A Generalization of Sachdev-Ye-Kitaev

David J. Gross, Vladimir Rosenhaus

Introduction

The Sachdev-Ye model , as recently revived and simplified by Kitaev , possesses, for large NN, three remarkable properties: conformal invariance in the infrared, solvability, and maximal chaos. While there are models that contain some of these properties, SYK is the first to have all three, as was recognized by Kitaev in a series of incredibly insightful seminars .

Broadly speaking, until recently two classes of large NN theories have been studied: matrix models and vector models, in which the dynamical variables transform in the adjoint or fundamental representation of a local or global SU(N)SU(N) or O(N)O(N) symmetry group, respectively. Matrix models are closely related to string theories , with the most concrete realization being the duality between supersymmetric gauge theories and string theory in Anti-de Sitter space . N=4\mathcal{N}=4 super Yang-Mills is conformally invariant, and at large ’t Hooft coupling the bulk gravity has black holes, so it should be maximally chaotic. However, it is not easily solvable. Vector models also have a long history and recently have been shown to be dual to interesting gravity theories. The critical O(N)O(N) vector model is conformally invariant and solvable, and the bulk dual is higher spin Vasiliev theory . However, it is integrable for large N{N}, so it is not likely to be chaotic. Roughly speaking, matrix models are too difficult to be explicitly solvable, while vector models are too simple to have the same rich properties. One would like a model that lies in between: one that is sufficiently complicated to be chaotic, while still simple enough to allow for direct analytic calculations for strong coupling. SYK is such a model.

At large NN, the dominant Feynman diagrams for matrix models are planar diagrams, whereas the dominant diagrams for vector models are bubble diagrams. The SYK model is dominated by a new class of Feynman diagrams, which have been referred to as sunset, or watermelon, diagrams. The SYK model may be just one example out of a much broader and new class of models. Past studies of large NN models have been extremely fruitful for understanding both quantum field theories and string theories. One may hope that the study of SYK-like models will also prove productive.

SYK is a quantum mechanics model, living in 0+10+1 dimensions. While two-dimensional CFTs have been extensively studied and categorized, one dimensional CFTs have not. In fact, it has been argued that 0+10+1 dimensional CFTs with nontrivial dynamics do not actually exist . SYK confirms this: the four-point function breaks the SL(2,R)SL(2,R) conformal invariance , consistent with holographic studies of AdS2 . It appears that in one dimension a theory can at best only be “nearly” conformally invariant. In SYK the breaking of conformal invariance, to leading order in 1/N1/N, is confined to a single dimension-two operator appearing in the OPE, so the power of conformal invariance is still largely applicable.

The SYK model consists of N≫1N\gg 1 Majorana fermions χi\chi_{i}, with a qq-body Hamiltonian with quenched disorder,

The model has qualitatively similar properties for any choice of even q≥4q\geq 4. The couplings Ji1,…,iqJ_{i_{1},\ldots,i_{q}} are independently chosen from a Gaussian, O(N)O(N) invariant, distribution with zero mean and a variance proportional to J2N1−qJ^{2}N^{1-q}. When evaluating observables, say correlation functions, a disorder average is performed at the end of the calculation. For the purposes of correlation functions, at large NN, the model is self-averaging for q>2q>2: randomly chosen, but fixed, Ji1,…,iqJ_{i_{1},\ldots,i_{q}} give the same results as disorder averaged Ji1,…,iqJ_{i_{1},\ldots,i_{q}}. One can alternatively think of the Ji1,…,iqJ_{i_{1},\ldots,i_{q}} as nearly static free bosonic fields; at leading order in 1/N1/N, this gives the same connected correlation functions , and furthermore, allows one to gauge the O(N)O(N) symmetry . To leading order in 1/N1/N the fermions are non-interacting, and the two-point function of the fermions satisfies a simple integral equation which can be explicitly solved near the infrared fixed point. The fermions start with dimension 00 in the UV, and flow to dimension Δ=1/q\Delta=1/q in the IR.

After the disorder average, the dynamics is invariant under an O(N)O(N) global symmetry, χi→Oijχj\chi_{i}\rightarrow O_{{ij}}\chi_{j}, with OOT=1OO^{T}=1, much like a vector model. The bilinear, primary, fermion operators, singlets under O(N)O(N), are schematically ∑i=1Nχi ∂τ2n+1χi\sum_{i=1}^{N}\chi_{i}\,\partial_{\tau}^{2n+1}\chi_{i}. In the UV, these operators have dimension 2n+12n+1. In the IR, the dimensions receive an order-one shift for small nn, and approach 2Δ+2n+12\Delta+2n+1 asymptotically for large nn. The standard AdS/CFT dictionary relates the dimensions of CFT single-trace operators for matrix theories, or bilinear singlet operators for vector models, to the masses of particles in the bulk dual. This would imply that the SYK dual has a tower of particles in the bulk, with masses, in units of the AdS radius, roughly spaced by two. This spectrum differs from N=4\mathcal{N}=4/AdS5×S5AdS_{5}\times S^{5} duality where for large ’t Hooft coupling only a small number of massless modes survive, or vector model/Vasiliev duality, where a tower of massless modes appears in the bulk. In it was noted that the bulk dual of SYK might be a string theory with the string scale comparable to the AdS radius, and thus non-local or stringy. But what the dual of SYK is, and the extent to which it is nonlocal, remains an open problem.

The goal of this paper is to generalize the SYK model. We would like to understand how large the class of such models is, and which features are generic and which are special to SYK. This paper will not add anything new to the bulk interpretation of SYK, but the dual bulk theory, whatever it is, should be able to incorporate this more general class of models.

Two seemingly important ingredients in SYK are: (a) 0+10+1 dimensions, where the fermions are dimensionless, thereby ensuring that any product of fermions is a relevant perturbation, and (b) quenched disorder, which plays an important role in the solvability at large NN. The generalization we explore is one in which there are ff flavors of fermions, χia\chi_{i}^{a}, where i=1…Nai=1\ldots N_{a} and a=1…fa=1\ldots f, with a Hamiltonian,

In Sec. 2 we derive the Schwinger-Dyson equation for the two-point functions of the fermions, and find that the model (1.2) generically has an IR fixed point. While the IR dimension for SYK was Δ=1/q\Delta=1/q, for the generalized model (1.2) a set of ff transcendental equations determine the dimensions Δa\Delta_{a}. In the limit of large qaq_{a}, these have simple analytic solutions. Furthermore, for large qaq_{a} one only needs to sum a particular subset of Feynman diagrams, thus yielding an explicit expression for the two-point function and the spectral function.

In Sec. 3 we study the spectrum of composite operators. After the disorder average, the generalized model (1.2) has an O(N1)×O(N2)×⋯×O(Nf)O(N_{1})\times O(N_{2})\times\cdots\times O(N_{f}) symmetry. The singlet bilinear operators are schematically ∑i=1Naχia ∂τ1+2nχia\sum_{i=1}^{N_{a}}\chi_{i}^{a}\,\partial_{\tau}^{1+2n}\chi_{i}^{a} for any a∈{1,…,f}a\in\{1,\ldots,f\}. So we expect there to be ff towers of operators. We derive equations determining the IR dimensions of these operators. We prove that for any choice of parameters: ff, NaN_{a}’s, qaq_{a}’s, there is always a dimension-two operator in the spectrum. In SYK, the dimension-two operator is responsible for both the breaking of conformal symmetry in the four-point function and for maximal chaos. The same properties hold for the generalized model.

An instructive case to study is the generalized model with all NaN_{a} equal to N/fN/f and all qaq_{a} equal to qq. It has the symmetry O(N/f)×⋯×O(N/f)O(N/f)\times\cdots\times O(N/f). The spectrum contains a tower identical to that of SYK with a qfqf body interaction, along with a new tower that appears with a degeneracy of f−1f-1. Indeed, this model is similar to SYK with NN fermions and a qfqf body interaction, but the full O(N)O(N) symmetry is broken and consequently more singlet operators exist, allowing for a richer model.

In Appendix A we consider the path integral for the generalized model. This provides an alternate way of computing the correlation functions, with the saddle point giving the Schwinger-Dyson equations for the two-point functions, and the leading 1/N1/N fluctuations about the saddle giving the four-point function. In Appendix B we consider (1.2) with an additional scalar; a special case of this includes supersymmetric SYK . Finally, Appendix C solves SYK for q=2q=2 at finite NN. SYK for q=2q=2 is like NN fermions with a random mass matrix; the randomness makes it nontrivial, though it is less interesting than q≥4q\geq 4. This appendix can be read independently of the rest of the paper.

Two-Point Function

Let us recall the SYK model . For recent studies of SYK, see . For some related studies of AdS2 and conformal symmetry breaking see . For earlier studies of a holographic interpretation of the SY model, see . While this paper was being completed, appeared, which considers a higher dimensional generalization of SYK. It contains NN Majorana fermions with the anticommutation relation {χi,χj}=δij\{\chi_{i},\chi_{j}\}=\delta_{ij}. The action is,

where the coupling Ji1,…,iqJ_{i_{1},\ldots,i_{q}} is totally antisymmetric and, for each i1,…,iqi_{1},\ldots,i_{q}, is chosen from a Gaussian ensemble. The two-point function of the Ji1,…,iqJ_{i_{1},\ldots,i_{q}} is taken to be,

At leading order in 1/N1/N, (2.2) is equivalent to the simpler normalization,

The particular scaling with NN in the choice (2.3) is in order to obtain a nontrivial large NN limit, while the other factors are for convenience. One can consider SYK for any even q≥2q\geq 2, with q=4q=4 being the prototypical case . At q=∞q=\infty there are some simplifications . The case q=2q=2 is simplest, and is equivalent to an O(N)O(N) vector fermion with a random mass matrix, although in many ways it is qualitatively different from the q>2q>2 models. We solve the q=2q=2 SYK at finite NN in Appendix C.

At zero coupling, the Euclidean two-point function ⟨Tχi(τ)χj(0)⟩≡G(τ)δij\langle T\chi_{i}(\tau)\chi_{j}(0)\rangle\equiv G(\tau)\delta_{ij} is given by,

where the factor sgn(τ)\text{sgn}(\tau) (sgn(τ)=1\text{sgn}(\tau)=1 for τ>0\tau>0 and sgn(τ)=−1\text{sgn}(\tau)=-1 for τ<0\tau<0) accounts for the fermion anticommutation. To leading order in 1/N1/N, the Schwinger-Dyson equations for the two-point function drastically simplify and are given by,

The first of these, (2.5), is the standard equation expressing the two-point function in terms of the one-particle irreducible self-energy Σ(ω)\Sigma(\omega). The second equation, which is written in position space, is a special feature of SYK (see Fig. 1). At leading order in 1/N1/N, the only diagrams that survive are nested sunset diagrams; all others are suppressed by some power of 1/N1/N. These equations can be combined into a single integral equation; however, an analytic solution to this equation is not known. At strong coupling, ∣Jτ∣≫1|J\tau|\gg 1 (equivalently, the infrared limit), one can drop the iωi\omega in (2.5), to get,

is a solution to (2.7) provided one takes,

The Fourier transform of G(τ)G(\tau), given in (2.8), is useful in verifying this,

What is special to SYK is that the IR Schwinger-Dyson equations (2.7) are invariant under reparameterization of time, τ→f(τ)\tau\rightarrow f(\tau), with the propagator transforming as G(τ1−τ2)→f′(τ1)Δf′(τ2)Δ G(f(τ1)−f(τ2))G(\tau_{1}-\tau_{2})\rightarrow f^{\prime}(\tau_{1})^{\Delta}f^{\prime}(\tau_{2})^{\Delta}\,G(f(\tau_{1})-f(\tau_{2})). Therefore, although (2.8) is at zero temperature, we can easily construct the finite-temperature two-point function by mapping the real line to a circle .

2. A Generalization of SYK

where II is a collective index, I=i1,…,iq1,…,j1,…,jqfI=i_{1},\ldots,i_{q_{1}},\ldots,j_{1},\ldots,j_{q_{f}}. The coupling JIJ_{I} is antisymmetric under permutation of indices within any one of the ff families, and is drawn from a Gaussian distribution,

where the disorder average ⟨JIJI⟩\langle J_{I}J_{I}\rangle is given by

It will be convenient to make the following definitions,

The class of models (2.12) for large NN is characterized by f−1f-1 independent continuous parameters 0<κk<10<\kappa_{k}<1, as well as the qkq_{k}, which can be any positive integers provided that their sum is even. After the disorder average, SYK (2.1) has O(N)O(N) symmetry, while in the generalized model (2.12) the symmetry is broken to the subgroup O(N1)×O(N2)×⋯×O(Nf)O(N_{1})\times O(N_{2})\times\cdots\times O(N_{f}).

The free two-point function for each χia\chi_{i}^{a}, is again given by (2.4). Away from the UV it will continue to be the case that the two-point function is diagonal in flavor and site space. Denoting the two-point function for the flavor kk fermion by Gk(τ)G_{k}(\tau), the self-energy for the flavor kk fermion is (see Fig. 2), The factors are as follows. The factor (∏qa!)2\left(\prod q_{a}!\right)^{2} comes from the square of the prefactor of the interaction term in (2.12). There is a factor of qkq_{k} from the number of contractions with the ingoing fermion, and another qkq_{k} with the outgoing fermion, and a (qk−1)!(q_{k}-1)! from the contraction of the remaining flavor kk fermions amongst themselves. There is also a factor of qa!q_{a}! from contractions of flavor aa fermions, for all the other flavors.

Making use of (2.14, 2.15), this simplifies to,

An alternative way to obtain (2.17) is by performing the replica trick to do the disorder average, introducing mean fields, integrating out the fermions, and taking the large NN saddle point; see Appendix A. For one flavor, (2.17) reduces to the SYK expression for the self-energy (2.6).

We first determine whether there is an IR fixed point and, if so, the IR dimension Δk\Delta_{k} of the fermions of flavor kk. In the IR, the two-point function should take the form,

To find the normalization bkb_{k} and dimension Δk\Delta_{k}, we first insert the above ansatz into (2.17) and take the Fourier transform, One should not confuse the usage of Σ\Sigma as the self-energy with the usage of Σ\Sigma as a sum.

Inserting (2.19) and (2.18) into the IR limit of (2.5), Σk(ω)Gk(ω)=−1\Sigma_{k}(\omega)G_{k}(\omega)=-1, gives,

The first equation is just the statement that the IR dimension of the coupling JIJ_{I} is zero. Simplifying the second gives,

Equating all the (2.22), for kk ranging from 11 to ff, gives f−1f-1 equations. Combined with (2.20), for any given choices of κk\kappa_{k} and qkq_{k}, we have a set of ff equations for the ff unknown dimensions Δk\Delta_{k}. These equations generically have solutions. The case of q1=1q_{1}=1 appears to be exceptional. For instance, taking two flavors with q1=1q_{1}=1, q2=3q_{2}=3, there is no solution for κ1<110\kappa_{1}<\frac{1}{10}. These equations have simple solutions in the limit of qa≫1q_{a}\gg 1, as we show in the next section.

3. Large qkq_{k}

If the number of fermions of flavor kk appearing in the interaction (2.12) is large, qk≫1q_{k}\gg 1, then from (2.20) we know that Δk≪1\Delta_{k}\ll 1. Let us assume qk≫1q_{k}\gg 1 for all kk. In this limit, (2.22) simplifies to ∏baqa=12κkQkΔk\prod b_{a}^{q_{a}}=\frac{1}{2}\kappa_{k}Q_{k}\Delta_{k}, with the solution,

Eq. 2.23 shows that a hierarchy in the qkq_{k}’s for different flavors, or in the κk\kappa_{k}’s, will lead to a hierarchy in the Δk\Delta_{k}’s.

The smallness of the dimensions Δa\Delta_{a} suggests one should be able to solve for the two-point function at all energies. This was done for SYK at large qq in . Here we perform an analogous computation for the generalized model in the large qkq_{k} limit. The two-point functions are taken to be,

Taking the Fourier transform, for which we use the shorthand F\mathcal{F},

Inverting to get Gk(ω)−1G_{k}(\omega)^{-1}, (2.5) allows us to identify,

where in the second equation we have done an inverse Fourier transform of the first. Combining with (2.17) gives,

We have such an equation for every kk. Thus, we can express gag_{a} in terms of gkg_{k} for any a,ka,k,

Summing (2.27) for all kk and using (2.28) gives,

where the rescaled J\mathcal{J} is kept finite in the large qkq_{k} limit. The solution to (2.29) is easily derived for finite temperature, namely with ga(τ)=ga(τ+β)g_{a}(\tau)=g_{a}(\tau+\beta) ,

where vv is defined implicitly in terms of J\mathcal{J}. At zero temperature (2.30) becomes,

where Δk\Delta_{k} is given by (2.23). Having the exact solution, we can take the IR limit J∣τ∣≫1J|\tau|\gg 1 to find the individual normalizations of the two-point function (2.18),

Recall that solving the IR limit of the Schwinger-Dyson equations only established the product of the normalizations, (2.22).

The two-point function in the large qq limit can alternatively be found by summing an appropriate set of Feynman diagrams. We will show how this works in SYK. Due to large qq combinatorics, the diagrams contributing to the self-energy that appear most often are like the ones shown in Fig. 3 (a), rather than those in Fig. 3 (b). The Feynman diagrams that are summed at large qq can be characterized as those diagrams that, under a single vertical cut, break up into two tree diagrams. The self-energy can therefore be found recursively, as shown in Fig. 3(c). The equation corresponding to Fig. 3(c) is,

where G0(ω)G_{0}(\omega) is the free two-point function (2.4). Rearranging (2.34) gives

where the second equation is the inverse Fourier transform of the first. Letting

3.2. Spectral Function

The frequency space two-point function follows from (2.24, 2.32),

and performing the τ\tau integral in Eq. 2.38 gives,

The spectral function (as defined in Appendix C by Eq. C.4) for the flavor kk fermion is therefore,

where Δk\Delta_{k} is given by (2.23). Since Δk≪1\Delta_{k}\ll 1, this is sharply peaked around small λ\lambda. If there is only one flavor, then Δ=1/q\Delta=1/q. This spectral function is for q≫1q\gg 1. For q=2q=2, the SYK spectral function is instead a Wigner semicircle (C.5).

4. Effective Action

We have so far discussed the model (2.12) directly in terms of the fermions, finding the two-point function at large NN through study of Feynman diagrams. It is useful to also consider the path integral approach. Employing the replica trick, one can carry out the disorder average, and then integrate out the fermions after the introduction of new (bilocal) fields G~a(τ1,τ2)\widetilde{G}_{a}(\tau_{1},\tau_{2}) and Σ~a(τ1,τ2)\widetilde{\Sigma}_{a}(\tau_{1},\tau_{2}). The result is (see Appendix A),

For one flavor, this reduces to the effective action for SYK (see for an analogous expression for the SY model, and for the Dirac fermion version of SYK). The large NN saddle point of the action gives the Schwinger-Dyson equations for the two-point function found previously from Feynman diagrams. In particular, varying SeffS_{eff} with respect to G~k(τ1,τ2)\widetilde{G}_{k}(\tau_{1},\tau_{2}), and assuming time-invariance, gives (2.17), while varying with respect to Σ~k(τ1,τ2)\widetilde{\Sigma}_{k}(\tau_{1},\tau_{2}) yields (2.5) for each flavor. The saddle point solutions are denoted by Gk(τ1,τ2)G_{k}(\tau_{1},\tau_{2}) and Σk(τ1,τ2)\Sigma_{k}(\tau_{1},\tau_{2}).

To leading order in 1/N1/N, the free energy is given by the saddle of (2.42),

Following , one can differentiate with respect to JJ to get,

For large qaq_{a}, Ga(τ)G_{a}(\tau) was found explicitly in Sec. 2.3. Also, since the partition function only depends on βJ\beta J, it follows that J∂J=β∂βJ\partial_{J}=\beta\partial_{\beta}. Thus for large qaq_{a},

where vv is defined in terms of J\mathcal{J} in (2.30). Up to the choice of normalization of the variance of the disorder, ⟨JIJI⟩\langle J_{I}J_{I}\rangle, this is the same as for SYK with NN fermions and a ∑a=1fqa\sum_{a=1}^{f}q_{a} body interaction. So the entropies are also the same. In order to see a distinction, one must study the 1/N1/N corrections.

Four-Point Function

The SYK model has an O(N)O(N) symmetry after the disorder average. The bilinear primary operators that are O(N)O(N) invariant are schematically ∑iχi ∂τ1+2nχi\sum_{i}\chi_{i}\,\partial_{\tau}^{1+2n}\chi_{i} for nonnegative integer nn. In the UV, these have dimension 2n+12n+1. The IR dimensions of the operators are computed by summing a class of ladder diagrams. The four-point function of the fermions is then given by a sum over conformal blocks, one for each of these composite operators.

For the generalized model (2.12), there is an O(N1)×O(N2)×⋯×O(Nf)O(N_{1})\times O(N_{2})\times\cdots\times O(N_{f}) symmetry after the disorder average, and the invariant operators are schematically ∑iχia ∂τ1+2nχia\sum_{i}\chi_{i}^{a}\,\partial_{\tau}^{1+2n}\chi_{i}^{a} for any a∈{1,…,f}a\in\{1,\ldots,f\}. So there are now ff towers of operators. In this section we compute the IR dimensions of these operators.

We begin by reviewing and adding some detail to the computation in for the IR dimensions of the SYK composite operators. The primary O(N)O(N) invariant bilinear operators are,

where the coefficients dnkd_{nk} are chosen so that the operators are primary. For instance,

The general form of dnkd_{nk} will not be important for us.

We would like to compute the overlap between the state created by the composite operator On\mathcal{O}_{n} acting at time τ0\tau_{0}, and two fermions at times τ1\tau_{1} and τ2\tau_{2}, respectively. In other words, the three-point function, ⟨χi(τ1)χi(τ2)O(τ0)⟩\langle\chi_{i}(\tau_{1})\chi_{i}(\tau_{2})\mathcal{O}(\tau_{0})\rangle, which we will denote by v(τ0;τ1,τ2)v(\tau_{0};\tau_{1},\tau_{2}). If the two fermions just propagated without interacting with each other, this would be found by Wick contractions,

Eq. 3.3 is the first diagram that appears in Fig. 4a. We must also include a sum over all the ladder diagrams in Fig. 4a. One can perform the sum by solving the equation (see Fig. 4b),

where the kernel is the operator that adds a single rung (see Fig. 4c),

where τab≡τa−τb\tau_{ab}\equiv\tau_{a}-\tau_{b}. Letting the composite have dimension hh, in the IR the solution to (3.4) will take the form of conformal three-point function,

For h>2Δh>2\Delta, the term GχχO0G^{0}_{\chi\chi\mathcal{O}} is much smaller than (3.6) in the IR, τ12≫1\tau_{12}\gg 1, so we can drop it in (3.4). Thus, (3.4) simplifies to (see Fig. 4d),

where g(h)=1g(h)=1. Eqn. 3.7 is telling us that v(τ0;τ1,τ2)v(\tau_{0};\tau_{1},\tau_{2}) are eigenvectors of the kernel with eigenvalues g(h)g(h). The dimensions hh of the composite operators are those hh for which the eigenvalue g(h)=1g(h)=1. It is helpful to think of the composite O(N)O(N) invariant operators as analogous to a bound state of two fermions. In the more familiar context of finding bound states in quantum field theory, Fig. 4d is the Bethe-Salpeter equation. There one is using this equation to find the masses of the bound states. Eq. 3.7 is the CFT analog of this, where instead of finding the masses of the bound states, one is finding the conformal dimensions hh.

The eigenvalue g(h)g(h) is independent of the choice of τ0\tau_{0}, so for evaluating (3.7) one can take the eigenvectors to be,

where 2α=2Δ−h2\alpha=2\Delta-h. By acting on (3.8) with the SL(2,R)SL(2,R) generators, one gets all of the eigenvectors (3.6) . Inserting (3.8) into (3.7) gives ,

where ψ(Δ)\psi(\Delta) was defined in (2.11). A plot of g(h)g(h) is given in Fig. 5. One can see that there is a tower of hh’s for which g(h)=1g(h)=1. For large hh the solutions to g(h)=1g(h)=1 are approximately h≈2Δ+2n+1h\approx 2\Delta+2n+1.

There are solutions to g(h)=1g(h)=1 for h<2Δh<2\Delta as well. These solutions immediately follow from the h>2Δh>2\Delta solutions due to the symmetry g(h)=g(1−h)g(h)=g(1-h). However, they do not correspond to dimensions of composite operators. Recall that dropping the first term in (3.4) was justified in the IR only for h>2Δh>2\Delta. (For h<2Δh<2\Delta, it is instead justified in the UV).

Knowing the dimensions of the “single-trace” operators, one can say something about the bulk dual of SYK. The AdS/CFT dictionary relates the dimensions of single-trace operators to the masses of bulk fields,

for AdS2. So the dual of SYK has a tower of particles in the bulk, one for each solution to g(h)=1g(h)=1 for h>2Δh>2\Delta. For large integer nn, these have approximate masses mn2≈(2Δ+2n+1)(2Δ+2n)m_{n}^{2}\approx(2\Delta+2n+1)(2\Delta+2n).

where the combinatorial factor in front is, The factor of NaqaN_{a}^{q_{a}}, for a≠l,ka\neq l,k, comes from the site index summation within the rung. For flavors k,lk,l, there are only qk−1,ql−1q_{k}-1,q_{l}-1 propagators in the rung, so those give factors of Nkqk−1N_{k}^{q_{k}-1}, Nlql−1N_{l}^{q_{l}-1}, respectively. There is then an additional factor of NlN_{l} because the Feynman diagrams are built by adding the kernel to the left (see Fig. 4); so the ll index will get summed over.

The diagonal components of the kernel are similar, but with slightly different propagator powers and combinatorial factors. Using (2.14, 2.15) and simplifying we get the diagonal and off-diagonal components,

where k≠lk\neq l and k,l∈{1,…,f}k,l\in\{1,\ldots,f\}. If there is only one flavor, K11K^{11} becomes (3.5).

As in SYK, we must find the eigenvectors and eigenvalues of the kernel. Letting gg be an eigenvalue, and va(τ12)v^{a}(\tau_{12}) the components of an eigenvector,

Following (3.8), an ansatz for an eigenvector is,

with some coefficients cac_{a}. Since the eigenvector and propagators in the kernel only depend on time differences, (3.15) factorizes nicely under a Fourier transform,

where the first term on the left is from the diagonal term in the kernel (3.13) and the second term is from the off-diagonal terms (3.14). Inserting the propagator (2.18) and evaluating gives,

In order to eliminate the dependance on ω\omega, we must choose,

In SYK we know that (3.8) is a special case of (3.6) with 2α=2Δ−h2\alpha=2\Delta-h. Similarly here, we let

which is consistent with (3.19). Thus, (3.18) becomes an eigenvector equation for the matrix K~\widetilde{K},

where the diagonal and off diagonal components of K~\widetilde{K} are,

In getting from (3.18) to (3.22) we made use of the product of normalizations of the propagators ∏baqa\prod b_{a}^{q_{a}} given in (2.21). If there is one flavor, K~11\widetilde{K}^{11} reduces to (3.9).

The next step is to find all hh for which there is an eigenvalue gg of K~\widetilde{K} (3.22) that equals 11. This is in principle straightforward: for any qaq_{a}, κa\kappa_{a} in (2.12) ones solves (2.20, 2.22) to find the IR dimensions Δa\Delta_{a} of the fermions, then for fixed hh one finds the ff eigenvalues of K~\widetilde{K}, and then for each of those eigenvalues solves for all hh such that the eigenvalue is equal to one. Aside from some special cases, we can not write a general and explicit answer for the hh’s. However, it is easy to see that there will always be a dimension 22 operator in the spectrum. For h=2h=2 (3.23) simplifies to,

Inserting this into (3.22), one can easily verify that the following vector

is an eigenvector of K~\widetilde{K} with eigenvalue one. Verifying this requires using ∑qaΔa=1\sum q_{a}\Delta_{a}=1, and nothing else. Perhaps surprisingly, it is not even required that the Δa\Delta_{a} are actual dimensions: one does not need to impose (2.22). The dimension-two operator is important: it leads to the breaking of conformal invariance and to maximal chaos; we will comment more on it in the next section. Another universal feature (for any number of flavors greater than one) is the seeming presence of a dimension-one operator. Inserting ρ(h=1)=−1\rho(h=1)=-1 into (3.22), one can verify that there are f−1f-1 eigenvectors of K~\widetilde{K} that have eigenvalue one. For any k∈{2,…,f}k\in\{2,\ldots,f\}, such an eigenvector has two nonzero components,

In fact, verifying this requires no assumptions on Δa\Delta_{a}. The presence of these dimension-one operators suggests a symmetry. In fact, this symmetry is simple to see from the effective action (2.42). We thank J. Maldacena for recognizing this. One can rescale G~1(τ1,τ2)→f(τ1)f(τ2)G~1(τ1,τ2)\widetilde{G}_{1}(\tau_{1},\tau_{2})\rightarrow f(\tau_{1})f(\tau_{2})\widetilde{G}_{1}(\tau_{1},\tau_{2}) and G~a(τ1,τ2)→[f(τ1)f(τ2)]−q1qaG~a(τ1,τ2)\widetilde{G}_{a}(\tau_{1},\tau_{2})\rightarrow[f(\tau_{1})f(\tau_{2})]^{-\frac{q_{1}}{q_{a}}}\widetilde{G}_{a}(\tau_{1},\tau_{2}), for any a≠1a\neq 1, while leaving the IR limit of (2.42) invariant.

1.2. Equal qaq_{a}, κa\kappa_{a}

A simple and instructive case is when all the qaq_{a} are equal to some qq, and all the κa\kappa_{a} are equal, for all flavors aa. The dimensions Δa\Delta_{a} are then, by symmetry, all equal to Δ=1fq\Delta=\frac{1}{fq}. The matrix K~\widetilde{K} in (3.22) factorizes,

where ρ(h)\rho(h) is given by (3.23) and is independent of the flavor. The eigenvalues of K~\widetilde{K} are thus,

where σk\sigma_{k} are the ff eigenvalues of K\mathcal{K}. The matrix K\mathcal{K} has a symmetric eigenvector (1,1,…,1)(1,1,\ldots,1) with eigenvalue σ=fq−1\sigma=fq-1, as well as f−1f-1 antisymmetric eigenvectors: (1,−1,0,…,0)(1,-1,0,\ldots,0), (1,0,−1,0,…,0)(1,0,-1,0,\ldots,0), …,(1,0,…,0,−1)\ldots,(1,0,\ldots,0,-1), all with the same eigenvalue σ=−1\sigma=-1. Setting gk(h)g_{k}(h) equal to 11 gives the dimensions hh. The eigenvalue σ=fq−1\sigma=fq-1 leads to the same tower of dimensions as SYK with an fqfq body interaction, while the eigenvalue σ=−1\sigma=-1 gives an additional and new tower of operators, see Fig. 7. The origin of the new towers is due to the more refined symmetry of the generalized model as compared to SYK: a product of ff O(N)O(N)’s instead of O(Nf)O(Nf).

An alternative way to think about the generalized model (2.12) for this case is that instead of having ff flavors of fermions with N1=N2=…=NfN_{1}=N_{2}=\ldots=N_{f} sites for each, there is one flavor with N1fN_{1}f sites. In other words, in the Hamiltonian (2.12),

where I=i1(1),…,iq(1),…,i1(f),…,iq(f)I=i^{(1)}_{1},\ldots,i^{(1)}_{q},\ldots,i^{(f)}_{1},\ldots,i^{(f)}_{q}, one makes the identification ik(p)=fnk+p−1i^{(p)}_{k}=fn_{k}+p-1, where nkn_{k} ranges from 11 to N1N_{1}, and gets rid of the flavor index on the fermions. There are now fN1fN_{1} sites; however, this is not the same as SYK with a qfqf body interaction, since the interactions are not all-to-all, being restricted to occur between particular qfqf sets of sites.

2. Four-Point Function

Having found the dimensions of the bilinear singlet operators Ona\mathcal{O}_{n}^{a}, the next step is to compute their OPE coefficient. The OPE between two fermions will include all the Ona\mathcal{O}_{n}^{a} and their descendants, and will take the form,

where cna,bc_{n}^{a,b} are the OPE coefficients and Cn(τ12,∂τ1)=1+…\mathcal{C}_{n}(\tau_{12},\partial_{\tau_{1}})=1+\ldots is fixed by conformal invariance. The OPE coefficient can be extracted by computing the three-point function between the two fermions and O\mathcal{O}, which in Sec. 3.1 was labelled as v(τ0;τ1,τ2)v(\tau_{0};\tau_{1},\tau_{2}) and satisfied Eq. 3.4. Thinking of KK as a matrix with indices (τ1,τ2)(\tau_{1},\tau_{2}), (τ3,τ4)(\tau_{3},\tau_{4}), the formal solution of (3.4) is,

where we have generalized (3.4) to account for multiple flavors. Notice that when we computed the dimensions in Sec. 3.1, we were allowed to drop the GχχO0G_{\chi\chi\mathcal{O}}^{0} term in (3.4), arguing it was unimportant in the IR. However, for finding the OPE coefficients one is interested in the UV, τ12≪1\tau_{12}\ll 1, so this term is essential.

We will also be interested in the four-point function. Defining the bilocal,

and proceeding formally, one can perform a double OPE expansion on the four-point function, Here nn ranges over the positive integers and is labeling the number of derivatives in the composite operator, see (3.1). The index ee is labeling the different flavors. In writing (3.33) we have assumed, as will generically be the case, that there are no degeneracies in the dimensions hn,eh_{n,e} of the composites.

The right-hand side is a sum of conformal blocks, given by hypergeometric functions of the conformally invariant cross ratio,

This is similar to two-dimensional CFTs, except here we have one cross-ratio instead of two.

At large NN, the leading and first subleading in 1/N1/N pieces of the four-point function are,

The 1/N1/N piece of the four-point function is found by summing ladder diagrams . What we have is a slight generalization of what occurs in SYK, as the four-point function is now a matrix in flavor space. Starting with

one uses the kernel (3.13, 3.14) to add rungs to the ladder. Summing all the ladder diagrams,

The technical challenge in evaluating (3.37) explicitly comes from inverting 1−K1-K. Recall the procedure used in SYK. One first finds a complete basis of eigenvectors of the kernel. This turns out to be given by (3.6) with hh ranging over even positive integers h=2,4,6,…h=2,4,6,\ldots, as well as h=1/2+ish=1/2+is where s>0s>0 . One then projects (3.37) onto this basis and performs the sum/integral over the discrete and continuous tower of hh’s to find (3.34) with OPE coefficients cnc_{n} ,

where g(h)g(h) is given by (3.9) and hnh_{n} are the solutions of g(hn)=1g(h_{n})=1.

Eq. 3.38 is for hn>2h_{n}>2. There is an additional complication that occurs for the h=2h=2 block. One can notice that g(h=2)=1g(h=2)=1, and since h=2h=2 is part of the basis of eigenvectors used to invert 1−K1-K, this causes the four-point function to diverge in the conformal limit. The h=2h=2 block must therefore be treated outside the conformal limit. Moving slightly away from the IR, the eigenvalue g(h=2)g(h=2) gets slightly shifted away from 11, and so the h=2h=2 block gives a finite but large, and non-conformal, contribution to the four-point function. Since its prefactor is dominant, its growth controls the behavior of the finite temperature out-of-time-order four-point function used to probe chaos . The growth of the h=2h=2 block occurs with a Lyapunov exponent 2πT2\pi T that saturates the chaos bound of . At strong coupling, the SYK Lyapunov exponent only depends on the temperature TT. At weak coupling, the SYK Lyapunov exponent scales with the coupling JJ . In Sec. 3.1.1 we found that the generalized model always contains a dimension-two operator; assuming its OPE coefficient doesn’t vanish, this implies that in the IR the generalized model, like SYK, both breaks conformal invariance and is maximally chaotic.

To compute the four-point function (3.37) for the generalized model with generic qaq_{a} and κa\kappa_{a}, one would need to repeat the procedure used for SYK, accounting for the additional complexity of having flavor. However, in the case that all the qaq_{a} are equal and all the κa\kappa_{a} are equal, it is simple to find the four-point function, and this is case we focus on.

2.1. Equal qaq_{a}, κa\kappa_{a}

If all the qaq_{a} are equal to qq, and all the κa=1/f\kappa_{a}=1/f, then the kernel matrix (3.13, 3.14) factorizes into a flavor-space matrix and a function of times,

where K\mathcal{K} was defined in (3.27). By symmetry, the two-point functions are flavor-independent, Ga(τ)≡G(τ)G_{a}(\tau)\equiv G(\tau). For concreteness, let us focus on the case of two flavors, f=2f=2. In Sec. 3.1.2 we diagonalized K\mathcal{K}, finding a symmetric eigenvector: (1,1)(1,1), with eigenvalue σS=2q−1\sigma_{S}=2q-1, and an antisymmetric eigenvector: (1,−1)(1,-1), with eigenvalue σA=−1\sigma_{A}=-1. Forming a matrix of the eigenvectors,

we diagonalize (3.37) in flavor space, forming OTFOO^{T}\mathcal{F}O, to find,

where F0=−G(τ13)G(τ24)+G(τ14)G(τ23)F_{0}=-G(\tau_{13})G(\tau_{24})+G(\tau_{14})G(\tau_{23}) is the diagonal component of F0\mathcal{F}_{0} in (3.36). Both of the terms appearing in Fab\mathcal{F}^{ab} are similar to what occurs in SYK, so we can write the answer,

Here α0(q)\alpha_{0}(q) is given by (3.38) and ρ(h)\rho(h) is given by (3.23) with fermion dimension Δ=1/2q\Delta=1/2q. To be clear, the hnh_{n} appearing in (3.45) and (3.46) are the solutions of (2q−1)ρ(hn)=1(2q-1)\rho(h_{n})=1 and −ρ(hn)=1-\rho(h_{n})=1, respectively. Recall that we found in Sec. 3.1.2 that with two flavors (with q1=q2=qq_{1}=q_{2}=q, κ1=κ2\kappa_{1}=\kappa_{2}), the spectrum of bilinear composite operators contains two towers: a tower that matches the 2q2q body SYK tower, and a new tower, see Fig. 7. The OPE coefficients cnSc_{n}^{S} are for the 2q2q body SYK tower. Note that (3.45) is for hn>2h_{n}>2; as discussed before, the contribution of the h=2h=2 block diverges in the conformal limit.

The OPE coefficients cnAc_{n}^{A} are for the new tower. Notice that this vanishes for the h=1h=1 operator. The OPE coefficients cn1c_{n}^{1} and cn2c_{n}^{2}, in terms of (3.45, 3.46), are given by,

where, for simplicity of presentation, rather than writing cna,bc_{n}^{a,b}, we have explicitly separated the two towers. The cn1c_{n}^{1} in (3.47) are the OPE coefficients for two fermions of flavor 11 going into the sum of On1\mathcal{O}_{n}^{1} and On2\mathcal{O}_{n}^{2} (each of which is given by (3.1) for the corresponding flavor), while the cn1c_{n}^{1} in (3.48) are the OPE coefficients for two fermions of flavor 11 going into the difference between On1\mathcal{O}_{n}^{1} and On2\mathcal{O}_{n}^{2} . Analogously for the fermions of flavor 22 and the cn2c_{n}^{2}. A more intuitive way to think about this four-point function is to define the symmetric and antisymmetric combinations of the bilocals (3.32),

The symmetric correlator probes only the SYK tower,

and matches the SYK 2q2q body four-point function. The antisymmetric correlator,

probes only the new tower. One can also reproduce (3.50, 3.51) from the path integral picture, see Appendix A.1.

Discussion

The SY model involves all-to-all interactions between spins in some representation of SU(M)SU(M), H=∑i,j=1N∑μ,ν=1MJijSi νμSj μνH=\sum_{i,j=1}^{N}\sum_{\mu,\nu=1}^{M}J_{ij}S_{i\,\nu}^{\mu}S_{j\,\mu}^{\nu}, with Gaussian-random couplings JijJ_{ij}. Writing the spins as products of two fermions, this becomes a four-fermion interaction. One of the key realizations of was that the model is solvable in the double scaling limit, N→∞N\rightarrow\infty, M→∞M\rightarrow\infty, M/N→0M/N\rightarrow 0. It was recognized in that a simpler model is one that avoids spins altogether and goes directly to the fermions, H=∑Jijkl χiχjχkχlH=\sum J_{ijkl}\,\chi_{i}\chi_{j}\chi_{k}\chi_{l}. There is then a clear generalization to a model with a qq-index coupling and a qq-body interaction .

In this paper, we have made another straightforward generalization, involving ff flavors of fermions with NaN_{a} sites for each flavor and a ∑a=1fqa\sum_{a=1}^{f}q_{a} body interaction. Perhaps surprisingly, the model has an infrared fixed point for most choices of parameters Na,qaN_{a},q_{a}. We found a set of equations determining the dimensions of the fermions in the infrared, as well as the matrix determining the infrared dimensions of the bilinear singlet operators that are invariant under the global O(N1)×O(N2)×⋯×O(Nf)O(N_{1})\times O(N_{2})\times\cdots\times O(N_{f}) symmetry.

It was recognized in that the SYK model simplifies in the limit q≫1q\gg 1. Here we pointed out that in the q≫1q\gg 1 limit, only a particular subset of Feynman diagrams need to be summed. For any even q≥4q\geq 4, the SYK model has qualitatively similar properties. In the generalized model introduced in this paper, there are more parameters to vary, and one may wonder if there are corners of parameter space which either lead to simplifications or qualitative differences.

We have only begun exploring the parameter space, focusing on the symmetric case of an equal number of sites for each flavor, as well as interaction orders qaq_{a} that are independent of the flavor. The main qualitative difference, as compared to SYK with a qfqf body interaction, is more singlet operators resulting from a symmetry that is a subgroup of the O(N)O(N) symmetry of SYK. One feature we found, that holds for any choice of parameters, is the presence of a dimension-two bilinear singlet operator in the infrared. Another was the presence of a dimension-one operator; however, in the symmetric case considered, its OPE coefficient vanished. It would be good to better understand this operator.

Nontrivial and solvable models are both rare and valuable. It is now clear that the class of SYK-like models is much larger than just the SY model. Just how large this class is, if there are further generalizations, and the precise characterization of the Feynman diagrams, at each order in 1/N1/N, are all still open problems. We may hope that exploring this structure will provide guidance towards understanding the dual string theory, if there is one.

Acknowledgements

We thank D. Anninos, T. Anous, D. Gaiotto, A. Kitaev, G. Korchemsky, J. Maldacena, Y. Nakayama, N. Nekrasov, J. Polchinski, B. Shraiman, and E. Silverstein for helpful discussions. This work was supported by NSF grant 1125915.

Appendix A Effective Action

In this appendix we compute the free energy (equivalently, the effective action) for the generalized model (2.12). The calculation is analogous to the one for SYK .

Employing the replica trick, instead of computing the disorder average of the logarithm of the partition function, one instead computes the disorder average of MM copies of the system. Starting with (2.12), this is given by,

where α\alpha is the replica index, α∈{1,…,M}\alpha\in\{1,\ldots,M\}, aa is the flavor, a∈{1,…,f}a\in\{1,\ldots,f\}, iai_{a} is the site index, ia∈{1,…,Na}i_{a}\in\{1,\ldots,N_{a}\}, and II is a collective site index, I=i1,…,iq1,…,j1,…,jqfI=i_{1},\ldots,i_{q_{1}},\ldots,j_{1},\ldots,j_{q_{f}}, and P[JI]P[J_{I}] is the probability distribution for the JIJ_{I} (2.13). Doing the Gaussian integral over the disorder, (A) becomes,

Having done the disorder average, we see that there is a O(N1)×O(N2)×⋯×O(Nf)O(N_{1})\times O(N_{2})\times\cdots\times O(N_{f}) symmetry. We thus introduce the collective fields,

where Σ~aαβ(τ1,τ2)\widetilde{\Sigma}_{a}^{\alpha\beta}(\tau_{1},\tau_{2}) acts as a Lagrange multiplier. We insert into (A.2) such a delta function for each replica index pair α,β\alpha,\beta and each flavor aa. This gives,

As is standard in studies of SYK, one assumes a replica symmetric saddle point, G~aαβ(τ1,τ2)=δαβG~a(τ1,τ2)\widetilde{G}_{a}^{\alpha\beta}(\tau_{1},\tau_{2})=\delta^{\alpha\beta}\widetilde{G}_{a}(\tau_{1},\tau_{2}), and so (A.6) becomes ZM‾=∫DΣ~a DG~aexp⁡(−MSeff) \overline{Z^{M}}=\int D\widetilde{\Sigma}_{a}\,D\widetilde{G}_{a}\exp\left(-MS_{eff}\right)~ where,

If there is only one flavor, we recover the SYK action ,

For SYK, one can expand (A.9) about the saddle G~=G+∣G∣2−q2g\widetilde{G}=G+|G|^{\frac{2-q}{2}}g and Σ~=Σ+∣G∣q−22σ\widetilde{\Sigma}=\Sigma+|G|^{\frac{q-2}{2}}\sigma, keeping terms up to second order, and then integrating out σ\sigma to get ,

where Kc−1K_{c}^{-1} is the inverse of KcK_{c}, thought of as a matrix with indices (τ1,τ2)(\tau_{1},\tau_{2}), (τ3,τ4)(\tau_{3},\tau_{4}), and given by,

The four-point function ⟨G~(τ1,τ2)G~(τ3,τ4)⟩\langle\widetilde{G}(\tau_{1},\tau_{2})\widetilde{G}(\tau_{3},\tau_{4})\rangle computed with (A.12), after doing the Gaussian integral, reproduces Eq. 3.37 for one flavor.

Now consider the generalized model, (A.8), for two flavors with q1=q2=qq_{1}=q_{2}=q and κ1=κ2=1/2\kappa_{1}=\kappa_{2}=1/2. From (A.8),

As noted in Sec. 2.4, the saddle point equation is the same as the equation for SYK with a 2q2q body interaction. Let us now study fluctuations about the saddle, G~a=G+∣G∣1−qga\widetilde{G}_{a}=G+|G|^{1-q}g_{a}, and Σ~a=Σ+∣G∣q−1σa\widetilde{\Sigma}_{a}=\Sigma+|G|^{q-1}\sigma_{a}. Expanding (A.13) to second order,

Integrating out σ1,σ2\sigma_{1},\sigma_{2} gives,

where gS/gAg_{S}/g_{A} are the symmetric/antisymmetric combinations of g1,g2g_{1},g_{2}, (3.49). The correlators ⟨G~S(τ1,τ2)G~S(τ3,τ4)⟩\langle\widetilde{G}_{S}(\tau_{1},\tau_{2})\widetilde{G}_{S}(\tau_{3},\tau_{4})\rangle and ⟨G~A(τ1,τ2)G~A(τ3,τ4)⟩\langle\widetilde{G}_{A}(\tau_{1},\tau_{2})\widetilde{G}_{A}(\tau_{3},\tau_{4})\rangle follow by analogy with (A.12), and reproduce (3.50) and (3.51).

Appendix B Model with a Scalar

In this appendix we consider a model with a boson field. It is a slight variant of (2.12) and has the action,

The only technical distinction between finding the IR dimensions for (B.1) compared with (2.12) is that the boson propagator is symmetric in time. The ansatz for the IR boson propagator is,

where ψ(Δ)\psi(\Delta) is defined in (2.11), while for the IR fermion propagator it is,

for k≥2k\geq 2. In the IR, one drops the free propagator appearing in the Schwinger-Dyson equation (2.5), so for both the boson and the fermions one has Σk(ω)Gk(ω)=−1\Sigma_{k}(\omega)G_{k}(\omega)=-1. The self-energy is again given by (2.16), with the disorder average normalization given in (2.14). Repeating the several steps in Sec. 2.2 gives the following equations,

The equations (B.4) are the same as for the generalized fermion model (2.12), while (B.5) is different.

For the case of f=2f=2 and κ1=κ2\kappa_{1}=\kappa_{2}, (B.4, B.5) have the simple solution,

For q2=2q_{2}=2 this gives the dimensions Δ1=2/3\Delta_{1}=2/3, Δ2=1/6\Delta_{2}=1/6 found in . We thank Yu Nakayama for sharing his results and explaining the supersymmetric model. Intriguingly, the difference between the boson dimension Δ1\Delta_{1} and fermion dimension Δ2\Delta_{2} is 1/21/2 for any q2q_{2}, as would be implied by supersymmetry. However, we have not checked that the model for general q2q_{2} is supersymmetric.

Appendix C Random Mass Matrix Fermions

The simplest SYK model is for q=2q=2: fermions with a random mass matrix. For this case, all computations can be performed exactly, without the restriction of being near the fixed points or working at large NN. In this appendix, we solve the q=2q=2 model. For infinite NN this is trivial, while for finite NN it is slightly more involved but follows from standard matrix model techniques. One should keep in mind that the q=2q=2 case has multiple features that are not representative of SYK at larger qq; in particular, it is not chaotic. In it was proposed that the q=2q=2 model satisfies the Eigenstate Thermalization Hypothesis.

The Schwinger-Dyson equations for the two-point function (2.5, 2.6) are integral equations for general qq, but become a simple quadratic equation for q=2q=2. The solution is

One can also find this directly by summing non-crossing rainbow diagrams (see Fig. 9),

where G0(ω)G_{0}(\omega) is the bare propagator (2.4), while CnC_{n} are the Catalan numbers,

The Catalan numbers are the number of different ways n+1n+1 factors can be completely parenthesized; here the parentheses are the rainbows. Summing (C.2) gives (C.1). One can also write (C.1) as,

where the spectral function ρ(λ)\rho(\lambda) is the Wigner semi-circle, with support for ∣λ∣<2J|\lambda|<2J,

At finite temperature, the frequencies in (C.1) should be viewed as the Matsubara frequencies, ωn=(2n+1)π/β\omega_{n}=(2n+1)\pi/\beta. Taking the discrete Fourier transform of (C.4) gives,

where 0<τ<β0<\tau<\beta. In the limit of zero temperature βJ≫1\beta J\gg 1, we can evaluate the integral to obtain,

where L1\boldsymbol{L}_{1} is the modified Struve function, and I1I_{1} is the modified Bessel function. While both L1\boldsymbol{L}_{1} and I1I_{1} grow exponentially, the two-point function (C.7) decays monotonically with ∣Jτ∣|J\tau|. The combination is sometimes denoted by M1≡L1−I1\boldsymbol{M}_{1}\equiv\boldsymbol{L}_{1}-I_{1}. We can do a strong coupling expansion of (C.7),

where we see that the first term matches what was expected from the IR limit of the Schwinger-Dyson equations (2.8, 2.9).

Comments

One comment is that in summing the Feynman diagrams giving (C.2) it is important to work at finite temperature. Each of the diagrams individually has IR divergences: the Fourier transform of any of the individual terms in (C.2) will diverge in the limit of β→∞\beta\rightarrow\infty. Of course, one could have chosen to regulate the IR divergence in some way other than working at finite temperature. However, finite temperature is natural. The point is just that the dimensionless expansion parameter is βJ\beta J.

Another comment is that aside from the implicit appearance of β\beta in the Matsubara frequencies, (C.2) has no explicit β\beta dependance. This is a property that is special to q=2q=2. For SYK with q≥4q\geq 4, one could solve the Schwinger-Dyson equations perturbatively around weak coupling, giving an expansion of the form,

with some coefficients gklg_{kl}. One can derive recursion relations for gklg_{kl}, but we have not found a way of solving them.

We have been considering Majorana fermions. One can instead study q=2q=2 with Dirac fermions,

At leading order in 1/N1/N, this gives the same two-point function (C.1). Working with Dirac fermions gives slightly more flexibility, as one can introduce a chemical potential. With no chemical potential, as in (C.10), one is at half-filling. Explicitly, consider a single free Dirac fermion H=ω0c†cH=\omega_{0}c^{\dagger}c. (Adding a chemical potential just corresponds to adding to (C.10) such a term for each fermion, with chemical potential μ=−ω0\mu=-\omega_{0}.) The finite-temperature two-point function is trivially,

Since we are at finite temperature, fields have the time range 0<τ<β0<\tau<\beta. The two-point function is a function of the difference between two times, and so naturally has the range −β<τ<β-\beta<\tau<\beta. However, from (C.11) we see that for 0<τ<β0<\tau<\beta, G(τ−β)=−G(τ)G(\tau-\beta)=-G(\tau). We can thus restrict to 0<τ<β0<\tau<\beta. The filling fraction Q\mathcal{Q} is defined as the expectation value of the occupation number,

We can choose the filling fraction by choosing ω0\omega_{0}. It is clear that for any finite temperature, if ω0=0\omega_{0}=0, then there is no energy cost to being in the state ∣1⟩|1\rangle versus ∣0⟩|0\rangle, and so the filling fraction is 1/21/2. Note that the limits of T→0T\rightarrow 0 and ω0→0\omega_{0}\rightarrow 0 do not commute. If we set T=0T=0 at finite ω0\omega_{0} (including ω0=0\omega_{0}=0), then we get zero filling: from (C.11), G(τ)=θ(τ)G(\tau)=\theta(\tau).

Finally, the q=2q=2 model sums rainbow diagrams. There are many other models that sum rainbow diagrams. For instance, two-dimensional QCD has the same rainbow diagrams, where the fermions are the quarks, and the disorder lines are the gauge field propagators. Also, the recently studied three-dimensional U(N)kU(N)_{k} Chern-Simons theory coupled to scalars or fermions also sums rainbow-like diagrams . A simple large NN quantum mechanics model that sums rainbow diagrams is the Iizuka-Polchinski model (see also, ). The IP model has a harmonic oscillator in the adjoint representation of U(N)U(N) plus a harmonic oscillator in the fundamental representation of U(N)U(N), coupled through a trilinear interaction. In the limit that the mass of the adjoint goes to zero, this is essentially the same as the model Eq. C.10, at leading order in 1/N1/N. The reason we say essentially the same is because in the IP model the fundamental is effectively at zero filling. In other words, its free two-point function is θ(τ)\theta(\tau) as opposed to 12sgn(τ)\frac{1}{2}\text{sgn}(\tau), and correspondingly, the infinite NN two-point function after summing the rainbow diagrams is only the first term, I1I_{1}, in (C.7). In addition, at subleading orders in 1/N1/N, differences will arise between the model Eq. C.10 and the IP model. This is because the adjoint propagator will receive quantum corrections, whereas the ⟨JijJij⟩\langle J_{ij}J_{ij}\rangle “propagator” in Eq. C.10 is always a constant.

Four-Point Function

It is simplest to write the four-point function in frequency space. This is defined as,

Written as a series in 1/N1/N, Fijkl=Fijkl(0)+1NFijkl(1)+…\mathcal{F}_{ijkl}=\mathcal{F}_{ijkl}^{(0)}+\frac{1}{N}\mathcal{F}_{ijkl}^{(1)}+\ldots . At leading order in 1/N1/N there is a disconnected piece,

At first subleading order in 1/N1/N, the four-point function is a sum of ladder diagrams, like SYK for general qq. However for q=2q=2 there is an extreme simplification, since the rungs only contain the disorder lines. Since there is no momentum exchange, summing the ladders in frequency space simply involves summing a geometric series, which gives,

It is only necessary to establish the first term in the ss-channel piece. The other term, as well as the tt and uu channels, follow from antisymmetry. Through a Fourier transform and analytic continuation of (C.14), one finds there is no exponential growth in the out-of-time-order four-point function , and so the q=2q=2 model is not chaotic.

C.2. Finite N

We now compute the two-point function at finite NN for the random mass matrix fermion, (C.10). For fixed coupling JijJ_{ij}, this is just NN free fermions with mass matrix JijJ_{ij}, so the nontrivial part is to perform the disorder average. Specifically,

where, We are using the same symbol JJ to denote both the matrix of couplings, as well as the number that appears as the variance of the distribution of couplings.

Consider first the trivial case of N=1N=1. This is just a fermion with a random mass. Then (C.15) reduces to (C.4) with a spectral function,

So at N=1N=1 the spectral function is a Gaussian, while at N=∞N=\infty it is the Wigner semicircle (C.5). The two-point function for N=1N=1 can also be found by summing Feynman diagrams,

Writing the double factorial as a Gaussian integral, and interchanging the integral and the sum, we recover (C.17). Explicitly performing the integral gives the two-point function in terms of the complimentary error function,

In the zero temperature limit we also find,

We now move on to the case of general NN, using the method of orthogonal polynomials to evaluate (C.15). We can write (C.16) in terms of the eigenvalues of JJ,

where we have used that JJ is Hermitian and the last equation is in terms of the Vandermonde,

This model is of course different from fermions with masses independently drawn from a Gaussian distribution; the masses here are eigenvalues of a Hermitian matrix and have repulsion, as encoded in the Vandermonde term in (C.21).

We now take linear combinations of the columns of (C.22), transforming it into a matrix with i,ji,j element, ϕj(λi)\phi_{j}(\lambda_{i}), where ϕj(λi)\phi_{j}(\lambda_{i}) is a polynomial with lowest element 11 and highest element λij\lambda_{i}^{j}. The determinant (C.22) remains invariant under these operations. We can write the determinant as a sum of permutations of the integers from 00 to N−1N-1,

The ϕn\phi_{n} will be proportional to the Hermite polynomials, defined as,

and so we find that the spectral function is,

where we have used that fk=J‾2k+12π k!f_{k}=\overline{J}^{2k+1}\sqrt{2\pi}\,k!, which follows from (C.26, C.27). A plot of (C.30) is shown in Fig. 10.

An alternative way to write the two-point function is to perform the integral over λ\lambda in (C.4) before evaluating the sum over kk appearing in the spectral function (C.29). After the introduction of a Schwinger parameter, the integration over λ\lambda yields a Laguerre polynomial. Using that the sum of the Laguerre polynomials is an associated Laguerre polynomial ∑k=0N−1Lk(x)=LN−11(x)\sum_{k=0}^{N-1}L_{k}(x)=L_{N-1}^{1}(x), we find

/N expansion

We would like to expand (C.31) in powers of 1/N1/N. Using the definition of the associated Laguerre polynomial,

and recalling that J‾2≡J2/N\overline{J}^{2}\equiv J^{2}/N, we exchange the order of the sums, and perform the integral over ss, to get,

An series expansion of B(p,N)B(p,N) in powers of 1/N21/N^{2} was also worked out in . The first few terms are,

Using this we can write the 1/N1/N expansion of the two-point function as,

The leading term in 1/N1/N, g(0)g^{(0)}, reproduces what we found from summing the planar diagrams, (C.1).

Here we compute the two-point function for the Majorana version of q=2q=2 SYK (2.1) at finite NN (note that NN must be even). This will be slightly different from the Dirac version studied in Sec. C.2. The two-point function is given by,

The matrix JJ is real and antisymmetric. The partition function (C.38) can be written terms of the eigenvalues of JJ ,

Defining an analog of the Vandermonde, one involving only even powers,

The procedure is now similar to the Dirac case. We can write the determinant as a sum of permutations of the even integers from 00 to N−2N-2,

The ϕn\phi_{n} are the same as in the Dirac case. The partition function now involves just the even normalization constants,

For evaluating the two-point function, note that since the eigenvalues come in pairs,

This is similar to (C.31), except it involves a sum only over the even Laguerre’s.

This is similar to the spectral function for the Dirac fermion (C.30), except for the addition of the last term in (C.46) that is 1/N1/N suppressed relative to the first two (and the trivial distinction that occurs at order 1/N1/N between J~\widetilde{J} and J‾\overline{J}).

References