation of its phase is compensated by the theta angle. The physical threshold lies near a real scale set by ∣m∣|m| after canonical normalization, but writing “μ=m\mu=m” for complex mm would conflate that real matching scale with the holomorphic source. Taking absolute values in the holomorphic equation destroys its anomalous covariance.

The formula assumes that mm is large compared with the low-energy strong scale, that the threshold is supersymmetric, and that the same holomorphic normalization is used above and below. A finite redefinition of either coupling multiplies the right-hand side by a convention constant. Canonical pole masses also contain wavefunction factors and should not be inserted into a holomorphic matching equation without translating schemes.

Begin with SU(Nc)SU(N_c) SQCD and Nf<NcN_f<N_c flavors. Write

bf=3Nc−Nf,k=Nc−Nf,b_f=3N_c-N_f, \qquad k=N_c-N_f,

and give the last flavor a mass,

Wf=k(Λfbfdet⁡M)1/k+mX,X=MNfNf.W_f=k\left(\frac{\Lambda_f^{b_f}}{\det M}\right)^{1/k} +mX, \qquad X=M^{N_f}{}_{N_f}.

On the flavor-symmetric branch relevant to decoupling, the off-diagonal heavy–light mesons vanish and

det⁡M=Xdet⁡M^,\det M=X\det\widehat M,

where M^\widehat M is the (Nf−1)×(Nf−1)(N_f-1)\times(N_f-1) light meson matrix. Define

A=(ΛfbfXdet⁡M^)1/k.A=\left( \frac{\Lambda_f^{b_f}} {X\det\widehat M} \right)^{1/k}.

The heavy F-term equation is

0=∂Wf∂X=−AX+m,0=\frac{\partial W_f}{\partial X} =-\frac{A}{X}+m,

so X=A/mX=A/m. Substituting this into the definition of AA gives

Ak+1=mΛfbfdet⁡M^.A^{k+1} =\frac{m\Lambda_f^{b_f}}{\det\widehat M}.

The solutions are branch labelled,

Aℓ=(mΛfbfdet⁡M^)1/(k+1)e2πiℓ/(k+1),Xℓ=Aℓm,ℓ=0,…,k.A_\ell= \left( \frac{m\Lambda_f^{b_f}}{\det\widehat M} \right)^{1/(k+1)} e^{2\pi i\ell/(k+1)}, \qquad X_\ell=\frac{A_\ell}{m}, \qquad \ell=0,\ldots,k.

The on-shell superpotential is

Wf−1,ℓ=kAℓ+mXℓ=(k+1)Aℓ.W_{f-1,\ell}=kA_\ell+mX_\ell=(k+1)A_\ell.

The low-energy theory has

bf−1=bf+1,Nc−(Nf−1)=k+1.b_{f-1}=b_f+1, \qquad N_c-(N_f-1)=k+1.

Using the holomorphic scale match

Λf−13Nc−Nf+1=mΛf3Nc−Nf,\Lambda_{f-1}^{3N_c-N_f+1} =m\Lambda_f^{3N_c-N_f},

we obtain

Wf−1,ℓ=(Nc−Nf+1)(Λf−13Nc−Nf+1det⁡M^)1/(Nc−Nf+1)e2πiℓ/(Nc−Nf+1).W_{f-1,\ell} =(N_c-N_f+1) \left( \frac{\Lambda_{f-1}^{3N_c-N_f+1}} {\det\widehat M} \right)^{1/(N_c-N_f+1)} e^{2\pi i\ell/(N_c-N_f+1)}.

This is exactly the Affleck–Dine–Seiberg superpotential with one fewer flavor. Analytic continuation of the phase of mm permutes the k+1k+1 branches. The calculation checks the exponent, coefficient, mass phase, and branch recursion. Repeating it transports the controlled Nf=Nc−1N_f=N_c-1 instanton normalization to every Nf<NcN_f<N_c; the general exact-superpotential and SQCD treatments are Intriligator, Leigh, and Seiberg 1994, §§ 2–3.2, pp. 1094–1101 and Intriligator and Seiberg 1996, § 4.1, pp. 12–15.

The decoupling limit is not obtained by simply deleting a row and column of MM while holding Λf\Lambda_f fixed. The meaningful limit is

m→∞,Λf→0,mΛfbf=Λf−1bf+1fixed.m\to\infty, \qquad \Lambda_f\to0, \qquad m\Lambda_f^{b_f}=\Lambda_{f-1}^{b_f+1} \quad\text{fixed}.

Then the high-energy theory is weak near the threshold while the low-energy strong scale remains finite. The heavy field is eliminated by its holomorphic F-term on a chosen branch before the limit is interpreted.

Off-diagonal mesons also have F-term equations. Setting them to zero is consistent on the branch used above, but in a more general superpotential they can mix with light fields and must be solved rather than silently discarded.

If mm crosses zero, the effective field content changes and the decoupled description fails. Analytic continuation around m=0m=0 can permute fractional-power branches. Matching is holomorphic on the punctured mass plane, not a claim of regularity through the massless threshold.

Suppose a low-energy Wilsonian superpotential Wlow(m,ga)W_{\mathrm{low}}(m,g_a) is known as a holomorphic function of a source mm and other couplings gag_a. Express every low-energy scale in terms of the fixed high-energy holomorphic scale ΛH\Lambda_H, mm, and the remaining sources before differentiating. If mm couples linearly to a chiral operator XX in the higher-energy description, the integrating-in prescription uses

X=(∂Wlow∂m)ΛH,ga.X=\left( \frac{\partial W_{\mathrm{low}}}{\partial m} \right)_{\Lambda_H,g_a}.

When this relation can be inverted locally for m=m(X,ga)m=m(X,g_a), define the Legendre transform

Whigh(X,ga)=Wlow(m,ga)−mX.W_{\mathrm{high}}(X,g_a) =W_{\mathrm{low}}(m,g_a)-mX.

Adding mXmX back and extremizing with respect to XX returns WlowW_{\mathrm{low}}. This is “integrating in.” It can reconstruct highly nontrivial exact terms from a simpler theory Intriligator 1994, § 2, Eqs. (2.1)–(2.7), pp. 2–3.

The required linearity principle and simple-threshold principle are hypotheses to test in each model, not general theorems. Additional source-independent terms or non-simple thresholds can invalidate the reconstruction even when a formal Legendre transform exists.

The transform has hypotheses:

  • mm must genuinely be the chiral source for XX with the stated normalization;
  • the Wilsonian superpotential must be linear in that source before XX is eliminated;
  • the m↔Xm\leftrightarrow X relation must be locally invertible on the selected branch;
  • threshold scales and anomalous charges must match; and
  • no extra holomorphic term independent of mm may be dropped without separate evidence.

Failure of invertibility often signals a singular locus or additional light fields. Integrating in is then not a globally valid change of coordinates.

Give all NfN_f SQCD flavors a full-rank mass matrix mm. Repeated threshold matching yields

ΛSYM3Nc=ΛNf3Nc−Nfdet⁡m.\Lambda_{\mathrm{SYM}}^{3N_c} =\Lambda_{N_f}^{3N_c-N_f}\det m.

Solving the meson F-terms in the massive ADS superpotential gives

Wℓ=Nc(ΛNf3Nc−Nfdet⁡m)1/Nce2πiℓ/Nc,W_\ell=N_c \left(\Lambda_{N_f}^{3N_c-N_f}\det m\right)^{1/N_c} e^{2\pi i\ell/N_c},

with ℓ=0,…,Nc−1\ell=0,\ldots,N_c-1. This equals NcΛSYM,ℓ3N_c\Lambda_{\mathrm{SYM},\ell}^3. The determinant, rather than ∣det⁡m∣|\det m|, is forced by holomorphy and reproduces the anomalous phase dependence.

Matching at a canonical pole mass in a holomorphic formula. The canonical mass contains ZZ factors. Either use the chiral mass source throughout or translate every coupling and wavefunction consistently.

Holding both strong scales fixed as m→∞m\to\infty. They are related by the threshold equation. The controlled decoupling limit fixes the low-energy scale while the high-energy scale changes.

Treating a Legendre transform as global. Multiple solutions for m(X)m(X) are distinct branches, and the map can fail at discriminant loci.

Starting with SU(Nc)SU(N_c) SQCD with two massive flavors of diagonal masses m1,m2m_1,m_2, integrate them out sequentially and show that the final scale is independent of the order.

Solution

Each pair changes bb by one. In either order,

ΛNf−23Nc−Nf+2=m2ΛNf−13Nc−Nf+1=m2m1ΛNf3Nc−Nf.\Lambda_{N_f-2}^{3N_c-N_f+2} =m_2\Lambda_{N_f-1}^{3N_c-N_f+1} =m_2m_1\Lambda_{N_f}^{3N_c-N_f}.

Because the masses are holomorphic numbers, multiplication commutes. For a nondiagonal full-rank mass matrix, the invariant generalization is the determinant of the heavy mass block.

Check that the scale-matching equation has the same mass dimension and anomalous axial charge on both sides.

Solution

Both sides have dimension bf+1b_f+1. Under the axial symmetry of the high-energy theory, qA(m)=−2q_A(m)=-2 while qA(Λfbf)=2Nfq_A(\Lambda_f^{b_f})=2N_f, so the right side has charge 2(Nf−1)2(N_f-1), equal to the charge of Λf−1bf+1\Lambda_{f-1}^{b_f+1} in the low-energy theory.

  • Kenneth A. Intriligator, “Integrating In and Exact Superpotentials in Four Dimensions,” Physics Letters B 336 (1994), 409–414, arXiv, DOI.
  • Kenneth A. Intriligator, Robert G. Leigh, and Nathan Seiberg, “Exact Superpotentials in Four Dimensions,” Physical Review D 50 (1994), 1092–1104, arXiv, DOI.
  • Kenneth A. Intriligator and Nathan Seiberg, “Lectures on Supersymmetric Gauge Theories and Electric–Magnetic Duality,” Nuclear Physics B Proceedings Supplements 45BC (1996), 1–28, arXiv, DOI.

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