Operator dimensions from moduli

We consider the operator spectrum of a three-dimensional N=2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{N}=2 $$\end{document} superconformal field theory with a moduli space of one complex dimension, such as the fixed point theory with three chiral superfields X, Y, Z and a superpotential W = XYZ. By using the existence of an effective theory on each branch of moduli space, we calculate the anomalous dimensions of certain low-lying operators carrying large R-charge J. While the lowest primary operator is a BPS scalar primary, the second-lowest scalar primary is in a semi-short representation, with dimension exactly J + 1, a fact that cannot be seen directly from the XYZ Lagrangian. The third-lowest scalar primary lies in along multiplet with dimension J + 2−c−3J−3 + O(J−4), where c−3 is an unknown positive coefficient. The coefficient c−3 is proportional to the leading superconformal interaction term in the effective theory on moduli space. The positivity of c−3 does not follow from supersymmetry, but rather from unitarity of moduli scattering and the absence of superluminal signal propagation in the effective dynamics of the complex modulus. We also prove a general lemma, that scalar semi-short representations form a module over the chiral ring in a natural way, by ordinary multiplication of local operators. Combined with the existence of scalar semi-short states at large J, this proves the existence of scalar semi-short states at all values of J. Thus the combination of N=2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{N}=2 $$\end{document} superconformal symmetry with the large-J expansion is more powerful than the sum of its parts.


Introduction
Generic CFT need not be weakly coupled, in the sense of lying in families -discrete or continuous -with limits that can be reduced to weakly interacting free fields or solved exactly in some more general way. However even individual theories that are strongly JHEP10(2017)089 coupled, may have families of observables with limits that are weakly coupled in this sense. The simplest such limit to study is that of large global charge.
In [1] and related work [2][3][4][5] it was noted that three dimensional CFT with global symmetries simplify in this sense in some familiar examples, when one considers the dimensions of low-lying operators of large global charge J. The theories considered in [1] are the critical O(2) model and the infrared fixed point of the N = 2 supersymmetric theory with a single chiral superfield Φ and superpotential W = Φ 3 . In each case, the operator dimension of the lowest operator with charge J is a scalar operator with dimension ∆ J = c 3 where the unknown coefficients c 3 2 , c 1 2 may differ between theories and the J-independent term is universal. 1 The common form of the large-J expansions for ∆ J follows from the fact that the two theories are both described by an effective theory in the same universality class. The effective theory describes a single compact scalar χ ≃ χ + 2π transforming as χ → χ + (const.) under the global symmetry. This effective theory can be used to calculate dimensions of operators using radial quantization on the sphere of radius r, taking the Wilsonian cutoff Λ to satisfy r −1 < < Λ < < √ J r . Then both quantum effects and higher-derivative terms are suppressed by powers of J, and the renormalization group equation at the conformal fixed point forces all Λ dependence cancel in observables, order by order in J. Crucially, conformal invariance is a symmetry of the effective theory at the quantum level, which constrains the Λ-independent terms to be classically scale invariant (indeed, Weyl invariant) and further determines the Λ-dependent terms uniquely in terms of the Λ-independent terms.
The J + 3 2 scaling in the O(2) and W = Φ 3 models is a consequence of the fact that neither theory has a continuous family of Lorentz-invariant vacua on flat spatial slices. As a result, the curvature of the space is irrelevant for high-energy states on the sphere, and so the relationship between the energy density H ≡ T 00 and the charge density ρ ≡ J 0 in the large-J ground state can only be H ∼ |ρ| + 3 2 . In the case of the N = 2 superconformal W = Φ 3 theory, the J + 3 2 scaling encodes the fact that SUSY is strongly spontaneously broken at large R-charge. That SUSY must be broken follows from the fact that the chiral ring truncates; the only BPS scalar primaries are 1 and φ itself. However the fact that the breaking is parametrically large at high J, cannot be understood in terms of the structure of the chiral ring, and only the use of the effective theory can uncover it.
The case of an infinite chiral ring is different. For N = 2 SCFT with infinite (finitely generated) chiral ring, there is a moduli space of Lorentz-invariant vacua on R 3 , whose holomorphic coordinate ring is the "radical" of the chiral ring -the chiral ring modulo its nilpotent elements [7]. Conversely, if there is a k-complex-dimensional moduli space, then it is described by a nilpotent-free chiral ring with k algebraically independent generators, or k + ℓ generators with ℓ relations.
The moduli space of vacua implies a degenerate spectrum when the curvature vanishes, and consequently the curvature is always relevant in the relationship between H and ρ on the sphere. For a theory with a moduli space of vacua, low-lying states of large R-charge JHEP10(2017)089 satisfy a relationship of the form H ∼ Ric 2 + 1 2 |ρ|, where Ric is the Ricci scalar curvature of the spatial slice. In radial quantization, this translates into a relationship ∆ J ∼ +1·|J| 1 , a relationship that is exact for the lowest operator with charge J, which is always BPS if a moduli space exists and J satisfies an appropriate quantization condition.
Possibly the simplest interacting theory with a moduli space is the XY Z model, the N = 2 superconformal infrared fixed point of three free chiral superfields X, Y, Z perturbed by a superpotential W = g XY Z where g is a coupling constant with dimension [g] = [mass] + 1 2 . At scales E < < g 2 this theory flows to a superconformal theory that is strongly coupled: the anomalous dimensions and OPE coefficients of the fields 2 X, Y, Z are all of O (1). The theory has exactly one marginal operator that breaks the U(1) 3 symmetry and lowers the dimension of the moduli space (as shown by a Leigh-Strassler type argument [8]), but no marginal operators neutral under the full global symmetry. The chiral ring of this theory is one-dimensional, corresponding to the case where k = 1 and ℓ = 2. The three generators X, Y, Z obey the relation XY = XZ = Y Z = 0, so that the moduli space consists of three branches, freely generated by X, Y , and Z respectively.
That is, the chiral ring consists of linear combinations of the elements, {X p , Y p , Z p , ∀p ≥ 0}. This theory has three independent U(1) global symmetries U(1) X,Y,Z under which X, Y, and Z carry charge +1, respectively, and the R-charge J R is a linear combination of the three, Scalar superconformal primary operators are in the chiral ring if they satisfy the BPS bound ∆ = J R . If an operator is not in the chiral ring, but satisfies (∆ − J R )/J R < < 1, we ought to be able to think of them as "near-BPS", and their anomalous dimensions should be computable in large-J perturbation theory.
The first examples of such a perturbation theory known to the authors are [9,10]. In those papers the authors used the additional simplifications of N = 4 SUSY in four dimensions, as well as the planar approximation at large N . In this paper we will show that near-BPS operator dimensions can be calculated straightforwardly in a large-J expansion in the XY Z model, which lacks these additional simplifications.
In particular, we will extend the approach of [1] to study the anomalous dimensions of near-BPS scalar operators with large R-charge on the "X branch", that is, operators with J R , J X > > 1, and J X − 3 2 J R and ∆ − J R of order 1. We will quantize the theory on S 2 spatial slices and use the effective field theory of the X branch of moduli space, to compute the operator dimension realized as the energy of the state on the sphere, via the state-operator correspondence. At large J, the moduli space effective theory becomes a controlled tool: both higher-derivative operators and Feynman diagrams with loops have their effects suppressed by powers of J.
We find some interesting results: • After the lowest operator, which is BPS, the next-lowest operator with the same charge is also a scalar and lies in a "semi-short" multiplet -itsQ 2 descendant is absent and its dimension is precisely J + 1.

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• The third-lowest operator with the same charges lies in a long multiplet and receives corrections to its dimension of order J −3 .
• The J −3 correction comes from a single insertion of the lowest-derivative super-Weylinvariant interaction term in the effective theory on moduli space.
• The coefficient of this effective term is not perturbatively calculable, but its sign is positive definite by virtue of the causality constraint discussed in [11]. As a result, the J −3 correction to the energy of the third-lowest scalar primary operator is negative definite.
2 Effective theory of the X branch As in the case of the O(2) model in [1], we begin by observing that the Wilsonian action at large values of the fields X, Y, Z has an expansion in powers of the cutoff over the UV scale defined by the scalar vevs themselves. In this regime the loop contributions to the RG equation, both the finite and Λ-dependent parts, are parametrically smaller than the action of a classical scale transformation, and the RG fixed point equation becomes the condition for classical scale invariance, with calculable corrections that simply determine the Λdependent terms from the Λ-independent terms. For the particular directions where one of the three fields is nonzero and the other two vanish, the other two fields are massive, with masses above the cutoff, and one can obtain an effective action for one of these fields alone.
Structure of the effective action. The effective theory of the X modulus has a relatively simple structure. In flat space, terms can be understood as full-superspace integrals, where I is an operator with J X = J R = 0. Terms in the effective Lagrangian can be classified into two types: classical and quantum terms. Classical terms are independent of the cutoff Λ and invariant under the Weyl transformation X → exp 2σ 3 X, with the superpartner of X transforming as ψ X → exp 7σ 6 ψ X . The scaling dimension of I classical must be exactly 1. Quantum terms are entirely dependent on the form of the regulator and scale as positive powers of the cutoff scale Λ. They are not Weyl-invariant or even scale invariant as terms in the action; scale invariance is explicitly broken by the Λ-dependence. These terms are of the form where I 1−q is an operator of dimension 1 − q and q > 0. It is important to note that the condition q > 0 satisfied by the quantum terms is not a universal rule in effective field theories: when we integrate out a shell of modes, between Λ and Λ − δΛ, the propagators are 1 Λ 2 and naively it would seem that Λ can appear to negative powers in the Wilsonian action. Rather, the q > 0 rule follows from the fact that the effective theory on moduli space is infrared-free. The 1PI effective action for X, JHEP10(2017)089 expanded around a nonzero vev, is therefore convergent, since X is an observable in the infrared theory. But the 1PI effective action is nothing more than the Λ → 0 limit of the Wilsonian effective action. So the Wilsonian action must be finite in the Λ → 0 limit.
There is less to the quantum terms than meets the eye. We are treating our theory as a Wilsonian theory in a perturbatively controlled regime by taking E IR < < Λ < < E UV , with E UV = |X| + 3 2 . The condition of conformal invariance dictates that the effect of integrating out a shell of modes and lowering the cutoff from Λ to Λ − δΛ must be exactly cancelled by rescaling the momenta by a factor of (1 − δΛ Λ ) −1 , with a redefinition of the fields to restore the normalization of the kinetic term. This allows us to write a renormalization group equation which can be solved to derive the coefficients of the Λ-dependent quantum terms from the Λ-independent classical action, order by order in Λ . The quantum terms, then, comprise a sort of epiphenomenon: once the regulator has been fixed and the conformal invariance of the underlying theory is taken as an input, the cutoff-dependent terms contain no independent information. Concretely, the RG evolution of the classical action is of the form 3 where O i is an operator of dimension ∆ i ≡ 3 − q i . Then the fixed point equation for RG evolution allows us to solve for L (a+1) in terms of L (a) by is the set of terms in the Lagrangian with canonical scaling dimension ∆ c . We do not need to know the concrete form of the quantum terms at all for most practical purposes. In correlation functions, their only role is to cancel the Λ-dependence from quantum amplitudes order by order in E IR /|X| 3 2 . In practice, we can simply quantize the classical action with a (sufficiently supersymmetric) cutoff, and add local counterterms with positive powers of Λ to cancel any divergences. Since the underlying theory is conformal, there is no danger of getting the wrong answer by doing this. For purposes of tree-level amplitudes we need not consider the Λ-dependent terms at all, and for one-loop amplitudes it is simplest to use a scale-free regulator such as ζfunction or dimensional regularization. We therefore need not consider the Λ-dependent terms further in this paper.
Weyl invariance and super-Weyl invariance. Weyl invariance constrains terms more strongly than simple scale invariance, and super-Weyl invariance constrains them more strongly still. Since the original CFT is Weyl invariant and can be formulated on an arbitrary geometry, 4 the same must be true of the effective theory of the X branch. This turns out to be rather constraining for possible effective operators.

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First, let us see why certain low-derivative terms that are scale invariant cannot be given a Weyl-invariant completion and therefore cannot appear as terms in the effective action of a CFT, even without considering constraints due to SUSY.
Defining the field 5 φ ≡ X we see that the leading scale-invariant term in three dimensions would be |φ| 6 = |X| 9 2 . This term is also Weyl-invariant although it is of course disallowed by supersymmetry. Note that when we say a term O in the Lagrangian is scale-invariant or Weyl-invariant, we mean this as a shorthand that the term transforms as a scalar density (a conformal tensor of weight 3), so that |g| d 3 x O is truly Weyl-invariant. The next term would be the kinetic term (∇ µ φ)(∇ µφ ). This term is scale-invariant but not Weyl-invariant and therefore not conformally invariant either. However it has a Weyl-invariant completion obtained by adding the conformal coupling to the Ricci scalar, Leading interaction term. Now let us discuss the interaction term and its effects on the spectrum of the X branch.
There are no Weyl-invariant bosonic operators with three derivatives. This is immediately clear on the basis of Lorentz invariance and parity. At the four-derivative level, there is a unique Weyl-invariant operator with four-derivatives [12][13][14][15][16] which in flat space takes the form of a supersymmetrized operator of Fradkin-Tesytlin-Paneitz-Riegert (FTPR) type [12,[17][18][19]: The curvature couplings of the FTPR operator have been worked out [12], and take the form where R µν = (Ric 3 ) µν is the Ricci tensor and R = Ric 3 is the Ricci scalar. For purposes of this paper, we need only know the Lagrangian on S 2 × R, which is conformally flat. So we could have worked out the curvature couplings for this particular geometry by Weyl-transforming the flat-space FTPR term under the transformation where w µ are the linear coordinates on R 3 and r is the radius of the sphere. The curvature couplings derived this way agree with the general form in (2.7) In principle, there may be terms in the effective theory that are Weyl-invariant but do not have a super-Weylinvariant completion. However the super-Weyl-invariant completion of the FTPR operator JHEP10(2017)089 exists and has recently been written down [20]. In flat space, it can be written as the superspace invariant where Φ ≡ φ+ √ 2θψ+· · · is a chiral superfield, whose complete expression is given in (A.4). By coupling this action to a background supergravity multiplet (see for instance [21,22]), we should in principle be able to derive the general curvature couplings of the fermions as well. However in practice, working out the component form of the super-FTPR term from the curved superspace expression is quite cumbersome. Since we only interested for purposes of this paper in the case of S 2 × R, it is more efficient to Weyl-transform the action directly from the flat-space expression. For a sphere of radius r, we obtain: (2.10) Here ∇ 2 is the full three-dimensional Laplacian, not the Laplacian on the spatial directions only.
Sign constraint. The four-derivative, zero-fermion term in the flat-space classical action comes entirely from the FTPR term (2.6). It has been pointed out [11] that such a term can only appear with a positive sign in the effective action for a massless field. A negative sign would give rise to superluminal signal propagation, as well as unitarity violation in moduli scattering, within the regime of validity of the effective theory. When we calculate the spectrum, we will see that the positivity of the coefficient (which we shall call α) shall translate directly into a negative sign for the coefficient of the leading large-J correction to the dimension of the lowest unprotected scalar operator of large R-charge J.
Global symmetries. In table 1, we present the action of the global symmetries on the fields of the UV description and on the φ, ψ fields of the moduli space of the X branch. Note that the φ-number and ψ-number symmetries are separately conserved as exact symmetries in the moduli space effective theory, not merely accidental symmetries. These separate boson-and fermion-number conservation laws simplify the classification of states and operators in the large-J effective theory to a considerable extent.

Quantization of the effective X branch theory
We now derive the Feynman rules for the quantization of the effective theory of the X branch. Our approach is the standard approach to the quantization of an effective field JHEP10(2017)089 Table 1. R and non-R global charges. The charge assignments in the effective theory are J φ = 2 3 J X + J R and J ψ = 2 3 J X − J R . The U(1) Y Z symmetry acts trivially on all light states on the X branch. The fermion-number symmetry U(1) ψ is unbroken even when φ gets an expectation value, and organizes Feynman rules in large-J states. theory. We have a double hierarchy E IR < < Λ < < M UV , where Λ is the cutoff (of unspecified form) and M UV is the ultraviolet scale set by the "vev" of |φ| 2 . We will be working in finite volume, so the "vev" is not truly a vacuum expectation value; however we shall refer to it as a "vev" anyway informally. Later on we will comment on the physically and mathematically precise meaning of the vev in the sense we use it. For now, it is sufficient to refer to it by its operational meaning: we define the path integral by dividing Φ ≡ X Vev and fluctuations. We begin by defining where F is presumed to satisfy the free-field equation of motion ∇ 2 φ = + 1 8 Ric 3 φ = 1 4r 2 φ, and ϕ 0 is constant. We then decompose the FTPR term into vev and fluctuations, retaining terms of four or fewer fluctuations. Note that substituting φ 0 into O super-FTPR will only yield zero, so that the classical correction vanishes.
We now list a few vertices that will be relevant later. By explicit computation, there are no corrections quadratic in fluctuations, modulo terms proportional to the leading-order equations of motion. By Lorentz invariance this must be so in flat space; by Weyl rescaling it is automatically the case on S 2 × R as well. There are also cubic vertices with three bosonic fluctuations, as well as two fermions and one bosonic fluctuation; however these do not contribute to the observables we will calculate and we do not list them. In general, the FTPR vertex with n B bosonic fluctuations and n F fermions, scales as |φ 0 | −(n B +n F +2) ,
The 4-point bosonic vertex is The vertex with two fermions and one bosonic fluctuation is and the vertex with four fermions and no bosonic fluctuations is As we will explain later when we give a precise definition of the "vev" φ 0 , the F field satisfies Feynman boundary conditions, thus has the usual Feynman propagator.
Feynman rules and J -scaling of diagrams. Having decomposed the field into vev and fluctuations, we can most easily understand the scaling of corrections by writing the Feynman rules for the f and ψ fields. A diagram with m FTPR vertices with k 1 , k 2 , · · · , k m lines on each vertex, will scale as |φ 0 | −2m− k i , and therefore as J −m− 1 2 k i .

Corrections to operator dimensions
Now we are going to study the theory in radial quantization, which means computing operator dimensions as energies on S 2 with radius r, in units of 1 r . We will focus on the lowest states with given global charges (in particular the R-charge), as well as low-lying excited states above the lowest. We will see that the lowest state is described by a classical solution with a particular symmetry, and that the fluctuations around the classical solution JHEP10(2017)089 are weakly coupled when the global charges are large. Thus the quantum properties of the lowest state and states of low excitation number above the lowest, are calculable in a perturbation series with expansion parameter 1 J .
Classical solutions with lowest energy for a given global charge. There is a particular family of classical solutions on S 2 × R that saturates the lower bound on the energy for a given R-charge, E ≥ J R /r, where r is the radius of the sphere. This solution exists regardless of the form of the terms in the effective action for X. This follows from a general fact in classical mechanics: the lowest classical solution with a given value of a conserved charge J, always preserves a "helical" symmetry, i.e., a combined symmetry under a time translation and action of the conserved charge J by Poisson brackets. Furthermore, the angular frequency of the global symmetry action is given by ω ≡ dE dJ . In the case where the global symmetry is an R-charge, the lowest classical solution with a given J R is invariant under a combined time translation and Rsymmetry rotation, and the angular frequency of the R-symmetry rotation is exactly 1/r for any value of the amplitude. That is, the lowest classical solution(s) carrying a given value of the R-charge have a helical symmetry, with X, Y, Z depending on time as exp{2it/3r}.
Due to the presence of the XY Z superpotential, there is no such solution with more than one of X, Y, Z turned on at a time, so the lowest classical solutions carrying a given R-charge are simply X = X 0 exp{2it/3r}, and then two other branches of solutions, with X replaced by Y or Z. These branches of solutions have X, Y, and Z charge equal to 3 2 times their R-charge, respectively. Due to the S 3 symmetric group permuting the three branches, we can ignore the Y and Z branches, and focus exclusively on the properties of the X branch.
We emphasize that we are not assuming any relation between classical solutions of the UV free XYZ model, and solutions of the moduli space EFT. Rather, we are simply using known structure of the moduli space and the known properties of the moduli space effective action to describe the large charge states in the infrared. In particular, each branch of moduli space has exactly one light complex scalar field with a particular combination of global charges.
Unlike the values of E and ω for a given J R , which are universal, the amplitude |X 0 | of the helical solution as a function of J R depends on the unknown form of the Wilsonian action. However we can estimate the value of |X 0 | on J R using dimensional analysis. All scale invariant bosonic terms take the form of polynomials in derivatives of X andX in the numerator, dressed with the appropriate power of |X| in the denominator to render the term scale invariant. So each additional derivative (or curvature) in the numerator costs an additional power of |X| 2 (or two) in the denominator. Thus the derivative (and curvature) expansion of the Lagrangian is also an expansion in inverse power of |X|, because of the underlying conformal invariance of the theory, which we use as an input in constraining the action. It follows that the leading term in the effective action for X, which is simply the free kinetic term with conformal coupling to the Ricci scalar, controls the leading large-J asymptotics of the magnitude of |X 0 | in the helical solution. Thus we conclude that |X 0 | is proportional to ( J r ) JHEP10(2017)089

Meaning of the "vev"
Free-field matrix elements with a "vev" are coherent state matrix elements. In finite volume, there is of course no such thing as spontaneous breaking of global symmetries. This can be seen easily from the fact that the expectation value of a charged operator in a state of definite charge, is always zero. This statement holds only if the state is an exact charge eigenstate. However states with exactly Gaussian correlation function for charged free fields can be constructed as coherent states. If a † ≡ (a † ) φ is a creation operator for an excitation of the φ field in the s-wave, then the coherent state has the property that and correlation functions of the oscillators in the state [v] are exactly Gaussian. Therefore free fields φ,φ built from the oscillators have the property that f ≡ φ − φ andf ≡ φ − φ have the same correlation functions as the vacuum correlation functions of φ andφ: where we have defined It remains to compare the expectation values in a large-J eigenstate with expectation values in a coherent state 6 and to show that the latter approximates the former in the large-J limit, with calculable corrections. Using , the definition (4.1) can be written and inverted to give (4.6) (Here, J denotes J φ , the charge of the φ-oscillator). This state has exactly Gaussian correlators, with a connected two-point function identical to that of the (uncharged) vacuum. It follows that the relation between the vacuum and coherent-state two-point function is simply a shift of the one-point functions, by a free classical solution. We can therefore use Feynman diagrams in a "background" given by the classical solution represented by the coherent state expectation value, to calculate arbitrary free-field correlation functions in the coherent state. So the usual Feynman diagrammatic perturbation theory with a "vev" given by a nontrivial free classical solution for the scalar JHEP10(2017)089 field, is simply a way of doing time-ordered perturbation theory in the coherent state in finite volume. This is relevant to the large-J expansion for definite-J matrix elements, because as we will now see, large-J matrix elements in charged Fock states are approximated at leading order by matrix elements in the corresponding coherent state.
Relationship between Fock states and coherent states. A consequence of this representation is that expectation values for Fock states are approximated at leading order in J by expectation values in coherent states, up to (calculable) subleading large-J corrections. To see this concretely, we need the following facts: • The definite-J Fock matrix element is given by a double contour integral of coherentstate matrix elements; • The double contour integral for a neutral operator can be evaluated by saddle point; • Fluctuation corrections to the saddle-point approximation are suppressed by powers of J; and • The leading saddle-point approximation is simply given by the coherent-state matrix element in the coherent state where the expectation value of the charge, is J.

First we write the expectation value
(4.7) One combination of the two integrals simply projects onto operators O that commute withĴ. Assume WLOG that O carries a definite charge, i.e., [Ĵ, O] = J O O. If J O = 0, then clearly its expectation value in Fock states must vanish. The first of the two contour integrals simply implements the projection that causes the Fock state expectation value to vanish.
If O is uncharged, the remaining contour integral is nonzero, and can be evaluated by saddle point when J is large, with fluctuation corrections that can be calculated as a series in 1 J . Define F (O) [J cl ] as the expectation value of an uncharged operator O in a coherent state of classical charge equal to J:

Then the Fock expectation value A (O) [J] is given by
where the leading coefficient R 00 is 1, and all the other coefficients are given by the generating function m,n≥0 R mn x m y n = e −xy (1 + y) x . (4.10)

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Note that R mn = 0 unless m ≤ n/2, so there are only a finite number of nonzero terms at a given order in J. Concretely, if we expand is the relative-order J −k contribution to the Fock-state expectation value, then 12) and the first few contributions are (4.13) As expected, the leading approximation A 0 [J] is simply equal to the coherent-state expectation value.
Conical deficit and φ-charge quantization. The change of variables φ ≡ X 3 4 is wellbehaved at large values of X (compared to the infrared scale) but singular at the origin. The classical helical solution never comes near the origin of field space, nor do fixed-energy perturbations of the helical solution in the limit of large J. So one would expect the singularity of the change of variables to be irrelevant in large-J perturbation theory.
On the one hand, this expectation is entirely accurate, in the sense that the details of the "resolution" of the singularity are indeed irrelevant to all orders in the 1/J expansion. Any two physically well-defined resolutions of the singularity, must necessarily correspond to different Hamiltonians H 1,2 that modify the moduli space effective action in a neighborhood of φ-field space of size M + 1 2 (equivalently, a neighborhood of X-field space of size M + 3 4 ), where M is some ultraviolet scale. If the correction terms scale like M k 2 /|φ| k at long distances in field space, then the corresponding large-J corrections go as (M/J) k 2 . If the two resolutions of the geometry are both exactly conical outside of a region of field space |φ| < M 1 2 , then the corrections to observables from the modified geometry vanish to all orders in J. This is the precise sense in which the singularity at the origin is "irrelevant" for large-J physics: at large J, the field doesn't live at the origin or anywhere near it.
However the conical deficit is a property of the geometry that is visible asymptotically, and the effective theory should know about all properties of the moduli space geometry where the vev is large compared to the infrared scale. The quantization rule for φ-charge is precisely the property of the quantum effective theory that encodes the conical deficit at large vev. For purposes of deriving a large-J asymptotic expansion in the effective field theory, one may simply take J X to be a multiple of 3 , in which case the number of φ-excitations is an integer, and in particular a multiple of 4.

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To verify that the only effect of the conical deficit is to alter the quantization rule, one can simply repeat any calculation in the φ effective theory, in terms of a logarithmic superfield defined as L ≡ ln(Φ). In terms of L, the only effect of the conical deficit is to alter the periodicity of the imaginary part of L; otherwise the Lagrangian is completely unaffected by the deficit. We conclude that the conical deficit has no effect on the energy spectrum to any order in perturbation theory, so long as the classical solution uniformly satisfies |φ| 2 > > E IR .

BPS property and vanishing of the vacuum correction
The classical energy of the large-J ground state. First, as a consistency check, we shall examine the energies of the BPS states, at the classical and one-loop level. By general multiplet-shortening arguments [24][25][26][27], these energies must remain uncorrected, and equal to the R-charge of the state. However even at the classical level, it is not immediately apparent that the super-FTPR term leaves the energies of the BPS states unaffected at the classical level. The term is a sum of many contributions with particular coefficients, none of which individually vanishes for the helical ground state classical solution. Nonetheless the sum of the terms in the FTPR expression (2.11) does indeed combine to give zero when evaluated on the helical solution: for any spherically homogeneous helical solution with frequency 1 2r , φ = exp{it/(2r)} φ 0 . This gives us some confidence in the applicability of the moduli space effective action to compute energies consistently.
Next, we shall compute the one-loop energies of the ground states, as well as semiclassical and one-loop energies of first-excited states as a consistency check, to build further confidence in our methods.
One-loop energy of the large-J ground state. We now check the one-loop energy of the large-J ground state, by expanding the action around the helical solution to quadratic order in fluctuations, and summing ±ω over bosonic and fermionic fluctuations with frequency ω, with the sign appropriate to the statistics. At the free level, the bosonic and fermionic fluctuations are paired at each frequency, and thus their contributions to the vacuum energy cancel mode by mode. The super-FTPR term could in principle have corrected the frequencies at order J −2 but it does not: as noted in section 3, the super-FTPR term, when expanded around the helical solution, contains no pieces quadratic in fermions or in bosonic fluctuations, and thus the energy is automatically uncorrected at absolute order J −2 (which is relative order J −3 ) even without any further nontrivial Bose-Fermi cancellation. So we see that the energy of the BPS ground state is therefore uncorrected up to and including order J −2 , as it must be to all orders in J. A nontrivial test of the large-J expansion would be to verify the cancellation of the correction to all orders in the loop expansion. It may be that some type of superfield formalism adapted to quantization about the helical ground state would make such cancellations more transparent.

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4.4 Semi-short property of the s-wave one-particle state Next we turn to the computation of first-excited energies at large J. The lowest state above the large-J ground state with the same U(1) quantum numbers, is the state with an additional φ excitation andφ excitation, both in the ℓ = 0 mode, i.e., the s-wave. At the free level, each has frequency ω = 1 2r , and we have seen that the frequency is unaffected by the interaction term up to and including order J −2 . So up to and including order J −2 , the energy of the first excited state is simply J + 1.
Since this state is not a BPS chiral primary, one might be interested to calculate corrections to its energy in the large-J expansion. However the one-loop correction actually vanishes.
Heuristically, the first-excited state can be thought of as obtained by shifting the φ charge of the vacuum from J → J + 1, and then cancelling it by adding a single quantum ofφ in the s-wave: Note that this linearized solution does not preserve the helical symmetry of the ground state; it isφ rather than φ that has a positive-energy mode excited. The one-loop correction to the energy of the state coming from a quartic vertex, can be seen to cancel explicitly. The one nontrivial aspect of this cancellation is the operator ordering of the quartic term: since the vev corresponding to the coherent BPS state breaks time-reversal invariance spontaneously, the ordering of operators is not simply described in terms of timeordered terms. The more convenient description is in terms of normal-ordered operators in the Hilbert space on the sphere: all operators appearing have at least twoφ-multiplet annihilation oscillators ordered to the right, and thus the perturbing Hamiltonian does not affect the energy of the semishort state, which has only a singleφ excitation. The existence of semishort states with the appropriate charges is visible at the level of the superconformal index; we have included an expression for the index in the appendix, as well as its expansion to several orders, so that the reader may see the agreement for herself. It is interesting to note that the semi-short states of the X-branch persist down to J = 0: the "moment map" operator is semi-short on general grounds, because it the superconformal primary whose descendant is the U(1) X current [28,29]. This operator can be thought of as the conformal Kähler potential itself for the effective theory of the X branch, namely K ∝ (XX) 3 4 . This representation in terms of the X field is not a welldefined, controlled operator for general purposes, but this expression is well-defined and precise in matrix elements between large-J states.
The one-particle states with nonzero spin are also in semi-short representations at the free-field level. At the interacting level, it is easy to prove in many cases that the semi-short property persists, because there are no states with the appropriate angular momentum, U(1) R , and U(1) X quantum numbers to fill out a full long representation at weak but finite coupling. For instance, the vector states obtained by acting on the BPS vacuum φ J+1 with the ℓ = 1 modes of theφ field, can be shown to be protected by such an argument. This prediction is also verified by the superconformal index.

Correction to the two-particle energies
Semi-short property means no disconnected diagrams. Say we calculate the energy correction to the state with twoφs on top of φ J . By expanding in VEV and fluctuations, two diagrams to consider at order J −3 are as follows: Incidentally, we know from the argument in the last subsection that this diagram should vanish: (4.17) Note that these Feynman diagrams with loops in them have scheme dependence, i.e., how you regularize and renormalize loop integrals -once we choose one scheme that is compatible with supersymmetry on S 2 × R, the expression is meaningful, and the diagram (4.17) gives exactly zero. Hence the only contribution to the energy correction at order J −3 is the diagram (4.15).
The above argument holds even when some of theφs are changed intoψ, theQdescendant ofφ. The only diagram that contributes to the energy correction to the statē ψφ φ J is

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Two-particle states energy correction. Now let us calculate the energy correction to the stateφφ φ J by expanding in VEV and fluctuations. Here note that we only have to care about spatially uniform field because of the argument in the last subsection. Truncating f to s-waves accordingly, we get the Lagrangian density for the fluctuation f (t), Above we have for simplicity set the radius r of the sphere to 1, as we shall continue to do in the rest of this section. Dots represent derivative with respect to t and the radius of S 2 is set equal to unity. We derive the Hamiltonian (4π times the Hamiltonian density) of the system from this Lagrangian. The conjugate momentum in terms of f andf is Π :=ḟ − i 2f andΠ :=ḟ + i 2 f , respectively. (4.21) As always we define creation and annihilation operators as and H int becomes We then evaluate the energy correction to the state a † a † |0 , which corresponds toφφ φ J : Likewise, the energy correction toψφ φ J andψψ φ J can be evaluated and gives the same number as that ofφφ φ J , as it should be due to supersymmetry. Detailed calculations are given in the appendix C. Note that the form of the operator perturbation is normal-ordered rather than timeordered. This is a consistency condition for supersymmetry, and it can be derived directly from the necessity of the existence of a set of operators implementing the N = 2 superconformal algebtra; in fact, it can be seen just from the consistency of a smaller algebra generated by half the generators, namely those preserving the BPS states X J . In appendix E, we demonstrate how the closure of the operator algebra in the interacting theory JHEP10(2017)089 directly dictates the form of the operator perturbation of the Hamiltonian in a toy model, obtained by truncating theφ multiplet down to its zero mode on the sphere.
In the matrix element (4.24), note that disconnected contributions coming from vacuum bubbles and propagator corrections are absent; the vanishing of these contributions follow from the nonrenormalization of the vacuum energy and semishort one-particle energy, respectively.
We also draw the attention to the relative negative sign between the parameter α in the Lagrangian, and the first correction to the non-BPS operator dimension. A positive value for α implies a negative anomalous dimension, and vice versa. As noted in section 2, the sign of α must be positive due to a superluminality constraint [11] and thus the order J −3 contribution to the anomalous dimension is negative.
We have also calculated, in appendix C, the energy shifts of the one-boson, one-fermion state with the fermion in the ℓ = 1 2 sector, and also the two-fermion state with both fermions in the ℓ = 1 2 mode. These are theQ andQ 2 -descendants of the primary state, respectively. The first-order interaction contributions to the anomalous dimensions are the same as for the two-boson state, which nontrivially checks that our formalism implements superconformal symmetry consistently.

Operator algebras and the semishort spectrum
In this section we return to the question of the semishort energy (non)correction. We have seen explicitly that the one loop correction to the scalar semishort energy cancels, and there is an algebraic argument that the scalar semishort energy is unrenormalized to all orders in large-J perturbation theory: the energy can only change if the semishort joins with other states to form a long multiplet, and there are no states with the correct quantum numbers, that are near energy ∆ = J R + 1 at large J, to fill out a long multiplet. This establishes that there is a scalar semishort at sufficiently large J. In this section we will see that this fact has consequences at low values of J due to the structure of the operator algebra: scalar semishorts form a module over the chiral ring, and as a result associativity will relate semishorts at high J to those at low J.
Nonsingularity of certain OPE structure functions. In any unitary N = 2 SCFT in three dimensions, all superconformal primary operators must satisfy [24][25][26][27], with the inequality saturated if and only if the state is annihilated byQ ↓ : SSSSP is annihilated byQ ↓ and alsoS ↑ , and therefore does saturate it: The scalar chiral primaries have a ring structure because their OPE is automatically nonsingular [30,31]. The argument follows immediately from rotational invariance, scale invariance, and the BPS formula (5.2).
If O 1,2 are two chiral ring elements, then their dimensions and R-charges satisfy ∆ 1,2 = R 1,2 . Their OPE is of the form where O i are operators of R-charge R i = R 1 + R 2 , dimension ∆ i , spin s i , and in particular third component of spin equal to s 3 i . The function f i has σ-scaling γ i ≡ ∆ i − ∆ 1 − ∆ 2 = ∆ i − R 1 − R 2 . So by (5.3) we have γ i ≥ s i , and so all the structure functions f i vanish at σ = 0 unless O i is a scalar. In the latter case the structure function has a finite limit, the OPE is nonsingular, and the product of two BPS scalar primaries at coincident points defines an associative multiplication which is the multiplicative structure of the chiral ring. Now we consider the operator product of a BPS scalar O BPS of R-charge R BPS with a scalar semi-short O SSS with R-charge R SSS . The dimensions of the operators are ∆ BPS = R BPS and ∆ SSS = R SSS + 1. In this case, there can be singular terms in the OPE, such as which will be of principal interest to us in this section. We would like to establish that this smooth and nonvanishing term (5.9) in the OPE defines an associative multiplication of the chiral ring on the scalar semi-shorts. We cannot draw this conclusion directly from the OPE above, because the nonsingular terms in a JHEP10(2017)089 generic OPE are not in general associative; only the sum of all terms, singular and not, generally satisfy associativity when taken together. However by taking aQ-descendant, we can establish associativity of (5.9) indirectly: by taking theQ ↑ descendant, we can define an associative action of the chiral ring on the superpartners O (↑) SSSSP ≡Q ↑ · O SSS of scalar semi-shorts.
Both O BPS and O α SSSSP ≡Q α · O SSS satisfy the BPS formula (5.2), so by the same arguments as above, any structure functions f i appearing in their OPE must scale as |σ| γ , with the exponent γ defined as where ∆ RHS and R RHS = R BPS + R SSS + 1 are the dimension and R-charge of the operator on the right hand side of the OPE. If the spin of the operator on the r.h.s. is s RHS , then the dimension satisfies the inequality (5.3), In the case where the r.h.s. is a scalar semishort superpartner, so s RHS = 1 2 , so This allows for two possible Lorentz-invariant tensor structures, It can be shown that the second of the two tensor structures can never appear in a paritysymmetric theory such as the XY Z model. The result is that the OPE of a chiral ring element with the superpartner of a scalar semishort operator is of the form where O α SSSSP is the scalar sem-short superpartner and the operator O α A is a spin-1 2 operator saturating the BPS bound. Any such operator is again necessarily theQ α descendant of a scalar semi-short, as shown by the following argument.
By virtue of the BPS bound, all other operators on the right-hand side of (5.14) vanish in the limit σ → 0. Therefore theQ-descendants of scalar semishorts form a module over the commutative ring of the chiral primaries: 7 From this, it follows that the scalar semishorts themselves form a module over the chiral ring. Naively this would appear to follow without any further justification, as one expects that the OPEs of descendants are completely determined by the OPEs of primary operators. For conformal invariance this is indeed the case, a fact synonymous with the JHEP10(2017)089 existence and uniqueness of the conformal blocks. For superconformally covariant OPEs, this argument does not generalize; there exist multiparameter families of nontrivial, fully superconformally invariant functions of three points in superspace [33]. Multiplying a supercovariant three-point function by such a function of three copies of superspace, yields another supercovariant three-point function. However, in the case where one of the three operators is a BPS scalar primary, this issue does not arise: the identity is the only function on three copies of superspace that is annihilated byD α acting on any one of the three points.
Heuristically, we can talk directly about the action of the chiral ring on scalar semishorts through the combined operation Since the chiral ring is annihilated byQ ↑ , the operator O BPS does indeed formally commute throughQ ↑ , justifying the above definition. However, the uniqueness of superconformal three-point functions with one chiral primary is necessary to make logical sense of equation (5.16). The property of scalar semishort operators, that they form a module over the chiral ring, has a remarkable consequence for the spectrum of the theory: it implies the existence of scalar semishorts at low J as well. Starting with the moment map operator (XX) 3 4 = φφ, we act J times with φ to obtain a scalar semishortφφ J+1 . Algebraically, this state could in principle vanish: a priori the representation of the chiral ring on the module of semishorts need not be faithful. However we have seen already that the scalar semishortφφ J+1 is nonvanishing for sufficiently large J, using the effective description! By associativity, then, it is impossible for any of the intermediate productsφφ k+1 to vanish, for any nonnegative value of k.
The presence of scalar semishorts for all k can of course in principle be seen via the superconformal index; and in the appendix we expand the index to several orders and verify the prediction. However it should be emphasized that the large-J picture yields the same conclusion with a far less laborious method.

Conclusions
In this note we have computed the dimensions of certain operators in the N = 2 superconformal XY Z model in three dimensions, to first nontrivial order in an expansion in large R-charge J R and large X-charge J X ∼ 3 2 J R . To do this, we treated the theory in radial quantization, and used the effective theory on the moduli space of the X branch. In this theory, both quantum corrections and higher-derivative interaction terms are suppressed by powers of |φ| = |X| 3 4 when |φ| is large, and |φ| scales as J + 1 2 . We have seen that the state with oneφ excitation in the s-wave is protected because its superconformal representation is semi-short [24][25][26][27] and has to candidate state with the correct quantum numbers to play the role of itsQ 2 descendant. The third-lowest scalar primary can be understood as twoφ quanta in the s-wave, on top of a sea of (2J R + 2) φ-quanta in the s-wave. This state is in a long multiplet and has an energy shift that is proportional to the coefficient of the first interaction term -the supersymmetric version of the FTPR term. By arguments based on unitarity and causality, the coefficient of the super-FTPR JHEP10(2017)089 term in the action must be positive, and as a result, the energy shift must be negativedefinite. There is an interesting formal similarity between the large-R-charge expansion of the anomalous dimension, and the large-spin expansion of the anomalous dimension of operators with large spin [34,35], despite the two expansions resting on rather different logical arguments. It would be interesting to understand these two expansions within a unified framework of operator dimensions with large quantum numbers.
One major virtue of the large-J expansion, in the case where a moduli space exists, is that it gives us the tools to connect properties of a superconformal field theory that are expressed in "bootstrap"-like language 8 -i.e., anomalous dimensions and operator algebra structure constants -with those that can be expressed in the language of effective field theory on the moduli space of vacua.
In moduli space dynamics, superconformal invariance is spontaneously broken and properties of the theory can be computed perturbatively in the low-energy effective theory. Such perturbative computations do not rely on any weak coupling in the underlying dynamics; the perturbative parameter in the context of moduli space EFT is the ratio of the infrared to the ultraviolet energy scale, which here is simply an inverse power of the total charge of the state. Thus our framework can be used to compute a 1/J expansion for properties of near-BPS states in a controlled fashion.
As a consistency check, we have verified that the appropriate BPS states with large X-charge do in fact exist. For chiral ring elements this is immediate, and it is slightly more nontrivial for semi-shorts scalar states. Interestingly, once we can verify the existence of scalar semishorts at high X-charge, the module structure of the semishorts over the chiral ring, immediately implies the existence of scalar semishorts at low X-charge as well. This prediction agrees with explicit calculations of the spectrum extracted with some effort from the superconformal index. Thus it appears the combination of holomorphy with the large-J expansion is more powerful than the sum of its parts. It may be hoped that this combination of points of view may be used to gain insights into the dynamics of other interesting superconformal theories as well.

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done with the help of the excellent Mathematica TM package diffgeo.m developed by M. Headrick [38].

B Uniqueness of the super-FTPR operator on flat space
We would like to show here that on flat space there is no supersymmetric dimension-3 operator constructed with four superderivatives, except for the super-FTPR operator (2.9). First of all, we do not have to consider operators containing any odd number of superderivatives acting on a single Φ orΦ, because such operators are always equal to ones containing only even number of superderivatives acting on a single Φ orΦ, modulo the leading-order superspace equations of motion,

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and especiallyD α D α Φ = 0. These identities are useful in decreasing the number of index structures. For instance, one can show that any candidate containing four superderivatives acting on a single Φ in any order vanishes modulo the leading-order superspace equations of motion. By the above consideration, we conclude that only the following operators possibly survive, 2 is equivalent to the super-FTPR operator (2.9), since D α ,D β = 2γ µ αβ ∂ µ . O 1 is also equivalent to the super-FTPR operator, becausē Here, by "∼" we mean modulo total superderivatives, the leading-order equations of motion, and numerical coefficients. So, there is only one supersymmetric dimension-3 operator with four superderivatives on flat space modulo total superderivatives, and it is nothing but the unique super-Weyl completion of the FTPR operator.

C Energy correction to one-boson one-fermion and two-fermion excitations
We assume the radius of S 2 to be unity throughout this section.

C.1 One-boson one-fermion excitation
Quantization of the lowest spin ψ α state must be done as follows: We also make use of the equation of motion for ψ: At the end of the quantization process we set

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as a normalisation condition. According to this quantization convention we get the free Dirac Hamiltonian, with the commutation relation being The interaction term in the Hamiltonian of order J −3 which includes 2-fermion 2-boson interaction is given by where α is a proportionality constant as in (4.20). Making use of the equation of motion and the fact that φ 0 = e it/2 ϕ 0 and then taking only the spin-1/2 and spin-0 contribution for the fermion and the boson field, respectively, we get Using the quantization of the boson field given in section 4.5 and that of the fermion field given above, we get which leads to the energy correction to the state a † β † + |0 is This agrees with the energy correction to the two-boson state, as it should be from supersymmetry.

C.2 Two-fermion excitation
The interaction term in the Hamiltonian of order J −3 which includes 4-fermion interaction is given by where α is a proportionality constant as in (4.20). Making use of the fact that φ 0 = e it/2 ϕ 0 and taking only the spin-1/2 contribution for the fermion field, we get

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where L = ψψ. Then by using (C.1) and the normalization condition, we get and and the resulting energy correction to the two-fermion state β † which agrees with the energy correction to the two-boson state, as it should be from supersymmetry.

D Superconformal index and scalar semi-short multiplets
In this appendix we check the superconformal index for the XY Z model to confirm that scalar semi-short multiplets really exist in the theory. The superconformal index for the XY Z model is given by the following plethystic exponential [39,40], Here, s 3 is the third component of the spin on S 2 , and t X and t Y Z are the fugacities for U(1) X and U(1) Y Z , respectively. F (x, t X , t Y Z ) is the so-called letter index, Because of the superconformal algebra, only protected multiplets can contribute to the superconformal index and therefore it is independent of the variable z in (D.1). In a BPS multiplet, the BPS primary operator and its ∂ ↑↑ -derivatives contribute to the index, whereas contributions from the other states in the BPS multiplet cancel between themselves. In a given scalar semi-short multiplet, it is theQ ↑ descendant of the semi-short primary operator and its ∂ ↑↑ -derivatives that contribute to the index. When the index is expanded with respect to x, contributions from BPS multiplets have positive coefficients,

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whereas those from semi-short multiplets have negative coefficients. The operators ∂ ↑↑ and Q ↑ are the partial derivatives and supercharges with spin +1 and + 1 2 along the z-axis. In principle, the superconformal index contains all information about operators in short or semi-short representations. In principle, even the terms in a full and explicit calculation of the index do not necessarily correspond one-to-one with operators satisfying (5.2), because cancellations can occur. Chiral ring elements contribute with a positive sign, while superpartners of scalar semishorts, for instance, contribute with a negative sign. In practice, cancellations occur frequently in many familiar theories, including the XY Z model in D = 3. These cancellations can be removed by organizing the index into characters of the particular short representations that appear.
We do not do this, since the organization into characters is cumbersome a and we are just calculating the some particular terms in the index to establish its agreement with the spectrum of semishort representations as computed with the large-J effective theory. Rather, we list both the positive and negative contributions to the index separately, noting the cancellations as they occur.
To see the existence of the scalar semi-short multiplets, we expand the superconformal index (D.1) with respect to x up to and including O(x 10/3 ). However, some contributions from semi-short multiplets are canceled by those from BPS multiplets, and therefore we cannot see all the contributions from semi-short multiplets just by expanding the index. So, we separate these two kinds of contributions order by order, by brute force. We also identify all the positive contributions up to and including O(x 10/3 ) with (descendants of) BPS operators. The superconformal index (D.1) is expanded with respect to x as follows: The negative contribution at O(x 2 ) is due to theQ ↑ descendants of the moment map operators D X and D Y Z , which trivially exist because of the U(1) X and U(1) Y Z symmetries. The negative contributions at O(x 8/3 ) and at O(x 10/3 ) are nontrivial, however. These cannot be descendants of the moment map operators on dimensional grounds. For instance,

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the −x 8/3 t X and −x 10/3 t 2 X terms are naturally identified with the which are theQ ↑ descendants of semishort operators of spin 0 and dimension 5/3 and 7/3, respectively. In terms of the almost-free φ variables, these semishorts can be represented as φ 0φ0 |X and φ 0φ0 X 2 , where as explained in section 4.2, the state X J can be thought of as φ 4J 3 0 |0 . Heuristically, these semi-short operators can be thought of as D X · X and D X · X 2 , respectively, where D X is the weight-1 scalar semishort "moment map" operator, whose descendant is the spin-1 X-number current. However this description is not fully precise, because the leading term in the OPE of D X with X J is not the semishort operator D X X J but rather the chiral primary X J , and the coefficient function is singular, |σ| −1 .
We emphasize that, for purposes of understanding the spectrum directly at sufficiently large J, the power of supersymmetric representation theory is useful mainly as a convenience: the explicit computations of the large-J effective theory simply agree with those of the index, with the spectrum computation becoming more reliable at large J.
The most important thing we learn directly is that there is a nonzero scalar semishort in the OPE of D X with X J , for sufficiently large J: where the structure constant C D X X J X J and can be calculated semiclassically from an expectation value of D X in the state X J , and is nonzero. This gives information about the index only asymptotically.
Combined with the power of associativity, the existence of semishorts at large J has more consequences: since the product · defines an associative multiplication, and since D X ·X J = 0, then all the lower-dimension products D X ·X, D X ·X 2 , · · · must automatically be nonzero as well. This is in agreement with the index as expanded above. So we see that large-J methods combined with associativity, yield information about semishort operators at low J as well.

E Semishort superalgebra
Let us try to set up a formalism of truncating the superalgebra to a finite degrees of freedom, which are creation and annihilation operators. This section is useful in understanding the vanishing of the 1-loop energy correction to the BPS and semi-short state with given charge J. For the consistency with the notation in A, upper the indices of the operators with dagger assigned.

E.1 Commutation relations
We work in radial quantization -then we have, as a basic building block of the algebra, ∆, the operator dimension, and † , the Hermitian conjugation. We are here doomed to dismiss either P or K at the very least, because of the fact that the bosonic conformal algebra can only be unitary represented in infinite-dimension Hilbert space. At any rate, however, we are trying to find a truncation of the algebra that contains as many supercharges as possible, under such a constraint.

E.3 Perturbation theory
Now let us set us perturbation theory. We wish to make a small change to the generators, at order ǫ, and demand that the structure of the superalgebra still be preserved at order Many first-order perturbations of the algebra are unphysical, and correspond merely to first-order redefinitions of the variables induced by transformations on Hilbert space; we fix much of this ambiguity by the condition that s a and J to be constant, independent of ǫ: Then use the notation and take the first ǫ-derivative of the algebra (E.4)-(E.9) {Q α (ǫ), Q † β (ǫ)} = δ αβ∆ (ǫ) + σ a βα s a , (E.20) and "hard" perturbation equations which involve two different perturbations: The "easy" perturbation equations (E.26) just express that the transformation laws of the perturbed generators under the "fixed" generators J, s a are the same as those of the corresponding unperturbed generators. Let us solve the hard perturbation equations. First, start with equation (E.29). Solving this in full generality may be difficult, but can be at least done in a sufficient condition way, i.e. this equation is solved by We can use the notation · for acting by commutation or anticommutation. We denote this by Q, and also define The meaning of the subscript [2] will become clear shortly. So then we have The ansatz we're going to make, to solve (E.3), is The first term would be present in flat-space SUSY. Indeed, the formula for ∆ ′ in terms of four supercharges acting on O [0] , is just an operator realization of superspace perturbation theory, with O [0] playing the role of the superspace integrand of D-term type. The second term on the r.h.s. of (E.39) is not present in flat-space SUSY, and corresponds to a nontrivial background curvature of superspace in the sense of [21,22].

E.4 A last bit of closure of the algebra
There is one last nontrivial equation that must be satisfied. It comes from eq. (E.31) (and its conjugate (E.32)). Equation

E.5 Examples
Now we would like to apply our formula to some examples of O [0] , which correspond to the superspace integrand of superspace perturbation theory, to see concretely how interaction terms made from the semishort zero mode correspond to perturbations ∆ ′ of the Hamiltonian. In particular, we will see that all such perturbations come out automatically normal-ordered, with at least one semishort zero mode annihilation operator on the right.

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Example: perturbation corresponding to quadratic deformations. So the simplest sort of deformation to add would of course be O [0] ≡ E a † a. Then using (E.10), we find that and the perturbation of the supercharges and dilatation operator simply vanish: Quartic perturbation. Now let us work out the formulae for the quartic perturbation. We define (E.43) Then we have (E.45) The first-order modification ∆ ′ of the operator Hamiltonian is (E.48) For p = 1, note that q α , a † α and ∆ ′ vanish, as we found earlier.