Semileptonic weak Hamiltonian to O ( αα s ) in momentum-space subtraction schemes

: The CKM unitarity precision test of the Standard Model requires a systematic treatment of electromagnetic and strong corrections for semi-leptonic decays. Electromagnetic corrections require the renormalization of a semileptonic four-fermion operator. In this work we calculate the O ( αα s ) perturbative scheme conversion between the MS scheme and several momentum-space subtraction schemes, which can also be implemented on the lattice. We consider schemes deﬁned by MOM and SMOM kinematics and emphasize the importance of the choice of projector for each case. The conventional projector, that has been used in the literature for MOM kinematics, generates QCD corrections to the conversion factor that do not vanish for α = 0 and which generate an artiﬁcial dependence on the lattice matching scale that would only disappear after summing all orders of perturbation theory. This can be traced to the violation of a Ward identity that holds in the α = 0 limit. We show how to remedy this by judicious choices of projector, and deﬁne two new schemes RI - MOM and RI - SMOM . We prove that the Wilson coeﬃcients in the new schemes are free from pure QCD contributions, and ﬁnd that the Wilson coeﬃcients (and operator matrix elements) have greatly reduced scale dependence. Our choice of the MS scheme over the traditional W -mass scheme is motivated by the fact that, besides being more tractable at higher orders, unlike the latter it allows for a transparent separation of scales. We exploit this to obtain renormalization-group-improved leading-log


Introduction
Leptonic and semi-leptonic decays of mesons and nuclear beta decays probe the CKM matrix and provide an electroweak precision test of the standard model (SM), see for example [1] and [2].The short-distance physics of meson and nuclear beta decays in the SM is described, to an excellent approximation, by an effective Hamiltonian that involves only a single charged-current operator where P L = (1 − γ 5 )/2 and G F is the Fermi constant.At tree-level, the respective Wilson coefficient is directly proportional to the G F and a single CKM matrix element, here V ud .
Traditionally, the calculation of the short distance contribution relies on current algebra and is performed in the W -mass renormalization scheme [21].This scheme preserves the QED Ward identity and ensures that all weak corrections to the Fermi decay can be absorbed into G F while the short distance corrections for the semi-leptonic decays comprise a large electromagnetic logarithm and electroweak corrections that are mostly absorbed into G F .QED corrections for leptonic and semi-leptonic decays were calculated both in the current algebra approach [22], in chiral perturbation theory ( [23][24][25]) or in a combined approach with chiral perturbation theory [26] where the electroweak box diagrams are calculated with lattice gauge theory [27,28].Another possible scheme is the MS scheme, which is already used for the calculation of QED corrections [29,30] to the Fermi theory that determine G F as defined in Ref. [31].This scheme is also used for the calculation of electroweak corrections to the weak effective Hamiltonian [32], where the electroweak matching corrections and next-to-leading order anomalous dimensions for the operator O are given in Ref. [33].In the MS scheme weak and hadronic scales are separated unlike in the W -mass scheme, and this scale separation simplifies the new physics interpretation and allows for a systematic inclusion of higher-order perturbative corrections.
The complete treatment of QED corrections on the lattice is a difficult task and has so far been performed for purely leptonic decays [34][35][36][37].A novel feature in the semi-leptonic decay is that the relevant operator renormalizes in the presence of QED corrections.Both the W -mass scheme and the MS scheme are defined perturbatively and cannot be implemented on the lattice.This limitation does not apply to momentum-space subtraction schemes, which can be implemented both on the lattice and in continuum perturbation theory.The renormalization in the RI'-MOM scheme with a lattice regulator was given in Ref. [36], including the one-loop perturbative matching to the W -mass scheme.
In this paper we will perform the perturbative matching at two-loop level for different momentum-space subtraction schemes.These schemes are regulator-independent (RI) and are defined through a condition on a projected renormalized Green's function for a particular off-shell momentum configuration.The choice of projector is an important part of the definition of a particular RI scheme.In particular, special choices of projectors are required to ensure that the weak currents do not receive a finite renormaliation in RI schemes [38,39].Similarly, it is preferable to choose renormalization conditions that do not result in a finite renormalization of the semileptonic operator O in the pure QCD limit, as a finite QCD renormalization would imply an artificial (residual) scale dependence that only (formally) disappears once all orders of perturbation theory are summed.
The remainder of this paper is organised as follows: In Section 2 we discuss different choices of renormalization scheme and show which choices of projectors lead to vanishing pure-QCD corrections.Section 3 describes salient technical aspects of our two-loop calculation, including the tensor reduction and the master integrals used in the loop calculations.In Section 4 we present the results, where we combine the two-loop lattice continuum matching corrections with the known short-distance corrections and perform a renormalization-group improvement showing explicitly the dependence on the scales µ W , µ b , and the lattice matching scale µ L .We also study in detail the cancellation of the dependence on the scale µ L between the RG-improved Wilson coefficient and the conversion factor (or matrix element).Section 5 contains our conclusion.

Renormalization conditions and change of scheme
In this section we define the MS, RI -MOM, RI-SMOM, RI-MOM, and RI-SMOM renormalization schemes for the fields and the operator O and express the scheme conversion factors in terms of two-and four point Green's functions (Figure 1).
Let us define the connected fermion two-point function S and the amputated four-point function with O-insertion Λ through (respectively) and where i, j represent colour indices, which are absent in (2.1) in the case of leptons.We recall that the 1PI two-point function is then given by S −1 .Fully defining the fields ψ f (f = u, d, ) and the operator O requires renormalization conditions.We note that, because O does not mix with other operators, any two schemes A, B differ only by a (finite) rescaling: The RI -MOM, RI-SMOM, RI-MOM, and RI-SMOM schemes are defined by imposing the renormalization conditions at suitable kinematics, where P is a constant Dirac tensor satisfying Λ (tree) αβγδ P αβγδ = 1.The difference between RI -MOM and RI-MOM (as well as RI-SMOM and RI-SMOM) is only in the choice of projector, with the latter schemes adding conditions to specify the projector which are not present in the former.We defer specifics to Section 2.2 below.
It follows that the scheme conversion factors satisfy with implicit dependence on the choice of kinematic point and projector.
Equations (2.7) and (2.8) are the master formulas allowing for the computation of the scheme conversion factors.We emphasize that they hold independently of the choice of regulator used in computing the two-and four-point functions, though defining the MS scheme in practice entails the use of dimensional regularization.

Dimensional regularization and MS renormalization
In our computations we employ dimensional regularization (with an anticommuting γ 5 ; no ambiguous traces will occur in the following), which at the same time is the basis for defining MS schemes.The relations between the MS-renormalized objects O MS and ψ MS and the bare objects O b , ψ b in dimensional regularization are analogous to (2.3), (2.4) but complicated by a regularization artefact, the evanescent operators.These are chosen such that their (renormalized) infrared-finite Green's functions vanish as d → 4; in particular they will vanish at the RI subtraction point.In our case and to the loop order of our calculation, a single evanescent operator suffices, the bare version of which can be chosen to be following the notation of [40] and where all fields are understood to be bare.
We define from which it follows that ) Explicitly, where α and α s represent the electromagnetic and strong coupling constant respectively, while ξ and ξ s represent the photon and gluon gauge fixing parameter.The objects Λ MS O and S MS then determine C MS→RI as previously described.

Specifics of the RI schemes and Ward identity
The main aim of the present paper is to compute the conversion factor between the MS scheme (as defined above) and improved versions of two momentum-space subtraction schemes defined in the literature: • RI -MOM [41]; • RI-SMOM [42].
The two schemes are characterised by different kinematics and projectors.In the RI -MOM scheme, all four external momenta in Figure 1 are equal, while RI-SMOM employs a symmetric configuration with two independent momenta such that RI -MOM : RI-SMOM : (2.18) In both schemes, the condition (2.5) is imposed.
The conventional definition of the projector P entering the condition (2.6) on the renormalized four-point function is [43] where P R = (1 + γ 5 )/2.This choice of the projector for (1.1) leads to a scale dependence of the semileptonic operator already in pure QCD.Such a scale dependence does not occur in the MS scheme and, as we explain in the following, its presence in the standard RI schemes can be traced to the violation of a Ward identity which appears in the pure-QCD limit.Such an artificial scale dependence is undesirable from a conceptual perspective and complicates error control when perturbative and lattice results are eventually combined.We derive projectors below which preserve the Ward identity and ensures that the running is of order α em .Correspondingly, the conversion factors C MS→RI between the lattice schemes and the MS scheme are modified at O(α s ) and O(α 2 s ) relative to the conventional projectors.The Ward-identity-preserving RI projectors are: (

2.21)
To see how these projectors are obtained, first note that, if electromagnetism is neglected, no diagrams with propagators connecting the quark and lepton lines occur.The lepton line just gives the tree-level leptonic current L µ = γ µ P L (again, we use open indices here).Hence (suppressing Dirac indices) note that, with our choice of Fierz ordering, this applies to the bare Green's functions in dimensional regularization.Now, Λ µ is the 1PI vertex function in pure QCD for the conserved current j µ = dγ µ P L u, which satisfies the Ward identity which in the exceptional configuration reads More precisely, these identities hold in dimensional regularization with anticommuting γ 5 , and continue to hold after minimal subtraction.(As is well known, there exist regularizations in which the Ward identity does not hold.)As a consequence, the current does not renormalize in MS, and for the semileptonic operator we have It follows that the anomalous dimension is O(α) and the Wilson coefficient does not run in MS in pure QCD.
As Gracey has pointed out in his work on momentum-space subtraction schemes for quark bilinear operators [39], preserving the Ward identity requires a judicious choice of projector.Unfortunately, (2.23, 2.24) do not hold (with QED neglected and Λ µ defined as above) for the RI -MOM and RI-SMOM projectors when applied to the semileptonic operators, and as a result Z RI OO = 1 + O(α s , α).The resulting pure QCD renormalization for these projectors is finite so that the Wilson coefficient still does not run at O(α s ).Yet, the resulting scheme conversion factor carries an implicit scale dependence, due to the truncation of the perturbation series, which leads to unnecessarily large theoretical uncertainties on the Wilson coefficient (or operator matrix element).
To find suitable replacements for the conventional projector (2.19), we extend the idea in Ref. [39] and expand the four-point function in a set of basis structures In pure QCD, for general kinematics, the following 6 structures are sufficient: (2.26) The ordering in T (6) is such that all structures but the first one vanish by the equations of motion (but of course not at general or SMOM kinematics).Note that no evanescent structures occur in the pure-QCD limit.For MOM kinematics (2.17) the shorter basis suffices.
All structures are easily rewritten with γ µ P L as the second ("leptonic") factor, e.g.
p and comparing coefficients of / p 1 and / p 2 on both sides of the Ward identity, the form factors must satisfy, for general kinematics, which, for p 2 1 = p 2 2 = −µ 2 , can be combined into a family of equations (2.29) whose left-hand side equates to Σ(−µ 2 ).This allows us to define an infinite 1 number of potential projectors parameterised by x.For MOM kinematics, the simpler condition As explained above, the conditions (2.29) and (2.30) are satisfied in the MS scheme.They will hold in a momentum-space subtraction scheme if the projector P is defined such that the projected amplitude results in the left-hand sides of (2.29) (for RI-SMOM) and (2.30) (for RI-MOM), in which case C MS→RI = 1 (in pure QCD) by virtue of (2.8).This is equivalent to the current conservation condition Z RI OO = 1 + O(α), and at the same time shows that the Wilson coefficient necessarily agrees with MS up to corrections suppressed by the electromagnetic coupling constant.In other words, we require To find solutions to (2.31) and (2.32) we define a "basis" of linearly independent projectors (six for SMOM and two for MOM) as (2.34) This projector reduces to the one defined in (2.21) for x = 1 2 , which we use as a reference value to present our results.As the conventional projectors appear among our basis projectors but do not agree with our solutions, it also follows that the standard schemes do not preserve the Ward identity.This is also evident from the known results for the Wilson coefficient, which has a scheme conversion factor different from unity, even in the absence of electromagnetism (see Section 4).

W -mass renormalization scheme and the definition of the Fermi constant
The W -mass renormalization scheme [21,22] was traditionally used in the determination of the Fermi constant G F and is still in use in the calculation of electroweak corrections for the semi-leptonic decays [21,26,36].In this scheme, the amplitude is regularized by splitting the photon propagator where q is the momentum carried by the photon and M W is the mass of the W-Boson.The first term of (2.35) acts as a massive photon propagator that contains all UV poles, which are absorbed by G F .The second term is UV finite, thanks to the W -boson mass acting as a hard UV cut-off, but results in an IR contribution to the Fermi constant of O(αm 2 µ /M 2 W ). When G F is used to normalize the weak Hamiltonian, such a contribution, while small, breaks the manifest separation of scales that is a main virtue of the effective-field-theory approach.
On the other hand the complete 2-loop QED corrections to the Fermi theory (leptonic weak Hamiltonian) have been calculated in the MS scheme [29,30] for the Fermi operator in its Fierz-rearranged form, and this scheme was used for the determination of G F from the muon lifetime in [31].This definition of G F is also used in the calculation of electroweak corrections to the weak effective Hamiltonian [32,33], where the normalization of the dimension-6 Hamiltonian to G F absorbs most electroweak corrections.In the present work, we employ the MS scheme for G F .Our Wilson coefficient results below can therefore directly be used with G F from [31], and allow for a transparent separation of contributions from different scales.
In order to be able to compare to the result in Ref. [36] we have however determined the scheme conversion from the MS scheme to the W -mass scheme to one loop.Neglecting O(αm 2 µ /M 2 W ) and O(αm 2 s /M 2 W ) corrections, we find that the conversion factor for the Fermi (leptonic) operator equals one, while the conversion factor for the semi-leptonic operator reads (2.36)

Details of the calculation
There are 21 relevant diagrams at O(αα s ) for the renormalization of semi-leptonic operator and example diagrams can be seen in Figure 2.
We kept open Dirac indices in the evaluation of the respective Feynman amplitudes and only took the traces with the projectors as defined in Section 2 after renormalization.This allows us to consider different projectors and has the additional benefit that possible ambiguities arising from the treatment of gamma matrices, specifically γ 5 , in d-dimensions are avoided.
In our loop calculations tensor integrals appear.At two-loops, the most complicated structure is given by where k and l are the loop momenta and D(p 1 , p 2 ) is a combination of the propagators involved in the loop.
We applied the Passarino-Veltman decomposition [44] to write the tensor integral as a linear combination of scalar form factors and tensor structures During this calculation, we found that we could relate all form factors of rank n to form factors of rank n − 1 or n − 2. The most complicated matrix inversion we needed to perform in order to do this was the inversion of the matrix (3.3) After reducing the problem to the level of scalar integrals, we made use of Reduze 2 [45] and FIRE6 [46] to perform an IBP reduction of the integrals.In some cases, the Feynman diagram could not be expressed in terms of a propagator basis which was conducive to IBP reduction.In these cases, once we had reduced the Feynman diagram to the level of scalar integrals, we processed these scalars using the method described in Ref. [47] such that we were left with a new set of scalar integrals in bases that were appropriate for direct application of IBP reduction.This left us with a set of Master Integrals, the topologies for which are given in Figure 3. Details regarding our set of Master Integrals, as well as sources used for integral values can be found in Tables 1 and 2. We found values for most of these master integrals in Ref. [48][49][50], but for those integrals for which there are no analytical results we made use of PySecDec [51] to evaluate them numerically.
We found a typo in eq. ( 29) of [48] where an extra factor of 2π 2 3 is present in the last line and hence we used the integral definition in eq. ( 28).Moreover, eq. ( 11) breaks down in This Work p --Fig.3i This Work p --Table 1: The master integrals for this work in the MOM kinematics.For master topologies, see Figure 3. some kinematic configuration, e.g.x = 4 and y = 1, and as a result eq. ( 9) needs to be evaluated numerically.
In some cases, we needed to improve the analytical expression of the integral found in the literature and in order to do so we made use of PySecDec to evaluate the missing parts in the -expansion numerically.
We have been able to retrieve the scale dependence of these integrals (which is logarithmic) by exploiting the fact that there is only one independent kinematic scale.This meant that we could rescale the master integral, leaving only dimensionless loop and external momenta before either performing the integration, or using PySecDec to perform the calculation.To illustrate, consider the loop integral I ex , with dimensionfull quantities k, a loop integral, and p, an external momentum.If we re-express these in terms of a dimensionfull scale, ν, and dimensionless variables, k and p, we retrieve As can be seen, we retain the overall mass dimension of the integral in the first prefactor, but are then able to retrieve the log behaviour of the integral through the second prefactor, upon expanding in .

Results and numerics
In this section we present our results for the conversion factors between the MS and the RI -MOM, RI-MOM and RI-SMOM schemes.The respective conversion factors exhibit a scale dependence that mirrors the scale dependence of the relevant semi-leptonic Wilson coefficient.Working in renormalization group improved perturbation theory, this scale dependence will cancel order-by-order in perturbation theory for the product of the Wilson coefficient and a given conversion factor.By studying the residual scale dependence of this product, we can estimate the uncertainty from unknown higher-order corrections.

Scale dependence
In the following we will combine the matching corrections with the renormalization-groupimproved Wilson coefficient.The results of our two-loop calculation together with (2.7) and (2.8) determine the conversion factor C MS→i O including its analytic dependence on the MS scale µ.The fact that the product of the Wilson coefficient C MS (µ) of the semi-leptonic operator (1.1) and the conversion factor is scale-independent implies the renormalization group equation where γ W is the anomalous dimension of the semi-leptonic operator.The two-loop anomalous dimension and the one-loop electroweak matching corrections for the Wilson at the electroweak scale are given in Ref. [33].This renormalization-group equation provides an additional check of our calculation.In the following, we study the residual scale dependence in the product , where µ L ∼ O(GeV) is the lattice scale and the large logarithms ln µ L /M W are summed in renormalization-group-improved perturbation theory.
To this end we write the Wilson coefficient at the lattice scale as a product of the Wilson coefficient at the electroweak scale and the evolution kernel U(µ, µ 0 ), where µ W is the weak scale, and where the evolution kernel fulfils the renormalization group equation In the following we will consider the expanded anomalous dimension up to O(αα 2 s ), since the value of γ W is sensitive to O(αα s ) scheme transformation of the effective theory.The value γ W is currently not known, but will play a part in our numerical analysis later.
The solution of (4.3), under the assumption that α(µ) = α(µ W ) = α is scale independent, is found to be where β the first two terms of the QCD beta function that determines the running of α s (µ); C F = 4  3 is the Casimir factor of the fundamental representation of SU (3), C A = 3 is Casimir factor of the adjoint representation of SU (3) and T F = 1 2 is the trace normalization of the fundamental representation, while N f is the number of flavours.
When evolving the Wilson coefficient down to the lattice scale we must take into account the threshold corrections due to the fact that we integrate out the heavy quarks.In order to do this, we split the evolution in three steps: Combining these steps and expanding in powers of α and α s as we obtain the final expression of the low-scale matching, where the superscript i denotes either of the RI schemes, C i α is the resummed QED contribution, C i αs is the leading O(α s ) effect and C i α,αs LL and C i α,αs NLL are the leading-log (LL) and next-to-leading-log (NLL) strong corrections to the electromagnetic contributions, with . We stress again that the contributions coming from C i αs will vanish to all orders for the renormalization schemes defined by the conditions (2.31) and (2.32) by virtue of the Ward Identity.

RI -MOM & RI-MOM
Here and in the following, we will collect the results for the different operator and field conversion factors.The explicit form of the operator conversion factor will depend on the renormalization kinematics and on the choice of projectors.Contrary to this, the field conversion factor is the same in the RI -MOM, RI-SMOM, RI-MOM, and RI-SMOM schemes and reads where ξ (ξ s ) is the photon (gluon) gauge parameter.The two-loop QCD correction is given in Ref. [38] while the O(αα s ) contribution is a novel result.
For MOM kinematics we give the operator conversion factor both for the RI -MOM scheme (using the projector in Eq. (2.19)) and our new RI-MOM scheme using the projector in Eq.
(2.20).Here we used the results in Ref. [38] to implement the two-loop QCD corrections to the operator conversion factors.For the RI -MOM scheme we find As a check, we combine this result with the scheme conversion factor (2.36) and find agreement with the one-loop QED result obtained in Ref. [36] (in our convention ξ = 1(0) in the Feynman (Landau) gauge).The choice of the conventional projector leads to the presence of O(α s ) and O(α 2 s ) corrections, where the latter correction does not even vanish for ξ = 0.The µ dependence of α s will introduce an artificial scale dependence into this conversion factor that is not related to the operator anomalous dimension.The resulting residual dependence of C RI -MOM O (µ L , p 2 ) on the scale µ L , shown of Figure 4, suggest at least an uncertainty of ±0.5% from unknown three-loop QCD corrections.
For the RI-MOM scheme using the projector which we derived (Eq.(2.20)), we find where we have explicitly checked that all pure QCD corrections vanish.(GeV)  , where we set ξ = ξ s = 0, −p 2 = 9 and γ (2) W = 0 (dark green curve).We can see the reduction of the scale dependence in going from C RI-MOM α,αsLL to C RI-MOM α,αsN LL , while the residual scale dependence is dramatically reduced compared to the RI -MOM scheme (Figure 4).The light green shaded area shows the effect of the unknown value of γ W on the next-to-leading-log contribution: the upper limit is obtained with γ (2) W = −100, while the lower limit is given by γ Combining the expression (4.7) with the values of the coefficients given by (4.11) and [33] we obtain the expression of the Wilson Coefficient in the RI-MOM scheme (4.12) We recall that γ( We can see that there is an exact cancellation of the µ dependence in the case of pure electromagnetic corrections. When we switch on QCD interactions, however, while the scale dependence of the LL term given by ln αs(µ L ) αs(µ b ) cancels with the explicit scale dependence of the NLL terms in the conversion factor, there is a residual scale dependence coming from the other NLL terms proportional to αs(µ L ) 4π γ(4) + C es O .This effect, nevertheless, is sub-leading with respect to the residual scale dependence in (4.10), which is dominant at the low scale.In order to explore the contributions from higher order corrections in our numerical analysis, we vary γ W < 100, since it is currently not known.This range was chosen to reflect the typical range of values for this type of quantity.This effect can be seen in the light green bands of Figs. 5 and 6 The resulting residual scale dependence of C RI-MOM O (µ L , p 2 ) is given in Figure 5 and suggest a very small, i.e. ±2 • 10 −4 , uncertainty from higher order corrections.While these uncertainty are encouraging, we would like to remind the reader that the uncertainties from higher order electroweak corrections are not included and that the contribution of γ W to the NLL QCD corrections is only estimated.

RI-SMOM
The field conversion factor for RI-SMOM equals the one for the other RI schemes given in eq.(4.9).For the operator conversion factor we only consider the RI-SMOM scheme (i.e. the one defined using the projector seen in (2.21)), which should not yield any pure QCD corrections.It reads The two-loop QCD computation needed for this check can be extracted from intermediate results that appear in the QCD renormalization of the vector current in the SMOM scheme [39].(GeV)  W on the NLL contribution: the top limit is obtained with γ (2) W = −100, while the bottom limit is given by γ  The resulting residual scale dependence of C RI-SMOM O (µ L , p 2 ) is given in Figure 6 and again suggests a very small, i.e. ±2 • 10 −4 , uncertainty from higher order corrections.Again, the uncertainties from higher order electroweak corrections are not included, while the contribution of γ W to the NLL QCD corrections is only estimated.

Conclusions
In this paper we have calculated the scheme conversions for the semi-leptonic weak effective operator between the MS scheme and the RI -MOM scheme, as well as to our newly defined RI-MOM and RI-SMOM schemes.We emphasized the importance of the projector in the definition of these schemes and found that a conventional choice of projector leads to an artificial QCD correction to the conversion factor with a bad perturbative convergence.Using the Ward identity in the pure-QCD limit, we defined modified vesions of the RI -MOM and RI-SMOM schemes that rectify this problem, by showing the existence of adequate new projectors, thereby defining the RI-MOM and RI-SMOM schemes.Performing an effective field theory analysis with renormalization-group-improved perturbation theory we showed that these schemes indeed exhibit an excellent perturbative convergence, when LL and partial NLL QCD corrections were added to the photonic corrections.We exhibited the dependence on the various thresholds µ W , µ b and the scheme conversion (lattice matching) scale µ L and studied the cancellation of the µ L dependence for the product of the MS Wilson coefficient and the conversion factor (or equivalently, for the RI Wilson coefficients or RI operator matrix elements).
Given the theoretical attractiveness and good perturbative convergence, we argue that the schemes defined with our proposed projectors should be used in future work on semileptonic decays in place of the coventional RI schemes.In particular, this should allow a better precision in determining CKM matrix elements in future phenomenological analyses.
Our approach also lends itself to a systematic improvement of short-distance contributions.We leave the evaluation of the relevant three-loop anomalous dimensions and two-loop electroweak matching calculations required for completing the NLL QCD corrections for future work.
) from which the relation C B O = C A→B O C A O for the Wilson coefficient follows.

Figure 2 :
Figure 2: Some examples of the two-loop diagrams calculated.They are from Basis 1, 2, and 4 respectively.

Figure 3 :
Figure 3: The topologies for all master integrals.All external momenta are incoming.A black dot represents a power of 2 on the scalar propagator.

Figure 4 :
Figure 4: Residual µ-dependence of the low-scale Wilson coefficient C RI -MOM O for the conventional projector choice, where we set ξ = ξ s = 0 and −p 2 = 9.It is evident that the leading strong corrections introduce an artificial scale dependence at low scales µ ∼ µ L .

Figure 5 :
Figure 5: Residual scale dependence of the low-scale Wilson coefficient C RI-MOM O

Figure 6 :
Figure 6: Residual scale dependence of the low-scale Wilson coefficient C RI-SMOM O , where we set ξ = ξ s = 0, −p 2 = 9 and γ(2)W = 0 (dark green curve).As in Figure5, the residual scale dependence is suppressed by α.The light green shaded area shows the effect of the value of γ(2)