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Dynamical Supersymmetry Breaking and Calculability

Dynamical supersymmetry breaking (DSB) means that a theory with no explicit supersymmetry-breaking parameter generates a strictly positive vacuum energy through quantum gauge dynamics. The strongest demonstrations combine an exact holomorphic obstruction to solving all FF- and DD-term equations with a tunable limit in which the vacuum lies at weak coupling. The classic SU(3)×SU(2)SU(3)\times SU(2) “3–2 model” has both features.

Required background. Chiral-theory anomaly constraints supplies the microscopic consistency checks; Nelson–Seiberg-type criteria supplies the RR-symmetry hypotheses; and quantum chiral rings and Konishi anomalies explains exact operator relations. Helpful background. The Witten index and its failure modes explains why a vanishing or ill-defined index is not a proof of breaking.

What a convincing DSB argument must exclude

Section titled “What a convincing DSB argument must exclude”

A positive-energy stationary point is not enough. A stable DSB conclusion must address:

  • all gauge and global anomalies, including discrete or global gauge anomalies;
  • every invariant branch and every supersymmetric solution at finite field values;
  • runaways on which V0V\to0 only at infinite distance;
  • the Kähler metric in the region where the vacuum is claimed;
  • extra vacua that enter from infinity when a deformation is varied;
  • whether an RR symmetry is exact, accidental, explicitly broken, or spontaneously broken.

Holomorphy can establish an incompatible set of FF-term equations, but a vacuum energy depends on the nonholomorphic Kähler metric. “Calculable DSB” therefore requires the vacuum to sit where the gauge couplings and Kähler corrections are parametrically controlled.

Take the simply connected product gauge group

G=SU(3)×SU(2)G=SU(3)\times SU(2)

and chiral fields

Q:(3,2),U:(3,1),D:(3,1),L:(1,2),Q:({\bf3},{\bf2}),\quad \overline U:(\overline{\bf3},{\bf1}),\quad \overline D:(\overline{\bf3},{\bf1}),\quad L:({\bf1},{\bf2}),

with

Wtree=λϵαβQαaDaLβ.W_{\mathrm{tree}}=\lambda\,\epsilon^{\alpha\beta} Q^a_{\alpha}\overline D_aL_\beta.

No nontrivial subgroup of the Z3×Z2\mathbb Z_3\times\mathbb Z_2 gauge center acts trivially on all four fields, so there is no quotient ambiguity for this matter content and no surviving electric one-form symmetry.

The SU(3)3SU(3)^3 anomaly cancels because the two SU(2)SU(2) components of QQ give two fundamentals against the two antifundamentals. The SU(2)SU(2) factor has four left-handed doublets—three colors of QQ plus LL—so its mod-two global gauge anomaly also vanishes. The one-loop coefficients are

b3=3(3)[2(12)+12+12]=7,b2=3(2)[3(12)+12]=4.\begin{aligned} b_3&=3(3)-\left[2\left(\frac12\right) +\frac12+\frac12\right]=7,\\ b_2&=3(2)-\left[3\left(\frac12\right)+\frac12\right]=4. \end{aligned}

Thus the two holomorphic scales are Λ37\Lambda_3^7 and Λ24\Lambda_2^4.

One anomaly-free ordinary symmetry and one anomaly-free RR symmetry can be represented by the scalar charges

QUDLX1423R1003\begin{array}{c|rrrr} &Q&\overline U&\overline D&L\\ \hline X&1&-4&2&-3\\ R&-1&0&0&3 \end{array}

The tree term has (X,R)=(0,2)(X,R)=(0,2). Direct substitution gives zero for both SU(3)2XSU(3)^2X and SU(2)2XSU(2)^2X, and for each mixed gauge–RR anomaly after including the charge-one gaugino. These checks ensure that the nonperturbative term below has the right selection rules; they do not generate it by themselves.

Choose a hierarchy Λ3Λ2\Lambda_3\gg\Lambda_2 and eventually take λ1\lambda\ll1. Viewed as an SU(3)SU(3) theory, QQ provides two fundamentals and (U,D)(\overline U,\overline D) two antifundamentals, so Nf=2=Nc1N_f=2=N_c-1. The exact ADS term is

W3=Λ37det(QQ),Q=(U,D).W_3=\frac{\Lambda_3^7} {\det(Q\overline Q)}, \qquad \overline Q=(\overline U,\overline D).

The full superpotential in this regime is

Weff=λQDL+Λ37det(QQ).W_{\mathrm{eff}} =\lambda Q\overline D L +\frac{\Lambda_3^7}{\det(Q\overline Q)}.

If all FF terms vanished at a finite point, FL=0F_L=0 would require QD=0Q\overline D=0. That makes the second column of the 2×22\times2 meson matrix vanish, hence det(QQ)=0\det(Q\overline Q)=0, precisely where the ADS term is singular. The equations therefore have no simultaneous finite solution. This is an exact holomorphic incompatibility, first exploited in Affleck, Dine, and Seiberg 1984, pp. 1678–1680.

The argument would be incomplete if the fields could run to infinity with every auxiliary field tending to zero. In the 3–2 model, the tree interaction grows along the classical flat directions on which the ADS term decreases, while the ADS term diverges on the directions that try to set QD=0Q\overline D=0. The gauge DD terms remove the remaining relative orientations. Their competition stabilizes the runaway at finite field values.

Let vv denote the common magnitude of the Higgsing expectation values, suppressing order-one ratios fixed by minimizing the DD terms. Dimensional analysis along the relevant branch gives

Wtreeλv3,W3Λ37v4.W_{\mathrm{tree}}\sim\lambda v^3, \qquad W_3\sim\frac{\Lambda_3^7}{v^4}.

Balancing their FF terms,

λv2Λ37v5,\lambda v^2\sim\frac{\Lambda_3^7}{v^5},

yields

vΛ3λ1/7,FΛ32λ5/7,VminΛ34λ10/7.v\sim\Lambda_3\lambda^{-1/7}, \qquad F\sim\Lambda_3^2\lambda^{5/7}, \qquad V_{\min}\sim\Lambda_3^4\lambda^{10/7}.

For λ1\lambda\ll1, vΛ3Λ2v\gg\Lambda_3\gg\Lambda_2. Both gauge groups are Higgsed where their couplings are weak, and corrections to the approximately canonical Kähler potential are suppressed by powers of Λ3/vλ1/7\Lambda_3/v\sim\lambda^{1/7} and weak logarithms. The order-one coefficients and the exact location require minimizing the full weak-coupling FF- and DD-term potential, but the parametric scaling and positive energy are controlled. This distinction—exact nonexistence of a supersymmetric solution versus perturbatively calculable vacuum location—is essential.

The vacuum spontaneously breaks the continuous RR symmetry, so its phase contains an RR axion in the limit that the symmetry is exact. Gauging additional interactions or adding higher-dimension terms can explicitly reduce that symmetry and change the light spectrum; those are deformations, not properties of the minimal model.

A different route couples singlets to composites on a quantum-modified moduli space. If the quantum constraint forbids all composites from vanishing while singlet FF terms demand that they do, the equations have a rank-condition obstruction. The SU(2)SU(2) model with four doublets and singlets developed by Intriligator and Thomas 1996, §§ 2–3, pp. 126–132 is the canonical example. Such a proof still needs Kähler control to compute the vacuum quantitatively; symmetry can sometimes locate it near a point where qualitative breaking is robust.

Two popular shortcuts are unsafe:

  • A zero Witten index permits breaking but does not require it. Noncompact directions and vacua arriving from infinity can invalidate deformation arguments.
  • The Nelson–Seiberg criterion assumes a generic superpotential in a specified set of infrared fields. Strong dynamics may add fields, constraints, or accidental symmetries, so the theory card and exact chiral relations must come first; the theorem’s hypotheses and exceptions are stated in Nelson and Seiberg 1994, pp. 46–62.

The controlled statement takes 0<λ10<\lambda\ll1 at fixed nonzero Λ3\Lambda_3 with Λ2/Λ3\Lambda_2/\Lambda_3 sufficiently small. Setting λ=0\lambda=0 first restores flat directions and sends the stabilized point to v=v=\infty. Raising Λ2\Lambda_2 to compete with Λ3\Lambda_3 removes the sequential-node derivation, even though holomorphy may continue some protected information. Neither altered limit disproves the finite-small-λ\lambda result; it changes the available control.

Stopping after incompatible F terms. One must also exclude DD-flat runaways and show that the potential has a finite minimum. The 3–2 tree interaction and ADS singularity do this together.

Calling a strong-coupling estimate calculable. Calculability here comes from v/Λ3λ1/71v/\Lambda_3\sim\lambda^{-1/7}\gg1. Without a tunable hierarchy, exact holomorphy does not determine the Kähler metric or vacuum energy.

Taking a deformation to zero in the wrong order. At λ=0\lambda=0 the vacuum escapes to infinity. Continuity at a fixed compact field point is therefore not a valid argument across that limit.

Verify the perturbative SU(3)3SU(3)^3 anomaly, the SU(2)SU(2) mod-two anomaly, and the two one-loop coefficients.

Solution

For SU(3)3SU(3)^3, QQ is two fundamentals and U,D\overline U,\overline D are two antifundamentals, giving 211=02-1-1=0. The SU(2)SU(2) factor sees 3+1=43+1=4 doublets, an even number. The index sums are 22 for each gauge factor, so b3=92=7b_3=9-2=7 and b2=62=4b_2=6-2=4.

Starting only from Wtreeλv3W_{\mathrm{tree}}\sim\lambda v^3 and W3Λ37/v4W_3\sim\Lambda_3^7/v^4, recover the powers of λ\lambda in v,Fv,F, and VV.

Solution

vW\partial_vW balances as λv2Λ37/v5\lambda v^2\sim\Lambda_3^7/v^5, so v7Λ37/λv^7\sim\Lambda_3^7/\lambda and vΛ3λ1/7v\sim\Lambda_3\lambda^{-1/7}. Then Fλv2Λ32λ5/7F\sim\lambda v^2\sim\Lambda_3^2\lambda^{5/7} and VF2Λ34λ10/7V\sim\lvert F\rvert^2\sim\Lambda_3^4\lambda^{10/7}.

  • Affleck, Ian, Michael Dine, and Nathan Seiberg. “Calculable Nonperturbative Supersymmetry Breaking.” Physical Review Letters 52 (1984): 1677–1680. DOI.
  • Intriligator, Kenneth, and Scott Thomas. “Dynamical Supersymmetry Breaking on Quantum Moduli Spaces.” Nuclear Physics B 473 (1996): 121–142. DOI; arXiv.
  • Nelson, Ann E., and Nathan Seiberg. “R Symmetry Breaking versus Supersymmetry Breaking.” Nuclear Physics B 416 (1994): 46–62. DOI; arXiv.
  • Skiba, Witold. “Dynamical Supersymmetry Breaking.” Modern Physics Letters A 12 (1997): 737–750. DOI; arXiv.