Comments on all-loop constraints for scattering amplitudes and Feynman integrals
Abstract
We comment on the status of “Steinmann-like” constraints, i.e. all-loop constraints on consecutive entries of the symbol of scattering amplitudes and Feynman integrals in planar super-Yang-Mills, which have been crucial for the recent progress of the bootstrap program. Based on physical discontinuities and Steinmann relations, we first summarize all possible double discontinuities (or first-two-entries) for (the symbol of) amplitudes and integrals in terms of dilogarithms, generalizing well-known results for to all multiplicities. As our main result, we find that extended-Steinmann relations hold for all finite integrals that we have checked, including various ladder integrals, generic double-pentagon integrals, as well as finite components of two-loop NMHV amplitudes for any ; with suitable normalization such as minimal subtraction, they hold for MHV amplitudes at three loops. We find interesting cancellation between contributions from rational and algebraic letters, and for the former we have also tested cluster-adjacency conditions using the so-called Sklyanin brackets. Finally, we propose a list of possible last-two-entries for -point MHV amplitudes derived from equations, which can be used to reduce the space of functions for higher-point MHV amplitudes.
1 Introduction
Recent years have witnessed enormous progress in computing and understanding analytic structures of scattering amplitudes in QFT. These developments have greatly pushed the frontier of perturbative calculations relevant for high energy experiments, and often they offer deep insights into the theory itself and exhibit surprising connections with mathematics. An outstanding example is the super-Yang-Mills theory (SYM), where one can perform calculations that were unimaginable before and discover rich mathematical structures underlying them. For example, positive Grassmannian Arkani-Hamed:2016byb and the amplituhedron Arkani-Hamed:2013jha have provided a new geometric formulation for its planar integrand to all loop orders.
On the other hand, the modern bootstrap program in perturbative QFT aims at computing scattering amplitudes and other physical quantities by directly imposing analytic structure and physical constraints, without ever needing Feynman diagrams or loop integrands. Again the perfect laboratory where very impressive perturbative orders have been achieved is the planar SYM amplitudes with Dixon:2011pw ; Dixon:2014xca ; Dixon:2014iba ; Drummond:2014ffa ; Dixon:2015iva ; Caron-Huot:2016owq ; Dixon:2016nkn ; Drummond:2018caf ; Caron-Huot:2019vjl ; Caron-Huot:2019bsq ; Dixon:2020cnr ; Golden:2021ggj (see Caron-Huot:2020bkp for a review). The key of the bootstrap program is the construction of a function space where the amplitude lives: for (or more generally MHV and NMHV amplitudes with any ) conjecturally it is the space of generalized polylogarithm functions, which depend on dual conformal invariant (DCI) cross-ratios, after subtracting infrared divergences e.g. by normalizing with Bern-Dixon-Smirnov (BDS) ansatz Bern:2005iz . As another deep connection between amplitudes and mathematics, it has been realized in Golden:2013xva that cluster algebras of Grassmannian are directly relevant for the singularities of -particle amplitudes, whose kinematics can be parametrized by momentum twistor Hodges:2009hk , or the space of mod torus action. More precisely, the so-called -coordinates of cluster algebras are related to symbol Goncharov:2010jf ; Duhr:2011zq letters of amplitudes: the letters of six-particle amplitudes and letters of seven-particle ones are nicely explained by and cluster algebras, respectively.
Apart from the overall symbol alphabet, more refined restrictions on scattering amplitudes and Feynman integrals have proved to be crucial for the bootstrap program to higher orders for . The most basic ones include the physical discontinuity Gaiotto:2011dt and the double discontinuity structure derived from the Steinmann relations Steinmann1960a ; Steinmann1960b , which have reduced possible first-two-entries to only and weight-two symbols for , respectively. Remarkably, the conjectural extended Steinmann (ES) relations, which basically extend Steinmann relations to higher multiple discontinuities, have been observed to hold for amplitudes and integrals for Caron-Huot:2016owq ; Dixon:2016nkn ; Caron-Huot:2019bsq . These ES relations impose similar constraints on any two consecutive entries of the symbol as Steinmann relations on the first two, which have been explicitly checked for (double-)pentagon ladders to arbitrary loops (and some for ) as well as amplitudes (up to ) and amplitudes (up to ), which are normalized by BDS-like subtraction Alday:2009dv and two-loop MHV amplitude with minimal subtraction Golden:2018gtk 111Interesting constraints similar to extended Steinmann relations have been found for Feynman integrals Bourjaily:2020wvq , form factors Dixon:2020bbt and even the wave-function of the universe Benincasa:2020aoj .. In these cases, the ES relations can be alternatively formulated as cluster adjacency conditions Drummond:2017ssj ; Drummond:2018caf ; Drummond:2018dfd : only coordinates that belong to the same cluster (for and for respectively) can appear adjacent in the symbol. As far as we know, ES relations/cluster adjacency has remained (mysterious) conjectures, and it is natural to ask if they extend to amplitudes and integrals for . It is in particular highly desirable to apply it to finite Feynman integrals to relatively high orders, as well as finite components of amplitudes, for higher multiplicities; among other things, such relations can provide powerful constraints on the function space for higher just as what they have achieved for . This is the main question we hope to address in the paper.
Beyond , Grassmannian cluster algebras for for become infinite, and a certain truncation is needed to obtain a finite symbol alphabet. As already seen for one-loop N2MHV, amplitudes with generally involve letters that cannot be expressed as rational functions of Plücker coordinates of the kinematics ; more non-trivial algebraic letters appear in computations based on equations CaronHuot:2011kk for two-loop NMHV amplitudes for and Zhang:2019vnm ; He:2020vob , requiring extension of Grassmannian cluster algebras to include algebraic letters. Solutions to both problems has been proposed using tropical positive Grassmannian speyer2005tropical and related tools for Drummond:2019qjk ; Drummond:2019cxm ; Henke:2019hve ; Arkani-Hamed:2019rds ; Arkani-Hamed:2020cig ; Herderschee:2021dez and Henke:2021avn ; Ren:2021ztg , as well as using Yangian invariants or the associated collections of plabic graphs Mago:2020kmp ; He:2020uhb ; Mago:2020nuv ; Mago:2021luw .
On the other hand, SYM has been an extremely fruitful laboratory for the study of Feynman integrals (c.f. ArkaniHamed:2010gh ; Drummond:2010cz ; Caron-Huot:2018dsv ; Henn:2018cdp ; Bourjaily:2018aeq ; Herrmann:2019upk and references therein).The connections to cluster algebras extend to individual Feynman integrals as well, e.g. the same and control multi-loop integrals in SYM Caron-Huot:2018dsv ; Drummond:2017ssj . Cluster algebra structures have also been discovered for Feynman integrals beyond those in planar SYM Chicherin:2020umh including a five-particle alphabet which has played an important role in recent two-loop computations Abreu:2018aqd ; Chicherin:2018old ; Chicherin:2018yne . The knowledge of alphabet and more refined information can be used for bootstrapping Feynman integrals Chicherin:2017dob ; Henn:2018cdp (see also Dixon:2020bbt ). In He:2021esx ; He:2021non , we have identified (truncated) cluster algebras for the alphabets of a class of finite, dual conformal invariant (DCI) Drummond:2006rz ; Drummond:2007aua Feynman integrals to high loops, based on recently-proposed Wilson-loop representation He:2020uxy ; He:2020lcu . For ladder integrals with possible “chiral pentagons” on one or both ends (without any square roots), we find a sequence of cluster algebras for their alphabets, depending on and the kinematic configurations; for cases with square root, such as the double-penta ladder integrals, we find a truncated affine cluster algebra which (minimally) contain rational letters and algebraic ones.
In this paper, we would like to use this rich collection of data for a systematic check of extended Steinmann relations beyond . Before proceeding, let us briefly list all finite integrals we use as data in this paper. As the main example, we consider double-penta ladder integral, with four massless corners labelled by , up to (whose alphabet contains letters mentioned above). Its collinear limit gives with an alphabet of cluster algebra ( rational letters). Simpler examples include penta-box ladder up to (alphabet is cluster algebra) and the well-known box ladder to all loops (alphabet is cluster algebra).
Besides these ladder integrals up to , we will also use the most general two-loop double-pentagon integrals computed in He:2020lcu , which we denote as . These integrals become generic at e.g. (depending on variables) whose alphabet has rational letters and multiplicative independent algebraic letters for each of the distinct square roots. For , we have e.g. (depending on variables) whose alphabet has rational letters and algebraic ones (with two different square roots).
Remarkably, these integrals directly give IR finite components of two-loop NMHV amplitudes to all multiplicities! More precisely, for non-adjacent the component of NMHV amplitude (after stripping off MHV tree)/Wilson loop is simply given by ; they represent the simplest class of NMHV components (while most generic for large ), which are also free of square roots Bourjaily:2019igt (as first computed for and for higher using method Zhang:2019vnm ; He:2020vob ).
In section 3, we will explicitly check ES relations and find positive answer for all these finite Feynman integrals (up to ) and two-loop NMHV (finite) amplitudes with ; note that the latter provides all-multiplicity evidence for ES relations for finite component amplitudes without the need of any subtraction/normalization. We will also confirm ES relations using the three-loop MHV amplitudes obtained very recently using equations by one of the authors and Chi Zhang Li2021 . Similar to the BDS-like subtraction for case, we need such normalization for higher-point MHV amplitudes and in particular for the case when is a multiple of , such as , the BDS-like subtraction is not defined and we need e.g. minimal subtraction. Note that for two-loop MHV amplitudes, cluster adjacency, which is closely related to ES relations, has been checked in Golden:2019kks using Sklyanin bracket, which also requires minimal subtraction for . It is not at all obvious to us that with the same subtraction, three-loop MHV amplitude also satisfies ES relations!
In all these cases except for and , we need to take into account algebraic letters, and while most ES relations directly hold for the rational part, naively there is a violation of ES relations in this part for remaining pairs which appear in cross-ratio of four-mass kinematics; it is remarkable that by including the algebraic part which also depends on such four-mass kinematics, the violation is cancelled and we have ES relations for the full answer. Note that while ES relations can be imposed without explicitly referring to the alphabet, it is more subtle to extend cluster adjacency to higher whose alphabet also contains algebraic letters; for rational ones, the so-called Sklyanin bracket Sklyanin:1983ig can be used, and we will see that for all those rational letters which do not violate ES relations, we can test that cluster adjacency is also satisfied.
In addition to ES relations which apply to all consecutive entries of the symbol, it is well known that the first two entries in general and last two entries for MHV amplitudes are not the same as before. As we have mentioned, given the physical discontinuity or the first entry condition, Steinmann-satisfying first two entries are much more constrained than subsequent pairs. In section 2, we will list all such (integrable) first-two-entries, which amounts to having the weight- space of Steinmann-satisfying dilogarithm functions. We list all such weight- functions for any , in terms of and . As extracted from the box functions, entries of the part will automatically DCI, while entries of functions are simply . We will give the general counting of these first-two-entries to all , and check this ansatz by all the data we have, including amplitudes and finite integrals.
In section 4 which has a different flavor than the rest of the paper, we will also provide a list of all possible last two entries for MHV amplitudes. The reason we study them is that last entries of MHV amplitudes have been known since Caron-Huot:2011dec which can be derived from equations and have played an important role for the bootstrap program. It is known again for that similar constraints can be derived for last two entries, again by using equations. We will explicitly go through the situations for and get all possible -coordinates pairs on the last-two-entries. Furthermore, for we reorganize the pairs into manifestly DCI integrable symbols, showing that there are allowed combinations. We will see that numbers of the last-two-entries from equations remain very limited as grows, leaving stronger constraints on the function space of MHV amplitudes.
2 First-two-entries from Steinmann relations
As a warm-up exercise, let us first present our conjecture for all possible first-two-entries of integrals/amplitudes. The starting point is that physical discontinuities, or the first entries of the symbol, for any amplitudes/integrals in planar SYM, must correspond to planar variables ; this is even true for any planar theory, and what is special about SYM is the dual conformal symmetry which forces the first entries to be DCI combinations. Note that out of all the planar variables, which we write as , of them are frozen variables ( for ), thus we have unfrozen Plücker variables which correspond to diagonals of -gon except for the “shortest” ones. Since we are interested in variables that are unfrozen, these are all we can have for the first entry, and equivalently one can construct the same number of DCI combinations e.g. . For example, for , these correspond to the well known and first entries, and for it is easy to see that we have first entries, which are given by for and for (or corresponding and ).
What about the first-two-entries? The most important constraint on the first-two-entries is the Steinmann relations, which says that the double discontinuities taken in overlapping channels of any amplitude should vanish. A convenient way to proceed is to start at one loop, where all finite amplitudes/integrals can be expanded in terms of (finite part of) box integrals. First we note that the only finite box integrals are the four-mass ones; given four dual points with cyclically ordered and each adjacent pair at least separated by , we have the (normalized) four-mass box integral
(1) | |||
(2) |
where and similarly for . It is straightforward to check that satisfies Steinmann relations as we will see in the next section. We can also go to lower-mass cases but they suffer from infra-red (IR) divergences, and certain regularization is needed. One way to preserve DCI is to introduce the DCI-regulator as in Bourjaily:2013mma , but we find that the resulting finite part of the lower-mass box integrals violate Steinmann relations. More precisely, it is possible to write the part of lower-mass boxes in a way that respects Steinmann relations, but the part does not, thus we will discuss these two parts separately for them. Our main conjecture is that for finite integrals and amplitudes to all loops, the first two entries that satisfy Steinmann relations can only be extracted from such box functions where the part need to be treated separately. In addition to the four-mass box cases, we will encounter the following functions for three-mass and two-mass-easy boxes 222For two-mass-hard or one-mass boxes, only a constant can appear in this part; as we are listing first-two-entries at the symbol level, we ignore such constant for now.:
(3) |
where one can check that indeed Steinmann relations are satisfied: the second-entry that can enter are just and . It is easy to count the total number of four-mass boxes and such functions for lower-mass cases: there are box functions and of them are two-mass-hard/one-mass boxes which only give , thus we have such functions. For example, for , there are and functions, which can be chosen to be for and for , respectively Dixon:2016nkn . Now for , we have four-mass boxes, and functions from lower-mass boxes, which we can choose to be with in
Having fixed all possible part, we move to the part, and it is clear which of them satisfy Steinmann relations:
(4) |
where means that the two diagonals (neither are the shortest ones) do not cross each other. Naively these do not respect DCI, but as we have mentioned above such can be converted to cross-ratios (with the help of frozen ones), which need to be done carefully with respect to Steinmann relations. For example, for , there are exactly and such functions respectively: with for , and and with for . For , we find functions for in
For general , it is straightforward to count that there are such functions. In total, there are first-two-entries which can be derived from box functions and satisfy Steinmann relations, and we conjecture that they are all we need for finite integrals and Steinmann-respecting amplitudes. For example, we have checked that in all two-loop finite Feynman integrals in Figure 1 and , exactly these first-two-entries for can appear. Moreover, we have checked first-two entries of minimally normalized of two-loop and three-loop MHV amplitudes for , exactly all first-two-entries appear.
3 Extended-Steinmann relations for integrals and amplitudes
As discussed in the last section, the Steinmann relations that restrict the for amplitudes or Feynman integrals give constraints on the first-two entries. The extended Steinmann relations are just generalizing these constraints to any two consecutive entries, thus restricting iterated discontinuity at any depth. Let us first write these relations as follows: define a linear “discontinuity” map in the space of symbols
(5) |
where we normalize the discontinuity map that computes the monodromy around such that . Then the extended Steinmann relations for a amplitude or Feynman integral of weight are
(6) |
for any and any two overlapping channels , , i.e. . For this reduces to the Steinmann relations (the second acting on the second-entry of the original symbol). Note that for , of a integrable symbol may not be integrable, so it’s not well-defined in the space of functions.
If any two letters of do not share the same branch point, for any two distinct letters and , then is given by clipping the -th entry off in the symbol of (after deleting all terms whose -th entry is not ), and ES relations simply become constraints of adjacent letters in the symbol. This is indeed how ES relations are checked for BDS-like normalized amplitudes for (up to and respectively) as well as certain Feynman integrals (such as double-pentagon ladders). Note that this is always the case when the alphabet contains only rational letters, which cannot share any branch point since by definition they are multiplicative independent. For instance, we have also checked the double-penta ladder integrals with and the penta-box ladders with up to , and find that they indeed satisfy ES relations in exactly the same way as finite integrals for .
Extended Steinmann relations with algebraic letters
However, generally amplitudes or Feynman integrals for involve square roots, and algebraic letters may share the same branch point , such that extended Steinmann relations cannot be directly formulated as constraints on which letters can appear next to each other in the symbol. Let us illustrate this phenomenon with the simplest case: we consider the Steinmann relations of (normalized) four-mass box function :
where
(7) |
The logarithms of these variables share 4 branch points , and only are two overlapping channels (the two diagonals cross each other), and now we consider the Steinmann relation for this pair.
Near the branch point ,
so or depending on the region of kinematics. Here we choose the second one, and then
Therefore, we see that algebraic letters can contribute to the discontinuity of a physical channel, and we can easily verify the Steinmann relation
and similarly .
A direct generalization of four-mass box is the box-ladder , which is the first example with square roots for checking extended Steinmann relations. The -loop box-ladder function Usyukina:1993ch ; Broadhurst:2010ds has a well-known expression:
(8) |
where and are defined by . Note the alphabet of for is simply :
and the only letter with non-zero discontinuity around the branch point or is or depending on the region of kinematics. Thus we have seen the advantage of using variables: the extended Steinmann relations for the box-ladder are simply the statement that there are no two consecutive or in the symbol of . This is quite clear from the expression eq.(8) that there is no two consecutive in and similarly for (obviously no contribution from powers of ).
Next we move to the class of integrals with more non-trivial algebraic letters, namely double-pentagon ladder , which have been computed up to with rational letters and independent algebraic letters He:2021non . First of all, since the algebraic letters only contain the square root as that of four-mass box , which only involve one pair of overlapping channels and as above. For any other pair of overlapping channels and , the extended Steinmann relations simply mean that rational letters and are not adjacent in the “rational” part of the symbol of . This is indeed the case as we have checked through .
What we have found is that the only minor violation in the “rational” part involves rational letters and in consecutive entries; in fact, they have only appeared next to each other at second and third entries. This is good news since the “irrational” part only contains algebraic letters at these two entries He:2021non , which also contribute to double discontinuities involving this pair. Recall that the algebraic letters are of the form for
with , defined as in eq.(7). Near the branch point , discontinuities of algebraic letters are given by
where the choices of depend on the kinematic region, but they should be the same on a given region. Similarly, we can calculate of these algebraic letters. Remarkably, after taking into account the contribution from “irrational” part, we find that the double discontinuity (at second and third entry) indeed vanishes, thus satisfy the extended Steinmann relations (at least up to )!
So far we have focused on integrals up to , but it is straightforward to also check ES relations for higher-point integrals/amplitudes. The two-loop double-pentagon integrals are all we need for MHV amplitudes (after regularizing divergences) as well as those finite components of NMHV amplitudes. Again the “rational” part of contains certain violation of ES relations at second and third entries, which require contributions from “irrational” part. What we find is that for each of the four-mass-box square roots (depending on four dual points ) 333For , generically we have choices for the dual points with , , , ., the double discontinuity around and is again cancelled nicely. Thus satisfies ES relations in exactly the same way.
An immediate consequence of this observation is that for , all components of two-loop NMHV amplitudes with non-adjacent also satisfy ES relations, since any such component is given by . In fact, these finite components are absent of algebraic letters, so ES relations for these components is nothing but the absence of adjacent unfrozen letters and for . This is a direct confirmation of ES relations to all multiplicities for finite amplitudes without any subtraction.
Three-loop MHV amplitudes and cluster adjacency
Given that finite double-pentagon integrals satisfy ES relations, so do two-loop MHV amplitudes if one can subtract IR divergences in a suitable way. In Golden:2019kks , cluster adjacency conditions have been checked for amplitudes with BDS-like subtraction or minimal subtraction when is a multiple of four, which imply ES relations when applied to letters of the form . Here we move to the three-loop MHV amplitude, whose symbol has only been computed very recently Li2021 using equations and two-loop NMHV amplitudes. This was a very non-trivial calculation: the raw data consists of roughly terms and further simplification is still underway. The alphabet consists of rational letters and algebraic ones, and quite remarkably it still has the nice feature that algebraic letters only appear at second and third entries, just as two-loop NMHV amplitudes and ladder integrals.
First we need to convert this result to the one with minimal subtraction:
where are -loop BDS-normalized amplitudes and is defined in the appendix A. Despite the huge size of the symbol, we can check ES relations exactly as before, and we find the same phenomenon as in and . The rational part of naively do not satisfy the extended Steinmann relations, which are broken at overlapping channels for each of the two four-mass boxes. We have only found such violation in the second and third entries, which is nicely in accordance with the position of algebraic letters. Quite remarkably, once we put these two parts together, the whole satisfies the extended Steinmann relations as in previous examples!
Note that for cases, it is remarkable that ES relations turn out to be equivalent to cluster adjacency conditions, which states that any two adjacent letters as cluster variables of the finite cluster algebra must belong to the same cluster. Given that all integrals and amplitudes we have checked satisfy ES relations, it is natural to ask if they also satisfy cluster adjacency conditions. Note that for , the relation between cluster adjacency and ES relations is unclear, except that for rational letters the latter follow from a special case of the former. It has been proven weaksep that two unfrozen Mandelstam-type -coordinates and are cluster adjacent if and only if in the -gon.
However, starting from , there are two main obstructions for studying cluster adjacency. First, it is known that not all letters are cluster variables of : algebraic letters or even more complicated functions can appear. Second, for is no longer a finite cluster algebra, which has infinite cluster variables, which makes it difficult to check whether a rational letter is a cluster variable and whether two cluster variables belong to a same cluster.
In Golden:2019kks , Sklyanin bracket Sklyanin:1983ig was introduced to resolve the second problem. Sklyanin bracket is a anti-symmetric Poisson bracket of two functions on . Suppose we parametrize by
then the Sklyanin bracket of two coordinates are given by
(9) |
and it is defined for any two functions by
(10) |
The main conjecture from Golden:2019kks is: two -coordinates , exist in the same cluster (thus cluster adjacent) if and only if their Sklyanin bracket is an integer or a half integer, i.e. .
For the first problem, since algebraic letters are no longer cluster -coordinates or -coordinates, we do not know a notion of cluster adjacency concerning them. Therefore, this check can only be performed for all pairs of rational letters. Before we apply it to more non-trivial cases, we first use this conjecture to check cluster adjacency conditions of , whose DCI alphabet forms a cluster algebra. By expanding the alphabet in -coordinates, we find that it becomes the union of
and
By computing the Sklyanin brackets for all pairs of letters, we find that only the following 15 pairs, which are exclusively contained in the second list, are not in , which means that they cannot appear next to each other in the symbol of :
We have checked this is indeed the case up to . Similar computation shows that the alphabet of contains -coordinates which are
and
Very nicely, we find again that pairs of letters have Sklyanin brackets that are not in , which only concern the letters in the second list. These are the pairs that cannot appear next to each other in the symbol , which we have also confirmed explicitly up to .
Note that a prior these cluster adjacency conditions based on (conjectural) Sklyanin bracket are different from the notion of adjacency for any pair of polynomials in a cluster-algebra alphabet as studied in He:2021non . However, we find that for the case, the latter is a consequence of the former! In other words, any two polynomials cannot appear to each other if and only if they appear in a forbidden pair of coordinates (with Sklyanin bracket not in ).
Next we apply this conjecture to check cluster adjacency conditions of integrals and amplitudes with algebraic letters. For , there is a pair and that appear in the second and third entries, which naively violate cluster adjacency. However, this must be an artifact of focusing on rational letters only, and the naive violation should be cancelled by contributions from algebraic letters (though we have not defined adjacency for the latter) similar to the case for ES relations. The non-trivial observation is that all other pairs of -coordinates in consecutive entries of the symbol indeed have brackets in , thus cluster adjacency is respected for them according to the conjecture.
We can proceed and check cluster adjacency conditions for finite integrals and component amplitudes, as well as three-loop MHV amplitudes with minimal subtraction. Remarkably, except for the letters corresponding to overlapping channels in four-mass boxes at entry , all other pairs of -coordinates in consecutive entries have brackets in . Provided the conjecture Golden:2019kks , we have thus confirmed cluster adjacency conditions for all cases we considered, except for the obvious violation which should be saved by algebraic letters. Naively these cluster adjacency conditions seem much stronger than ES relations but this can change if we impose them for bootstrap; we leave a systematic study of ES relations/cluster adjacency for octagon bootstrap (including algebraic letters), to future works.
4 Last-two-entries for MHV amplitudes from equations
Finally, let us turn to the discussion of the last-two-entries for loops -points MHV amplitude. Unlike extended Steinmann relations which are expected to hold for any (finite) integrals and amplitudes, a prior we do not expect such universal constraints on the last entry (let alone last two entries). However, for MHV amplitudes with BDS normalization, it has been known since CaronHuot:2011ky that dual supersymmetry restrict the last entry to be of the form ( unfrozen variables in total), and by studying the RHS of equations for MHV amplitude a bit more carefully, we can fix the last two entries as well.
We will first quickly review basic ingredients of formalism CaronHuot:2011kk , which offers an efficient method to calculate amplitudes of higher loops from the lower-loop ones. Equipped with the enumeration of all possible last entries (times R invariants) of NMHV He:2020vob , it becomes possible to use equations to determine all possible last-two-entries for MHV amplitudes. To do so, it is important to use the symbol integration algorithm presented in CaronHuot:2011kk , which computes the symbol of integral purely from the symbol of the integrand. This allows us to convert those “last entry R invariants”, into last-two-entries for MHV amplitude. This can be done for any , but we will mostly focus on , which suffices to illustrate our method.
As proposed in CaronHuot:2011kk , anomaly of the -loop BDS-normalized -matrix is related to those of higher and but lower , according to the perturbative expansion of the equation. Since kernel of is trivial for , after the anomaly is determined, we can directly replace by to get the total derivative , hence the symbol . This makes equation a powerful tool for computing NMHV (MHV) amplitudes from N2MHV (NMHV) amplitudes, and even more so for determining (all-loop) last entries. The anomaly of MHV amplitudes,can be obtained from -point NMHV amplitudes:
(11) |
where are weight multi-polylog functions. According to the equations, after taking the collinear limit with and in , formally we are performing integrals as
(12) |
which allows us to obtain (thus total differential) of -point MHV amplitudes. General will lead to divergences when taking the residue at . However, such divergences cancel in the combination of RHS of equations, and all we need are finite part of ’s in the limit . (for general we do not know or need explicit form of these ’s). The upshot is CaronHuot:2011kk :
(13) |
for , and similarly
(14) |
with and . The integrals vanish for other R-invariants.
Practically, these integrations are performed at the symbol level following the algorithm presented in the appendix of CaronHuot:2011kk . Last entries of the integrand together with the form fully determine the last-two-entries for the result. Nicely, all last entries for NMHV amplitudes have been given in He:2020vob , which we list in Appendix B for completeness. This is our starting point for computing all possible last-two-entries for MHV amplitudes.
Now we present some details of our calculation for possible last-two-entries of -point MHV amplitudes. Following (12) and (4), only terms proportional to () contribute non-trivial results after performing the Grassmannian integration and taking the residue at . Hence we firstly list all the possible pairs , where are NMHV last entries and are arbitrary unknown entries, both after applying the collinear limit. Secondly, we perform the Grassmannian integration over the Yangian part of these pairs following (12) and (4). To take the finite part at , we can simply set overall factors of to and other to . Finally, we integrate on , obtaining a list of symbols associated with . We record last-two-entries of this list, which gives an all-loop prediction for MHV amplitudes.
We first take MHV as an illustration. There are R-invariants of -point NMHV which give non-trivial contributions. For instance, is associated with , which are in the first class of NMHV last entries, and a non-trivial one is in the second class. For the latter one, we take and parametrize in collinear limit. then factorizes out an factor which is set to while other . Finally, after performing the -integration we get eight possible pairs
as last-two-entries for MHV amplitudes from this contribution.
Following the same logic and collect all possible contributions, we find that equations in fact leave no constraints for possible last-two-entries of , i.e. for each as last entries, all -coordinates are allowed to appear before it. It will not be that case for higher however, and we will see that the equation impose stronger constraints as increases.
For -point MHV amplitudes, there are two independent unfrozen last entries up to cyclicity, which are chosen as and . Naive computation shows that there are both possible -coordinates allowed to appear before them. However, since and are related by the dihedral symmetry , letters before them should also preserve such a symmetry. Thus we need to delete all those -coordinates before that are not dihedral images of those before and vice versa, ruling out letters in each list.
Moreover, for -point amplitudes we have the canonical choice of the symbol letters in the DCI form
(15) |
together with all from cyclically relabeling by times. Each contains only one unfrozen -coordinates, such that every pair of unfrozen letters is in one-to-one correspondence with a pair like . Hence we can recover DCI by simply replacing each unfrozen -coordinates by its corresponding . Note that the unfrozen last entries correspond to for .
In this way, we find exactly allowed letters before , which are
with . Letters before other last entries can be obtained by cyclic rotation and dihedral symmetries. In total there are DCI pairs and we have checked that our prediction matches the explicit results of -point MHV amplitudes up to , for both the BDS-subtracted amplitude Drummond:2014ffa and the one after BDS-like subtraction Dixon:2016nkn . Note that our list does not preserve extended Steinmann relations since we are using standard BDS-subtraction. However,at the BDS-like subtraction Alday:2009dv only reduces the possible pairs for last-two-entries comparing to BDS-subtraction. Therefore our prediction still holds for amplitudes with BDS-like subtraction.
Furthermore, we reorganize these weight- symbols by applying the integrability condition , and conclude that there are independent functions. of them are of the form , where . And the remaining functions live in cyclic orbits, whose initial seeds can be chosen as
where the symbol of the last one reads 444The weight- function can be easily obtained but we suppress the expression since it is much longer than the symbol.:
We remark that the length of the last orbit is only (thus there are functions in total), since after cyclic rotation times the image turns out to be a linear combination of the first functions in this orbit. This gives all integrable weight- symbols for the last two entries.
It is straightforward to extend the computation to any , but since the simplification of the -coordinates becomes more and more complicated, the list becomes more and more intricate as grows. We will not attempt to find such lists for all multiplicities, but content ourselves with last-two-entries for , which are generic enough. Note that since we do not have a confirmed alphabet beyond , it is not clear how they can be organized into DCI letters or how to apply integrability conditions without any ambiguities.
For , we have two independent unfrozen last entries and up to cyclic shift and dihedral symmetry ; explicit computation shows that there are unfrozen -coordinates before and before , which are recorded in the appendix C. Note that this represents a significant reduction of the weight- symbols in the last two entries, as naively there can be order letters for any last entry. We have checked that our prediction holds for -point BDS-subtracted amplitudes up to Li2021 .
For there are also independent unfrozen last entries, e.g. , up to cyclic shift and dihedral symmetries. There are allowed unfrozen letters before and before . As discussed in Henke:2021avn ; Ren:2021ztg using the tropical Grassmannian, naively there can be thousands of rational letters before each last entry. Our computation, however, drastically reduces this number, showing that the possible pairs are in fact very limited. Thus we have seen a significant reduction of function space for from these last-two-entry conditions, and the fraction of reduction grows rapidly with .
independent (unfrozen) | ||||||
num. of allowed (unfrozen) letters | 9 | 25 | 45 | 46 | 70 | 71 |
5 Conclusion and Discussions
In this paper, we have provided further evidence that extended-Steinmann relations hold for individual (finite) Feynman integrals as well as scattering amplitudes beyond , including various ladder integrals up to four loops, two-loop double-pentagons and NMHV finite components to all multiplicities, as well as three-loop MHV amplitudes with minimal subtraction. In all cases with algebraic letters, the contribution from algebraic letters is needed for ES relations to hold, and we have also checked cluster adjacency for rational letters in terms of Sklyanin bracket. For the first two entries, we have also listed all dilogarithm functions which satisfy Steinmann relations. Finally, for MHV amplitudes we have computed all possible last two entries using equations, which provide further constraints on their function space, as summarized in the Table 1 above for up to .
Our result on ES relations provides new evidence for their validity for Feynman integrals and amplitudes beyond : unlike MHV amplitudes where ES relations only hold with suitable normalization, individual Feynman integrals and finite components of non-MHV amplitudes do not require any subtraction thus ES relations hold in a “cleaner” way; on the other hand, it is already non-trivial that ES relations hold for two-loop MHV amplitudes with minimal subtraction Golden:2019kks , and we find it remarkable that they hold for three-loop amplitudes in the same normalization. Our result has further supported the claim that ES relations is a general property for any QFT (at least in the planar limit in the way we have formulated it). It would be highly desirable to understand these relations better, especially for divergent integrals/amplitudes where subtraction or regularization is needed. It would be fascinating to see if one could identify some underlying principle responsible for these remarkable relations.
Another mysterious property of some Feynman integrals and scattering amplitudes (in and beyond planar SYM) is that their symbol alphabet seems to fit into a cluster algebra (or truncated ones He:2021non with algebraic letters). In the presence of such cluster algebras, ES relations become closely related to cluster adjacency conditions, and we have established cluster adjacency conditions using -coordinates in all these integrals and amplitudes, modulo subtlety with algebraic letters. It would be highly desirable to formulate similar (truncated) cluster adjacency conditions including the algebraic letters, and to understand connections with ES relations e.g. for case. These ES relations/cluster adjacency can be used as extremely powerful constraints for bootstrap, at least for case which seems within reach. The starting point is the space of weight- functions we have constructed, and it would be interesting to continue building ES/adjacency-satisfying space at higher weights, which can be used for bootstrapping multi-loop amplitudes/integrals for .
Last but not least, although we have focused on studying ES relations for multiple polylogs (MPL) at the symbol level, as constraints on iterative discontinuities they apply to more general functions such as elliptic MPL. For example, it is clear that the fully massive double-box integral (finite component of two-loop N3MHV amplitudes) Kristensson:2021ani satisfies Steinmann relations, and we leave the study of ES relations for integrals/amplitudes beyond MPL to future works.
Acknowledgement
It is a pleasure to thank Yichao Tang and Chi Zhang for collaborations on related projects. This research is supported in part by National Natural Science Foundation of China under Grant No. 11935013,11947301, 12047502,12047503.
Appendix A Minimally-normalized Amplitude
The minimally-normalized (MHV) amplitude is defined by
where is the BDS-normalized amplitude, then
The function is defined by
where
where breaks dual conformal symmetry. For our purpose, we write the symbol of from that of and as
Appendix B Last-entries for all-multiplicity NMHV amplitudes
Let us summarize all possible last entries (dressed with Yangian invariants) for -point NMHV amplitudes He:2020vob , where we have three classes (note the second term on the right hand side of equations also belongs to the first class):
-
1.
last entries:
(16) -
2.
last entries:
(17) where , and the abbreviation .
-
3.
last entries:
(18) where .
For computing -point MHV amplitudes using equations, we take and plug these on the RHS of equations for MHV.
Appendix C Last-two-entries for MHV amplitudes
For , there are two independent unfrozen last entries up to cyclicity and dihedral symmetries, and . We list allowed unfrozen -coordinates
which can appear before , and
which can appear before .
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