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Supersymmetry algebra and BPS states of super Yang-Mills theories on noncommutative tori PDF

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Supersymmetry algebra and BPS states of super Yang-Mills theories on 9 noncommutative tori 9 9 1 Anatoly Konechny and Albert Schwarz n a J Department of Mathematics, University of California 8 Davis, CA 95616 USA 1 [email protected], [email protected] 1 v January 15, 1999 7 7 0 Abstract 1 0 Weconsider 10-dimensional super Yang-Mills theory with topological 9 terms compactified on a noncommutative torus. We calculate supersym- 9 metry algebra and derive BPS energy spectra from it. The cases of d- / h dimensionaltoriwithd=2,3,4areconsideredinfulldetail. SO(d,d,Z)- t invarianceoftheBPSspectrumandrelationofnewresultstotheprevious - p work in this direction are discussed. e h : 1 Introduction v i X In this paper we consider supersymmetric gauge theories on non- r a commutative tori. It was shown in [3] that such gauge theories can beobtainedascompactifications ofM(atrix) theory. Moreprecisely we can consider compactifications of BFSS Matrix model ([1]) on a noncommutative d-dimensional torus T . Another way to look at θ this model is by considering first a compactification of IKKT model [2] (as it was suggested in [3]) on a (1 + d)-dimensional torus of the form T = S1 ×T and then performing a Wick rotation of that θ theory with the S1 factor corresponding to the time direction. For the case of commutative torus our calculations agree with well known results (see for example [11]). They agree also with calculations performed in [10] in the context of Born-Infeld theory. 1 Partial answer to the problem we consider is contained also in [7], [8]. The terms that were taken into account in these papers agree with our results. Thepaperisorganizedasfollows. Insection2wecalculatesuper- symmetry algebra of the model and derive the expression for BPS energy spectrum out of it. In section 3 we calculate BPS spectra for d = 2,3,4explicitly in terms of topologicalnumbers and eigenvalues of the total momentum and the zero mode of electric field. In sec- tion 4 we discuss the invariance of the BPS spectra with respect to SO(d,d|Z) transformations. Finally, we discuss the case of modules admitting a constant curvature connection. We show that for this case our new results can be reproduced by the method used in our previous paper [9] for the analysis of modules admitting constant curvature connection over two-dimensional tori. 2 Supersymmetry algebra and BPS spectrum Let T be a d-dimensional noncommutative torus specified by an θ antisymmetric d×d matrix θ. Such a torus can be defined by means of generators U ,...,U satisfying 1 d U U = e2πiθkjU U . k j j k Let us consider derivations δ of T determined by the following i θ relations δ U = 2πiδ U (1) k j kj j where δ is the Kronecker symbol. These derivations span an kj abelian Lie algebra denoted by L . θ Consider an abelian 10-dimensional Lie algebra L that acts on T θ by means of derivations belonging to L . This means that for every θ X ∈ L we have an operator δ ∈ L obeying δ (ab) = δ (a)b + X θ X X aδ (b) for any a,b ∈ T. Then a connection ∇ on E can be defined X X as a set of linear operators ∇ : E → E, X ∈ L satisfying the X Leibnitz rule: ∇ (ae) = a∇ e+(δ a)e (2) X X X for any a ∈ T, e ∈ E. (We assume that δ and ∇ depend linearly X X on X.) We also suppose that L is equipped with a Minkowski signa- 2 ture metric. These data are sufficient to define an action functional of the M(atrix) theory (BFSS model) compactified on T . θ Letusadopt thefollowing conventions aboutindices. Thecapital LatinindicesI,J,...runfrom0to9,Greekindices µ,ν,...runfrom 0 to d, the small Latin indices i,j,... take values from 1 to d, and the tilted small Latin indices˜ı,˜,... take values from d+1 to 9. We assume that one can fix a basis X of the Lie algebra L such that I δ = δ , δ = 0, and the metric tensor g in this basis satisfies Xi i ˜ı IJ g = −R2, g = 0 if I 6= 0, g = 0, g = δ . The conditions on 00 0 I0 i˜ ˜ı,˜ ˜ı,˜ g mean that it can be written as the following block matrix IJ −R2 0 0 ... 0 0 0 (g ) ... 0 0  ij  g = 0 ... 1 ... 0 (3)  0 ... ... ... 0       0 0 ... ... 1      where g stands for a d × d matrix that defines a metric on the ij spatial torus. The Minkowski actionfunctional ofM(atrix) theory compactified on a noncommutative torus T can be written as θ −V S = Tr(F +φ 1)(FIJ +φIJ1)+ 4g2 IJ IJ YM iV + Trψ¯ΓI[∇ ,ψ] (4) 2g2 I YM where ∇ is a connection on a T -module E, ψ is a ten-dimensional I θ Majorana-Weyl spinor taking values in the algebra End E of en- Tθ domorphisms of E, φ is an antisymmetric tensor with the only IJ non-vanishing components φ , and Γ are gamma-matrices satisfy- ij I ing {Γ ,Γ } = −2g . It follows from our conventions on δ that I J IJ XI ∇ = X where X are endomorphisms of E (scalar fields). ˜ı ˜ı ˜ı In [9] we discussed the quantization of Yang-Mills theory on a noncommutative torus in the ∇ = 0 gauge. Those considerations 0 can be easily generalized to the supersymmetric case at hand. Let us briefly describe the quantization procedure. The Minkowski ac- tion functional (4) is defined on the configuration space ConnE × (ΠEnd E)16 where ConnE denotes the space of connections on E, Tθ 3 Π denotes the parity reversion operator. To describe the Hamil- tonian formulation we first restrict ourselves to the space M = Conn′E×(End E)9×(ΠEnd E)16 where Conn′E stands for the Tθ Tθ space of connections satisfying ∇ = 0, the second factor corre- 0 sponds to a cotangent space to Conn′E. We denote coordinates on that cotangent space by PI. Let N ⊂ M be a subspace where the Gaussian constraint [∇ ,Pi] = 0 is satisfied. Then the phase space i of the theory is the quotient P = N/G where G is the group of spatial gauge transformations. The presymplectic form (i.e. a degenerate closed 2-form) ω on M is defined as V ω = TrδPI ∧δ∇ −i Trδψ¯Γ0 ∧δψ. (5) I 2g2 YM It descends to a symplectic form on the phase space P which deter- mines Poisson brackets {.,.} . PB The Hamiltonian corresponding to (4) reads g2 R2 H = Tr YM 0PIg PJ + IJ 2V V +Tr (F +φ ·1)gIKgJL(F +φ ·1)+ 4g2 IJ IJ KL KL YM +fermionic term. (6) The action (4) is invariant under the following supersymmetry transformations i δ ∇ = ǫ¯Γ ψ ǫ I I 2 1 δ ψ = − F ΓIJǫ (7) ǫ IJ 4 ˜ ˜ δ ψ = ǫ, δ ∇ = 0 (8) ǫ ǫ I The corresponding supercharges are given by expressions iR iVR Q = 0TrPIψtΓ Γ + 0TrF ψtΓIJ , (9) 2 0 I 4g2 IJ YM iVR Q˜ = − 0Trψ. (10) g2 YM 4 (Supersymmetrytransformationsareoddvectorfieldspreserving the symplectic form and therefore are generated by odd functions on the phase space - supercharges.) As one can readily calculate using (7) and (9), (10) the super- symmetry algebra has the form 1 R V i{Q ,Q } = (H −Φ)+ 0γIP − γ[ijkl]C α β PB 2 2 I 16g2 ijkl YM −R V i{Q˜ ,Q } = 0γ pI + γijC α β PB 2 I 4g2 ij YM V i{Q˜ ,Q˜ } = dimE (11) α β PB g2 YM where H is the Hamiltonian (6), Φ = V Tr(φ φij1 + 2F φij), 4g2 ij ij YM pI = TrPI, P = TrF PJ + fermionic term, C = TrF , C = I IJ ij ij ijkl TrF F . In (11) we use the Euclidean nine-dimensional gamma- ij kl matrices γI = R Γ0ΓI satisfying {γI,γJ} = 2gIJ. Note that in (11) 0 we assume that the index I does not take the zero value. When calculating Poisson brackets (11) it is convenient to use the identity {A,B} = 1(a(B) − b(A)) where a, b denote the Hamiltonian PB 2 vector fields corresponding to functions A and B respectively. After quantization the supersymmetry algebra (11) preserves its form (one only needs to drop factors of i on the LHS’s), provided Q , Q˜ , H, P , and pI are considered as self-adjoint operators in α α I a Hilbert space. The quantities C , C , Φ, dimE are central ij ijkl charges. As usual we define BPS states as states annihilated by a part of supersymmetry operators. The energy H eigenvalues of BPS states can be expressed via values of central charges and eigenvalues of operators P , pI (the operators H, P , and pI all commute with I I eachother). The energyofa1/4-BPSstateonad-dimensionaltorus for d ≤ 4 is given by the formula R2g2 E = 0 YM pIg pJ + IJ 2VdimE V + (C +dimEφ )(Cij +dimEφij)+ 4g2 dimE ij ij YM +R kvk2 +P2 +(π/g )4(C )2. (12) 0 ˜ı YM 2 q 5 where kvk2 = v gijv stands forthe normsquared of ad-dimensional i j vector v = (P −(dimE)−1C pj), and i ij 1 C = ǫijkl(C −(dimE)−1C C ). 2 8π2 ijkl ij kl In formula (12) we use the same notations P , pI for the eigenvalues I of the corresponding operators. Note that when the term with the square root vanishes we get a 1/2-BPS state. Here we would like to make few remarks on how to obtain formula (12). First one notices that commutators of supercharges (11) form a block matrix M . αβ The BPS condition means that this matrix has a zero eigenvector. As the block {Q˜ ,Q˜ } is non-degenerate one can reformulate the α β BPS condition as the degeneracy condition on some square matrix of dimension twice smaller than that of M . At that point one αβ can apply the standard technique of finding zero eigenvalues of ma- trices expressed in terms of Gamma matrices (for example see [11] Appendix B). Note that operators P , p˜ have a continuum spectrum. Every- ˜ı where below we restrict ourselves to the zero eigenvalue subspace for these operators. Moreover, we will not consider any effects of scalar fields on the spectrum. Below P denotes the operator TrF Pj. i ij The phase space P of the theory at hand is not simply connected. It is well known that in such a case there is some freedom in quan- tization. Namely, in the framework of geometric quantization (see [12] or Appendix A of paper [9] for details) we can assign to every function F on a phase space an operator Fˇ defined by the formula ∂F Fˇφ = Fφ+ωij ∇ φ (13) ∂xj i where ∇ φ = h¯∂ +α is a covariant derivative with respect to U(1)- i i i gauge field having the curvature ω . Here ω is a matrix of sym- ij ij plectic form ω and ωij is the inverse matrix. The operator Fˇ acts on the space of sections of a line bundle over the phase space. The transition from F to Fˇ is called prequantization. It satisfies [Fˇ,Gˇ] = ih¯({F,G})∨ where {F,G} = ∂F ωij ∂G is the Poisson bracket. Notice that re- ∂xi ∂xj 6 placing α with α+δα we change Fˇ in the following way Fˇ = Fˇ +δα(ξ ) = Fˇ +δα ξi (14) old F old i F where ξ stands for the Hamiltonian vector field corresponding to F the function F. To define a quantization we should introduce the so called polarization, i.e. exclude half of the variables. Then for every function F on the phase space we obtain a quantum operator Fˆ. If the gauge field in (13) is replaced by a gauge equivalent field we obtain an equivalent quantization procedure. However, in the case when the phase space is not simply connected the gauge class of ∇ in (13) is not specified uniquely. The simplest choice of the i 1-form α in the system we consider is V α = TrPIδ∇ −i Trψ¯Γ0δψ. (15) I 2g2 YM But we can also add to this α any closed 1-form δα, for example δα = λiTrδ∇ +λijkTrδ∇ ·F (16) i i jk where λijk is an antisymmetric 3-tensor and λi is a 1-tensor. One can check that for d ≤ 4 we obtain all gauge classes by adding (16) to (15) (for d > 4 one should include additional terms labeled by antisymmetric tensors of odd rank ≥ 5). In the Lagrangian for- malism one can include topological terms into the action functional. The addition of all topological terms to the Lagrangian corresponds to the consideration of all possible ways of (pre)quantization in the Hamiltonianformalism. The topologicalterms canbeinterpreted as Ramond-Ramond backgrounds from the string theory point of view (see [10], [8] for more details). The additional terms in the action can be expressed in terms of the Chern character. In particular, the consideration of the form α+δα given by (15), (16) corresponds to adding the following terms to the action S = λiTrF +λijkTrF F . (17) top 0i 0i jk Let us make one general remark here. Assume that a first order linear differential operator L defined by L F = {A,G} obeys A A PB e2πLA = 1 (in other words the Hamiltonian vector field correspond- ing to A generates the group U(1) = R/Z). Then it is easy to check 7 that e2πAˇFˇe−2πAˇ = Fˇ (18) for any function F on the phase space. It follows from (18) that after quantization we should expect e2πiAˆ = const. We see that the eigenvalues of Aˆ are quantized; they have the form m+µ where m ∈ Z and µ is a fixed constant. Now let us discuss the spectrum of the operators Pˆ , pˆi. Our i considerations will be along the line proposed in [10]. Consider a Hamiltonian vector field ξ corresponding to the gauge invariant P i momentum functional P = TrF Pj. The variation of ∇ under i ij j the action of ξ is equal to F . Let us fix a connection ∇0 on the Pi ij i module E. Then anarbitrary connection has the form∇ = ∇0+X i i i where X ∈ End E. Hence, we have i Tθ ξ (∇ ) = F = −[∇ ,X ]+[∇0,∇ ]. (19) Pi j ij j i i j Here the first term corresponds to infinitesimal gauge transforma- tion. Therefore, up to a gauge transformation, P generates a vector i field acting as δ∇ = [∇0,∇ ]. Now one can check using (1), (2) and j i j the identity eδj = 1 that the operator exp(∇0) is an endomorphism, j i.e. exp(∇0)U exp(−∇0) = U j i j i and since it is unitary it represents a global gauge transformation. This means that on the phase space of our theory (after taking a quotient with respect to the gauge group) the identity exp(L ) = 1 P j is satisfied. Here L stands for the differential operator correspond- P j ing to P . As we already mentioned this identity leads to a quan- j tization of Pˆ eigenvalues. Namely, for some fixed constant µ the j j eigenvalues of Pˆ have the form j P = 2π(µ +m ) (20) j j j where m is an integer. The quantization condition (20) is valid for j every choice of quantization procedure (for every α+δα). However, the constants µ depend on this choice. Using the freedom that we j 8 have in the quantization we can take µ = 0 when δα = 0. In the j case of non-vanishing α we obtain using (14) and (19) P = 2πm +C λk +C λjkl. (21) j j jk ijkl Quantization of the electric field zero mode TrPi comes from pe- riodicity conditions on the space Conn′E/G. It was first noted in [10] one can consider the operator U exp(−θjk∇ ) that commutes j k with all U and thus is an endomorphism. Being unitary this op- i erator determines a gauge transformation. As one can easily check this gauge transformation can be equivalently written as an action of the operator δ exp((2πδ −θjlF ) ) (22) jk lk δ∇ k on the space Conn′E. Therefore, on the space Conn′E/G this oper- ator descends to the identity. The Hamiltonian vector field defined bytheexponentialof(22)correspondstothefunctional2πpk−θkiP . i Hence, asweexplainedabovethequantumoperatorpˆk−(2π)−1θkiPˆ i has eigenvalues of the form ni + νi where ni ∈ Z and νi is a fixed number. Proceeding as above we obtain the following quantization law for eigenvalues of TrPˆi pi = ni +θijm +λidimE +λijkC (23) j jk where ni is an integer and m is the integer specifying the eigenvalue j of total momentum operator (21). 3 Energies of BPS states for d = 2,3,4 Now we are ready to write explicit answers for d = 2,3,4. For d = 2 the Chern character can be written as ch(E) = (p−qθ)+qα1α2 where p and q are integers such that p − qθ > 0. Hence dimE = p−qθ, C = πǫ q, C = 0 and we get the following answer for the ij ij 2 energies of BPS states R2g2 E = 0 YM (ni +θikm +λidimE)g · k ij 2VdimE 9 ·(nj +θjlm +λjdimE)+ l R2 2πR + 0 (πq+φdimE)2 + 0 kvk (24) 2Vg2 dimE dimE YM where is a two-dimensional vector v = (m p−qǫ nj). i ij For a three-dimensional torus the Chern character has the form 1 1 ch(E) = p+ trθq + q αiαj ij 2 2 where p is an integer and q is an antisymmetric matrix with integral entries. Substituting the expressions dimE = p+ 1trθq, C = πq , 2 ij ij C = 0 into the main formula (12) and using (23), (21) we obtain 2 R2g2 E = 0 YM (ni +θikm +λidimE +πλiklq )g · k kl ij 2VdimE ·(nj +θjrm +λjdimE +πλjrsq )+ r rs V + (πq +dimEφ )gikgjl(πq +dimEφ )+ 4g2 dimE ij ij kl kl YM πR + 0 kvk (25) dimE where v = (m dimE −q (nj +θjkm )). i ij k Finally let us consider the case d = 4. The Chern character now reads as 1 1 ch(E) = p+ trθq +sθ+ (q +∗θs) αiαj +sα1α2α3α4 ij 2 2 where p and s are integers, q is an antisymmetric 4×4 matrix with ij integral entries, (∗θ) = 1ǫ θkl, and θ = 1θijǫ θkl = detθ ij 2 ijkl 8 ijkl ij stands for the Pfaffian of θ. From this expression for chq(E) we obtain 1 dimE = p+ trθq +sθ, C = π(q+∗θs) ij ij 2 C = π2ǫ s, C = (dimE)−1(ps−q). [ijkl] ijkl 2 Substituting the above expressions into (12) we obtain the following answer for the BPS spectrum R2g2 dimE E = 0 YM (ni +λidimE +πλikl(q +∗θs) +θikm )g · kl k ij 2V 10

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