The (2, 0) superalgebra, null M-branes and Hitchin’s system

We present an interacting system of equations with sixteen supersymmetries and an SO(2) × SO(6) R-symmetry where the fields depend on two space and one null dimensions that is derived from a representation of the six-dimensional (2, 0) superalgebra. The system can be viewed as two M5-branes compactified on S−1×T2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ {S}_{-}^1\times {\mathbb{T}}^2 $$\end{document} or equivalently as M2-branes on ℝ+×ℝ2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ {\mathbb{R}}_{+}\times {\mathbb{R}}^2 $$\end{document}, where ± refer to null directions. We show that for a particular choice of fields the dynamics can be reduced to motion on the moduli space of solutions to the Hitchin system. We argue that this provides a description of intersecting null M2-branes and is also related by U-duality to a DLCQ description of four-dimensional maximally supersymmetric Yang-Mills.


Introduction
M-theory is generally viewed as a non-perturbative completion of string theory. While string theory is based on a perturbative quantization of strings there is no similar construction in M-theory. Branes of various types are known to play an important role in string theory. These often have a perturbative definition in terms of open strings and have decoupling limits leading to non-gravitating theories in any dimension less than ten. In Mtheory one finds just M2-branes and M5-branes but embedded into an eleven-dimensional spacetime. Each of these admits a decoupling limit leading to interacting quantum field theories in three and six dimensions but there is typically no perturbative description (at least for smooth eleven-dimensional spacetime). These theories are of great interest as they are inherently strongly coupled and understanding them is thought to be a big step in the general understanding of M-theory.
In [1,2] a closed system of equations for various six-dimensional fields was obtained that are invariant under the (2, 0) superalgebra which is associated to the worldvolume of M5branes embedded in an eleven-dimensional spacetime. The fields take values in a 3-algebra, except for the gauge field that takes values in the Lie-algebra (specifically su(2) ⊕ su (2) for the case at hand) that acts on the 3-algebra. The system can be thought of as a set of dynamical equations for the scalars, fermions and self-dual three-form as well as constraints for the additional gauge and vector fields that it contains. In addition the system depends JHEP10(2017)126 on a choice of abelian three-form C µνλ . For C µνλ = 0 it reproduces various descriptions of two M5-branes [1,3,4]. For C µνλ spacelike the constraints reduce it to the equations two M2-branes [2]. The purpose of this paper is to explore the system for a null choice of C µνλ . We will see that this leads to a novel supersymmetric system of equations on R 2 times a null direction R + . Alternatively, via an M-theory version of T-duality, we can think of this system as describing intersecting M2-branes which are tangent to a null direction.
A similar system of equations but defined on R 4 times a null direction R + was obtained in [1] (and is therefore also a solution to the constraints of [2]). These were analysed in [3] where it was shown they reduce to dynamics on instanton moduli space with the null direction playing the role of 'time'. From the origin of these equations in the (2, 0) superalgebra it is clear that the resulting system describes two M5-branes compactified on a null circle with corresponding null momentum given by the instanton number. This is in agreement with the DLCQ prescription of [5,6]. We similarly expect that the system here corresponds to two M5-branes compactified on T 2 and carrying momentum along the null direction. We show that the system reduces to quantum mechanics on Hitchin moduli space and provides a description of intersecting null M2-branes. We note that there is a similar DLCQ description of four-dimensional maximally supersymmetric SU(N ) Yang-Mills with null momentum K which is also based on quantum mechanics on Hitchin moduli space [7,8]. We will argue that this construction is related to our system by U-duality.
Another motivation for our work is to find and study field theories which have symmetry groups corresponding to branes embedded into eleven dimensions. From the field theory point of view an embedding into eleven dimensions, as opposed to just ten, corresponds to enhanced R-symmetries, presumably arising at strong coupling. It is therefore of interest to obtain any such theories and study their interpretation: both as corresponding to objects in M-theory as well as strong coupling limits of field theories.
The rest of this paper is organised as follows. In section two we review the system of [2] and then examine it for the case of a null background 3-form C 3 . In section three we analyse this new system and in particular show how, for a particular choice of fields, it reduces to supersymmetric dynamics on the moduli space of solutions to Hitchin's equations. In section four we provide a physical interpretation of our system in terms of intersecting M2-branes. Section five contains our comments and conclusions on our results. We also provide an appendix with several conventions.

The system
Let us start by reviewing the (2, 0) system of [2] (which itself is a generalization of [1]). The fields Y µ , X i , H µνλ , Ψ all take values in a Lie-3-algebra, that is in a vector space endowed with a totally anti-symmetric product [ , , ] from the vector space to itself. Here µ, ν = 0, 1, 2, 3, 4, 5 and i = 6,7,8,9,10. If we expand all in fields in terms of a basis for the 3-algebra

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where the structure constants of the 3-algebra f ABC D are anti-symmetric in the upper indices. Furthermore the triple product is required to satisfy the fundamental identity which reads 2) or equivalently, the structure constants need to satisfy: We also require the existence of a symmetric inner-product which is invariant under the action of the 3-algebra, which allows the definition of a metric structure In addition there is a gauge field A µ which takes values in linear maps from the 3-algebra to itself and a covariant derivative: Lastly there is an abelian, constant, 3-form C µνλ .

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In addition to these equations of motion one has the constraints: This system is invariant under the supersymmetry transformations (2.10)

A null C and SO(2) × SO(6)
In this paper we wish to analysis this system for the choice where In particular we will see that the solution of the constraints leads to fields that only depend on x + , x 1 , x 2 . Although the system we started with has an SO L (1, 5) × SO R (5) symmetry turning on C +34 breaks the Lorentz group SO L (1, 5) to an SO L (2) that acts as rotations in the (x 1 , x 2 )-plane along with an SO R (2) that acts as rotations in the (x 3 , x 4 )plane and which is now viewed as an R-symmetry. Somewhat surprisingly we find that there is an enhancement of the original SO R (5) R-symmetry to SO R (6) so that the final system has an SO L (2) × SO R (2) × SO R (6) symmetry.

Solving the constraints and equations of motion
Our first task is to solve the constraints. From the last constraint in (2.10) we see that only Y − , Y 3 , Y 4 are non-vanishing. The third and fourth equations in (2.10) can be reduced to algebraic equations if we take ∂ − , ∂ 3 , ∂ 4 to vanish. Thus all fields are functions of x + , x 1 , x 2 . Solving the resulting algebraic equations from the third and fourth equations in (2.10) one finds that (2.14) Next we can use the second equation in (2.10) to determine the components of H µνλ . Using self-duality we find

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To proceed it is useful to introduce the complex coordinates and fields Here, and in what follows, a bar denotes complex conjugation and not the Dirac conjugate. In addition we introduce an SO(6) multiplet of scalar fields X I , I = 5, 6, . . . , 10, defined by We first note that there is one independent component of H µνλ that is not determined from the constraints above and so we define The remaining constraints can now be evaluated to give where the I = 5 component actually arises from the (DH) zz+− equation. The only other new equation that arises from the (DH) µνλ equation comes from the (DH) zz+3 and (DH) zz+4 terms and gives The fermion equations are Here we see that the equations of motion have a natural SO L (2) × SO R (2) × SO R (6) symmetry. In particular the field Y − has enhanced the original SO R (5) to SO R (6).

Supersymmetry
The supersymmetry transformations can also be expressed as The variation of H = H +z3 requires special attention as self-duality implies that H = iH +z4 . Evaluating these gives (2.26)

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Demanding that these are equal gives the condition (2.27) As required this vanishes as a consequence of the fermion equation (2.22). As a result we find It is worth commenting that the identification H +z3 = iH +z4 maps the SO R (2) action as rotation by θ on We also note that a rescaling of l can be absorbed by a rescaling of x + and H. Henceforth we simply take l = 1.

Energy-momentum and superalgebra
The general form for the supercurrent and energy-momentum tensor were given in [2] as: Setting the fermions to zero we find that in the case at hand

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In the system here the role of time is played by x + so we define as well as the topological term Here V 3 is a three-dimensional volume factor that arises from the fact that T µν , as defined above, has dimension six as appropriate for a six-dimensional theory. Given that there is only one length scale in our system it is natural to take V 3 = l 3 . After some calculations one finds that the superalgebra takes the form The central charges are given by where anti-symmetrization on all free I, J, K, L indices is understood.

Reduction to dynamics on moduli space
We now turn to an analysis of the dynamical equations that we found above. We view x + as 'time' and take the Hamiltonian to be −P + . They are a novel system of differential equations for a set of three-algebra valued fields (X I , Z, H, Ψ + , Ψ − ) along with a Lie-algebra valued gauge field (A + , A z , Az) all of which depend on two space and one null directions (z,z, x + ) and are invariant under 16 supersymmetries generated by Q + and Q − .

Abelian case
To gain some insight it is helpful to first solve the abelian case where the triple product vanishes and we set the gauge fields to zero. The equations of motion are simply The solutions to these equations are readily seen to be given by taking Z to be an arbitrary x + dependent holomorphic function of z and X I can be taken to be the real part of an arbitrary x + dependent holomorphic function. For H we find

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where h is a holomorphic function which also has an arbitrary dependence on x + . Looking at the fermions we find where η ± are spinors which satisfyΓz η ± = 0 . (3.4) and which are also holomorphic functions and arbitrary functions of x + . Thus the solution space is a set of holomorphic functions with arbitrary x + -dependence. To recover some physics we note that for generic solutions the energy P + will diverge due to the poles in the holomorphic functions. Thus on physical grounds we should take all holomorphic functions to be constant. In this case P + will still diverge due to the integral over z however we could imagine putting the theory on a torus, reducing the system to a quantum mechanical model. In that case global consistency requires that In this way we see the recover the familiar free-dynamics of Ψ + and Z, although the x + dependence of X I , H and Ψ − remain unconstrained. Looking that the on-shell supersymmetry in this case we see that Even in the non-abelian case one sees that there are no standard kinetic terms for X I , H and Ψ − . Indeed there are no D + derivatives on H or Ψ − and D + only appears linearly on X I and within a triple product. Thus we will interpret X I , H and Ψ − as, possibly x + -dependent, background fields. Given a particular choice of these fields as functions of z and x + the equations of motion then determine the behaviour of Z and Ψ + .

Vacua of the non-Abelian system
Next we look at the form of the supersymmetry algebra. Here one sees that Q − is broken unless However this implies that DZ = 0 and hence F zz (Z) = 0. This effectively reduces the system back to the abelian case. Thus in what follows we assume that Q − is broken and JHEP10(2017)126 set − = 0. We then wish to examine the system where only Q + acts dynamically. The role of Q − can then be thought of as mapping between different backgrounds defined by choices of X I , H and Ψ − . In this paper we will only consider backgrounds which preserve all of the Q + supersymmetries. In particular for a generic + one sees that such backgrounds are of the form Ψ − = 0, H = 0 with D + X I = 0 and [X I , X J , X K ] = 0. Henceforth we will only consider such solutions. In this case the gauge fields are also invariant under Q + . Therefore the dynamical fields are Z and Ψ + . For simplicity we will also set Ψ + = 0 with the understanding that their dynamics can be recovered by applying the Q + supersymmetry to the bosonic equations.
To begin we note that the ground states with P + = 0 correspond to Since the X I are covariantly constant: DX I =DX I = 0 this equation is essentially just that of a Hitchin system [9] but in a three-algebra format as we now detail.
To continue we consider the specific case of a positive-definite 3-algebra with generators T A , A = 1, 2, 3, 4 whose inner-product is T A , T B = δ AB and triple product where k is a constant (usually taken to be integer). The gauge field takes values in so(4) = su(2) ⊕ su(2) and the fields X I and Z are in the vector of SO(4). Solutions for X I that satisfy [X I , X J , X K ] = 0 can be expanded in terms of two constant SO(6) vectors u I , v I : For generic choices of u I and v I the gauge group is completely broken and the vacuum equations have no non-trivial solutions. In particular Z is also restricted to lie in the T 3 and T 4 directions of the 3-algebra and the gauge field is locally flat. As with the abelian case above all the non-zero components of the fields are given by holomorphic functions. However demanding that W and P + be finite requires that these holomorphic functions are constant and space is compactified. However if we take all the X I to be aligned in the 3-algebra, say X I = v I T 4 then there is an unbroken SO(3). If we expand Z = Z A T A then DX I =DX I = 0 implies ∂v I =∂v I = 0 and A z4 b = A za 4 = 0, a, b, = 1, 2, 3. The solutions are then given bȳ

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where a bold face indicates that the components are orthogonal to T 4 in the three-algebra and re-expressed as elements of the SO(3) Lie algebra: is the usual Lie-bracket. 2 In other words bold-faced fields can be viewed as taking values in the unbroken su(2) Lie algebra. This is precisely the Hitchin system for gauge algebra su(2) [9]. The equations of motion allow for Z 4 to be any holomorphic function but demanding that W is finite implies that Z 4 is constant. Thus the vacuum solutions are in a one-to-one correspondence with solutions to the Hitchin system for su (2).
It is useful to recall here that the Hitchin system itself is the dimensional reduction of the four-dimensional self-duality equations to two-dimensions. In particular let us define (3.13) Equation (3.12) can then be written as (recall that z = x 1 + ix 2 ) which are indeed the self-duality conditions and W is the dimensional reduction of instanton number and as such is no longer integer.

Dynamical evolution
Next we allow for x + dependence and allow Z to be dynamical, although we continue to restrict to the Q + invariant sector: D + X I = H = [X I , X J , X K ] = Ψ − = 0. For simplicity we also set Ψ + = 0 with the understanding its dynamics can be restored using the Q + supersymmetry. Keeping X I = v I T 4 and Z 4 = w this requires that ∂ + v I = 0 and A a + 4 = −A 4 + a = 0. It is helpful then to rewrite the equations for the various remaining fields which we now express in their su(2)-valued form.
We start with the observation that (B) b c = ε ab c A a z 4 is not necessarily zero since DX I need not vanish. This implies that the holomorphic constraintDZ = 0 leads to the equations∂ w + 1 2 tr(BZ) = 0 for the A = 4 and A = a components respectively. Thus a non-zero w and B lead to change in the holomorphic constraint on Z.
Next we recall that the Hitchin equation  From the F +z equation we learn that arising from to the A = 4 and A = a components respectively. Lastly we also simply find We see that non-vanishing B and w lead to a z-dependent v I and hence to a modification of Hitchin's system. Our approach here is to treat X I and hence v I as a background field. Elementary manipulations of the first equation in (3.20) show that v I dv I = 1 2 tr(B † B)|v| 2 + |∂v I | 2 + |∂v I | 2 ≥ 0 . To understand these equations we recall that (A, Z) are required to solve the Hitchin equations for all x + . Thus motion can only take place on the moduli space solutions so that under where δA and δZ are fluctuations of the solution to Hitchin's equations: i.e. solutions to the linearised Hitchin equations. In particular these linearised equations are (3.25)

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Using the second equation in (3.23) we see that is the natural metric on the moduli space. As shown by Hitchin [9] this space is hyper-Kahler and therefore, by standard arguments, the dynamics can be extended to include fermions in such a way as to preserve the 8 supersymmetries generated by Q + . Next we can consider the effect of a non-zero w but we still keep v I constant and hence B = 0. We see that for static solutions with ∂ + = A + = 0 we still reduce to Hitchin's system however for A + , ∂ + = 0 there is a modifcation. To see what happens we can differentiate (3.16) with respect to ∂ + to find (recall that D 2 + Z = ∂ 2 + w = 0): This generalises the first equation in (3.25) and the rest of the analysis continues as before.
One sees that the analysis in (3.26) still goes through one still finds that (3.23) imply the first equation in (3.25). However (3.31) is now modified tō

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The rest of the equations remain unchanged. In particular the Hamiltonian is the same except for an additional term in P + : This will diverge unless ∂ + w = 0 as w is holomorphic (although it would be finite for constant w if we are on a compact Riemann surface). Lastly we can quantize the system in a natural way by considering wavefunctions ψ(ξ m ) and replacing Thus the dynamics reduces to quantum mechanics on Hitchin moduli space.

Physical interpretation
So far in this paper we have solved the constraints of the (2, 0) superalgebra of [2] for a particular choice of three-form C = l 3 dx 3 ∧dx 4 ∧dx + . We showed that the resulting system of equations had a vacuum configurations consisting of solutions to the Hitchin system on R 2 . We also saw that the dynamical evolution consisted of motion on the moduli space H K (su(2), R 2 ) of such solutions. Here H n (g, Σ) denotes the moduli space of the charge n Hitchin system with gauge algebra g on a Riemann surface Σ. Therefore it is of interest to see how our construction fits in with other known descriptions of M-branes.
To begin with we recall that to solve the constraints of the original (2, 0) algebra we had to dimensionally reduce the full six-dimensional system on x 3 , x 4 and x − . However it is clear from the subsequent analysis that the resulting system still carries information about the momentum around x − in the form of the topological term W ∼ T −− . Thus we should view the system as two M5-branes compactified on T 2 × S 1 − but with a fixed null momentum P − ∼ W.
We can view a null compactification as a limit of a boosted spacelike compactification where x 5 is taken to be compact with a radius that vanishes so that in the limit of a null boost the radius R − remains finite. Therefore let us review the case where C = l 3 dx 3 ∧dx 4 ∧dx 5 is spacelike and the constraints imply that the fields have no dependence on x 3 , x 4 , x 5 . It was shown in [2] that the (2, 0) superalgebra reduces to the description of two M2-branes with a transverse R 8 . From a brane perspective we can think of this as a toroidal compactification on x 3 , x 4 , x 5 , sending all the radii to zero, accompanied by a U-duality transformation which decompactifies the dual torus. This can be thought of as an M-theory version of T-duality that takes N M5-branes wrapped on T 3 to N M2-branes which are transverse to a dualT 3 . 4 In particular the U-duality we require consists of reducing to string theory on x 5 , leading to N D4-branes wrapped on a T 2 with a coupling g 2 Y M ∼ R 5 , and then performing T-dualities along x 3 and x 4 to find N D2-branes with a transversê If we now shrink the original radii to zero we obtain the strong coupling limit of N D2-branes in a transverse R 7 or equivalently N M2-branes in a transverse R 8 .
Let us repeat these steps with K units of momentum along x 5 . In addition to the N D4-branes we also find K D0-branes. After T-duality these become K D2-branes along x 3 , x 4 . Taking all the radii to zero leads to N M2-branes along x 0 , x 1 , x 2 and K M2-branes along x 0 , x 3 , x 4 . The Hitchin system can then be thought of as the BPS condition for K M2branes intersecting the original N M2-branes, generalising the familiar abelian holomorphic condition∂Z = 0 for intersecting branes. We also see that there will be an SO L (2) × SO R (2) × SO R (6) symmetry from rotations in the (x 1 , x 2 ), (x 3 , x 4 ) and (x 5 , . . . , x 10 ) planes respectively.
Lastly we need to perform the light-like boost along x 5 which is transverse to all the M2-branes. In terms of static gauge this corresponds to replacing X 5 with −vx 0 + X 5 and taking the limit v → 1. For v = 0 this will break the SO R (6) symmetry of the total transverse space to SO (5). However one can see that the breaking only occurs through the time derivative kinetic terms. The spatial gradient terms will remain invariant under SO R (6). The interaction terms also remain invariant since X 5 → −vx 0 + X 5 is a shift by the centre of mass degree of freedom which is non-interacting. 5 If we take the limit v → 1 then the M2-brane tension vanishes, the kinetic terms diverge and we are forced to set them to zero. Thus the SO R (6) symmetry is restored. In addition we can allow the moduli to evolve such that ∂ 0 ξ m ∼ O( √ 1 − v 2 ). In this case the SO R (6) symmetry remains unbroken as these moduli are invariant under rotations of the total transverse space. In the limit that v → 1 the Manton approximation of slow motion on the moduli space of solutions becomes exact and the dynamics reduces exactly to motion on H K (su(2), R 2 ).
This agrees with the results that we have found in the previous section. Stated somewhat differently boosting the intersecting M2-branes leads to 'fast' modes corresponding

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Lastly let us examine the formula for W in the case that we considered in section 3.3 and propose an interpretation for it as the M5-brane momentum P − . It is known that there are no finite action regular solutions to the Hitchin system on R 2 [11] (more recently see [12]) but here we will make a proposal on how to interpret certain multivalued solutions. Restoring the factor of l, identifying A, B = − 1 2 tr(AB) (valid in the case considered in section 3.3) and replacing the integral over x 3 , x 4 , x − by the volume factor V 3 = (2π) 3 R 3 R 4 R − that we would get by taking x 3 , x 4 , x − to be periodic we have For a smooth solution the integral is only over the sphere at infinity. Let us assume that for large z we can treat Z as abelian and ignore A (which can either be subleading or simply commuting with Z). Then up to a gauge transformation we can expand where J 3 is a real anti-hermitian generator of so(3) normalised to tr(J 2 3 ) = −2 and the ellipsis denotes subleading terms. We have assumed this asymptotic form so that W = 0. Even so the expression for W is problematic as there is a divergence: However if we cut-off the divergent terms at some large by finite r = |z| they become where we have introduced a branch cut for ln z that runs along the negative real axis and written w = ln r + iθ. Therefore we find Next we observe that Z is not single valued: under a rotation z → e 2πi z we see that Z ∼ = Z+2πaJ 3 . We recall that Z = Y 4 +iY 3 where Y 4 and Y 3 are real anti-symmetric matrices. These have imaginary eigenvalues y 4 and y 3 respectively which, after multiplication by i, can be thought of as positions of the two M5-branes along x 4 , x 3 directions. The above identification then implies that y 4 ∼ = y 4 + 2πRea and y 3 ∼ = y 3 + 2πIma. We learn from this that Y 3 and Y 4 must be treated as periodic and hence we identify a = R 4 + iR 3 .

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This means that the divergent term only depends on R 3 , R 4 , R − . Unfortunately we do not have a physical interpretation for this divergence, it would be interesting to find one. However in this discussion we only want to consider solutions that correspond to fixed radii and so we will simply ignore the divergence and consider instead Let us write C = cJ 3 + . . . where the ellipsis denotes terms that are orthogonal to J 3 . Thus The multivalued nature of Z also means that in the space of solutions, those which differ by c → c + 2πa must be identified with each other. Therefore if we write c = 2πR 4 n 4 + 2πiR 3 n 3 , (4.8) then solutions that differ by (n 3 , n 4 ) → (n 3 + 1, n 4 + 1) are identified with each other. As a result we have This suggests that we should identify l 3 = V 3 = (2π) 3 R 3 R 4 R − and so recover the KK spectrum of a null compactification on x − , provided that n 4 − n 3 is an integer. Putting this another way: in order to arrive at the interpretation of our model as describing a null compactification M5-branes we should assume (Y 3 , Y 4 ) are periodic and impose on our Hitchin system the boundary condition Z ∼ −i(R 4 + iR 3 )J 3 lnz + 2π(R 4 n 4 + iR 3 n 3 )J 3 where n 4 − n 3 is an integer. Lastly we mention that, according to the previous discussion, we are ultimately required to let R 3 , R 4 , R 5 → 0. However when viewed as the limit of a null boost, the spacelike radius is sent to zero in such that a way that R − is fixed. In this case W finite remains finite.

Conclusion
In this paper we presented a solution to the constraints of the (2, 0) system derived in [2]. The result was a system of equations for 3-algebra valued fields Z, H, X I , Ψ ± , along with an associated gauge field one-form A, that are defined on a plane R 2 times a null direction R + which we used as 'time'. We saw that for choices of the fields X I , H, Ψ − that preserve the Q + supersymmetries the system reduced to supersymmetric dynamics (with supersymmetry generator Q + ) on the moduli space of an SO(3) Hitchin system. We also gave a physical interpretation of the resulting system as a re-formulation of the M5-brane on T 2 × S 1 − as intersecting null M2-branes or alternatively a DLCQ of four-dimensional maximally supersymmetric Yang-Mills.

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The original Hitchin system arises in our system for one particular choice of background. In addition our equations admit generalizations such as a non-zero Z 4 and nonconstant X I . It would be interesting to examine these backgrounds and their associated dynamics. It is also possible to include impurities giving by sources in the Hitchin equations as done in [7,8]. We also expect that our results can be naturally extended to a Lorentzian 3-algebra and hence to an arbitrary gauge group. We also note that Hitchin's system has also appeared before in conjunction with class-S theories derived from the M5-brane [13][14][15][16][17].
Lastly we note that the Hitchin system is generally thought of as applying to a Riemann surface Σ of genus g. However here we have taken the coordinates (z,z) to be those of the flat plane, or possibly a torus, which admit covariantly constant spinors. Due to the SO R (2) symmetry we may twist our theory by taking Killing spinors of the diagonal group of SO L (2)×SO R (2). Alternatively we could break the transverse SO(5) → SO(3)×SO(2) and use the later to twist the theory. Thus we expect to be able to extend our supersymmetric system to a generic Riemann surface and possibly make contact with the class-S theory literature (or at least toroidal compactifications of them). In doing so we should also allow for singularities at marked points on the Riemann surface.

A Conventions
In the text we introduced the coordinates In these coordinates we find For spinors we find it useful to introduce the following conventions: