Abstract

A number of features and applications of subleading-color amplitudes of 𝒩=4 SYM theory are reviewed. Particular attention is given to the IR divergences of the subleading-color amplitudes, the relationships of 𝒩=4 SYM theory to 𝒩=8 supergravity, and to geometric interpretations of one-loop subleading-color and 𝑁𝑘MHV amplitudes of 𝒩=4 SYM theory.

1. Introduction

Planar amplitudes of 𝒩=4 SYM theory have been extensively studied by a variety of methods, see, for example, [123]. For a recent overview, see [24] and the special issue of Journal of Physics A, devoted to “Scattering amplitudes in gauge theories." Subleading-color (i.e., nonplanar) amplitudes, however, usually receive less attention [2533]. Nevertheless interesting insights are available from various applications of subleading color amplitudes. One case in point is a possible weak/weak duality between 𝒩=4 SYM theory and 𝒩=8 supergravity [15, 3446]. Since nonplanar graphs appear on an equal footing with planar graphs in 𝒩=8 supergravity, one needs to understand the nonplanar graphs in 𝒩=4 SYM if the weak/weak duality is to be explored.

This paper will cover three significant topics. Section 2 discusses the IR divergences of various subleading-color amplitudes. In Section 3 the interplay between subleading-color amplitudes of 𝒩=4 SYM theory and amplitudes of 𝒩=8 supergravity will be considered. Section 4 presents various geometric interpretations of one-loop subleading-color amplitudes, primarily using the tools of momentum twistors and the accompanying polytope interpretation.

In the remainder of this section, we define the notation for the color decomposition, the loop expansion, and the 1/𝑁 expansion.

At tree level, we can decompose the amplitudes 𝒜𝑛 of 𝒩=4 SYM into color-ordered tree amplitudes 𝐴𝑛𝒜tree𝑛(12𝑛)=𝑔𝑛2𝜎𝑆𝑛/𝑍𝑛Tr(𝑇𝑎𝜎(1)𝑇𝑎𝜎(𝑛))𝐴tree𝑛(𝜎(1)𝜎(𝑛))=𝑔𝑛2𝑃(23𝑛)Tr(𝑇𝑎1𝑇𝑎𝑃(2)𝑇𝑎𝑃(𝑛))𝐴tree𝑛(1𝑃(2)𝑃(𝑛)),(1.1) where in the second line, 1 is fixed and 𝑃(23𝑛) is a permutation of 2,3,,𝑛 and 𝑇𝑎 are SU(𝑁) generators in the fundamental representation, normalized according to Tr(𝑇𝑎𝑇𝑏)=𝛿𝑎𝑏. The color-ordered amplitudes 𝐴𝑛 depend on the momenta and polarizations of the external particles.

The color-ordered amplitudes are not independent. For 𝑛-point amplitudes, there is a basis of (𝑛2)! amplitudes out of the total 𝑛!, called the Kleiss-Kuijf (KK) basis [47], and we can find the others easily in terms of it [40]. It is based on the existence of the Kleiss-Kuijf relations [47] 𝐴𝑛(1,{𝛼},𝑛,{𝛽})=(1)𝑛𝛽{𝜎}𝑖OP𝛽{𝛼},𝑇𝐴𝑛1,{𝜎}𝑖,,𝑛(1.2) where 𝜎𝑖 are ordered permutations, that is, ones that keep the order of {𝛼} and of {𝛽𝑇} inside 𝜎𝑖. Thus the KK basis is 𝐴𝑛(1,𝒫(2,,𝑛1),𝑛), where 𝒫 are arbitrary permutations. All the other 𝐴𝑛’s can be recovered from it by the use of the KK relations and cyclicity and reflection invariance 𝐴𝑛(12𝑛)=(1)𝑛𝐴𝑛(𝑛21).(1.3)

At one loop, we can write a similar expansion in color-ordered amplitudes 𝒜1loop𝑛(12𝑛)=𝑔𝑛[]𝑛/2+1𝑗=1𝜎𝑆𝑛/𝑆𝑛;𝑗𝐺𝑟𝑛;𝑗(𝜎)𝐴𝑛;𝑗(𝜎(1)𝜎(𝑛)),𝐺𝑟𝑛;1(1)=𝑁Tr(𝑇𝑎1𝑇𝑎𝑛),𝐺𝑟𝑛;𝑗(1)=Tr(𝑇𝑎1𝑇𝑎𝑗1)Tr(𝑇𝑎𝑗𝑇𝑎𝑛).(1.4) However, the subleading piece in the 1/𝑁 expansion can be obtained from the leading piece by 𝐴𝑛;𝑗(12,𝑗1,𝑗,𝑗+1,𝑛)=(1)𝑗1𝜎COP{𝛼},{𝛽}𝐴𝑛;1(𝜎),(1.5) where COP are cyclically ordered permutations, again keeping the order of {𝛼} and {𝛽} fixed up to cyclic permutations.

At arbitrary loops, the decomposition of the four-gluon amplitude takes a form with only single and double traces 𝒜4(1234)=𝑔2𝜎𝑆4/4Tr(𝑇𝑎𝜎(1)𝑇𝑎𝜎(2)𝑇𝑎𝜎(3)𝑇𝑎𝜎(4))𝑁𝐴4;1(𝜎(1)𝜎(2)𝜎(3)𝜎(4))+𝑔2𝜎𝑆4/32Tr(𝑇𝑎𝜎(1)𝑇𝑎𝜎(2))Tr(𝑇𝑎𝜎(3)𝑇𝑎𝜎(4))𝐴4;3(𝜎(1)𝜎(2)𝜎(3)𝜎(4)).(1.6) We also define an explicit basis [48] of single and double traces: 𝒞[1]=Tr(𝑇𝑎1𝑇𝑎2𝑇𝑎3𝑇𝑎4),𝒞[4]=Tr(𝑇𝑎1𝑇𝑎3𝑇𝑎2𝑇𝑎4),𝒞[7]=Tr(𝑇𝑎1𝑇𝑎2)Tr(𝑇𝑎3𝑇𝑎4),𝒞[2]=Tr(𝑇𝑎1𝑇𝑎2𝑇𝑎4𝑇𝑎3),𝒞[5]=Tr(𝑇𝑎1𝑇𝑎3𝑇𝑎4𝑇𝑎2),𝒞[8]=Tr(𝑇𝑎1𝑇𝑎3)Tr(𝑇𝑎2𝑇𝑎4𝒞),[3]=Tr(𝑇𝑎1𝑇𝑎4𝑇𝑎2𝑇𝑎3),𝒞[6]=Tr(𝑇𝑎1𝑇𝑎4𝑇𝑎3𝑇𝑎2),𝒞[9]=Tr(𝑇𝑎1𝑇𝑎4)Tr(𝑇𝑎2𝑇𝑎3),(1.7) in terms of which the four-gluon amplitude can be expanded as 𝒜4(1234)=𝑔29𝑖=1𝐴[𝑖]𝒞[𝑖].(1.8)

The loop expansion of color-ordered amplitudes 𝐴[𝑖]=𝐿=0𝑎𝐿𝐴[𝑖](𝐿),𝑁𝐴4;1=𝐿=0𝑎𝐿𝐴(𝐿)4;1,𝐴4;3=𝐿=0𝑎𝐿𝐴(𝐿)4;3(1.9) is in terms of the natural ‘t Hooft loop expansion parameter [7] 𝑔𝑎2𝑁8𝜋2(4𝜋e𝛾)𝜖,(1.10) where 𝛾 is Euler’s constant and 𝜖=(4𝐷)/2. Note that at 𝐿 loops, the amplitude is at most of order 𝑁𝐿, which means that 𝐴(𝐿)[𝑖] starts at 𝒪(𝑁0).

For a general 𝑛-point amplitude, we will have an expansion in an arbitrary number of multitrace color-ordered amplitudes 𝐴𝑛;𝑗1,𝑗2,,𝑗𝑘.

Besides the loop expansion in the ‘t Hooft parameter 𝑎, we still have a 1/𝑁 expansion of the amplitudes, which can be understood in ‘t Hooft’s double line notation as an expansion in the topology of the diagrams. For 𝒜4, the expansion in single-trace 𝐴4;1 and double-trace 𝐴4;3 amplitudes corresponds to the topology of the outside lines, forming boundaries of the diagrams. For example, at one-loop, the contribution in 𝐴4;1 to the amplitude is leading, that is, of order 𝑁 (thus 𝐴4;1 of order 1), coming from a diagram with the topology of 4 external lines and a boundary, whereas the contribution of 𝐴4;3 is subleading, that is, of order 𝑁0, and comes from a nonplanar diagram with 4 external lines, but arranged on two boundaries. It can be obtained by taking two twists of the ‘t Hooft double lines on opposite sides of the box, or twists on all 4 sides. Thus the multitrace expansion comes as an expansion in the topology associated with the external lines (number of boundaries for them) and is an expansion in integer powers of 1/𝑁, corresponding to the number of boundaries of the diagram.

On top of that, we also have an expansion in integer powers of 1/𝑁2, independently for 𝐴4;1 and 𝐴4;3, corresponding to nonplanar diagrams with handles (a handle gives a factor of 1/𝑁2). The expansion terminates at order 𝒪(𝑁0) for the amplitude, since in the amplitude the powers of 𝑁 can only be positive. Thus at 𝐿-loops, we have 𝐴(𝐿)4;1=𝒪(1) to 𝒪(1/𝑁𝐿) and 𝐴(𝐿)4;3=𝒪(1/𝑁) to 𝒪(1/𝑁𝐿). Taken together, we will say that the gluon amplitudes have a 1/𝑁 expansion.

2. IR Divergences for Subleading 𝒩=4 Four-Gluon Amplitudes

2.1. General Formalism

𝒩=4 SYM is a UV-finite theory, but IR divergences arise due to the exchange of soft and collinear gluons. These divergences can be regulated using dimensional regularization in 𝐷=42𝜖 dimensions, in which they appear as poles in a Laurent expansion in 𝜖.

In gluon-gluon scattering in 𝒩=4 SYM, IR divergences arise both from soft gluons and from collinear gluons, each of which gives rise to an 𝒪(1/𝜖) pole at one loop, leading to an 𝒪(1/𝜖2) pole at that order. At 𝐿 loops, the leading IR divergence of the scattering amplitude is therefore 𝒪(1/𝜖2𝐿), arising from multiple soft gluon exchanges.

Subleading-color amplitudes 𝐴(𝐿,𝑘), that is, those suppressed by 1/𝑁𝑘 relative to the leading-color amplitude at 𝐿 loops, have less severe IR divergences, being only of 𝒪(1/𝜖2𝐿𝑘) at 𝐿-loops.

In this section, we review the derivation of a compact all-loop-order expression for the IR-divergent part of the 𝒩=4 SYM four-gluon amplitude given in [41, 49]. This result is expressed in terms of the soft (cusp) anomalous dimension 𝛾(𝑎), the collinear anomalous dimension 𝒢0(𝑎), and the soft anomalous dimension matrices Γ() and relies on the assumption that the soft anomalous dimension matrices are mutually commuting, which follows if they are all proportional to Γ(1), as has been conjectured in [30, 31, 33, 50]. This compact expression is then used to obtain the coefficient of the leading IR pole (and some subleading poles) of all the subleading-color amplitudes. Explicit values for the anomalous dimensions can be obtained by comparison with various exact results.

We organize the 4-point color-ordered amplitudes 𝐴[𝑖] defined in (1.8) into a vector in color space [25, 26] ||𝐴𝐴=[1],𝐴[2],𝐴[3],𝐴[4],𝐴[5],𝐴[6],𝐴[7],𝐴[8],𝐴[9]𝑇,(2.1) where ()𝑇 denotes the transposed vector. The vector of color-ordered amplitudes factorizes into [27, 29] ||||𝐴𝑠𝑖𝑗𝜇2𝑄,𝑎,𝜖=𝐽2𝜇2𝐒𝑠,𝑎,𝜖𝑖𝑗𝑄2,𝑄2𝜇2||||𝐻𝑠,𝑎,𝜖𝑖𝑗𝑄2,𝑄2𝜇2,,𝑎,𝜖(2.2) where |𝐻, which is IR-finite as 𝜖0, characterizes the short-distance behavior of the amplitude and where the prefactors 𝐽 and 𝐒 encapsulate the long-distance IR-divergent behavior. The soft function 𝐒 is written in boldface to denote that it is a matrix acting on the vector |𝐻. Also 𝑠𝑖𝑗 is the kinematic invariant (𝑘𝑖+𝑘𝑗)2, 𝜇 is a renormalization scale, and 𝑄 is an arbitrary factorization scale which serves to separate the long- and short-distance behavior.

Because 𝒩=4 SYM theory is conformally invariant, the product of jet functions 𝐽 may be explicitly evaluated as [7] 𝐽𝑄2𝜇21,𝑎,𝜖=exp2=1𝑎𝜇2𝑄2𝜖𝛾()(𝜖)2+2𝒢0(),𝜖(2.3) where 𝛾() and 𝒢0() are the coefficients of the soft (or the Wilson line cusp) and collinear anomalous dimensions of the gluon, respectively. The explicit values for these anomalous dimensions may be obtained from the exact expressions for the planar four-gluon amplitude [7]: 𝛾(𝑎)==1𝑎𝛾()=4𝑎4𝜁2𝑎2+22𝜁4𝑎3𝒢+,0(𝑎)==1𝑎𝒢0()=𝜁3𝑎2+4𝜁5+103𝜁2𝜁3𝑎3+.(2.4) The soft function 𝐒 is given by [27, 29] 𝐒𝑠𝑖𝑗𝑄2,𝑄2𝜇2=,𝑎,𝜖P1exp2𝑄20𝑑𝜇2𝜇2𝚪𝑠𝑖𝑗𝑄2,𝑎𝜇2𝜇2,,𝑎,𝜖(2.5) where 𝚪𝑠𝑖𝑗𝑄2=,𝑎=1𝑎𝚪(),𝑎𝜇2𝜇2=𝜇,𝑎,𝜖2𝜇2𝜖𝑎,(2.6) suppressing the explicit dependence of Γ() on 𝑠𝑖𝑗/𝑄2 to lighten the notation.

At this point, we make the assumption that the soft anomalous dimension matrices Γ() all commute with one another. (This assumption was also used to simplify the IR divergences of QCD in [33]. The assumption is certainly valid through two loops, since Γ(2)=(1/4)𝛾(2)Γ(1), as shown in [28, 29]. In [32], it was established that Γ(3)=(1/4)𝛾(3)Γ(1) for the nonpure gluon contributions. Further, Γ(𝐿)=(1/4)𝛾(𝐿)Γ(1) has been conjectured to hold to all orders in [30, 31, 33, 50]. Difficulties may arise at four loops, however, due to the possibility of quartic Casimir’s terms [31, 32, 51, 52].) Therefore, the path ordering in (2.5) becomes irrelevant, allowing us to explicitly integrate it, obtaining𝐒𝑠𝑖𝑗𝑄2,𝑄2𝜇21,𝑎,𝜖=exp2=1𝑎𝜇2𝑄2𝜖𝚪().𝜖(2.7) Combining the exponents of the jet and soft functions into [27, 41] 𝐆()𝑁(𝜖)=2𝜇2𝑄2𝜖𝛾()𝜖2+2𝒢0()𝜖1𝟙+𝜖𝚪(),(2.8) we may express the four-gluon amplitude in the compact form||𝐴(𝜖)=exp=1𝑎𝑁𝐆()||(𝜖)𝐻(𝜖),(2.9) or equivalently ||𝐻(𝜖)=𝐿=0𝑎𝐿||𝐻(𝐿𝑓)=(𝜖)𝟙=1𝑎𝑁𝐅()||(𝜖)𝐴(𝜖).(2.10) where the matrices 𝐅()(𝜖) will be defined below. (Henceforth we suppress 𝑠𝑖𝑗, 𝑄, 𝜇, and 𝑎 in the arguments of the amplitudes.) Expanding (2.10) through three loops, we obtain the expressions given in [27, 41] ||𝐴(1)=1(𝜖)𝑁𝐅(1)||𝐴(𝜖)(0)+||𝐻(1𝑓),||𝐴(𝜖)(2)=1(𝜖)𝑁2𝐅(2)||𝐴(𝜖)(0)+1𝑁𝐅(1)||𝐴(𝜖)(1)+||𝐻(𝜖)(2𝑓),||𝐴(𝜖)(3)=1(𝜖)𝑁3𝐅(3)||𝐴(𝜖)(0)+1𝑁2𝐅(2)||𝐴(𝜖)(1)+1𝑁𝐅(1)||𝐴(𝜖)(2)+||𝐻(𝜖)(3𝑓),(𝜖)(2.11) which will be useful in extracting the IR-divergent terms of leading- and subleading-color amplitudes in the following section. (Note that, because of the presence of poles in 𝐅(𝜖), we will need to know positive powers of 𝜖 in the expansion of lower loop amplitudes to obtain all the IR-divergent contributions to the 𝐿-loop amplitude 𝐴().)

The equivalence of (2.9) and (2.10) follows if the matrices 𝐅()(𝜖) are defined through the equation 𝟙=1𝑎𝑁𝐅()(𝜖)exp=1𝑎𝑁𝐆()(𝜖)=𝟙.(2.12) First define the functional 𝑋[𝑀] via [7] 1+=1𝑎𝑀()exp=1𝑎𝑀()𝑋()[𝑀](2.13) so that 𝑋(1)[𝑀]=0,𝑋(2)[𝑀]=(1/2)[𝑀(1)]2,𝑋(3)[𝑀]=(1/3)[𝑀(1)]3+𝑀(1)𝑀(2), and so forth. This functional was defined for scalar functions 𝑀(), but we can also use it for commuting matrices. We have assumed that Γ() and therefore 𝐆() are mutually commuting, and thus so are 𝐅(), as a result of (2.12). Thus 𝟙=1𝑎𝑁𝐅()(𝜖)=exp𝐿=0𝑎𝑁𝐅()(𝜖)𝑋()[],𝐅(2.14) and so (2.12) is equivalent to 𝐅()(𝜖)=𝑋()[]𝐅+𝐆()(𝜖)(2.15) which defines 𝐅() recursively in terms of 𝐆() and 𝐅() with <. The explicit expressions up through three loops 𝐅(1)(𝜖)=𝐆(1)𝐅(𝜖),(2)1(𝜖)=2𝐅(1)(𝜖)2+𝐆(2)𝐅(2𝜖),(3)1(𝜖)=3𝐅(1)(𝜖)3𝐅(1)(𝜖)𝐅(2)(𝜖)+𝐆(3)(3𝜖).(2.16) agree (up to rescaling by a factor of 𝑁𝐿) with the expressions given in [27] when specialized to the case of 𝑔𝑔𝑔𝑔 in 𝒩=4 SYM theory.

2.2. 1/𝑁 Expansion of IR Divergences

In this subsection, we will use the results of the previous subsection to expand the IR-divergent contributions of the four-gluon amplitude in powers of 1/𝑁.

The 𝐿-loop color-ordered amplitudes may be written in a 1/𝑁 expansion as ||𝐴(𝐿)=(𝜖)𝐿𝑘=01𝑁𝑘||𝐴(𝐿,𝑘),(𝜖)(2.17) where |𝐴(𝐿,0) are the leading-color amplitudes, arising from planar diagrams and |𝐴(𝐿,𝑘), 1𝑘𝐿, are the subleading-color amplitudes, which include contributions from nonplanar diagrams as well. The single-trace amplitudes (𝑖=1,,6) only contain even powers of 1/𝑁 (relative to the leading-color amplitude), while the double-trace amplitudes (𝑖=7,,9) only contain odd powers of 1/𝑁.

We begin by expanding (2.9): ||𝐴(𝜖)=𝐿𝐿=0𝑘=0𝑎𝐿𝑁𝑘||𝐴(𝐿,𝑘)=(𝜖)=1𝑛1𝑛!𝑎𝐆()(𝜖)𝑁𝑛0=00𝑘0=0𝑎0𝑁𝑘0||𝐻(0,𝑘0).(𝜖)(2.18) In the derivation of (2.18), we assumed that the soft-anomalous dimension matrices are mutually commuting. We now assume further that the higher-loop soft-anomalous dimension matrices are all proportional to the one-loop soft-anomalous dimension matrix 𝚪()=𝛾()4𝚪(1)(assumption)(2.19) as has been conjectured (see footnote 1). This allows us to rewrite (2.8) as 𝐆()(𝜖)𝑁=12𝜇2𝑄2𝜖𝛾()(𝜖)2+2𝒢0()𝛾𝜖𝟙+()𝚪4𝜖(1).(2.20) The one-loop soft anomalous dimension matrix can be written [29]: 𝚪(1)1=𝑁44𝑖=1𝑗𝑖𝐓𝑖𝐓𝑗log𝑠𝑖𝑗𝑄2,(2.21) where 𝐓𝑖𝐓𝑗=𝑇𝑎𝑖𝑇𝑎𝑗 with 𝑇𝑎𝑖 the SU(𝑁) generators in the adjoint representation. On the basis of (1.7), it has the explicit form [48], 𝚪(1)+2=2𝛼00𝛿𝑁,0𝛽𝛾0(2.22) where ,𝛼=𝒮+𝒯000000𝒮+𝒰000000𝒯+𝒰000000𝒯+𝒰000000𝒮+𝒰000000𝒮+𝒯,𝛽=𝒯𝒰0𝒮𝒰𝒰𝒯𝒮𝒯00𝒯𝒮𝒰𝒮0𝒯𝒮𝒰𝒮𝒰𝒯𝒮𝒯0𝒯𝒰0𝒮𝒰𝛾=𝒮𝒰𝒮𝒯00𝒮𝒯𝒮𝒰0𝒰𝒯𝒰𝒮𝒰𝒮𝒰𝒯0𝒯𝒰0𝒯𝒮𝒯𝒮0𝒯𝒰,𝛿=2𝒮0002𝒰0002𝒯(2.23) with 𝑠𝒮=log𝑄2𝑡,𝒯=log𝑄2𝑢,𝒰=log𝑄2.(2.24) If the assumption (2.19) is valid, then the 1/𝑁 expansion of 𝐆()(𝜖)/𝑁 terminates after two terms 𝐆()(𝜖)𝑁=𝑔+1𝑁𝑓,(2.25) where 𝑔 and 𝑓 can be read from (2.20) and (2.22). We rewrite (2.18) as ||𝐴(𝜖)=𝐿𝐿=0𝑘=0𝑎𝐿𝑁𝑘||𝐴(𝐿,𝑘)=(𝜖)=1𝑛1𝑛!𝑎𝑔+𝑎𝑁𝑓𝑛0=00𝑘0=0𝑎0𝑁𝑘0||𝐻(0,𝑘0)(𝜖)(2.26) making all 𝑁 dependence explicit.

We now determine the power of the leading IR pole of |𝐴(𝐿,𝑘)(𝜖). Consider an individual term on the right-hand side of (2.26). By counting powers of 𝑎 and 1/𝑁, one sees that this term contributes to |𝐴(𝐿,𝑘)(𝜖), with 𝐿=0+=1𝑛,𝑘=𝑘0+𝑘1,(2.27) where 𝑘1 is the number of factors 𝑓 present in the term. From (2.20) and (2.22), it is apparent that 𝑔 has a double pole in 𝜖, but 𝑓 only has a single pole. The leading IR pole in the term under consideration is therefore 1/𝜖𝑝, where 𝑝=2=1𝑛𝑘1.(2.28) Combining (2.27) and (2.28), we find 2𝑝=2𝐿𝑘=1(1)𝑛+20𝑘0.(2.29) Since 𝑘00, the term in square brackets is nonnegative, and we conclude that ||𝐴(𝐿,𝑘)1(𝜖)𝒪𝜖2𝐿𝑘.(2.30) This behavior was previously conjectured in [41] and shown in [49] (subject to the assumptions stated above).

Next we review the derivation [41, 49] of the coefficient of the leading IR pole of |𝐴(𝐿,𝑘)(𝜖). Terms in (2.26) contribute to the leading IR pole only when the expression in square brackets in (2.29) vanishes, which occurs when 𝑛=0 for 2, and 0=𝑘0=0 (with 𝑛1 unconstrained). In other words, the leading IR divergences are given by [41, 49] ||𝑎𝐆𝐴(𝜖)exp(1)(𝜖)𝑁||𝐴(0)(leadingIRdivergence).(2.31)

Recalling that𝐆(1)(𝜖)𝑁=𝜇2𝑄2𝜖2𝜖21𝟙+𝜖+1𝛼00𝛿,𝑁𝜖0𝛽𝛾0(2.32) we use (2.31) to obtain the coefficient of the leading IR pole||𝐴(𝐿,𝑘)=(𝜖)(2)𝐿𝑘1𝑘!(𝐿𝑘)!𝜖2𝐿𝑘0𝛽𝛾0𝑘||𝐴(0)1+𝒪𝜖2𝐿𝑘1,(2.33) where the tree-level amplitudes are ||𝐻(0,0)=||𝐴(0)=4𝑖𝐾𝑠𝑡𝑢(𝑢,𝑡,𝑠,𝑠,𝑡,𝑢,0,0,0)𝑇,(2.34) where 𝑠=(𝑘1+𝑘2)2,𝑡=(𝑘1+𝑘4)2 and 𝑢=(𝑘1+𝑘3)2 are the usual Mandelstam variables, obeying 𝑠+𝑡+𝑢=0 for massless external gluons. The factor 𝐾, defined in (7.4.42)of [53], depends on the momenta and helicity of the external gluons and is totally symmetric under permutations of the external legs.

The leading IR pole of the planar amplitude is simply ||𝐴(𝐿,0)=((𝜖)2)𝐿𝐿!𝜖2𝐿||𝐴(0)1+𝒪𝜖2𝐿1.(2.35) The remaining IR divergences, from 𝒪(1/𝜖2𝐿1) to 𝒪(1/𝜖), are all proportional to |𝐴(0) and are given by the (generalized) ABDK equation [7] (see Appendix A of [49]).

We now write an explicit expression for the coefficients of the leading IR poles of subleading-color amplitudes. First we use (2.34) and (2.23) to show 𝛾𝑢𝑡𝑠𝑠𝑡𝑢111111𝑋=2(𝑠𝑌𝑡𝑋),𝛾𝛽=22+𝑌2+𝑍2111(2.36) with 𝑡𝑋=log𝑢𝑢,𝑌=log𝑠𝑠,𝑍=log𝑡.(2.37) Hence, the leading IR divergence of the subleading-color amplitudes is given by ||𝐴(𝐿,2𝑚+1)=(𝜖)4𝑖𝐾𝑠𝑡𝑢(1)𝐿12𝐿𝑚𝑋2+𝑌2+𝑍2𝑚(𝑠𝑌𝑡𝑋)(2𝑚+1)!(𝐿2𝑚1)!𝜖2𝐿2𝑚10000001111+𝒪𝜖2𝐿2𝑚2,(2.38)||𝐴(𝐿,2𝑚+2)=(𝜖)4𝑖𝐾𝑠𝑡𝑢(1)𝐿2𝐿𝑚1𝑋2+𝑌2+𝑍2𝑚(𝑠𝑌𝑡𝑋)(2𝑚+2)!(𝐿2𝑚2)!𝜖2𝐿2𝑚20001𝑋𝑌𝑍𝑋𝑌𝑍𝑌𝑍𝑍𝑋𝑋𝑌+𝒪𝜖2𝐿2𝑚3.(2.39) The results (2.38) and (2.39) were derived in [49], generalizing expressions derived in [41].

2.3. IR Divergences of 𝐴(𝐿,1)

In this subsection, we consider the subleading-color amplitude |𝐴(𝐿,1) and derive the first three terms in the Laurent expansion. (It is straightforward to obtain further terms in the Laurent expansion as needed.) Consider all terms in (2.26) for which the expression in square brackets in (2.29) is ≤2: ||𝐴(𝐿)=1(𝜖)𝑔𝐿!1+1𝑁𝑓1𝐿||𝐴(0)+1𝑔𝑁(𝐿1)!1+1𝑁𝑓1𝐿1||𝐻(1,1)+1(𝜖)𝑔(𝐿2)!1+1𝑁𝑓1𝐿2𝑔2+1𝑁𝑓2||𝐴(0)+1𝑔(𝐿1)!1+1𝑁𝑓1𝐿1||𝐻(1,0)+1(𝜖)𝑁2𝑔(𝐿2)!1+1𝑁𝑓1𝐿2||𝐻(2,2)((𝜖)+threeleadingIRpoles),(2.40) where we use (2.20) and (2.22) to write 𝑔1=𝜇2𝑄2𝜖2𝜖21𝟙+𝜖𝛼00𝛿,𝑓1=1𝜖𝜇2𝑄2𝜖,𝑔0𝛽𝛾02=𝜇2𝑄22𝜖𝛾(2)8𝜖2+𝒢0(2)𝛾2𝜖𝟙+(2)8𝜖𝛼00𝛿,𝑓2=𝛾(2)𝜇8𝜖2𝑄22𝜖.0𝛽𝛾0(2.41) To extract the |𝐴(𝐿,1) amplitude, we employ the identity𝑔1+1𝑁𝑓1𝐿||||1/𝑁piece=𝐿𝑔1𝐿1𝑓1+𝐿2𝑔1𝐿2𝑓1,𝑔1+𝐿3𝑔1𝐿3𝑓1,𝑔1,𝑔1+𝑓1,𝑔1,𝑔1,𝑔1,(2.42) in which the first term on the right-hand side has an expansion that starts with 1/𝜖2𝐿1, the second term has an expansion that starts with 1/𝜖2𝐿2, and so forth. Thus, keeping only the terms proportional to 1/𝑁 in (2.40), and only the first three terms in the Laurent expansion, we obtain||𝐴(𝐿,1)=1𝑔(𝐿1)!1𝐿1𝑓1||𝐴(0)+12𝑔(𝐿2)!1𝐿2𝑓1,𝑔1||𝐴(0)+1𝑔(𝐿1)!1𝐿1||𝐻(1,1)+1(𝜖)6𝑔(𝐿3)!1𝐿3𝑓1,𝑔1,𝑔1||𝐴(0)+1𝑔(𝐿2)!1𝐿2𝑓2||𝐴(0)+1𝑔(𝐿3)!1𝐿3𝑓1𝑔2||𝐴(0)+1𝑔(𝐿2)!1𝐿2𝑓1||𝐻(1,0)1(𝜖)+𝒪𝜖2𝐿4,(2.43)as obtained in [49].

2.4. IR Divergences of 𝐴(𝐿,𝐿)

In this subsection, we derive an expression for the coefficient of the IR divergences of the first two terms in the Laurent expansion of the most subleading-color amplitude |𝐴(𝐿,𝐿).

The only terms in (2.26) that contribute to |𝐴(𝐿,𝐿) are those with as many factors of 1/𝑁 as of 𝑎. Thus, only 𝑓1 and |𝐻(0,0) can contribute, giving||𝐴(𝐿,𝐿)=(𝜖)𝐿0=01𝐿0!𝑓𝐿01||𝐻(0,0),(𝜖)where𝑓1=1𝜖𝜇2𝑄2𝜖0𝛽𝛾0(2.44) exact to all orders in the 𝜖 expansion. Keeping just the first two terms in the Laurent expansion, we find ||𝐴(𝐿,𝐿)=1(𝜖)𝑓(𝐿1)!1𝐿11𝐿𝑓1||𝐴(0)+||𝐻(1,1)1(𝜖)+𝒪𝜖𝐿2=11(𝐿1)!𝜖𝐿10𝛽𝛾0𝐿1||𝐴(1,1)1(𝐿𝜖)+𝒪𝜖𝐿2.(2.45) This was derived in [49] and confirms the conjecture made in (4.45) and (4.46) of [41].

2.5. Exact Expressions at One and Two Loops

𝒩=4 SYM scattering amplitudes may be expressed in terms of planar and nonplanar scalar loop integrals. The two-loop four-gluon scattering amplitude was first computed by Bern et al. [54] (see also [36]). Explicit expressions for these IR-divergent integrals as the Laurent expansions in 𝜖 were later obtained by Smirnov in the planar case [55] and by Tausk in the nonplanar case [56]. In this subsection, we review these results and some formulas for the 1/𝑁 expansion of these divergences.

Recall from (2.17) that 𝐴(𝐿,𝑘)[𝑖] denotes the 𝐿-loop color-ordered amplitude which is subleading by a factor of 1/𝑁𝑘 in the 1/𝑁 expansion. Single-trace amplitudes are denoted by 𝑖=1,,6 and double-trace amplitudes by 𝑖=7,,9 (see (1.7)).

At one loop, the single-trace amplitudes are given by [34] 𝐴[1](1,0)=𝑀(1)(𝑠,𝑡)𝐴[1](0)=2𝑖𝐾𝐼4(1)(𝑠,𝑡)(2.46) with the other single-trace amplitudes 𝐴(1,0)[2] and 𝐴(1,0)[3] obtained by letting 𝑡𝑢, and 𝑠𝑢, respectively. The identities 𝐴(𝐿)[1]=𝐴(𝐿)[6], 𝐴(𝐿)[2]=𝐴(𝐿)[5], and 𝐴(𝐿)[3]=𝐴(𝐿)[4] are satisfied at all loop orders. In (2.46), 𝐼4(1)(𝑠,𝑡) denotes the scalar box integral 𝑀(1)1(𝑠,𝑡)=2𝑠𝑡𝐼4(1)𝐼(𝑠,𝑡),4(1)(𝑠,𝑡)=𝐼4(1)(𝑡,𝑠)=𝑖𝜇2𝜖e𝜖𝛾𝜋𝐷/2𝑑𝐷𝑝𝑝2𝑝𝑘12𝑝𝑘1𝑘22𝑝+𝑘42,(2.47) an explicit expression for which is given, for example, in [7].

The one-loop double-trace amplitudes are given by [34] 𝐴[7](1,1)=𝐴[8](1,1)=𝐴[9](1,1)𝐴=2[1](1,0)+𝐴[2](1,0)+𝐴[3](1,0)(2.48)𝐼=4𝑖𝐾4(1)(𝑠,𝑡)+𝐼4(1)(𝑡,𝑢)+𝐼4(1).(𝑢,𝑠)(2.49) Relation (2.48) follows from the one-loop U(1) decoupling identity [57].

At two loops, the leading-color single-trace amplitude is given by [54] 𝐴[1](2,0)=𝑀(2)(𝑠,𝑡)𝐴[1](0)=𝑖𝐾𝑠𝐼4(2)𝑃(𝑠,𝑡)+𝑡𝐼4(2)𝑃,(𝑡,𝑠)(2.50) where 𝐼4(2)𝑃(𝑠,𝑡) denotes the scalar double-box (planar) integral 𝑀(2)1(𝑠,𝑡)=4𝑠𝑡𝑠𝐼4(2)𝑃(𝑠,𝑡)+𝑡𝐼4(2)𝑃,𝐼(𝑡,𝑠)4(2)𝑃(𝑠,𝑡)=𝑖𝜇2𝜖e𝜖𝛾𝜋𝐷/22𝑑𝐷𝑝𝑑𝐷𝑞𝑝2(𝑝+𝑞)2𝑞2𝑝𝑘12𝑝𝑘1𝑘22𝑞𝑘42𝑞𝑘3𝑘42,(2.51) an explicit expression for which is given, for example, in [7]. The double-trace amplitude is [54] 𝐴[7](2,1)𝑠=2𝑖𝐾3𝐼4(2)𝑃(𝑠,𝑡)+2𝐼4(2)𝑁𝑃(𝑠,𝑡)+3𝐼4(2)𝑃(𝑠,𝑢)+2𝐼4(2)𝑁𝑃𝐼(𝑠,𝑢)𝑡4(2)𝑁𝑃(𝑡,𝑠)+𝐼4(2)𝑁𝑃𝐼(𝑡,𝑢)𝑢4(2)𝑁𝑃(𝑢,𝑠)+𝐼4(2)𝑁𝑃,(𝑢,𝑡)(2.52) and the subleading-color single-trace amplitude is [54] 𝐴[1](2,2)𝑠𝐼=2𝑖𝐾4(2)𝑃(𝑠,𝑡)+𝐼4(2)𝑁𝑃(𝑠,𝑡)+𝐼4(2)𝑃(𝑠,𝑢)+𝐼4(2)𝑁𝑃𝐼(𝑠,𝑢)+𝑡4(2)𝑃(𝑡,𝑠)+𝐼4(2)𝑁𝑃(𝑡,𝑠)+𝐼4(2)𝑃(𝑡,𝑢)+𝐼4(2)𝑁𝑃𝐼(𝑡,𝑢)2𝑢4(2)𝑃(𝑢,𝑠)+𝐼4(2)𝑁𝑃(𝑢,𝑠)+𝐼4(2)𝑃(𝑢,𝑡)+𝐼4(2)𝑁𝑃,(𝑢,𝑡)(2.53) where 𝐼4(2)𝑁𝑃(𝑠,𝑡) denotes the two-loop nonplanar integral 𝐼4(2)𝑁𝑃(𝑠,𝑡)=𝑖𝜇2𝜖e𝜖𝛾𝜋𝐷/22𝑑𝐷𝑝𝑑𝐷𝑞𝑝2(𝑝+𝑞)2𝑞2𝑝𝑘22𝑝+𝑞+𝑘12𝑞𝑘32𝑞𝑘3𝑘42,(2.54) an explicit expression for which is given in [56]. All the other single- and double-trace amplitudes 𝐴(2,𝑘)[𝑖] are obtained by making the appropriate permutations of 𝑠,𝑡, and 𝑢 in these expressions.

It is well known [7] that planar amplitudes have the property of uniform transcendentality. It is less obvious but nevertheless true [41] that subleading-color 𝒩=4 amplitudes at one and two loops (and presumably beyond) also have uniform transcendentality. What makes this surprising is that the nonplanar integral 𝐼4(2)𝑁𝑃(𝑠,𝑡) that contributes to 𝐴(2,1) and 𝐴(2,2) does not have uniform transcendentality [39, 58]. The subleading transcendentality parts, however, cancel out in the expressions (2.52) and (2.53). (The same thing happens for the two-loop four-point amplitude of 𝒩=8 supergravity [39, 58].)

The two-loop amplitudes obey the following group theory relations [59]: 𝐴[7](2,1)𝐴=2[1](2,0)+𝐴[2](2,0)+𝐴[3](2,0)𝐴[3](2,2),𝐴[8](2,1)𝐴=2[1](2,0)+𝐴[2](2,0)+𝐴[3](2,0)𝐴[1](2,2),𝐴[9](2,1)𝐴=2[1](2,0)+𝐴[2](2,0)+𝐴[3](2,0)𝐴[2](2,2)(2.55) and may be easily verified using (2.50), (2.52), and (2.53). In addition, we have 𝐴[1](2,2)+𝐴[2](2,2)+𝐴[3](2,2)=0,(2.56) also easily verified using (2.53). Together these equations imply63𝑖=1𝐴[𝑖](2,0)9𝑖=7𝐴[𝑖](2,1)=0(2.57) which is the two-loop generalization of the U(1) decoupling relation (2.48). Both (2.56) and (2.57) are encapsulated in the equation 63𝑖=1𝐴[𝑖](𝐿)𝑁9𝑖=7𝐴[𝑖](𝐿)=0,𝐿2,(2.58) which is valid through two loops.

At one loop, we also saw that one can relate all the subleading-color amplitudes 𝐴𝑛;𝑗 to the leading amplitude 𝐴𝑛;1 via the group theory relation (1.5).

We now list some explicit formulas for the IR-divergent pieces of one- and two-loop amplitudes that will be of use in the following section. At one loop, the leading 4-point amplitude is given by (2.46) with 𝑀(1)1(𝑠,𝑡)=𝜖2𝜇2𝑠𝜖1𝜖2𝜇2𝑡𝜖+12log2𝑠𝑡+2𝜋23+𝒪(𝜖),(2.59) while the exact relation (2.48) can be used to write both the IR-divergent and IR-finite contributions to the double-trace subleading-color amplitude||𝐴(1,1)=(𝜖)8𝑖𝐾𝜇𝑠𝑡𝑢2𝑢𝜖(𝑠𝑌𝑡𝑋)𝜖111(𝑠+𝑡)𝑋𝑌+𝒪(𝜖),(2.60) where we have only included the [79] components of 𝐴(1,1)[𝑖] as the others vanish.

At two loops, the planar amplitude is given by (2.50) with [60] 𝑀(2)1(𝜖)=2𝑀(1)(𝜖)2𝜁2+𝜖𝜁3+𝜖2𝜁4𝑀(1)𝜋(2𝜖)472+𝒪(𝜖).(2.61) The two-loop double trace amplitude has an IR divergence given by the general formula (2.38), which yields ||𝐴(2,1)=(𝜖)8𝑖𝐾𝑠𝑡𝑢(2)(𝑠𝑌𝑡𝑋)𝜖31111+𝒪𝜖2.(2.62) Finally, the subleading-color single-trace amplitude is given by (2.45) which in this case yields ||𝐴(2,2)=1(𝜖)𝜖𝐴𝑋𝑌𝑍𝑋𝑌𝑍𝑌𝑍𝑍𝑋𝑋𝑌[7](1,1)𝜖(2𝜖)+𝒪0.(2.63) Only the [1] through [6] components are listed, as the [7] through [9] components vanish.

3. Subleading-Color Amplitudes of 𝒩=4 SYM and Amplitudes of 𝒩=8 Supergravity

The AdS5/CFT4 correspondence provides a strong/weak duality between 𝒩=4 SYM and 𝒩=8 supergravity. These relationships have been extensively explored and exploited. There are also numerous indications of a weak/weak duality between the two theories, although this latter possibility is much less developed. Nevertheless this may be a very fruitful approach in attempts to understand relationships between the two theories. A lot of work has been done to relate the perturbation expansions of these two theories [15, 3438, 4146, 61, 62]. Part of this program is the extension of the tree-level KLT theories, but many relations have been found at loop level as well. Since this work is extensive, we will not attempt to review it all here. Since nonplanar graphs appear on an equal footing with planar graphs in 𝒩=8 supergravity, it seems important to understand nonplanar graphs in 𝒩=4 SYM if a weak-weak duality is to be explored. This is the focus of this section.

We will review the known exact relations between the 4-point functions of subleading 𝒩=4 SYM and those of 𝒩=8 supergravity, at one and two loops. For more than two loops, the known relation for 𝑛=4 is for the leading IR singularity only. One application of these ideas for 𝑛=5 at one loop is a new form of (tree level) KLT relations. Others are possible relations between 𝒩=4 subleading-color amplitudes and 𝒩=8 sugra for 𝑛5.

3.1. One and Two-Loop Relations

In this subsection, we demonstrate the existence of some exact relations between 𝒩=4 SYM amplitudes and 𝒩=8 supergravity amplitudes at the one- and two-loop levels. The 𝐿-loop 𝑁-independent SYM amplitude 𝐴(𝐿,𝐿) may be expected to be related to the 𝐿-loop supergravity amplitude, as both have 𝒪(1/𝜖𝐿) leading IR divergences. Other subleading-color SYM amplitudes 𝐴(𝐿,𝑘) have 𝒪(1/𝜖2𝐿𝑘) leading IR divergences and consequently satisfy relations involving lower-loop supergravity amplitudes. The normalization of 𝐴(𝐿,2𝑚+1)SYM(𝑠,𝑡) is arbitrary. We have chosen one that is most natural in the context of the SYM/supergravity relations presented in this subsection.

In this section we use the notation𝐴(𝐿,2𝑚)SYM(𝑠,𝑡)=𝑎𝐿𝐴[1](𝐿,2𝑚),𝐴(𝐿,2𝑚+1)SYM𝑎(𝑠,𝑡)=𝐿2𝐴[8](𝐿,2𝑚+1),(3.1) noting that the other components 𝐴(𝐿,𝑘)[𝑖] are obtained by permutations of 𝑠, 𝑡, and 𝑢. However, we omit the argument (𝑠,𝑡) for functions that are completely symmetric under permutations of 𝑠, 𝑡, and 𝑢.

Factor out the tree amplitude to define𝑀(𝐿,𝑘)SYM𝐴(𝑠,𝑡)=(𝐿,𝑘)SYM(𝑠,𝑡)𝐴(0)SYM,(𝑠,𝑡)(3.2) so that the coupling constant 𝑎𝐿 is now included in the definition of 𝑀(𝐿,𝑘)SYM(𝑠,𝑡), and where. 𝐴(0)SYM(𝑠,𝑡)=4𝑖𝐾.𝑠𝑡(3.3)

In what follows we denote 𝐴treeSYM(𝑖𝑗𝑘)=𝐴(𝑖𝑗𝑘) (see also (2.34)). Recall that the one-loop 𝑁-independent SYM four-gluon amplitude is given by (2.47), obtaining 𝐴(1,1)SYM=2𝑔2𝑖𝐾2𝑁8𝜋2(4𝜋e𝛾)𝜖𝐼4(1)(𝑠,𝑡)+𝐼4(1)(𝑡,𝑢)+𝐼4(1).(𝑢,𝑠)(3.4) The one-loop supergravity four-graviton amplitude may be expressed as [34, 36] 𝐴(1)SG=8𝑖𝐾2(𝜅/2)28𝜋2(4𝜋e𝛾)𝜖𝐼4(1)(𝑠,𝑡)+𝐼4(1)(𝑡,𝑢)+𝐼4(1).(𝑢,𝑠)(3.5)after stripping off a factor of (𝜅/2)2 for a four-point amplitude. The supergravity amplitude is proportional to 𝐾2 rather than 𝐾 due to the KLT relations [63] (a manifestation of the relation “closed string = (openstring)2”). This factor is also present in the tree-level supergravity amplitude, so we can factor it out as follows:𝐴(1)SG=𝐴(0)SG𝑀(1)SG=16𝑖𝐾2𝑀𝑠𝑡𝑢(1)SG.(3.6) Defining 𝜆SYM=𝑔2𝑁 and 𝜆SG=(𝜅/2)2, one observes that the one-loop SYM and supergravity amplitudes are related by𝑀(1,1)SYM(𝑠,𝑡)=2𝜆SYM𝜆SG𝑢𝑀(1)SG.(3.7) In other words, the ratio of the one-loop subleading-color SYM and the one-loop supergravity amplitudes (after factoring out the tree amplitudes) is simply proportional to the ratio of coupling constants, where we encounter the effective dimensionless coupling 𝜆SG𝑢 for supergravity because 𝜆SG is dimensionful.

Finally, rewrite (3.7) in the manifestly permutation-symmetric form13𝜆SG𝑢𝑀(1,1)SYM(𝑠,𝑡)+c.p.=2𝜆SYM𝑀(1)SG,(3.8) (where c.p. denotes cyclic permutations of 𝑠, 𝑡, and 𝑢) even though 𝑢𝑀(1,1)SYM(𝑠,𝑡) is already symmetric under permutations. A similar symmetrized relation can be written for the one-loop leading-color amplitude 𝜆SG𝑢𝑀(1,0)SYM(𝑠,𝑡)+c.p.=𝜆SYM𝑀(1)SG(3.9) obtained from the one-loop decoupling relation (2.48) together with (3.7).

Now turn to two loops. There are some relations between SYM and supergravity amplitudes that hold only for the IR-divergent terms. The easiest case to analyze is the two-loop 𝑁-independent SYM amplitude 𝐴(2,2)SYM(𝑠,𝑡), since, from (2.63), 𝐴(2,2)SYM(𝑠,𝑡)=2𝑎𝑋𝑌𝜖𝐴(1,1)SYM𝜖(2𝜖)+𝒪0.(3.10) This can be rewritten as𝑀(2,2)SYM𝜆(𝑠,𝑡)=2𝑎SYM𝜆SG𝑢𝑋𝑌𝜖𝑀(1)SG𝜖(2𝜖)+𝒪0,(3.11) where 𝑋=log(𝑡/𝑢),𝑌=log(𝑢/𝑠),𝑍=log(𝑠/𝑡), as in (2.37), thus obtaining a relation to the one-loop supergravity amplitude.

Using the relation 𝑀(2)SG(𝜖)=(1/2)[𝑀(1)SG(𝜖)]2+𝒪(𝜖0) between the one- and two-loop supergravity amplitudes [41, 58, 64, 65], we can write this as13𝜆SG𝑢2𝑀(2,2)SYM(𝑠,𝑡)+c.p.=2𝜆2SYM𝑀(2)SG,(3.12) where this relation is exact (!), as may be easily verified by using the exact expression for the 𝑁-independent SYM amplitude [54] and from (2.53) 𝑀(2,2)SYM𝑎(𝑠,𝑡)=2𝑠𝑡2𝑠𝐼4(2)𝑃(𝑠,𝑡)+𝐼4(2)𝑁𝑃(𝑠,𝑡)+𝐼4(2)𝑃(𝑠,𝑢)+𝐼4(2)𝑁𝑃𝐼(𝑠,𝑢)+𝑡4(2)𝑃(𝑡,𝑠)+𝐼4(2)𝑁𝑃(𝑡,𝑠)+𝐼4(2)𝑃(𝑡,𝑢)+𝐼4(2)𝑁𝑃𝐼(𝑡,𝑢)2𝑢4(2)𝑃(𝑢,𝑠)+𝐼4(2)𝑁𝑃(𝑢,𝑠)+𝐼4(2)𝑃(𝑢,𝑡)+𝐼4(2)𝑁𝑃(𝑢,𝑡)(3.13) and that for the two-loop supergravity amplitude [36] 𝑀(2)SG𝑠=3𝑡𝑢4(𝜅/2)28𝜋2(4𝜋e𝛾)𝜖2𝐼4(2)𝑃(𝑠,𝑡)+𝐼4(2)𝑁𝑃(𝑠,𝑡)+𝐼4(2)𝑃(𝑠,𝑢)+𝐼4(2)𝑁𝑃+(𝑠,𝑢)c.p.,(3.14) where 𝐼4(2)𝑃 and 𝐼4(2)𝑁𝑃 are the two-loop planar and nonplanar 4-point functions.

Now consider the two-loop subleading-color amplitude 𝑀(2,1)SYM. The two-loop decoupling relation (2.57) can be rewritten as2𝑢𝑀(2,1)SYM(𝑠,𝑡)+c.p.=6𝑢𝑀(2,0)SYM(𝑠,𝑡)+c.p..(3.15) Using the ABDK relation [60] 𝑀(2,0)SYM1(𝜖)=2𝑀(1,0)SYM(𝜖)2+𝑎𝑓(2)(𝜖)𝑀(1,0)SYM(2𝜖)+𝒪(𝜖),𝑓(2)𝜁(𝜖)=2+𝜖𝜁3+𝜖2𝜁4,(3.16) together with (3.9), we can rewrite (3.15) as13𝜆SG𝑢𝑀(2,1)SYM(𝑠,𝑡)+c.p.+12𝜆SG𝑢𝑀(1,0)SYM(𝑠,𝑡)2+c.p.=2𝜆2SYM8𝜋2(4𝜋e𝛾)𝜖𝑓(2)(𝜖)𝑀(1)SG(2𝜖)+𝒪(𝜖).(3.17) Unlike (3.12), however, (3.17) only holds through 𝒪(𝜖0), which relates to the one-loop supergravity amplitude rather than the two-loop one.

Note that (3.8) and (3.12) can be written as 13𝜆SG𝑢𝐿𝑀(𝐿,𝐿)SYM(𝑠,𝑡)+c.p.=2𝜆SYM𝐿𝑀(𝐿)SG(3.18) for 𝐿=0, 1, and 2. Can this relation be valid at higher loops? It turns out not to be the case, but we can still find some relations valid for 𝐿3.

3.2. Three or More Loops

On the supergravity side, there is an exact exponentiation formula [64, 65], which implies𝑀(𝐿)SG=1𝑀𝐿!(1)SG𝐿1+𝒪𝜖𝐿2=1𝐿!𝜆SG(𝑠𝑌𝑡𝑋)8𝜋2𝜖𝐿1+𝒪𝜖𝐿1.(3.19) Since the leading IR divergences of 𝐴(𝐿,𝐿) is 𝒪(1/𝜖𝐿), one can show that the following relations hold: 𝜆2SG𝑠2+𝑡2+𝑢23𝑘13𝜆SG𝑢𝑀(2𝑘+1,2𝑘+1)SYM(𝑠,𝑡;𝜖)+c.p.=𝜆2𝑘+1SYM22𝑘+1/2𝑀(2𝑘+1)!(2)SG1(𝜖)+6𝜆SG8𝜋22𝑠𝑋+𝑡𝑌+𝑢𝑍𝜖2𝑘𝑀(1)SG1(𝜖)+𝒪𝜖2𝑘,(3.20) for 𝐿=2𝑘+1𝜆2SG𝑠2+𝑡2+𝑢23𝑘13𝜆SG𝑢2𝑀(2𝑘+2,2𝑘+2)SYM(𝑠,𝑡;𝜖)+c.p.=𝜆2𝑘+2SYM22𝑘+2𝑀(2𝑘+2)!(2)SG1(𝜖)+6𝜆SG8𝜋22𝑠𝑋+𝑡𝑌+𝑢𝑍𝜖2𝑘𝑀(2)SG1(𝜖)+𝒪𝜖2𝑘+1(3.21) for 𝐿=2𝑘+2 (where 𝑘=0,1,2,).

That is, we have an exact relation at 𝐿-loops for the leading IR divergence ~𝒪(1/𝜖𝐿), with an untested relation for the subleading divergence of 𝒪(1/𝜖𝐿1); see also (2.45).

An interesting fact is that either (3.18) or (3.20) and (3.21) without the extra term, and also the relation (3.17), have a possible interpretation in terms of the ‘t Hooft string picture of the 1/𝑁 expansion. Thus at least in the case of 𝐿=1,2, (3.18) and (3.17) still do, so one can hope that there is a correct relation at higher 𝐿 yet to be determined.

3.3. New KLT Relations

One of the pioneering connections between SYM and supergravity theories are the KLT relations [63], originally proved using string theory methods [35, 63]. More recently, alternate versions of KLT relations have been presented based on field theoretic techniques at the tree level [44, 45]. One form of these new relations has manifest (𝑛3)! permutation symmetry for the 𝑛-point functions, and another has (𝑛2)! symmetry, but requires regularization as a consequence of singularities. They are part of a flurry of recent activity relating 𝒩=4 SYM and 𝒩=8 supergravity, including [40, 42, 43, 46, 61, 6668] (among older works see also [37, 69, 70]). Recent work applying the KLT relations includes [7174]. In our quest for SYM-supergravity relations, we first review previous KLT relations; we then note that 𝐴5;3 and the 1-loop supergravity amplitude both have 1/𝜖 IR divergences. We present here a tree-level KLT relation for the 𝑛=5-point amplitudes derived in [75], using information from one-loop SYM and supergravity amplitudes and their IR divergences. This results in a KLT relation for 5-point functions with 2(𝑛2)! manifest symmetry, without the need for regularization. These KLT relations are proved explicitly using the helicity spinor formalism and the Parke-Taylor formula. In analogy with Section 3.1 on 4-point functions of 𝒩=8 supergravity and subleading-color 𝒩=4 SYM theories, both with the 1/𝜖 IR divergence, we explore the possibility that the 1-loop 5-point supergravity amplitude can be expressed as a linear combination of the 𝐴5;3 SYM amplitudes. In particular a linear relation is proposed among the 1/𝜖 IR divergences of the two theories.

At tree level, the KLT relations are quadratic relations between the 𝑛-point amplitudes of 𝒩=4 SYM and those of 𝒩=8 supergravity. In these relations, the helicity information is all contained within the amplitudes, and the coefficients are all function of the kinematic invariants 𝑠𝑖𝑗 only.

These relations relate graviton tree amplitudes with sums of squares (products) of gauge tree amplitudes. The original KLT relations were derived from string theory in the 𝛼0 limit [35, 63] and can be expressed as (we use the notation of [37]) 𝐴tree𝑛,sugra(12𝑛)=(1)𝑛+1𝐴𝑛(12𝑛)perms𝑓𝑖1𝑖𝑗𝑓𝑙1𝑙𝑗×𝐴𝑛𝑖1,,𝑖𝑗,1,𝑛1,𝑙1,,𝑙𝑗𝑓𝑖,𝑛+𝒫(2,,𝑛2)1,,𝑖𝑗=𝑠1,𝑖𝑗𝑗1𝑚=1𝑠1,𝑖𝑚+𝑗𝑘=𝑚+1𝑔𝑖𝑚,𝑖𝑘,𝑓𝑙1,,𝑙𝑗𝑙=𝑠1,𝑛1𝑗𝑚=2𝑠𝑙𝑚+,𝑛1𝑚1𝑘=1𝑔𝑙𝑘,𝑙𝑚,(3.22) where “perms’’ are (𝑖1,,𝑖𝑗)𝒫(2,,𝑛/2),  (𝑙1,,𝑙𝑗𝒫(𝑛/2+1,,𝑛2),  𝑗=𝑛/21,𝑗=𝑛/22, and 𝑔𝑖,𝑗=𝑠𝑖𝑗 if 𝑖>𝑗 and zero otherwise.

In [44, 45], new forms of the KLT relations for any 𝑛-point function were found. They are both written in terms of the functions:𝒮𝑖1𝑖𝑘𝑗1𝑗𝑘=𝑘𝑡=1𝑠𝑖𝑡1+𝑘𝑞>𝑡𝜃𝑖𝑡,𝑖𝑞𝑠𝑖𝑡𝑖𝑞,𝒮𝑖1𝑖𝑘𝑗1𝑗𝑘=𝑘𝑡=1𝑠𝑗𝑡𝑛+𝑘𝑞<𝑡𝜃𝑗𝑞,𝑗𝑡𝑠𝑗𝑞𝑗𝑡,(3.23) where 𝜃(𝑖𝑡,𝑖𝑞) is zero in (𝑖𝑡,𝑖𝑞) has the same order in both sets ={𝑖1,,𝑖𝑘} and 𝒥={𝑗1,,𝑗𝑘} and is 1 otherwise, and similarly for 𝜃(𝑗𝑞,𝑗𝑡).

A form of KLT relations was found in [44], but needs to be regularized, due to a singular denominator 𝐴tree𝑛,sugra=(1)𝑛𝛾,𝛽𝐴𝑛𝑛,𝛾2,𝑛1𝒮𝛾,12,𝑛1,𝛽2,𝑛1𝑝1𝐴𝑛1,𝛽2,𝑛1,𝑛𝑠12𝑛1,𝐴tree𝑛,sugra=(1)𝑛𝛽,𝛾𝐴𝑛𝑛,𝛽2,𝑛1𝒮𝛽,12,𝑛1,𝛾2,𝑛1𝑝𝑛𝐴𝑛1,𝛾2,𝑛1,𝑛𝑠23𝑛.(3.24) However they have a large (𝑛2)! manifest symmetry. Another set was proven in [45] which is nonsingular 𝐴tree𝑛,sugra=(1)𝑛+1𝜎𝑆𝑛3𝛼𝑆𝑗1𝛽𝑆𝑛𝑗2𝐴𝑛1,𝜎2,𝑗,𝜎𝑗+1,𝑛2𝒮𝛼,𝑛1,𝑛𝜎(2),𝜎(𝑗)𝜎2,𝑗𝑝1×𝒮𝜎𝑗+1,𝑛2𝛽𝜎(𝑗+1),𝜎(𝑛2),𝑛𝑝𝑛𝐴𝑛𝛼𝜎(2),𝜎(𝑗),1,𝑛1,𝛽𝜎(𝑗+1),𝜎(𝑛1),𝑛(3.25) but with only (𝑛3)! manifest symmetry.

The original KLT relation for the 5-point function is𝐴tree5,sugra=𝑠12𝑠34𝐴(12345)𝐴(21435)+𝑠13𝑠24𝐴(13245)𝐴(31425)(3.26) and has (𝑛3)!=2! symmetry, whereas the KLT relations (3.25) become, explicitly, 𝐴tree5,sugra=𝜎,𝜎𝑆2𝐴45,𝜎23𝐴,11,𝜎23𝑆,45𝜎2,3𝜎2,3𝑝1=𝑠12𝑠13(𝐴(45231)𝐴(12345)+𝐴(45321)𝐴(13245))+𝑠13𝑠12+𝑠23𝐴(45231)𝐴(13245)+𝑠12𝑠13+𝑠23𝐴𝐴(45321)𝐴(12345),tree5,sugra=𝜎,𝜎𝑆2𝐴14,𝜎23𝐴,51,𝜎23𝑆𝜎,452,3𝜎2,3𝑝4=𝑠24𝑠34[]𝐴(12345)𝐴(14235)+𝐴(13245)𝐴(14325)+𝑠34𝑠24+𝑠23𝐴(12345)𝐴(14325)+𝑠24𝑠34+𝑠23𝐴(13245)𝐴(14235)(3.27) and have (𝑛3)!=2! symmetry.

We now derive another KLT relation for 5-point amplitudes using information about subleading one-loop amplitudes.

As we saw in (1.5), the 𝐴𝑛;𝑗 are related to the 𝐴𝑛;1 via group theory. In particular, for 5-point amplitudes, one has a single-trace amplitude 𝐴5;1 and a double-trace amplitude 𝐴5;3 related by [76] 𝐴5;3(45123)=𝜎COP4123𝐴5;1(𝜎(1),,𝜎(4),5).(3.28)

The single-trace amplitude is given by 𝐴5(1,0)(12345)𝐴5;11(12345)=4𝐴(12345)cyclic𝐹(1)𝑠,𝑡,𝑚2,(3.29) where𝐹(1)𝑠,𝑡,𝑚2=𝑠𝑡𝐼5(1)𝑠,𝑡,𝑚2(3.30) is the dimensionless one-mass box, and 𝐼(1)(𝑠,𝑡,𝑚2) is the 1-loop scalar box integral (2.47) with momenta 3,4 in the same corner and 𝑚2=𝑃2=(𝑝3+𝑝4)2.

Substituting in (3.28), we find 𝐴5;3(𝑓𝑔;𝑖𝑗)=𝑎𝑏𝑐𝑑𝑒30xedterms𝑠𝐹(𝑐𝑑𝑒;𝑎𝑏)𝑎𝑏𝑐𝑑𝑒;+;𝑓𝑔𝑖𝑗𝐴(𝑎𝑏𝑐𝑑𝑒)+𝑠𝑎𝑏𝑐𝑑𝑒;;𝑓𝑔𝑖𝑗.𝐴(𝑎𝑏𝑒𝑑𝑐)(3.31) Here 𝑠𝑎𝑏𝑐𝑑𝑒;±;𝑓𝑔𝑖𝑗 are signs, defined as follows. The relative sign is plus if 𝑎𝑏 belong to 𝑖𝑗, and minus otherwise, and the overall sign is plus if the permutation of 𝑖𝑗 inside 𝑎𝑏𝑐𝑑𝑒 is even, and minus if it is odd.

The 1-loop 𝒩=8 supergravity amplitude is [62], written in terms of the scalar 1 m box 𝐼(123,45) (with momenta 4,5 on the same corner of the box), and the dimensionless box 𝐹(123;45) is𝐴1-loop5,sugra12𝑞3𝑞2𝑞11=230perms𝑠𝑞2𝑞1𝑠12𝑠2𝑞3𝐴12𝑞3𝑞2𝑞1𝐴12𝑞3𝑞1𝑞2𝐹12𝑞3;𝑞2𝑞1(3.32) or𝐴1-loop5,sugra1(12345)=230perms𝐹(𝑐𝑑𝑒;𝑎𝑏)𝑠𝑐𝑑𝑠𝑑𝑒𝑠𝑎𝑏𝐴(𝑐𝑑𝑒𝑎𝑏)𝐴(𝑐𝑑𝑒𝑏𝑎).(3.33)

The IR behavior of the 1-loop 1 m scalar box is 𝐼4,1𝑚𝑠,𝑡,𝑚2=𝑟Γ𝑠12𝑠232𝜖2𝑠12𝜖+𝑠23𝜖𝑠45𝜖+nite𝑟𝐹(𝑐𝑑𝑒;𝑎𝑏)Γ𝜖2𝑠𝑐𝑑𝜖+𝑠𝑑𝑒𝜖𝑠𝑎𝑏𝜖+nite𝑟Γ=Γ(1+𝜖)Γ2(1𝜖),Γ(12𝜖)(3.34) where 𝐷=42𝜖.

3.3.1. IR Behavior of the Double-Trace 1-Loop SYM Amplitude 𝐴5;3

Using (3.34), we find𝐴5;3(𝑓𝑔;𝑖𝑗)=𝑎𝑏𝑐𝑑30terms𝑠𝐹(𝑐𝑑𝑒;𝑎𝑏)𝑎𝑏𝑐𝑑𝑒;+;𝑓𝑔𝑖𝑗𝐴(𝑎𝑏𝑐𝑑𝑒)+𝑠𝑎𝑏𝑐𝑑𝑒;;𝑓𝑔𝑖𝑗𝑟𝐴(𝑎𝑏𝑒𝑑𝑐)Γ𝜖2𝑎𝑏𝑐𝑑30terms𝑠𝜖𝑐𝑑+𝑠𝜖𝑑𝑒𝑠𝜖𝑎𝑏𝑠𝑎𝑏𝑐𝑑𝑒;+;𝑓𝑔𝑖𝑗𝐴(𝑎𝑏𝑐𝑑𝑒)+𝑠𝑎𝑏𝑐𝑑𝑒;;𝑓𝑔𝑖𝑗.𝐴(𝑎𝑏𝑒𝑑𝑐)(3.35) Organizing the coefficients of each divergence, we find𝐴5;3𝑟(𝑓𝑔;𝑙𝑚𝑛)Γ𝜖2𝑖<𝑗𝑠𝑖𝑗𝜖𝑎𝑏𝑐𝑖,𝑗𝜖𝑙𝑚𝑛[],𝐴(𝑖𝑗𝑎𝑏𝑐)(3.36) where 𝜖𝑙𝑚𝑛[𝐴(𝑖𝑗𝑎𝑏𝑐)] means 𝐴(𝑖𝑗𝑎𝑏𝑐) is multiplied by the sign of the permutation of 𝑙,𝑚,𝑛 inside 𝑖,𝑗,𝑎,𝑏,𝑐, and the sum over 𝑎,𝑏,𝑐 contains all the 6 terms of the arbitrary permutation of the 𝑎,𝑏,𝑐𝑖,𝑗.

The leading (1/𝜖2) divergence of 𝐴5;3(45;123), given by 𝑖<𝑗𝑎𝑏𝑐𝑖,𝑗𝜖123[],𝐴(𝑖𝑗𝑎𝑏𝑐)(3.37) vanishes by explicit computation, so that the leading IR divergence of 𝐴5;3 is 1/𝜖, as expected from a generalization of the subleading-color amplitude of the 4-gluon amplitude [39, 49]. (The vanishing of the 1/𝜖2 IR divergence of (3.37) is also a consequence of (4.7).)

3.3.2. IR Behavior of 𝒩=8 Supergravity One-Loop Amplitudes and KLT Relations

Using (3.32), we obtain𝐴1-loop5,sugra1(12345)=230perms𝐹(𝑐𝑑𝑒;𝑎𝑏)𝑠𝑐𝑑𝑠𝑑𝑒𝑠𝑎𝑏1𝐴(𝑐𝑑𝑒𝑎𝑏)𝐴(𝑐𝑑𝑒𝑏𝑎)2𝜖230perms𝑠𝜖𝑐𝑑+𝑠𝜖𝑑𝑒𝑠𝜖𝑎𝑏𝑠𝑐𝑑𝑠𝑑𝑒𝑠𝑎𝑏𝐴(𝑐𝑑𝑒𝑎𝑏)𝐴(𝑐𝑑𝑒𝑏𝑎).(3.38) Organizing the terms by IR divergences, we obtain 𝐴1-loop5,sugra1𝜖2𝑖<𝑗𝑠1𝜖𝑖𝑗×𝑑𝑠𝑐𝑑𝑠𝑑𝑒𝐴(𝑖𝑗𝑐𝑑𝑒)𝐴(𝑖𝑗𝑒𝑑𝑐)+𝑐𝑠𝑖𝑐𝑠𝑎𝑏+𝐴(𝑖𝑗𝑎𝑏𝑐)𝐴(𝑖𝑗𝑏𝑎𝑐)𝑐𝑠𝑗𝑐𝑠𝑎𝑏.𝐴(𝑖𝑗𝑐𝑏𝑎)𝐴(𝑖𝑗𝑐𝑎𝑏)(3.39)

On the other hand, we know that the IR behavior of the 1-loop 𝑛-point supergravity amplitude is [77] 𝐴1-loop𝑛,sugra1(1𝑛)𝜖2𝐴tree𝑛,sugra(1𝑛)𝑖<𝑗𝑠1𝜖𝑖𝑗(3.40) which means that we must have the KLT relation 𝐴tree5,sugra(12345)=𝑑𝑠𝑐𝑑𝑠𝑑𝑒𝐴(𝑖𝑗𝑐𝑑𝑒)𝐴(𝑖𝑗𝑒𝑑𝑐)+𝑐𝑠𝑖𝑐𝑠𝑎𝑏+𝐴(𝑖𝑗𝑎𝑏𝑐)𝐴(𝑖𝑗𝑏𝑎𝑐)𝑐𝑠𝑗𝑐𝑠𝑎𝑏𝐴(𝑖𝑗𝑐𝑏𝑎)𝐴(𝑖𝑗𝑐𝑎𝑏),(𝑖𝑗).(3.41) Note that it has the larger manifest symmetry of 2×(𝑛2)!=2×3! and has no need to be regularized.

The tree-level KLT formula (3.41) has been derived using the IR behavior of 1-loop computations. However it can be proved explicitly. To do so, use the helicity spinor formalism and the Parke-Taylor formula [78], which states that𝐴tree𝑛,SYM1+2+𝑖𝑗𝑛+=𝑖𝑗4,1223𝑛1(3.42) or for our case, for instance choosing 12, 𝐴123+4+5+=124.1223344551(3.43) A similar formula exists for the supergravity amplitude [37] 𝐴tree5,sugra123+4+5+=128𝜖(1234),𝑁(5)(3.44) where𝜖(𝑖𝑗𝑘𝑙)=4𝑖𝜖𝜇𝜈𝜌𝜎𝑘𝜇𝑖𝑘𝜈𝑗𝑘𝜌𝑘𝑘𝜎𝑙,𝑁(5)=45𝑖=1𝑗=𝑖+1𝑖𝑗.(3.45)

A specific case of (3.41) is proved, namely,𝐴tree5,sugra(12345)=𝑠34𝑠45𝐴(12345)𝐴(12543)+𝑠53𝑠34𝐴(12534)𝐴(12435)+𝑠45𝑠53𝐴(12453)𝐴(12354)+𝑠23𝑠45𝐴(12345)𝐴(12354)+𝑠24𝑠35𝐴(12435)𝐴(12453)+𝑠25𝑠34𝐴(12534)𝐴(12543)+𝑠13𝑠45𝐴(21345)𝐴(21354)+𝑠14𝑠35𝐴(21435)𝐴(21453)+𝑠15𝑠34𝐴(21534)𝐴(21543).(3.46) The others follow from permutations and symmetry.

One makes use of helicity spinor identities to verify that the right-hand side of (3.46) is equal to (3.44), proving the KLT relation.

3.3.3. Relation between 𝐴one-loop5,sugra and 𝐴5;3

Motivated by the fact that the leading IR divergence of the 𝑛=5-point supergravity amplitude and that of 𝐴5;3 are both of order 1/𝜖 at 1 loop, one investigates whether 𝐴1-loop5,sugra can be expressed as a linear combination of 𝐴5;3 amplitudes. One uses information from (3.34) to (3.38) and finds a relation valid for IR divergences, and then one conjectures how one possibly could extend to a relation for the full amplitudes.

Based on what happened at 4 points at 1 and 2 loops, as discussed in Section 3.1, we want to find 𝐴1-loop5,sugra as a linear combination of the 𝐴5;3 amplitudes.

In analogy with the 4-point function, we would like to find a relation of the type𝐴1-loop5,sugra(12345)=𝑖𝑓𝑔𝑖𝑗𝛽𝑖𝐴5;3=(𝑖)𝑎𝑏𝑐𝑑𝑒30xedterms𝐹(𝑐𝑑𝑒;𝑎𝑏)𝑖𝑓𝑔𝑖𝑗𝛽𝑖𝑠𝑎𝑏𝑐𝑑𝑒;+;𝑖𝐴(𝑎𝑏𝑐𝑑𝑒)+𝑠𝑎𝑏𝑐𝑑𝑒;;𝑖.𝐴(𝑎𝑏𝑒𝑑𝑐)(3.47) On the other hand, 𝐴1-loop5,sugra(12345)=𝑎𝑏𝑐𝑑𝑒30xedterms𝐹(𝑐𝑑𝑒;𝑎𝑏)𝛼𝑎𝑏𝑐𝑑𝑒,(3.48) where from (3.33), 𝛼𝑎𝑏𝑐𝑑𝑒1=2𝑠𝑐𝑑𝑠𝑑𝑒𝑠𝑎𝑏𝐴(𝑐𝑑𝑒𝑎𝑏)𝐴(𝑐𝑑𝑒𝑏𝑎)(3.49) which means that we need 𝛼𝑎𝑏𝑐𝑑𝑒=𝑖𝑓𝑔𝑖𝑗𝛽𝑖𝑠𝑎𝑏𝑐𝑑𝑒;+;𝑖𝐴(𝑎𝑏𝑐𝑑𝑒)+𝑠𝑎𝑏𝑐𝑑𝑒;;𝑖𝐴(𝑎𝑏𝑒𝑑𝑐)(3.50) to be satisfied, which are 30 equations for 10 unknowns (𝛽𝑖), so (3.50) is not guaranteed to have solutions.

The 30 equations can then be rewritten, using the explicit form of 𝛼𝑎𝑏𝑐𝑑𝑒, and a new notation that will prove useful, as 12𝑠𝑎𝑏𝑠𝑏𝑐𝑠𝑑𝑒𝐴(𝑎𝑏𝑐𝑑𝑒)𝐴(𝑎𝑏𝑐𝑒𝑑)=𝑓𝑔;𝑖𝑗𝛽(𝑓𝑔)𝜖𝑖𝑗[]𝐴(𝑎𝑏𝑐𝑑𝑒)1𝜖𝑖𝑗(𝑑𝑒)𝐴(𝑎𝑏𝑐𝑒𝑑),𝐴(𝑎𝑏𝑐𝑑𝑒)(3.51) where 𝜖𝑖𝑗(𝑑𝑒) is plus if both 𝑑,𝑒 belong to ,𝑖,𝑗, and minus otherwise.

In order to see if a unique solution for the 𝛽𝑖 is possible, one can match the IR behaviors on the two sides of (3.47). Expressing the IR behaviors of the lhs and the rhs, 1𝜖2𝐴tree5,sugra(12345)𝑖<𝑗𝑠𝑖𝑗𝑠𝑖𝑗𝜖=𝑟Γ𝜖2𝑘𝑓𝑔;𝑙𝑚𝑛𝛽𝑘𝑖<𝑗𝑠𝑖𝑗𝜖𝑎𝑏𝑐𝑖,𝑗𝜖𝑙𝑚𝑛[]𝐴(𝑖𝑗𝑎𝑏𝑐)(3.52) which means that one requires, using the vanishing of the 1/𝜖2 IR divergence, 𝐴tree5,sugra(12345)𝑠𝑖𝑗=𝑘𝑓𝑔;𝑙𝑚𝑛𝛽𝑘𝑎𝑏𝑐𝑖,𝑗𝜖𝑙𝑚𝑛[].𝐴(𝑖𝑗𝑎𝑏𝑐)(3.53) If we denote the 𝐴tree5,sugra(12345) by just 𝑀5, then the lhs is a vector column of (𝑖𝑗),𝑀5𝑠𝑖𝑗. Also denote 𝑎𝑏𝑐𝑖,𝑗𝜖𝑙𝑚𝑛[𝐴(𝑖𝑗𝑎𝑏𝑐)] as 𝑁(𝑖𝑗),(𝑓𝑔), so that𝑁(𝑖𝑗),(𝑓𝑔)𝛽(𝑓𝑔)=𝑀5𝑠𝑖𝑗𝛽(𝑓𝑔)=𝑁(𝑖𝑗),(𝑓𝑔)1𝑀5𝑠𝑖𝑗.(3.54) Note that the index (𝑓𝑔) on the matrix 𝑁 has 10 values, and these values can also be identified by the 𝑙𝑚𝑛 of 𝜖𝑙𝑚𝑛[𝐴(𝑖𝑗𝑎𝑏𝑐)], since it corresponds to the same 10 terms, picking out a group (𝑓𝑔) or (𝑙𝑚𝑛) out of 1,2,3,4,5.

At this point, however, note that the vanishing of the leading IR divergence in (3.37) means that (𝑖𝑗)𝑁(𝑖𝑗),(𝑓𝑔)=0,(3.55) that is, that the matrix 𝑁 has rank 9 instead of 10. One then needs to work with the corresponding 9×9 reduced matrix 𝑁red;(𝑖𝑗),(𝑓𝑔) and give the 10th coefficient 𝛽(𝑓𝑔) an arbitrary value.

Therefore one has found a linear relation, (3.47), with coefficients obtained from (3.54), which is satisfied by the IR divergences, and containing an arbitrary parameter. Of course, it is still not clear that the remaining 𝛽(𝑓𝑔) are unique. For that, one must calculate the rank of 𝑁red. If its rank is less than 9, the solution is parametrized by more than one parameter, since then some of the remaining 𝛽’s will be undetermined. As the algebra is quite involved, this is a project for further work.

In order to see if (3.47) is also satisfied for the full amplitude, one must substitute the solution for 𝛽(𝑓𝑔) back in (3.51) and see if these equations are satisfied, since now one needs to check whether the 30 equations are satisfied by substituting the 10 unknowns 𝛽(𝑓𝑔) solved as in (3.54). The verification of (3.47) for 𝑛=5 is analogous with that for the (successful) relation (3.9) for 𝑛=4. Therefore, it would be interesting if (3.47), (3.50) were true. (As (3.18) exemplifies for 𝐿=1,𝑛=4, (3.47) may not be the only equation relating 𝒩=8 supergravity to 𝒩=4 SYM for 𝐿=1,𝑛=5.)

In principle the strategy described above can be applied to higher 𝑛-point amplitudes. Namely, one can analyze the IR behavior of the results for 𝒩=4 SYM and 𝒩=8 supergravity at 1 loop and compare these to the known behavior, which would imply a relation among tree amplitudes from SYM and a KLT-type relation from the supergravity. Finally, one can relate the subleading-color SYM and supergravity amplitudes and use the consistency of the IR behavior to fix the proposed relation. For 𝑛=6,𝐿=1, the results of Bjerrum-Bohr et al. [38] are suitable for this purpose.

4. Geometric Interpretations of Subleading-Color Amplitudes

4.1. Polytope Picture
4.1.1. Polytopes for MHV Leading Amplitudes

In [79], a simple picture was found for the 1-loop color-ordered leading amplitudes of 𝒩=4 SYM theory, in terms of the volume of a closed polytope in 𝐴𝑑𝑆5. In [80], it was generalized to subleading-color amplitudes. The picture for the leading MHV amplitude was obtained as follows. We start by writing the amplitude in a space dual to momenta, thus trivializing momentum conservation 𝑖𝑝𝑖=0, by 𝑝𝑖=𝑥𝑖𝑥𝑖+1. Then, for example, the 1-loop dimensionless massless box function (in 4 dimensions, which is of course IR divergent) 𝐹0𝑚(1234)=(1/2)𝑠𝑡𝐼4(1)(𝑠,𝑡), with 𝐼4(1)(𝑠,𝑡) in (2.47) becomes𝐹0𝑚𝑑(1,2,3,4)=𝑖4𝑥02𝜋2𝑥1𝑥32𝑥2𝑥42𝑥0𝑥12𝑥0𝑥22𝑥0𝑥32𝑥0𝑥42.(4.1)

We then construct 𝑥𝛼̇𝛼=𝑥𝜇(𝜎𝜇)𝛼̇𝛼 and finally map𝑥𝛼̇𝛼𝑋𝐴𝐵=12𝜖𝛼𝛽𝑥2𝑖𝑥𝛼̇𝛽𝑖𝑥𝛽̇𝛼𝜖̇𝛽̇𝛼.(4.2) Here the 𝑋’s, satisfying 𝑋212𝜖𝐴𝐵𝐶𝐷𝑋𝐴𝐵𝑋𝐶𝐷𝑋=0,𝑖𝑋𝑗𝑥=𝑖𝑥𝑗2(4.3) are coordinate patches on the quadric 𝑋𝑋=0 in 𝑅𝑃5, with 𝑋𝐴𝐵𝜆𝑋𝐴𝐵 being their homogeneous coordinates. These 𝑋’s are considered as vertices situated at the boundary of an AdS5 and are simple bitwistors living in twistor space, that is, there exist twistors 𝐴𝐴 and 𝐵𝐵 such that 𝑋𝐴𝐵=𝐴[𝐴𝐵𝐵] (a twistor 𝐴𝐴 is made of (𝐴𝛼,𝐴̇𝛼)).

Consider a box function characterized by vertices 𝑋1,𝑋2,𝑋3,𝑋4. Then the following function of the Feynman parameters 𝛼𝑖(0,1) with 𝛼𝑖=1, 𝑋(𝛼)=𝛼1𝑋1+𝛼2𝑋2+𝛼3𝑋3+𝛼4𝑋4,(4.4) is a map to 𝑅𝑃5, but such that 𝑋(𝛼)𝑋(𝛼)0, and in fact they vary over a tetrahedron in 𝑅𝑃5. After normalizing by 𝑌(𝛼)=𝑋(𝛼),𝑋(𝛼)𝑋(𝛼)(4.5) one obtains 𝑌(𝛼)𝑌(𝛼)=1, which means that 𝑌(𝛼) lies in the Euclidean AdS5. Since straight lines 𝑋(𝛼) are mapped to geodesics in AdS5, the edges and faces of the tetrahedron in AdS5 are geodesic, which by definition makes the tetrahedron ideal.

The value of the IR-finite 4-mass box matches twice the volume of the tetrahedron in AdS5. The IR-divergent lower mass functions need to be regularized, either in dimensional regularization, or using a mass regularization as in [79], modifying 𝑋2=0 to 𝑋𝑋=𝜇2(𝑋𝐼), with 𝐼 being a fixed point (a useful choice of 𝐼 is 𝑋𝑖𝐼=1,forall𝑖).

The one-loop MHV  𝑛-point amplitudes divided by the tree MHV amplitudes are given by the sum of 1-mass and 2-mass easy box functions with coefficient one, which add up to the volume of a closed 3-dimensional polytope (without a boundary) with 𝑛 vertices.

Note that by this definition, the volume of a tetrahedron comes with a sign, determined by the order of the dual space vertices 𝑥𝑖 in the box function 𝐹(𝑖,𝑗,𝑘,𝑙). That also induces an orientation (sign) for the triangular faces of the tetrahedron, determined by whether the missing vertex from (𝑖𝑗𝑘𝑙) is in an even or odd position. Faces with same vertices and different orientation (sign) can be glued together, forming a continuous object.

4.1.2. Polytopes for MHV Subleading-Color Amplitudes

For subleading-color amplitudes, we want to use (1.5) to relate to the leading amplitudes and expand in the KK basis (1.2), where we will obtain a nice geometrical interpretation.

We start with the 5-point amplitude as an example. The ratio of the leading 1-loop MHV to the tree level MHV amplitudes is the volume of a boundary of a 4-simplex, 𝐴MHV5;1(12345)𝐴MHV5(12345)𝑀MHV5(12345)=cyclic𝐼𝑥1,𝑥2,𝑥3,𝑥4,𝑥5𝑥𝑉1,𝑥2,𝑥3,𝑥4,𝑥5.(4.6) Here 𝐼(𝑥1,𝑥2,𝑥3,𝑥4,(𝑥5)) is the volume of the tetrahedron with vertices 𝑥1,𝑥2,𝑥3,𝑥4, equal to 𝐹(1,2,3,4), and the missing vertex (𝑥5) is added in brackets since the cyclicity involves all 5 points; 𝑉(𝑥1,𝑥2,𝑥3,𝑥4,𝑥5) is the volume of the boundary of the 4-simplex in twistor space, with (𝑦)𝑖(𝑌)𝑖; that is, we map the arguments of 𝑉 into twistor space.

Using (1.5) and writing the tree amplitudes in terms of the KK basis, we obtain 𝐴5;3(12345)=𝐴5𝑀(12345)5(12345)𝑀5+𝑀(41235)5(43125)𝑀5(31245)+𝐴5(𝑀12435)5(12435)𝑀5(+𝑀31245)5(34125)𝑀5(41235)+𝐴5𝑀(14235)5(14235)𝑀5+𝑀(31425)5(34125)𝑀5(41235)+𝐴5(𝑀13245)5(23145)𝑀5(+𝑀42315)5(43125)𝑀5(31245)+𝐴5𝑀(13425)5(23145)𝑀5+𝑀(31425)5(43125)𝑀5(24315)+𝐴5(𝑀14325)5(23145)𝑀5(+𝑀31425)5(34125)𝑀5(.23415)(4.7) We see that for each KK basis member we have the sums of two terms which are some simple differences of 𝑀5’s. In fact these differences can be written as the differences of two polytope volumes, which in turn can be written as the volume of a simple polytope. For instance, the coefficient of the KK basis element 𝐴5(12345) in (4.7) is𝑀MHV5(12345)𝑀MHV5+𝑀(41235)MHV5(43125)𝑀MHV5=𝑉𝑥(31245)1,𝑥2,𝑥3,𝑥4,𝑥5𝑥𝑉4𝑥5+𝑥1,𝑥1,𝑥2,𝑥3,𝑥4+𝑉𝑥4,𝑥1+𝑥4𝑥5,𝑥1,𝑥1𝑥3+𝑥4,𝑥2𝑥3+𝑥4𝑥𝑉1,𝑥1𝑥3+𝑥4,𝑥2𝑥3+𝑥4,𝑥4,𝑥5.(4.8) In the two brackets, the two volumes of opposite sign correspond to polytopes with 𝑛1=4 points common out of 𝑛=5, and the relative sign is such that we can write this as the volume of the polytope obtained by the taking the union of the two polytopes.

By examining the 𝑛=6 case [80] as well, we can understand the general pattern for 𝐴𝑛;3. The general formula is 𝐴MHV𝑛;3(𝑛1,𝑛,1,2,.,𝑛2)={𝜎}𝑖OP𝛽{𝛼},𝑇𝑗max𝐴MHV𝑛1,{𝜎}𝑖×,𝑛𝑛1{𝛼},{𝛽};𝑗max{𝛼},{𝛽}()𝑛𝛽𝑀MHV𝑛({𝛽},1,{𝛼},𝑛)(4.9) with 𝑀MHV𝑛 being the volume of a closed polytope and pairs of opposite sign 𝑀𝑛’s adding up to another closed polytope. It is obtained as follows. In the above, just from (1.5), we have 𝑀𝑛({𝛽},1,{𝛼},𝑛), where 𝑛1 is either in {𝛼} or in {𝛽}, and otherwise {𝛼} contains 2,3,,𝑘 and {𝛽} contains 𝑘+1,,𝑛2.

For the tree amplitude prefactors, when using the KK relations (1.2), from {𝛼} and {𝛽} we form the permutation {𝜎}𝑖 which contains {𝛼} and {𝛽𝑇}, keeping the ordering, that is, in the KK basis amplitude, we have 𝐴(1,{𝜎},𝑛). Here if we extract the 𝑛1, then {𝛼}=2,,𝑗max is ordered; that is, it goes from left to right in the permutation, and then {𝛽}=𝑗max+1,,𝑛2 is transposed and still ordered; that is, it goes from right to left. The same 𝑗max (extracted from the resulting KK basis member) is obtained from either 𝑘 or 𝑘+1. That means that there are exactly 4 terms corresponding to the same KK basis member, corresponding to both 𝑗max and 𝑛1 belonging to either {𝛼} or {𝛽}.

The sign of the terms is obtained from the sign in the KK relations (1.2), that is, (1)𝑛𝛽, where here {𝛽} refers to the individual 𝑀𝑛({𝛽},1,{𝛼},𝑛) term. The fact that 𝑗max belongs to either {𝛼} or {𝛽} means that in 𝑀𝑛({𝛽},1,{𝛼},𝑛) we have 𝑗max either at the end of {𝛼}, or at the beginning of {𝛽}; that is, we have a flip of 𝑗max𝑛 versus 𝑛𝑗max in between terms with different signs, hence a different 𝑛𝛽 (with or without 𝑗max). The exception is when actually (𝑛1) is at the end of {𝛼}, and not 𝑗max, in which case the same flip is now (𝑛1)𝑛 versus 𝑛(𝑛1), and the same relative minus sign applies.

Since the pair in the difference in the () bracket multiplying KK basis members has the same 𝑛2 permutation, and the remaining two terms are flipped, we have the difference of two 𝑛-polytopes with a common 𝑛1-polytope, just as in the 5-point case.

We can generalize to 𝐴𝑛;𝑗 also, obtaining𝐴MHV𝑛;𝑗(=𝑛𝑗+2,,𝑛,1,,𝑛𝑗+1){𝜎}𝑖OP𝛽{𝛼},𝑇𝑗max{1,,𝑛𝑗+1},𝑙max{𝑛𝑗+2,,𝑛1}𝐴MHV𝑛1,{𝜎}𝑖×,𝑛{𝑛1,,𝑛𝑗+2}{𝛼},{𝛽};𝑗max{𝛼},{𝛽}()𝑛𝛽+𝑗1𝑀MHV𝑛({𝛽},1,{𝛼},𝑛),(4.10) where again we have pairs of 𝑀MHV𝑛’s of different signs and with 𝑛1 common vertices adding up to give other closed polytopes (of 𝑛+1 vertices).

The new features with respect to the 𝐴𝑛;3 are as follows. The KK basis elements that we get are of a special type: if we take out 𝑛1,,𝑛𝑗+2 from the amplitude, then the situation should be like the one for 𝑛=3, namely, in the remaining permutation we go from 1 to a 𝑗max towards the right, and then towards the left. But moreover, in 𝑛1,,𝑛𝑗+2, we also have some ordering: some of them are in {𝛼}, some in {𝛽𝑇}, which means that 𝑛1,,𝑙max+1 is cyclic (i.e., towards the right), and 𝑛𝑗+2,,𝑙max is also cyclic (i.e., we change the direction of the cyclicity at 𝑙max).

The number of terms multiplying a KK basis member is even, corresponding to having 𝑗max in {𝛼} or {𝛽} and any number of the 𝑗2 terms {𝑛1,,𝑛𝑗+2} in {𝛼} and the rest in {𝛽}. They come in pairs, the pairs corresponding to 𝑗max being just before 𝑛 or just after, or otherwise one of the {𝑛1,,𝑛𝑗+2} being either just before, or just after 𝑛, and the pairs as before having different sign. The sign of the terms is then simply (1)𝑗1+𝑛𝛽. In terms of polytopes, the two terms of different sign correspond as before to polytopes with only a vertex differing between them, which means they again add up to another polytope with one more vertex.

As a simple application of this analysis, we note that (4.7), (4.9), and (4.10) show that the amplitudes 𝑀𝑛 come in alternating pairs. Each of these 𝑀𝑛 has leading IR singularity 1/𝜖2+𝒪(1/𝜖) and therefore at one-loop 𝐴𝑛,𝑗 has only a 1/𝜖 IR singularity.

4.1.3. Polytope Picture for the 6-Point Leading 𝑁MHV Amplitude

The leading (planar) gluon amplitudes 𝐴𝑁MHV6;1 for the split-helicity configuration are [81] 𝐴𝑁MHV6;11+2+3+456=𝑐Γ2𝐵1𝑊6(1)+𝐵2𝑊6(2)+𝐵3𝑊6(3),(4.11) where 𝑊6(𝑖) are cyclic permutations of 𝑊6(1), and 𝑊6(𝑖+3)𝑊6(𝑖), given in terms of box functions by𝑊6(𝑖)=𝐹1𝑚6𝑖+𝐹1𝑚6𝑖+3+𝐹2𝑚62;𝑖+1+𝐹2𝑚62;𝑖+4,(4.12) and the 𝐹’s are dimensionless boxes. We can write polytope interpretations for the 𝑊6(𝑖)’s based on the fact that the 𝐹’s have polytope interpretation. Denoting for instance by (4561(23)) what was previously called 𝐼(𝑥4,𝑥5,𝑥6,𝑥1(𝑥2,𝑥3)), we write𝑊6(1)=(4561(23))+(1234(56))+(12(3)4(5)6)+(45(6)1(2)3)𝐴1+𝐴3+𝐴2+𝐴4,𝑊6(2)=(5612(34))+(2345(61))+(23(4)5(6)1)+(56(1)2(3)4)𝐴5+𝐴7+𝐴6+𝐴8,𝑊6(3)=(6123(45))+(3456(12))+(34(5)6(1)2)+(61(2)3(4)5)𝐴9+𝐴11+𝐴10+𝐴12,(4.13) where the 𝐴’s are tetrahedra defined in the order they appear in the 𝑊6(𝑖) above, while for example for the 6-point MHV amplitude, we have𝐴MHV6;1([(]𝐴123456)=𝐴(123456)12(3)45(6))+(23(4)56(1))+(34(5)61(2))+(1234(56))+(2345(61))+(3456(12))+(4561(23))+(5612(34))+(6123(45))=𝐴(123456)13+𝐴14+𝐴15+𝐴3+𝐴7+𝐴11+𝐴1+𝐴5+𝐴9,(4.14) where again the various 𝐴’s are defined in the order they appear. However, because of the spin coefficients of 𝑊6(𝑖), we cannot find a simple polytope interpretation for the subleading-color amplitudes.

4.2. Momentum Twistor Representation
4.2.1. Momentum Twistor Representation for Leading 𝑁𝑘MHV Amplitudes

Instead, we can use a momentum twistor [17, 20] representation for the 𝑁𝑘MHV superamplitudes in order to find a simple formula for the subleading 𝑁𝑘MHV amplitudes.

The MHV tree-level color-ordered superamplitudes are given by the Nair formula [82], a supersymmetric generalization of the Parke-Taylor formula [78, 83], 𝒜𝑛,2𝛿(12𝑛)=4𝑛𝑖=1𝜆𝑖̃𝜆𝑖𝛿8𝑛𝑖=1𝜆𝑖̃𝜂𝑖,1223𝑛1,𝑛𝑛,1(4.15) where as usual 𝑖𝑗𝜖𝛼𝛽𝜆𝛼(𝑖)𝜆𝛽(𝑗), ̃𝜂 is a spinor with an index 𝐼=1,,4 for supersymmetries suppressed, and the 2 in 𝐴𝑛,2 refers to 𝑅-charge, since the 𝑁𝑘MHV amplitude has 𝑚=𝑘+2  𝑅-charge.

The leading singularities of an amplitude are the discontinuities of the amplitude over the singularities where we put a maximum number of propagators on-shell, as explained in [18], where a conjecture for these leading singularities was proposed.

In terms of supermomentum twistors 𝑍𝑖, the leading singularity of the (color-ordered, planar, i.e., leading) 𝑁𝑘MHV superamplitude is [19, 23] 𝑛,𝑚=𝛿4𝜆̃𝜆𝛿8𝜆̃𝜂𝑑1223𝑛1𝑛𝑘𝒟𝑉𝑜𝑙(𝐺𝑙(2))𝑘𝜇=1𝛿4|4𝑛𝑖=1𝒟𝜇𝑖𝑍𝑖(12𝑘)(23𝑘+1)(𝑛12𝑘1)=𝑛,2×𝑛,𝑘,(4.16) where 𝑘=𝑚2. The prefactor 𝑛,2 is the tree MHV amplitude (4.15), and the integral 𝑛,𝑘=𝑛,𝑚2, is Yangian invariant. This object is dual conformal covariant, only 𝑛,𝑘 being dual conformal invariant, and the tree amplitude is covariant.

The one-loop amplitudes of 𝒩=4 SYM can be reduced to just boxes via the van Neerven and Vermaseren procedure, with some coefficients. The leading singularities also coincide with the coefficients of these box functions [18]. For one-loop MHV, the coefficients of the boxes are known to be just the MHV tree amplitudes, agreeing with the result above.

4.2.2. Subleading 𝑁𝑘MHV Amplitudes in Momentum Twistor Space

The planar (leading) color-ordered 𝑁𝑘MHV amplitude is a sum of permutations of boxes with coefficients equal to the leading singularities, 𝐴𝑛;1(1𝑛)=𝜎𝑛,𝑘(𝜎)𝐼𝑛;4(𝐴𝜎)=MHV𝑛(𝜎)𝑅𝑛;𝑘(𝜎)𝐼𝑛;4(𝜎),(4.17) where 𝐼𝑛;4 are boxes. At 6 points, the permutations 𝜎 combine such that we can organize the sum as a sum over cyclic permutations, with several boxes having the same coefficient [18]. For this coefficient we can factorize the tree MHV amplitude, which is cyclically invariant, so that it appears as a common factor 𝐴6;1(16)=𝐴MHV6(16)𝜆=cyclic𝑅6;𝑘(𝜆)𝜎/𝜆𝐼6;4(𝜎).(4.18) At higher 𝑛-point, the situation is slightly more complicated. The box diagrams are ordered in groups that can be cyclically permuted, for each group having a given formula for the residue, but unlike 6-point, the residue is not universal for all the groups [18]. However, all the diagrams still have the external legs in the original order, which means, since the MHV tree amplitude is cyclically invariant, that we can again factorize the MHV tree amplitude, obtaining for planar 𝑁𝑘MHV amplitudes𝐴𝑛;1(1𝑛)=𝐴MHV𝑛(1𝑛)groupsofdiagrams𝜆=cyclic𝑅𝑛;𝑘(𝜆)𝜎/𝜆𝐼𝑛;4(𝜎)𝐴MHV𝑛(1𝑛)𝑀𝑛;𝑘(1𝑛)(4.19) which implicitly defines 𝑀𝑛,𝑘.

We now finally note that we have the same formula for 𝐴𝑛;1(1𝑛) in terms of 𝐴MHV𝑛 and 𝑀𝑛;𝑘 from the previous section on polytopes, so we can apply the same calculations we used to obtain the MHV𝐴𝑛;𝑗 in terms of 𝐴𝑛;1 in Section 2. We just have to change the definition of 𝑀𝑛;𝑘 as in (4.19) and thus also drop the polytope interpretation of 𝑀𝑛,𝑘. But otherwise the same (4.10) found in the MHV case holds in the general 𝑁𝑘MHV case as well, as can be seen from (4.9).

4.2.3. Application to the 6-Point 𝑁MHV Amplitude

For the superamplitude, we use an explicit form of the twistor formula (4.18), doing the twistor space integrals over the 1-loop 𝑁MHV contours. The result is [84, 85] 𝐴(1)𝑁MHV6;1𝑎(123456)=2𝐴(0)MHV6×𝑅(123456)413+𝑅146𝑊6(1)+𝑅524+𝑅251𝑊6(2)+𝑅635+𝑅362𝑊6(3)𝐴(0)MHV6(123456)𝑀(1)𝑁MHV6(123456).(4.20) From the 𝑅𝑛;𝑘 terms in (4.18), one gets the sum of basic dual conformal invariant 𝑅-invariants 𝑅𝑗,𝑗+3,𝑗+5 above. Here the 𝑅𝑗,𝑗+3,𝑗+5 are given by 𝑅𝑟𝑠𝑡=𝑠1𝑠𝑡1𝑡𝛿(4)Ξ𝑟𝑠𝑡𝑥2𝑠𝑡𝑟||𝑥𝑟𝑡𝑥𝑡𝑠||𝑟||𝑥𝑠1𝑟𝑡𝑥𝑡𝑠||𝑠𝑟||𝑥𝑟𝑠𝑥𝑠𝑡||𝑟||𝑥𝑡1𝑟𝑠𝑥𝑠𝑡||𝑡,Ξ𝑟𝑠𝑡=𝑟1𝑡𝜂𝑖𝑖||𝑥𝑡𝑠𝑥𝑠𝑟||𝑟+𝑠1𝑟𝜂𝑖𝑖||𝑥𝑠𝑡𝑥𝑡𝑟||𝑟,𝑥𝑠𝑡=𝑥𝑠𝑥𝑡=𝑡1𝑖=𝑠𝑝𝑖.(4.21)

As explained before, we can then perform the same combinatorics that led us to (4.9), just that now we use 𝑀(1)𝑁MHV6(123456) instead of the 𝑀6(123456).

5. Summary

We have reviewed a number of features of subleading-color amplitudes of 𝒩=4 SYM theory, a subject considerably less developed than that of the leading (planar) amplitudes. Nevertheless this topic should not be ignored if the structure of perturbative 𝒩=8 supergravity and its relationship to 𝒩=4 SYM theory are to be understood, as nonplanar graphs appear on an equal footing in 𝒩=8 supergravity.

After presenting a detailed description of the IR divergences of 𝒩=4 SYM theory, we obtained the leading (and some subleading) IR divergences of subleading-color amplitudes at 𝐿 loops and tested these against known exact results for one- and two-loop four-point functions. These ideas applied to the one-loop five-point function led to a new KLT relation, as well as possible new relations between 𝒩=4 SYM and 𝒩=8 supergravity amplitudes. A geometric interpretation of the one-loop subleading and 𝑁𝑘MHV amplitudes of 𝒩=4 SYM was presented in the last section.

Since reformulations and extensions of known results frequently lead to new insights, we advocate that continued study of subleading-color amplitudes is likely to be fruitful. In particular, it would be important for our understanding of the relation of 𝒩=4 SYM to 𝒩=8 supergravity to extend (3.20) and (3.21) to subleading IR divergences, and to higher 𝑛-point functions. An example of the latter is the speculative (3.47) for 𝐿=1 and 𝑛=5. However, (3.8) and (3.17) remind us that (3.47) may not be the only way to relate the two theories, so that the subjects discussed in this paper should provide many opportunities for future work.

Acknowledgments

We have benefited from numerous insights and suggestions from Lance Dixon throughout our work on the various topics of this paper, for which we are extremely grateful. The research of S. G. Naculich is supported in part by the NSF under Grant PHY-0756518. The research of H. J. Schnitzer is supported in part by the DOE under Grant DE-FG02-92ER40706. The research of H. Nastase is supported in part by CNPQ Grant 301219/2010-9.