Penrose limits and spin chains in the GJV/CS-SYM duality

We examine Penrose limits of the duality proposed by Guarino, Jafferis and Varela between a type IIA massive background of the type of a warped, squashed $AdS_4\times S^6$, and a 2+1 dimensional IR fixed point of ${\cal N}=8$ super Yang-Mills deformed by Chern-Simons terms to ${\cal N}=2$ supersymmetry. One type of Penrose limit for closed strings corresponds to a large charge closed spin chain, and another, for open strings on giant graviton D-branes, corresponds to an open spin chain on sub-determinant operators. For the first limit, we find that like in the ABJM case, there are functions $f_a(\lambda)$ that interpolate between the perturbative and nonperturbative (string) regions for the magnon energy. For the second, we are unable to match the gravity result with the expected field theory result, making this model more interesting than ones with more supersymmetry.


Introduction
The AdS/CFT correspondence was started in 3+1 dimensions with the duality of N = 4 super Yang-Mills (SYM) and string theory in an AdS 5 × S 5 background [1] (see [2] for an introduction to the correspondence). But many of the results obtained there were dependent on the large amount of symmetry, including supersymmetry and conformal invariance, so it was not clear a priori how much of it could be applied to the case of most interest, QCD. Then in 2+1 dimensions the ABJM duality between the N = 6 supersymmetric SU (N ) × SU (N ) superconformal Chern-Simons (CS) gauge theory and strings in an AdS 4 × S 7 background was used as a toy model mostly for condensed matter purposes, but again the large amount of symmetry stands in the way of generalizing the lessons observed there to physical contexts.
But an interesting duality was proposed by Guarino, Jafferis and Varela (henceforth GJV) in [3] that combines some of the best features of both cases, but with less symmetry and more parameters, offering the possibility of getting a little closer to real world predictions. On the gravity side it has a background solution of the massive type IIA string theory of the type of a warped, squashed AdS 4 × S 6 , and on the field theory side it was proposed that we have an IR fixed point for an N = 2 supersymmetric 2+1 dimensional SU (N ) SYM gauge theory obtained from the N = 8 one through deforming by a supersymmetric CS terms at level k. The CS level is related to the Romans mass m of type IIA by k = 2πl s m.
Like the ABJM theory, this theory is potentially rich for condensed matter phenomenology (as we said, the ABJM model is the standard toy model for condensed matter), yet because of its low amount of supersymmetry and extra parameter, can be closer to realistic models. The presence of Chern-Simons terms means first of all relevance to anyonic physics (see for instance [4] for a review). Also, since the standard description of the Fractional Quantum Hall Effect (FQHE) involves Chern-Simons terms (see the lectures [5]), one can hope to embed a holographic description of the FQHE in the GJV background, perhaps modified, like it was done in the case of the ABJM model in [6][7][8] (description corrected in [9]). The ABJM model has been also at the center of attempts to describe the quantum critical phase [10][11][12], and compressible Fermi surfaces [13], but its lack of flexibility (and of parameters) hampered a precise description; perhaps now it will have a better chance.
Another area of interest for theories in 2+1 dimensions with Chern-Simons terms is particle-vortex duality. A path integral formulation was started in [14], and developed and embedded in the ABJM model in [15]. An Sl(2, Z) action on states [14], including particlevortex duality, was shown to constrain correlators of CFTs [5], and similar constraints were found from AdS/CFT in [16]. Moreover, particle-vortex duality was shown to be part of a web of dualities for 2+1 dimensional theories with Chern-Simons terms, whose basic unit is a fermionic version of particle-vortex duality [17][18][19], and which can give information about condensed matter systems. It is likely that the CS-SYM theory dual to the GJV background can be embedded in a web of dualities also, though we have not yet considered this.
It is well known that the de Wit-Nicolai four dimensional N = 8 SO(8)-gauged supergravity can be obtained by a consistent truncation of the eleven dimensional supergravity on the seven sphere [20][21][22]. On the other hand, it has been shown that this solution belongs to a parametric family of supergravities whose parameter, ω ∈ [0, π/8], is given by a linear combination of the SO(8) electric and magnetic gauge fields. From this perspective, the de Wit-Nicolai solution corresponds to the purely electric case [23][24][25].
Naturally, one would like to know if this parametric family of supergravity solutions can be embedded into the string/M-theory framework. Unfortunately, it has been recently proved [26] that we cannot give a general stringy interpretation for this family of solutions and that de Wit-Nicolai supergravity solution is an exceptional point in this one-parameter space. Remarkably, there are also dyonic supergravity solutions with symmetry group ISO (7), which is closely related to the group SO (8), and with consistent embeddings of its purely electric case into the D = 11 supergravity through consistent truncations on S 6 × S 1 [24,27,28].
In contrast to the SO(8)-dyonic solution, it has been shown that the ISO(7)-dyonically gauged supergravity solutions can be obtained from a massive type IIA solution compactified on a squashed six-sphere, provided that the magnetic coupling constant is identified with the Romans mass [3,[29][30][31][32].
Given that the internal manifold is (topologically) a sphere, one can conjecture that the origin of this ISO(7) solution is the near-horizon of a stack of N D2-branes probing flat space with a Chern-Simons term inducing the Romans mass on the brane worldvolume. Using this brane construction, it is conceptually important to replace the transverse flat space by something more general, for example, a Calabi-Yau singularity.
Therefore, taking N D2-branes probing a Calabi-Yau threefold singularity in massive type IIA supergravity, the field theory on the brane worldvolume is an N = 2 Chern-Simons quiver gauge theory with group U (N ) G , where G is the Euler number of the resolved manifold, which flows to a field theory dual to a resolution of N = 2 AdS 4 × S 6 in the low energy limit [33].
In a previous paper by two of the authors [34], the analysis of the GJV/CS-SYM duality was started, with the study of various semi-classical observables, such as baryon vertex operators, which are dual to wrapped branes; Wilson loops, the anomalous dimensions of operators of high spin coming from large strings, and giant gravitons that are D-branes moving on cycles. Furthermore, the analysis of giant magnons was started in the same work.
In this paper, we consider the analysis of spin chains in the duality, based on the model of the closed string spin chain, dual to the Penrose limit, defined in [35], and of the open string spin chain, first defined in [36], applied to the ABJM case, for open strings ending on D-branes, in [37]. We first find a Penrose limit whose closed string excitations on the pp-wave give a closed spin chain. We then find Penrose limits for which the open string excitations, for strings ending on D-branes in the pp-wave, give open spin chains embedded into larger operators.
The paper is organized as follows. In section 2 we present the GJV/CS-SYM duality: after a review of the gravity solution, we discuss in some detail the general CS-SYM field theories, and the particular case of the dual to the gravity solution, with emphasis on the IR physics. In section 3 we present the relevant Penrose limits of the GJV geometry. We start with a classification of the useful null geodesics, namely ones that move on isometry directions, corresponding to a large charge in the field theory. These are then analyzed separately: motion in a direction ψ for closed strings, and in possible directions σ, φ, and σ + φ for open strings. Then in section 4 we analyze the spin chains dual to the Penrose limits: we analyze in some detail the one for closed strings, and then we sketch the one for open strings, as we could not match properly with the field theory. In section 5 we conclude. The Appendix contains N = 1 theories and N = 2 supersymmetric CS-matter theories in 3 dimensions in superspace. The duality proposed in [3] is between a well-defined gravitational background, and a CS-SYM gauge theory in 2+1 dimensions, which is defined somewhat implicitly, so in this section we will define it better.
We start with a review of the warped, squashed AdS 4 × S 6 solution of [3,33]. We then consider the relevant N = 2 CS matter theories [38,39], and specialize them to our case.
As is common practice in the literature, we denote the Romans mass m = F 0 . Explicitly, we write the AdS 4 metric as We also take the opportunity to record the field strength H 3 = dB, For constant α and ψ, the internal manifold is topologically CP 2 , and for λ = π/2 and fixed σ we have (topologically) a CP 1 . The points α = 0 and α = π correspond to isolated conical singularities. The isometries of the metric are SO(2, 3) for AdS 4 and the SO (7) symmetry of the internal manifold is broken down to SU (3) × U (1) for the CP 2 and the S 1 fiber ψ through various warp factors.
The constants in the solution are expressed in terms of the Romans mass m and another parameter g 2 by L 2 ≡ 2 −5/8 3 −1 g −25/12 m 1/12 and e φ 0 ≡ 2 1/4 g 5/6 m −5/6 . (2.9) Charge quantization in this background leads to (see [3,33,34]) where k ∈ Z is an integer that will be associated with the CS level in the field theory dual and s = √ α is the string length, and allows the relations 11) where N ∈ N will be associated with the rank of the gauge group in the field theory dual.

CS-SYM field theory action
The conjecture of [3] relates the supergravity solution of [3,33] to the IR fixed point of the field theory on a stack of N D2-branes with Romans mass deformation m.
The worldvolume field theory on a stack of N D2-branes in flat space is an N = 8 D = 3 SYM theory with gauge group SU (N ), containing the gauge field, 7 scalars (the transverse directions to the D2-brane) and 8 fermions, all of them in the adjoint representation of the gauge group.
Similarly to the ABJM case, the fixed point for the D2-brane theory on a background with a mass deformation m induces a Chern-Simons term on the D2-brane worldvolume, where k ∈ Z is the Chern-Simons level [3,33], which is related to the Romans mass by k = 2πl s m.
The Chern-Simons term by itself breaks all the supersymmetries, but by supersymmetrizing it and adding appropriate couplings, we can preserve up to N = 3 supersymmetries [3,28,29,31,32].
The GJV gravitational solution is an N = 2 background in massive type IIA, so the conjectured field theory dual should have the same amount of supersymmetry. In N = 2 notation, the IR fixed point theory has an SU (N ) vector multiplet V and three chiral multiplets Φ i for i = 1, 2, 3. The theory has a superpotential given by with all fields in the adjoint of SU (N ). The field content and superpotential are exactly the same as in 4D N = 4 SYM [2,40].
The theory has an U (1)×SU (3) symmetry, where the U (1) = SO(2) is the R-symmetry, and SU (3) rotates the complex scalars in the chiral multiplets. As we saw, this symmetry is realized in the dual gravitational background as the isometry of the internal space: the deformation (squashing) of the six-sphere breaks the original SO(7)-isometry down to SU (3) × U (1), respectively the isometries of CP 2 and the S 1 parametrized by the fiber coordinate ψ in the geometry.
The chiral superfield is expanded as usual into a scalar φ, a fermion ψ and an auxiliary field F , Φ = φ + √ 2θψ + θθF. (2.14) Note that the dimension of the superpotential coupling is [g] = 1/2, so the superpotential term dominates at low energies (in the IR, close to the conformal point Superconformal CS theories in 2+1 dimensions have been studied by Schwarz [38], Gaiotto and Yin [39]. The CS matter action in the presence of a superpotential W can be written as (see appendix A for more details) 15) and the complete expression is given in (A.34). The superpotential action is (2.16) Note that the CS and matter terms in the action are conformal, but the superpotential term is not.
The sextic (conformal) potential term for the scalars in (A.34), can be rewritten as The other term in the scalar potential is the non-conformal one that comes from the superpotential, which, since ijk ipq = 2δ jk pq , is

Comments on dimensions and the IR fixed point
In order to understand the IR fixed point of the above theory, we must understand the dimensions of various quantities relevant in the IR, and what is the interaction term relevant in the IR.
Gaiotto and Yin [39] consider the case of a system of D2-branes and D6-branes in massive type IIA theory, with a superfield Φ 1 corresponding to the D2-brane coordinates transverse to the D6-brane (overall transverse), and Φ 2 , Φ 3 to the D2-brane coordinates parallel to the D6-brane (relative transverse), whereas Q,Q are the "bifundamental", or D2-D6, coordinates. Then they consider the superpotential in the IR where, due to quantum corrections, in the IR we have Φ 1 of dimension 1 (whereas the fields Φ 2 , Φ 3 , Q,Q have the classical dimension 1/2), so that W is a marginal operator, i.e. it has the classical dimension of 2.
But this is only possible because in the IR Φ 1 is auxiliary, i.e. it has lost its kinetic term d 4 θΦ 1 Φ 1 , which would have meant (since θ has always dimension 1/2) the classical dimension 1/2. Then in fact we can introduce a further auxiliary term Tr Φ 2 1 /2, which means that by eliminating it we obtain the usual quartic potential for Φ 2 , Φ 3 , Q,Q, (2.20) But that was only possible since we have singled out Φ 1 , as being the superfield for the coordinates transverse to the D6-branes (overall transverse), and to the fact that in the IR, quantum corrections dominate and kill the kinetic term for Φ 1 . In their absence, this should not be possible. Then Φ 1 , Φ 2 , Φ 3 should appear symmetrically in the action, and this is the case that we have now.
In fact, [3] argue that Φ 1 , Φ 2 , Φ 3 have R-charge q R = 2/3, which would mean that W has R-charge 2. As an operator, W can stay chiral if ∆ = q R , so that would mean that the dimensions of Φ 1 , Φ 2 , Φ 3 are also 2/3, for a total dimension of 2.
But that is the same condition as would be obtained by considering instead a superpotential with coefficient g of dimension 1/2, understood in the quantum theory as having dimension coming from a µ δ factor, which therefore would dominate at low energies. Then the potential coming from it must be put to zero at low energies, again obtaining (2.23) The relation between the two pictures described above is a rescaling of the Φ i 's by g 1/3 , which would imply that after it, the kinetic term has a coefficient with dimension. Either way, the result is the same, namely φ i 's should commute in order to avoid having an infinite potential term in the IR.
But that still leaves us with the conformal term in the potential, which survives the IR limit unchanged. This is given in (2.17b).
Then in the IR (at low energies), for the picture with mass dimension [g 2 ] = 1, there will be no conformal point unless the commutator of φ i 's vanishes, which means that we will be restricted to live on the space of solutions with (2.24) Note that this still leaves the possibility that [φ i ,φ i ] = 0. Indeed, this is needed in order to have the conformal term in the potential be nonzero. 3

Penrose limits of the GJV background
In this section we will study various Penrose limits [35,41] 4 of the GJV background from the last section. For any Penrose limit, near a null geodesic moving in any direction x in 3 Indeed, note that for instance as an example of such a case for N = 2 (in the SU (2) gauge group case). Moreover, it is possible to have also [φi, φj] = 0, yet [φi,φj] = 0, for instance the background, we can consider in principle closed strings or open strings and quantize them (find the worldsheet Hamiltonian). Closed strings would be dual to a spin chain that selects the scalar Z dual to the direction x as special.
Alternatively, we can consider giant gravitons, i.e. D-branes wrapping some cycle and moving at the speed of light, and the Penrose limit near a null geodesic moving in a direction y along the giant gravitons. Then consider open strings ending on the D-brane, in the Penrose limit, i.e. open string states on the pp-wave, corresponding to open strings moving on the D-brane in this direction y.
Either way, the starting point for all these exercises is finding the Penrose limit near a null geodesic moving in some direction in the background. In this section, we turn our attention to this task and study various Penrose limits of the geometry (2.1). Case by case, we find it convenient to shift the ω term by a constant piece that does not change J , so it does not affect the solution.

Useful null geodesics for Penrose limit
The only thing we need strictly speaking in order to define a Penrose limit is a null geodesic. We will however also consider the concept of a "useful limit", which will mean for us a Penrose limit in an isometry direction. This should correspond in the dual field theory to a spin chain that singles out a large charge J for the corresponding field theory symmetry.
The equation of motion for a null geodesic parametrized by λ, moving in 10D spacetime with coordinates x i , is If we have motion (velocity) in the direction x λ , that is dx i /dλ = δ i λ , we need have no acceleration in the other directions, so Note that we also have dt/dλ = c (constant), but we will deal with static metrics, ∂ t g ij = 0, and also diagonal metrics with g 0i = g 0i = 0. Thus, it is easy to see that the geodesic equation for i = t is satisfied, and moreover j, k = t does not contribute to the equations for i = t.
Moreover, if we consider motion in an isometry direction, i.e. a direction for which ∂ λ g µν = 0, then the condition becomes simply The three internal isometry directions of the GJV metric are σ, ψ, φ, since as we can see, ∂ σ g µν = ∂ φ g µν = ∂ ψ g µν = 0. Thus in our case, the metric is a matrix in the (σ, φ, ψ) (isometries) space, and is diagonal in the (α, λ, θ) (non-isometries) space. Specifically, we have Note, in displaying the above metric, we have allowed for a shift ω → ω − dσ/4, which doesn't change the solution.
While we can consider in principle the Penrose limit around any null geodesic, it is more useful to consider the motion around null geodesics in isometry directions, since that guarantees, as we said, that in the dual field theory we have a spin chain with some large charge J associated with a symmetry direction matching the isometry of the geodesic. As we emphasized, we can consider closed strings for Penrose limits in any of the (σ, φ, ψ) directions, and they would correspond to spin chains with some large charge in the field theory.
But in particular, we will be interested in the Penrose limit for the motion in ψ, since as we said, this is the U (1) isometry corresponding in the field theory to the U (1) R-symmetry. Thus, we will be considering closed strings, and giant gravitons, i.e. D4-branes wrapping the CP 2 and moving at the speed of light, both in the ψ direction. These objects have to be situated at a point in AdS 4 (i.e. we consider the null geodesic fixed at a point in AdS 4 ), usually taken to be the center, ρ = 0. The rest of the conditions on the position of the null geodesic need to be defined by the need to get a nontrivial pp-wave (corresponding to a nontrivial spin chain in field theory) and by the solutions to the geodesic conditions (3.3).
Given the above considerations, the motion of the open strings attached to the giant graviton is described by the Penrose limit of null geodesics around another isometry direction, one that can be considered parallel to the D4-branes, i.e. along the CP 2 . This means either σ or φ, or even σ + φ, or some other combination of them. For both motion in σ and φ, it is natural to consider an expansion around θ = π/2, since in the φ case we want the coefficient sin 2 θ of the free dφ 2 (the one not mixing with dσ) to be nonzero, and more specifically extremum (maximal), and in the σ case, we want σ not to mix with φ, so cos θ = 0. On the other hand, for motion in σ + φ, we want to have this combination in the metric, so we need cos θ = 1, i.e. θ = 0.

Case 1: motion in ψ
We remind the reader that here we consider the shifted ω, i. e. ω → ω − 1/4dσ. Now g ψψ is, as we saw, only a function of α, so the geodesic conditions reduce to The solutions to this equation are α = 0, π/2, π, but in order to have a nontrivial Penrose limit we need to have a nonzero metric g ψψ , which means sin 2 α = 1.
That leaves only α = π/2 as a possibility. As usual, we choose also ρ = 0, meaning that the geodesic is fixed at the center of AdS 4 , and λ = 0, though any λ 0 would do.

Case 2: motion in σ
The geodesic conditions, are automatically satisfied since ψ and φ are isometric directions, and (as well as the similar ones in the AdS directions) are satisfied since ∂ θ g σσ = 0.

Case 3: Motion in φ
In this case, we consider the original unshifted ω (2.5). The geodesic conditions g σσ ∂ σ g φφ = g ψψ ∂ ψ g φφ = 0, (3.11) are automatically satisfied since ψ and σ are isometric directions, and where i are the AdS directions, are satisfied since ∂ i g φφ = 0.
We now see that λ = π/2 solves the second equation. Indeed, since we need sin 2 λ (from the coefficient of the metric in φ direction) to be nonzero, λ = π/2 is the unique valid solution. We also need sin 2 α = 0 for the same reason, which means that the unique valid solution to the last equation is α = π/2. All in all, in this case, we need to expand around the geodesic with λ = π/2, α = π/2, θ = π/2. Also as usual, ρ = 0 (the center of AdS), is chosen by convention (we can always change coordinates in order to put the center where we want).

Useful pp-wave for closed strings: motion in ψ
In this subsection we consider the Penrose limit of the GJV solution near a null geodesic moving on the U (1) isometry coordinate ψ, which is dual to R-symmetry. As highlighted in the previous section (case 1) we should expand around α = π/2, λ = 0 and ρ = 0. Before proceeding, it is worth noting that there are no pp-wave solutions to a massive theory, so in the process of zooming in on the null geodesic, the final solution we encounter is a solution to massless IIA supergravity. Therefore, ensuring that the equations of motion of the theory are satisfied provides an important consistency check that we have performed the limit correctly.
To perform the Penrose limit, we first rescale as usual the coordinates in the vicinity of the null geodesic, consistent with α = π/2, λ = 0, ρ = 0, for the R ≡ e φ 0 4 L → ∞ limit (the near-geodesic limit) 5 Taking the limit R → ∞, the metric reduces to (3.30a) 5 Observe that the limit R → ∞, corresponds to the case where (m, g) → 0, with e φ 0 ∼ g m 5/6 is fixed Changing from spherical (ρ, ϑ, ϕ) to Cartesian coordinates (y 1 , y 2 , y 3 ), and using the Hopf map coordinates (z 1 , In order to write this metric in the standard Brinkmann pp-wave form [51], so that it is quadratic in transverse coordinates, we consider the scaling Finally, we get We can also take the same limit on the remaining fields, with the result, To confirm that there is no mistake, it is prudent to check the geometry is indeed a solution to massless IIA supergravity. For our purposes, we will confine our attention to the Einstein equation, where further details of notation can be found in [52]. The immediate advantage of Brinkmann coordinates is that the only nonzero component of the Ricci tensor is R ++ = − 1 2 ∇ 2 g ++ , where we have introduced the Laplacian on the eight-dimensional space transverse to the null-coordinates (x + , x − ). A quick calculation reveals that R ++ = 5 and this is the only nonzero term on the LHS of equation (3.35). Evaluating the RHS, one confirms the same result, so that the Einstein equation is satisfied.
However, even without checking the Einstein equation, we know the solution is correct. In particular, it can be checked that the above pp-wave solution is the same as the Penrose limit of the AdS 4 × CP 3 spacetime [48,53], which allows us to import the following analysis from the literature [37,41].
The metric, which is warped product of AdS 4 with a squashed S 6 , has isometry SO(2, 3) × SU (3) × U (1), with the U (1) R-symmetry. In the Penrose/large R-charge limit, the U (1) combines with the SO(2) (scaling) part of SO(2, 3), becoming the U (1) ∆+R ≡ U (1) ± of the field theory. The Penrose limit of the gravitational background rearranges and breaks the isometry into Here SO(3) r = SU (2) r rotates the coordinates y 1 , y 2 , y 3 , U (1) u gives translations along u and SU (2) L acts on the complex coordinates w 1 , w 2 . Note that these would be four real coordinates, acted upon by SO(4) = SU (2) L × SU (2) R , were it not for the redefinition (3.32), which breaks SU (2) to its Cartan subalgebra, the action with e +iα and e −iα on the diagonal, which is identified with U (1) ± , since x + takes the role of the α parameter in (3.32).
In this case, we find for the lightcone momenta on the pp wave, in terms of the anomalous dimension ∆ of the field theory and the charge J ψ associated with motion on ψ in the gravitational background, In the field theory, we will identify 2 3 J ψ with J, the (large) charge of operators. In the picture where ∆[φ i ] = 1/2 (as in the classical case), J[φ i ] = 1/2.

Closed string quantization on the pp wave
Using the definitions of [54], the Green-Schwarz action for the type IIA closed string on the pp-wave above is found to be (like in the ABJM case) where we consider the identification X 1 = u, (y 1 , y 2 , y 3 ) ≡ X A = (X 2 , X 3 , X 4 ) and finally (w i ,w i ) ≡ X B = (X 5 , X 6 , X 7 , X 8 ) (see [37,41]). Therefore, the light-cone Hamiltonian for the closed string on the pp-wave is (we could rescale x + by µ as usual, and then H would have a common µ factor to give it dimensions, but we keep it like this for ease of comparison with the field theory) (3.39) If n/(α p + ) 1, we find four modes, corresponding to X 1 = u, (X 2 , X 3 , X 4 ) = (y 1 , y 2 , y 3 ), with energies and four modes, corresponding to (X 5 , X 6 , X 7 , X 8 ), with energies (3.41)

Useful pp-waves for (closed and) open strings on D-branes: motion on σ
In this subsection, we consider the Penrose limit of the GJV solution near a null geodesic moving in the coordinate σ, with α = π/2, λ = π/4, θ = π/2 and ρ = 0 (also φ = 0, ψ = 0), as we discussed for case 2 in the first subsection. As we mentioned, this limit will be more useful for open strings on D-branes in the geometry than for closed strings. The D4-brane giant graviton wraps CP 2 , i.e. coordinates (λ, θ, φ, σ), and moves in the ψ direction, like the closed strings. The open strings must move in one of the isometry directions parallel to the D4-brane, so the σ direction fits the bill.
In order to boost on σ, we consider the transformation σ →σ = √ 3 4 σ and the definitions where, as before, R = e φ 0 4 L. To find the required Penrose limit, we consider the expansion near the null geodesic above, namely Moreover, for a nontrivial Penrose limit in the direction σ, we make use of the fact that there is a freedom in the definition of ω in the metric, so that we consider the modification which obeys dω = dω , as we explained when analyzing case 2 for the Penrose limit. As a result, we can then write η = dψ + ω .
Taking the limit R → ∞, the metric becomes a pp-wave, 46) and the fields supporting the geometry may be expressed as follows: In contrast to the solution presented in the last section, which preserved twenty-four supersymmetries, here it is easy to confirm that only sixteen supersymmetries are preserved. To see this, recall the dilatino variation of type IIA supergravity (see [52] for notation) Plugging in the solution, while ignoring the obvious projection condition that preserves sixteen supersymmetries, i. e. Γ + = 0, we encounter the projection condition: It is easy to convince oneself that this is not a good projection condition and does not permit any supernumeracy Killing spinors, namely those beyond the obvious sixteen.
To tidy up and bring the pp-wave solution to the standard Brinkmann form, we make the coordinate transformation in order to change the g +µ , µ = +, term in the metric, (3.51) Defining complex coordinates we obtain To bring the metric to Brinkmann form (3.31), we consider the coordinate transformations, after which the metric takes the form we want: (3.55) where we have introduced x i , i = 1, 2, 3 to parametrize theρ directions and have employed the redefinitions: v = y 4 , Re(w 1 ) = y 5 , Im(w 1 ) = y 6 , Re(w 2 ) = y 7 , Im(w 2 ) = y 8 . Rewriting the remainder of the solution in terms of Brinkmann coordinates, one finds: where we have employed gauge symmetry to bring B to the above form.
Given the fact that the energy is E = i∂ t , which in the dual field theory corresponds to the conformal dimension ∆, and that the angular momentum for motion in σ is J σ = −i∂ σ , the lightcone momenta on the pp-wave are written in terms of ∆ and J σ as
We expand these coordinates as follows: In addition, we also redefine so that the metric in the pp-wave limit (R = e φ 0 4 L → ∞) becomes, We also perform the same limiting procedure on the rest of the solution: To make sure that everything is correct, one can quickly check that the Einstein equation (3.35) is satisfied. Note that R ++ = 35 24 is the only nonzero component of the Ricci tensor. Having established that we have taken the pp-wave limit correctly, one can bring it to the Brinkmann form by redefining 6 : The end result may be expressed as: where we have dropped tildes.
It is easy to see from supersymmetry analysis, the details of which we omit, that only sixteen supersymmetries are preserved.

Useful pp waves for (closed and) open strings on D-branes:
motion in φ + σ Yet another alternative for open strings on D4-brane giant gravitons is to take the Penrose limit on some combination of σ and φ. We can choose it for simplicity to be σ + φ, as in case 4 of our general analysis.
Then we must expand around the null geodesic with λ = π/4, α = π/2, θ = 0, ρ = 0, and we can choose ψ = 0. Thus we expand the variables as In addition, we redefine to obtain the pp-wave metric, Taking the same limit on the rest of the solution, one finds: where we have used gauge symmetry to drop a total derivative from the B-field. Using R ++ = 35 12 , the only nonzero component of the Ricci tensor, it is an easy exercise to convince oneself that the Einstein equation is satisfied. In fact, it is worth noting that the solution is modulo coordinate redefinitions and irrelevant signs 7 , the same as the pp-wave limit for motion on the σ direction (3.46). To bring it to the same form, one can introduce cartesian coordinates z 1 = z sinφ, z 2 = z cosφ, in addition to shifting x − → x − + 1/(2 √ 6)z 1 z 2 . As a result, the rewriting of the pp-wave in terms of Brinkmann coordinates reduces to the previous analysis and we omit further details.

Open string quantization on the pp-waves
In this subsection we consider open string quantization making use of the pp-wave limits identified in the previous subsections. We will encounter difficulties in solving the entire system, but we will find a common sector that can be solved for all the pp-waves we have identified. As a result, we focus our attention on the pp-wave obtained for motion in the σ direction.
The bosonic sector of type IIA string theory, in the presence of a B-field, is described by the Polyakov action where we have used the conformal gauge √ −hh ab = η ab = diag(−1, 1) and 01 = 1. To avoid confusion, we write the worldsheet coordinates as (σ 0 , σ 1 ).
For the pp-wave corresponding to motion on σ, inserting the pp-wave solution (3.55) and (3.56), and making a rescaling x + → µx + and x − → µ −1 x − , along with the identifications X i = x i , i = 1, 2, 3, Y i = y i , i = 4, 5, 6, 7, 8, the string action on the pp-wave becomes (in the light-cone gauge µ x + = σ 0 ) (3.69) The equations of motion read (3.70b) We are interested in open strings attached to a D4-brane wrapping the R t × CP 2 space spanned by the coordinates (t, λ, θ, φ, σ), which become (x ± , x, y, z) in the pp-wave limit, or after the redefinitions, (x ± , y 7 , y 8 ) and y 5 cos [36,55]. Therefore, we impose Neumann boundary conditions along these directions and Dirichlet boundary conditions in the remaining directions, (3.71) Note that consistency necessarily implies that x ± satisfy Neumann boundary conditions.
The coupled system of Y 4 , Y 5 , Y 6 is difficult to solve, but X i , Y 7 , Y 8 are simple. For them, we find In principle, the remaining equations can be solved numerically, but we postpone this to future work.
In fact, we can check that the part of the string action (3.69) involving X i , Y I is the same for all three pp-wave metrics, namely for motion on φ, on σ, or on φ+σ, and therefore the solutions (3.72) and the eigenenergies (3.73) are the same for all. We will see that a puzzle arises when we try to construct an open string spin chain in the field theory: it has to correspond to one of the pp-waves, and all of them have the same energies (3.73) for the modes (3.72). In spite of this, we cannot get the zeroth order spin chain energies to agree with (3.73).

Spin chains in the field theory IR limit
As we have seen in section 2, in the IR limit of the field theory, if we choose the picture where we use the classical description of the theory, we have states satisfying [φ i , φ j ] = 0, ∀ i, j = 1, 2, 3, and for these states the bosonic interaction Hamiltonian is given by (2.17b), which we repeat here for convenience

Closed string spin chain
The symmetry of the theory is SO(2, 3) conf. ×SU (3)×U (1), and in the field theory Penrose limit, which should be a large R-charge limit, we expect, based on the gravitational Penrose limit on the ψ direction, the U (1) to combine with the SO(2) (scaling) part of the conformal SO(2, 3) to give U (1) ± , and the SU (3) will break to SU (2) L . We expect also an extra U (1) u symmetry.
This breaking coincides with the idea of picking out, as usual, a special complex field charged under the U (1), let us call it Z, among the φ i , i = 1, 2, 3. We call the remaining complex scalars φ m , m = 1, 2. Then the bosonic interaction Hamiltonian in the IR is We want to construct the closed string spin chain, whose vacuum must have charge J, corresponding to momentum p + on the pp-wave. We have to define the charge of Z (the unit of charge), and we define it to be such that (in our picture using classical dimensions) ∆ − J = 0 for Z, i.e. J = 1/2. In (3.37), we saw that 2p − = ∆ − (2/3)J ψ , and we said that we identify ( Then the unique object of ∆ − J = 0 (corresponding to E = p − = 0) and J = 1/2 (corresponding to p + = 1/2) is Z, so the vacuum has to be made from it only. At ∆ − J = 1/2 we have both φ m andφ m , m = 1, 2, which have J = 0. At ∆ − J = 1 we haveZ and D a , a = 1, 2, 3 (covariant derivatives in the field theory direction).
We can use the same vacuum as in the BMN [35] case, since we want a vacuum with J units of p + , i.e.
or more precisely Introducing oscillators on top of them is trickier, since now (in the "classical" picture) [φ i , φ j ] = 0 (but [φ i ,φ j ] = 0). We can imagine introducingφ m as oscillators, since they do not commute with Z, though it is less clear what to do about φ m , since they do.
Another possibility, since now also [φ m ,φ m ] has nonzero commutator with Z, we can put insertions of [φ m ,φ m ] instead. In that case, for instance a nontrivial insertion would be In total, we could insert the 3+4+1=8 oscillators of ∆ − J = 1, But this has the disadvantage that the classical dimension (at λ = g 2 Y M N = 0) would be ∆ − J = 1 for all the oscillators, yet we have seen that half the closed string oscillators in the pp-wave in ψ have energy 1 at n = 0 and half have energy 1/2.
We can easily see that the gravity dual picture is instead matched by the simplest possibility, namely the same one as in the 3+1 dimensional N = 4 SYM case. Namely, the oscillators are φ m ,φ m , m = 1, 2, of ∆ − J = 1/2, corresponding to the 4 modes of energy 1/2 at λ = 0, n = 0 on the pp-wave (modes B), and D a , a = 1, 2, 3 andZ, both of ∆ − J = 1, corresponding to the 4 modes (modes A) of energy 1 at λ = 0, n = 0 on the pp-wave. Defining then a generic insertion as their insertion inside the trace corresponds to a string oscillator as usual, Note then that if Φ "hops" to the right when acting on the state with the Hamiltonian, it acquires a e ip factor (p = 2πn/J), and if it "hops" to the left, it acquires a e −ip factor, etc.
If we would consider commutator insertions, then among the terms in H int , the first and the second give the interaction of [Z,Z] and [φ m ,φ m ], and the third, fourth, fifth and sixth will not contribute in the dilute gas approximation, since at the planar level they would need to have two oscillators next to each other (at the same site) to contribute. As a result, the terms that contribute are However, there are also the mixing terms on the last line (seventh and eight).
This in effect is the same kind of interaction as in N = 4 SYM, once we replace the oscillators φ m by [Z, Z] or [φ m , φ m ], so the result would be the same. However, as we said above, already at tree level we get a different result from the gravity dual, so we need to consider instead just the usual insertions of 3+1 dimensional N = 4 SYM.

Commutator [Z, Z] insertion
To set up the procedure, let us start with the simplest case (though we showed it doesn't match the gravity dual) of commutator insertion. Then the above term in the interaction Hamiltonian is considered as the interaction for the commutator, and we rewrite it as  We write the planar diagrams implied by this interaction in the dilute gas approximation (dual to the pp-wave limit)  Note that there are vertices with two insertions, e.g. Z Φ ΦZ and Φ Z Z Φ , but in the dilute gas approximation we neglect these, since they are subleading.
Then the total factor associated with these planar diagrams is This would be the factor arising from the expansion in λ of the BMN eigenenergies.
It is associated with a term in the effective discretized string Hamiltonian obtained from rewriting the diagrams above in terms of "fields at site j" φ j , as This is just (minus) the N = 4 SYM result.

Insertion ofZ
Now we move to the physical case, of insertion of fundamental fields, and we start with ā Z insertion. In this case, we need to remember that the space of physical states is defined by [φ i , φ j ] = 0, so we can freely commute φ m past Z's, andφ m pastZ. We then have the following diagrams: • The interaction term Tr (ZZZZZZ) gives two diagrams Z ZZ ZZ Z and ZZ Z Z ZZ . Both diagrams are planar, since the vertex is sextic, but again we neglect the second diagram since we are in the dilute gas approximation. The coefficient of the first diagram is −4 and its phase is trivial (=1).
• The interaction term Tr (ZZZ 2 Z 2 ) gives three relevant diagrams The total factor for these diagrams is then total factor = fZ(p) = −4 + 2(1 + e ip + e −ip ) − (e 2ip + e −2ip ) = 8 sin 2 p 2 1 − 2 sin 2 p 2 . (4.14) To find the Hamiltonian for these excitations, we note that, for φ j representing the field at site j, the 5 diagrams give the following terms (where the sum over j is implicit) (4.15) The discretized Hamitonian would be obtained by substituting φ j = (b j + b † j )/ √ 2 and adding a free piece. But for matching we are in any case only concerned with small lattice momentum p. And note that the above interacting Hamiltonian is the discretization of (4.16) So at small p, only the first term, 2φ 2 → 2(φ j+1 − φ j ) 2 , remains, and this is, up to factor of 2, the same Hamiltonian as for N = 4 SYM (therefore the same as in the case of the commutator insertions).

Insertion ofφ m .
We now need to do a similar calculation for theφ m insertion. We first expand the interaction Hamiltonian, the terms with two φ's only (the only ones relevant in the dilute gas approximation) and obtain and we can rewrite this expression as We write separately the contributions of each term to the spin chain Hamiltonian, obtaining 9 diagrams: 1st line: • The terms Tr (φφZZZZ) and Tr (φφZZZZ) don't contribute.
• The term Tr (φφZ 2 Z 2 ) gives the (relevant) diagram φZZ φ Z Z with coefficient +2 and trivial phase.   The Hamiltonian is found in the same way as forZ insertion. The 9 diagrams give the contributions (as before, the sum over j is implicit) which is the discretization for We see that, at small p, we have 5 times the result of theZ insertion.

Insertion of φ m .
We now look at the φ m insertion. In this case, the insertion can propagate throughout the chain with no change. However, for the first nontrivial correction to the energy, planarity (which, if violated, carries a penalty of a 1/N 2 factor) requires that the fields interact only "3 sites down with the corresponding 3 sites up", just like in the previous cases.
We have now in principle the same 9 diagrams as in the case of theφ m insertion, just that now, because we can commute freely φ inside the Z's, they all come from the same interaction. The vertices are all equivalent (under the commutation), and are equivalent to φ mφmZ2 Z 2 . The result is that we have the same phase factors as forφ insertion, but all have the same coefficient, which is now −2/3, namely: with phases e −2ip and e 2ip , respectively.
(4.22) However, exactly like in the BMN case for N = 4 SYM [35], there will be also other Feynman diagrams involving gauge fields and fermions, which come with a trivial phase (the scalars are not "hopping" on the chain, but going straight up, and the gauge fields and fermions are making various connections to the scalar lines), and their result will be such that at p = 0 we should have a total vanishing contribution, since the p = 0 operator is a chiral primary field. The result of this is that we can replace the coefficient of the trivial phase, −(2/3)3, with the one that cancels the rest at p = 0, namely with −(2/3)(−6), so that in the final expression for the total factor we remove the constant −6, and have At small p, we get the same result as for theφ m insertion, except for an extra factor of 2/5.
For the construction of the Hamiltonian, we do the same as before. We obtain from the diagrams above the contribution which is the discretization of Again at small p, we get the same Hamiltonian, except for an extra factor of 2/5.
So in all these cases, except for overall factors, the interacting Hamiltonian at small lattice momentum p is the same as in the N = 4 SYM case, so the calculation of the energy gives the same square root, except for an overall factor of the interaction part.

Eigenenergies and comparison with gravity dual
The factors calculated above must still be multiplied by the same basic scalar diagram. In three dimensions the scalar propagator in position space is P (x, y) = 1/(4π|x − y|). The basic correction, a "two-loop" Feynman diagram, which we consider has one operator O(0) at zero, and its conjugateŌ(x) at x, is integrated over a vertex at y, and has 3 propagators from the vertex to each of the operators, so [P (y, 0)] 3 [P (x, y)] 3 . Since we want to compare with the free case (tree diagram), we divide the result by the tree result [P (x, 0)] 3 , obtaining and we also have an N 2 factor coming from the sum over the 't Hooft double lines, for a total Feynman diagram factor, correcting the tree result, of (F(x) ≡ O(x)Ō(0) ) 8 More generally, in a conformal theory we can use a conformal transformation to put the field theory on R × S d−1 . Therefore, we calculate a general integral as and dΩ d−1 = 2π d/2 /Γ(d/2). For our case of d = n = 3, we have (4.28a) Doing the y integral, we have an IR divergence and a divergence for y = x. We introduce the infrared cut-off Λ, and then also Λ = x − max(y), obtaining where f i (p) are the total factors fZ(p), fφ(p) and f φ (p) calculated in the previous subsections. This is to be compared with the expected form (4.31) to finally write Note that the numerical coefficient multiplying f i (p) is different than in 3+1 dimensional N = 4 SYM, since the basic Feynman diagram is different. We also find the "two-loop" λ 2 factor instead of λ, since now the vertex is sextic.

Commutator insertions.
For completeness, we start by considering the case of [Z, Z] insertions, and then from (4.12) we obtain (since p = 2πn/J and (∆ − J)(tree) = 1) where the last result was for small p (small n).
Since the spin chain Hamiltonian at small p is (up to a numerical factor) always the same as for 3+1 dimensional N = 4 SYM, the full result is the square root that has the above as the first correction, i.e.
Like in the case of the ABJM spin chain, all the more so since we have less than maximal supersymmetry, we expect the coefficient of sin 2 p/2 to have some function of the 't Hooft coupling λ = N/k, i.e. we expect that such that for small λ, f [Z,Z] (λ) 4λ 2 .
For the case of giant magnons, p is not infinitesimal anymore. In this case, we can neglect the 1 in the square root, and get (4.36) As described in [34], where giant magnons were analyzed in the GJV gravitational background, the dual giant magnon energy, given by the string action, is proportional to (since the Polyakov action is essentially the metric in string frame) This means that at large λ, we have Moreover, this result is valid for any type of spin chain insertion, corresponding to any direction for the giant magnon excitation.
On the pp-wave, i.e. in the BMN limit, the scale factor is the same L 2 string , so we should obtain in general at large λ f i (λ) ∝ λ 2/3 . (4.39)

Field insertions
As we said, the physical case seems to be for insertions of the basic fields, rather than the commutators. For each case, we will have a set of different functions where the last two equalities are only valid for small p. But for matching with the pp-wave result, we must only consider small p, so we can neglect the sin 4 p/2 terms in f i (p).
The tree level value (∆ − J) 0 for ∆ − J is, as we already explained, 1 for D a andZ insertions, and 1/2 for φ m andφ m insertions. From matching with the pp-wave results (3.40) and (3.41) for n = 0, we see that D a insertions correspond to X 2 , X 3 , X 4 insertions on the pp-wave,Z insertions to X 1 = u insertions, and φ m ,φ m to X 5 , X 6 , X 7 , X 8 insertions.
Since, as we saw, p + = J/L 2 string , to translate from the pp-wave result we use the map, valid at λ → ∞, (4.42) • ForZ insertions, from fZ(p) in (4.14), we get which from the spin chain Hamiltonian would be • Forφ m insertions, from fφ(p) in (4.19), we get which from the spin chain Hamiltonian would be at small p, and at small λ we have fφ(λ) 40λ 2 . By comparing with the small p result on the pp-wave, eq. (3.41), we see that at large λ, which from the spin chain Hamiltonian would be at small p, and at small λ we have f φ (λ) 16λ 2 . By comparing with the small p result on the pp-wave, eq. (3.41), we see that at large λ, Note that the functions f i (λ) are the same ones for the usual magnons (dual to the pp-wave) as they are for the giant magnons (corresponding to the calculation from [34]) since the scale in both gravity backgrounds is L 2 string , which means we have the map (4.42). In conclusion, we find matching with the pp-wave results, but only by introducing independent functions of coupling f i (λ), one for each field insertion.

Sketch of field theory spin chain for open strings on D-branes
We will now attempt to describe the spin chain for open strings on the giant graviton D4branes, in the same way as it was done in [37] for the ABJM case. We will only sketch the analysis, since we will see that we have an important puzzle, which we could not resolve.
From the point of view of the analysis for closed strings excitation modes, we have the scalars Z,Z, charged under a U (1) symmetry with charge J, and φ m ,φ m , m = 1, 2, which we will split as W, T , forming an SU (2) sector, and their conjugates,W ,T .
A maximal giant graviton D4-brane, wrapping the CP 2 parametrized by (λ, θ, φ, σ), thus with transverse coordinates ρ (AdS radial coordinate) and angles α and ψ, where its motion is on the same direction ψ as for the closed strings, will be described by a determinant operator made up of Z, the complex scalar charged under the rotation on ψ, i.e.
A non-maximal giant graviton will correspond to a sub-determinant operator, and it is more complicated (Schur polynomials in general), so we will stick with the maximum one.
On the other hand, the open string must move in an isometry direction A ∈ CP 2 parallel to the D4-brane giant, which restricts it to be A = σ, φ or a combination thereof (like σ+φ). This corresponds indeed to the directions in which we took the Penrose limits for the open string pp-wave. That means that the direction A is charged under a different U (1) chargē J = J. Since the direction α, rescaled to u, corresponds (as we saw in the last section) to theZ insertion in field theory (it has the same energy vs. ∆ − J), it means that the rotation angle A corresponds to (rotation of) a different φ m ,φ m insertion. Let us define the complex scalar field charged underJ to be W , and define it to have chargeJ = 1/2 (so thatW has chargeJ = −1/2).
Among the modes of the open strings, in the three Penrose limit directions analyzed, as we have explained in section 3.6, we have some modes that we cannot calculate precisely, and five modes that are identical over the three different limits: the modes X i , i = 1, 2, 3, and the modes Y 7 , Y 8 , see (3.72) and (3.73). This means that no matter how we choose the field theory open spin chain, there should be a universality in the result.
But when looking at the modes of the open string on the pp-wave, we see that only the D a modes, corresponding to the X i excitations, with energies ω (i) n , match the p = 0 values for the energy (∆ −J in the field theory), and only if we rescale (reabsorb in the implicit µ scale for the energy) a 1/ √ 2 factor for ω's.
After the rescaling by √ 2, the modes Y 7 , Y 8 (with E = µ/ √ 6 at n = 0) on the ppwave have energies E = µ/ √ 3 at zero momentum, which however disagrees with both ∆ −J = 1/2 of Z,Z, T,T , or the ∆ − J = 1 ofW . It is not clear how we could fix this mismatch.

Conclusions
In this paper we have studied Penrose limits of the GJV duality between the IR fixed point of N = 2 SYM-CS theories in 2+1 dimensions and a warped product geometry of the form AdS 4 × S 6 , where the six-sphere is squashed. On the gravitational side, we have calculated all the nontrivial Penrose limits along isometries of the background.
On the field theory side, after describing the Lagrangian and IR fixed point of the theory, we described a spin chain that corresponds to closed strings in one of the pp-waves, more concretely the Penrose limit along the R-symmetry direction. We obtained matching, only at the expense of introducing independent functions f i (λ) for the various field theory insertions Φ i , and after restricting to small spin chain momentum p, so that sin 2 p/2 1.
This situation is different from either of the more established examples, notably 3+1 dimensional N = 4 SYM (when there are no functions of the coupling), or 2+1 dimensional N = 6 superconformal CS theory (ABJM model), where there is only one function. We attribute this feature to the fact that there is less supersymmetry (N = 2 instead of the maximal N = 8) and more parameters, which makes the GJV duality more interesting. Even more so, since as we see, we can use a combination of the methods used in the N = 4 SYM and ABJM cases to analyze the model. It should be interesting to use methods based on quantum spectral curves to perform an analysis of these functions [56,57].
In the process of completing this work, an unresolved puzzle arose with respect to the open strings on D4-brane giant gravitons. A pp-wave corresponding to such a situation was found for each of the σ, φ, σ + φ directions, but neither of these logical possibilities seem to match the result obtained in the field theory at zero spin chain momentum p. We are unsure how to resolve this but, coupled with the fact that in the closed string case we have matching only for small p, suggests that this less supersymmetric case is more complicated and interesting than the standard N = 4 SYM and ABJM cases.
in T/U-dualities and Generalized Geometries" in Zagreb for providing a stimulating work environment, where the finishing touches to this paper were made.
In this section we review 3D N = 1 superspace. Our motivation to do so stems from the fact that recent treatments in the literature, for example [38,39], have favoured working with components and the superspace conventions have not been comprehensive enough to stand alone. In this section, we will recapitulate some of the earlier work in this direction [58,59].
We adopt the spacetime metric η µν = diag(−1, 1, 1), with gamma matrices, noting that γ µ γ ν = η µν + µνρ γ ρ , with 012 = γ 012 = 1. We next introduce αβ = iσ 2 , αβ = −iσ 2 , α, β = 1, 2, allowing us to raise/lower indices on spinors and construct Lorentz invariants,ψ To construct superfields, we introduce a two-component Majorana spinor comprising Grassmann coordinates θ α , α = 1, 2. With N = 1 supersymmetry, one can construct two different types of multiplets, namely scalar and gauge multiplets. We begin by defining a real scalar multiplet, consisting of two real scalars φ(x), C(x) and a Majorana spinor ψ: We note that there are two real bosonic and two real fermionic degrees of freedom. The generator of the N = 1 supersymmetry transformation Q α is given by, The covariant superderivative is defined as The supersymmetry variations follow from which in terms of the component fields, leads to the variations 9 : From the scalar superfield Φ one can construct a scale invariant action of the form 10 , To see that this is scale invariant, we assign dimensions, Now that we have introduced the scalar multiplet, we can introduce the gauge multiplet. The gauge multiplet is contained in a Majorana spinor superfield Γ α , which consists of two two-component Majorana spinors, χ α , λ α , a real scalar a(x) and a vector potential A µ (x), Once again, we note that one has an equal number of bosonic and fermionic degrees of freedom, i. e. four real degrees. The infinitesimal gauge transformation of the spinor superfield is δΓ α = −iD α Φ, where Φ is a real superfield. In terms of components, one finds δA µ = −∂ µ φ, δλ = 0, δχ = ψ, δa = −2C. Noting that λ α = i 2 iD β D α Γ β | θ=0 is gauge invariant, the natural field strength superfield is, where gauge invariance follows from the identityD β D α D β = 0. The Chern-Simons action is obtained from the action where we have evaluated the action in the supersymmetric gaugeDΓ = 0, which corresponds to setting a = 0, ∂ µ A µ = 0 and λ = γ µ ∂ µ χ. The generalisation to the non-Abelian case is straightforward.
(A.20b) Under these definitions, it's easy to show that the chiral superfield Φ, defined byD a Φ = 0 has the most general expansion Φ(y) = φ(y) + √ 2θψ(y) + θθF (y), that is, In addition, we can define the anti-chiral superfield Φ † ≡Φ, such that D αΦ = 0, then Φ(ȳ) =φ(ȳ) − √ 2θψ(ȳ) −θθF (ȳ), that is The vector field V in the Wess-Zumino gauge is given by and using the identities (A.18), we can easily show that V = V † and Therefore, we have the following D-terms Using these results, the N = 2 Chern-Simons action is ♣ Charged Matter Lagrangian Let us consider, for the sake of generality, a family of chiral superfields, that is Φ i , i = 1, · · · , n. The gauged Lagrangian for charged matter fields is . (A.28) and also Superpotential: The superpotential Lagrangian is (A.31) Consider that the matter fields X are Lie-algebra valued. Therefore, the fields in the gauge multiplet, denoted collectively by G, act in the matter fields X adjointly, for example where the trace is normalized as 2Tr(T a T b ) = δ ab . Integrating out the auxiliary fields, we find Tr ψ i T a φ i ,χ a = 8π k Tr φ i † T a ψ i , (A. 33) so that kTr(Dσ) = −2πTr(φ i † Dφ i ).