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Precise Determination of the Bottom-Quark On-Shell Mass Using Its Four-Loop Relation to the ¯MS-Scheme Running Mass

  • Corresponding author:

    Xu-Dong Huang, Email: huangxd@cqnu.edu.cn

  • Received Date: June 26, 2024
  • Published Date: September 19, 2024
  • We explore the properties of the bottom-quark on-shell mass (Mb) by using its relation to the ¯MS mass (¯mb). At present, this ¯MS-on-shell relation has been known up to four-loop QCD corrections, which however still has a 2% scale uncertainty by taking the renormalization scale as ¯mb(¯mb) and varying it within the usual range of [¯mb(¯mb)/2,2¯mb(¯mb)]. The principle of maximum conformality (PMC) is adopted to achieve a more precise ¯MS-on-shell relation by eliminating such scale uncertainty. As a step forward, we also estimate the magnitude of the uncalculated higher-order terms by using the Padé approximation approach. Numerically, by using the ¯MS mass ¯mb(¯mb)=4.183±0.007 GeV as an input, our predicted value for the bottom-quark on-shell mass becomes Mb5.372+0.0910.075 GeV, where the uncertainty is the squared average of the ones caused by Δαs(MZ), Δ¯mb(¯mb), and the estimated magnitude of the higher-order terms.
  • Article Text

  • Quark masses are important parameters for the quantum chromodynamics (QCD) theory, which need to be renormalized in higher-order calculations. In perturbative QCD (pQCD) theory, two schemes are frequently adopted for renormalizing the quark masses, e.g., the on-shell (OS) scheme[1] and the modified minimal subtraction (MS¯) scheme.[2,3] The OS mass, also known as the pole mass, offers the advantage of being grounded in a physical definition which is gauge-parameter independent and scheme independent. It ensures that the inverse heavy-quark propagator exhibits a zero at the location of the pole mass to any order in the perturbative expansion. On the other hand, the MS¯ scheme focuses solely on removing the subtraction term 1/ϵ + ln(4π)–γE from the quantum corrections to the quark two-point function. By combining this with the bare mass, one can derive the expression for the renormalized MS¯ mass. In high-energy processes, the MS¯ mass is preferred for its lack of intrinsic uncertainties. It has been found that for the high-energy processes involving the bottom quark, such as the B meson decays, when their typical scales are lower than the bottom quark mass, the using of MS¯ mass becomes less suitable and the OS mass is usually adopted. Practically, the relation between the OS mass and the MS¯ mass that is affected by renormalons,[46] resulting in a perturbative series with poor convergence. Thus for precision tests of the Standard Model, accurate determination of the OS mass is important.

    It is noted that the OS mass can be related to the MS¯ mass by using the perturbative relation between the bare quark mass (mq, 0) and the renormalized mass in either the OS or MS¯ scheme, where q denotes the heavy charm, bottom, and top quark, respectively. For example, we have mq,0=ZmOSMqOS and mq,0=ZmMS¯m¯q(μr), where μr is the renormalization scale. Here, ZmOS and ZmMS¯ represent the quark mass renormalization constants in the OS and MS¯ scheme, respectively. At present, the relation between the OS mass and the MS¯ mass, called the MS¯-on-shell relation, has been calculated up to four-loop QCD corrections.[716] Many attempts have also been finished to estimate the higher-loop contributions.[1719] Those improvements enable the possibility of precise determination of the bottom quark OS mass with the help of the experimentally fixed MS¯ mass. Both αs and m¯q are scale dependent, whose scale running behaviors are governed by the renormalization group equations (RGEs) that involve either the β-function[2025] or the quark mass anomalous dimension γm-function.[2628] Thus the crucial point for this determination is how to fix the precise values of αs and the MS¯ running mass m¯q simultaneously.

    Practically, researchers usually use the guessed renormalization scale and vary it within a certain range to estimate its uncertainty for a fixed-order pQCD series. This naive treatment leads to mismatches among the strong coupling constant and its expansion coefficients, which directly breaks the standard renormalization group invariance[29,30] and results in the conventional renormalization scale and scheme ambiguities. The effectiveness of this treatment depends heavily on the convergence of the pQCD series. Unfortunately, the bottom quark MS¯-on-shell relation exhibits poor convergence. The MS¯-on-shell relation up to four-loop QCD corrections still has a scale uncertainty about 100 MeV,[14,15] which significantly exceeds the current uncertainty of the MS¯ mass of the bottom quark issued by the Particle Data Group,[31]m¯b(m¯b)=4.183±0.007 GeV.

    In the process of renormalization, a renormalization scale needs to be introduced. For the original truncated perturbative series, if the renormalization scale is chosen improperly, the perturbative series will depend on the choice of renormalization scale and renormalization scheme. However, with methods such as the principle of maximum conformality (PMC),[3237] the improved perturbative series leads to a prediction without renormalization scale ambiguity in the fixed order. The PMC offers a systematic approach for determining the correct value of αs by using the RGE-involved {βi}-terms of the pQCD series. After using those {βi}-terms, the initial pQCD series changes into a newly scheme-independent conformal series. It has been found that the resultant PMC series is independent of any choice of renormalization scale, and the scale-invariant PMC series is also valuable for estimating the contributions of uncalculated higher-order (UHO) terms.[38] The comprehensive exploration of the PMC can be found in the review articles.[39,40]

    Recently, an improved PMC scale-setting procedure has been proposed in Ref. [41]. This approach simultaneously determines the correct magnitudes of αs and the quark mass m¯q by utilizing the RGEs for determining the magnitudes of the running coupling αs and the running mass under the same scheme such as the MS¯ scheme. Upon implementing the new scale-setting procedure to the MS¯-on-shell relation, the renormalization scale ambiguity inherent in the pQCD series is effectively eliminated. Additionally, the renormalon terms associated with the β-function and γm-function of the pQCD series can also be removed. In Ref. [41], we have made a detained discussion on the top-quark pole mass. In this Letter, we intend to utilize the PMC scale-setting approach to determine the bottom-quark OS mass. Furthermore, the Padé approximation approach (PAA),[4244] which offers a systematic method for approximating a finite perturbative series into an analytic function, will be employed to estimate the (n+1)th-order coefficient by incorporating all known coefficients up to order n. The PAA has been shown to be effective both in predicting unknown higher-order coefficients and in summing the perturbative series.

    The relationship between the bottom-quark MS¯ quark mass and its OS quark mass can be expressed as

    Mbm¯b(μr)=ZmMS¯ZmOS=n0asn(μr)cm(n)(μr),

    (1)

    where as = αs/(4π), cm(0)(μr)=1, and cm(n)(μr) is a function of ln(μr2/m¯b2(μr)). Subsequently, the determination of the bottom-quark OS mass can be achieved using the following relationship:

    Mb|conv.=m¯b(μr){1+C1(μr)as(μr)+C2(μr)as2(μr)+C3(μr)as3(μr)+C4(μr)as4(μr)+O(as5)},

    (2)

    where conv. stands for the initial pQCD series given under the MS¯ scheme. As mentioned above, the expansion coefficients Ci have been known up to N4LO-level, which need to be transformed as the β-series so as to fix the correct values of αs and m¯b. This transformation can be performed by using the general QCD degeneracy relations, and the results were given in Ref. [41]. Then, by applying the PMC scale-setting procedures, Eq. (2) can be transformed into the following conformal series:

    Mb|PMC=m¯b(Q*){1+r1,0as(Q*)+r2,0as2(Q*)+r3,0as3(Q*)+r4,0as4(Q*)+O(as5)},

    (3)

    where ri, 0 are conformal coefficients. Here Q* represents the PMC scale, whose logarithmic form ln(Q*2/m¯b2(Q*)) can be represented as a power series in as(Q*):

    lnQ*2m¯b2(Q*)=i=0nSiasi(Q*),

    (4)

    where the coefficients Si can be determined up to next-to-next-to-leading log (NNLL) accuracy[41] by using the given four-loop pQCD series. It is found that Eq. (4) is independent of the choice of renormalization scale. This property ensures that both the running mass m¯b and the running coupling constant αs are concurrently determined. By matching the μr-independent conformal coefficients ri, 0, the resulting PMC series becomes devoid of the conventional renormalization scale ambiguity.

    We are now ready to calculate the bottom-quark OS mass Mb through its perturbative relation to the MS¯ mass. To do the numerical computations, we adopt αs(MZ) = 0.1180±0.0009 and m¯b(m¯b)=4.183±0.007 GeV.[31] The scale running of αs(μr) is calculated by using the package RunDec.[45]

    Using Eq. (2) and setting all the input parameters to be their central values, we present the bottom-quark OS mass Mb under conventional scale-setting approach in Fig. 1. Figure 1 shows how the bottom-quark OS mass Mb changes with the renormalization scale and demonstrates that the conventional renormalization scale dependence diminishes as more loop terms have been incorporated. Numerically, we have

    Mb|Conv.=4.1830.111+0.782+0.399+0.0620.584+0.199+0.0270.162+0.145+0.007+0.023+0.1360.001+0.036=5.0620.016+0.095(GeV),

    (5)

    whose central values are for μr=m¯b(m¯b), and the uncertainties are for μr[m¯b(m¯b)/2,2m¯b(m¯b)]. The relative magnitudes of the leading-order terms (LO): the next-to-leading-order terms (NLO): the next-to-next-to-leading-order terms (N2LO): the next-to-next-to-next-to-leading-order terms (N3LO): the next-to-next-to-next-to-next-to-leading-order terms (N4LO) are approximately 1 : 9.5% : 4.8% : 3.5% : 3.3% for the case of μr=m¯b(m¯b). Equation (5) shows that the magnitudes of each loop terms are highly scale dependent, and the perturbative behavior of the whole series is different for different scale choices. Within this scale range, the absolute scale uncertainties are about 21%, 162%, 95%, 16%, and 27% for the LO, NLO, N2LO, N3LO, and N4LO terms, respectively. The overall scale uncertainty of the four-loop prediction of Mb becomes ∼ 2.2% due to the large cancelation of scale dependence among different orders.

    Fig. 1.  The bottom-quark OS mass Mb versus the renormalization scale (μr) under conventional scale-setting approach up to various perturbative orders.

    Similarly, using Eq. (3), we present Mb under the PMC scale-setting approach in Fig. 2. The PMC scale Q* can be fixed up to N2LL accuracy by using Eq. (4), i.e.,

    lnQ*2m¯b2(Q*)=72.8957as(Q*)+137.61as2(Q*)17177.2as3(Q*),

    (6)

    which is independent of any choice of μr and leads to Q* = 1.917 GeV. The flat lines in Fig. 2 indicate that the PMC prediction is devoid of renormalization scale ambiguity at any fixed order. Numerically, we have

    Mb|PMC=5.100+0.6670.4390.153+0.197=5.372(GeV).

    (7)

    It shows that the relative importance of the LO : NLO : N2LO : N3LO : N4LO terms in the PMC series is 1 : 13.0% : −8.6% : −3.0% : 3.9%.

    Fig. 2.  The bottom-quark OS mass Mb versus the renormalization scale (μr) under PMC single-scale approach up to different perturbative orders.

    It has been found that for the case of top quark,[41] whose αs(m¯t)0.11 and αs(Qt*=123.3GeV)0.11, there is good perturbative behavior for both the conventional and PMC series. However, for the present case of bottom quark, whose αs(m¯b)0.22 and αs(Qb*=1.917GeV)0.31, the αs power suppression fails to counterbalance the influence of the substantial numerical coefficients even after applying the PMC, e.g., Eq. (5) shows that the relative importance of the N2LO : N3LO : N4LO terms for conventional series is 1 : 73% : 68% for μr=m¯b(m¯b), 1 : 454% : 465% for μr=m¯b(m¯b)/2, and 1 : 67% : 60% for μr=2m¯b(m¯b), respectively; and Eq. (7) shows that such relative importance changes to 1 : 35% : 45% for the scale-invariant PMC series. At present, the relatively large magnitude of the N4LO-terms indicates that the magnitude of the N4LO conformal coefficients, which are unrelated to the RGE-involved β-terms or the quark mass anomalous dimension involved γm-terms, is large. However, such scale-invariant perturbative behavior can be treated as the intrinsic perturbative behavior of the MS¯-on-shell relation. By properly choosing the scale, the perturbative behavior of conventional series will be close to the PMC one. Thus for those cases, a proper scale-setting approach to achieve a scale-invariant series is very important. Moreover, in comparison of the N2LO-terms and N3LO-terms, the sizable magnitude of the N4LO-terms indicates the importance of knowing whether the UHO-terms can give sizable contributions and present the wanted convergent behavior. For the purpose, we adopt the PAA to estimate the magnitude of the UHO contributions.

    The PAA is a kind of resummation to create an appropriate generating function such as the fractional generating function; and it offers a systematic way for approximating a finite perturbative series into an analytic function. For a given pQCD series that can be written as ρ(Q)=i=1nCiasi, its [N/M]-type fractional generating function is defined as[4244]

    ρN/M(Q)=as×b0+b1as++bNasN1+c1as++cMasM,

    (8)

    where N and M are integers, N≥0, M≥1, N+M+1 = n. The coefficients bi∈[0, N] and ci∈[1,M] can be fixed by requiring the coefficients Ci∈[1, n] defined in the following expansion series

    ρN/M(Q)=i=1nCiasi

    (9)

    to be the same. The coefficients Ci=Ci and Ci = ri, 0 for in for the conventional series and PMC conformal series, respectively. Using Eqs. (2) and (3), the MS¯-on-shell relation up to mth-loop level can be written as

    Mb|PAAN/M=m¯b(μ)[1+ρN/M(μ)],

    where N + M = m–2 due to n = m–1 (the perturbative series of Mb|PAAN/M is one-order higher than the perturbative series of ρN/M(μ), since the perturbative series of Mb|PAAN/M includes αs0-order terms after factoring m¯b(μ); m and n denote the accuracies of the Mb|PAAN/M and ρN/M(μ), respectively), μ = μr for conventional series and μ = Q* for the PMC series. The PAA works for m ≥ 3. Following the standard PAA procedures described in detail in Ref. [38], we obtain the different types of PAA predictions by using the known two-, three-, and four-loop pQCD series and put them in Tables 1 and 2.

    Table  1.  The mth-loop PAA predictions Mb|PAAN/M (in units of GeV) for the conventional series with μr=m¯b(m¯b), where N + M = m–2.
    m = 3m = 4m = 5
    Mb|PAAN/M[0/1] 4.976[0/2] 5.216[0/3] 5.586
    [1/1] 5.317[1/2] 3.441
    [2/1] 7.090
     | Show Table
    DownLoad: CSV
    Table  2.  The mth-loop PAA predictions Mb|PAAN/M (in units of GeV) for the PMC series, where N + M = m–2.
    m = 3m = 4m = 5
    Mb|PAAN/M[0/1] 5.295[0/2] 5.161[0/3] 5.355
    [1/1] 4.939[1/2] 5.335
    [2/1] 5.261
     | Show Table
    DownLoad: CSV

    Due to the presence of divergent renormalon terms associated with the β-function and γm-function in each loop term, the PAA prediction derived from the conventional series exhibits significant uncertainty. The PAA prediction is generally [N/M]-type dependent, which provides the systematic error of the PAA approach. More explicitly, Table 1 shows that the relative magnitudes of the allowable types of PAA predictions are Mb|PAAm=3:Mb|PAAm=4:Mb|PAAm=5=1 : 1.05–1.07 : 0.69–1.42 for the conventional series, respectively. On the contrary, the PMC conformal series, which is free of renormalon terms associated with the β-function and γm-function, can be a more reliable foundation for predicting UHO contribution. Table 2 shows that the relative magnitudes of the allowable types of PAA predictions are Mb|PAAm=3:Mb|PAAm=4:Mb|PAAm=5=1 : 0.93–0.97 : 0.99–1.01 for the PMC series, respectively. It has been found that the [0/n–1] or [0/m–2]-type PAA predictions are self-consistent for the PMC method itself,[38] which agrees with the GM-L scale-setting procedure[46] to obtain scale-independent perturbative QED predictions. Moreover, one may also observe that the [0/n–1]-type PAA predictions under different orders exhibit better stability than other types. Thus, we adopt the [0/n–1]-type PAA predictions as an estimate of the UHO contributions, i.e.,

    ΔMb|Conv.Highorder=±|Mb|PAA,Conv.[0/3]Mb|Conv.|=±0.524(GeV),

    (10)

    ΔMb|PMCHighorder=±|Mb|PAA,PMC[0/3]Mb|PMC|=±0.017(GeV).

    (11)

    Due to the elimination of divergent renormalon terms, the PMC series predicts a much smaller uncertainty from the UHO-terms. It is also found that the PAA works better when more terms have been known. We define a ratio, κi=|(Mb|PAA[0/n1]MbO(αsn))/MbO(αsn)| with n = (2, 3, 4), which shows more explicitly how more loop terms affect the accuracy of the PAA prediction. For conventional series, we have κ2 : κ3 : κ4 = 0.041 : 0.059 : 0.104; and for the PMC conformal series, we have κ2 : κ3 : κ4 = 0.028 : 0.033 : 0.003.

    In addition to the uncertainties due to UHO-terms, there are also uncertainties from the Δαs(MZ) and Δm¯b(m¯b). Using αs(MZ) = 0.1180±0.0009[31] as an estimate, we obtain

    ΔMb|Conv.Δαs(MZ)=(0.026+0.028)(GeV),

    (12)

    ΔMb|PMCΔαs(MZ)=(0.073+0.089)(GeV).

    (13)

    Using the RGE to fix the correct magnitude of αs, the PMC series thus depends heavily on the precise αs running behavior. The more sensitivity of the PMC series on the value of αs(MZ) makes it inversely be a better platform to fix the reference point value from comparison of experimental data.[47]

    Regarding the uncertainty arising from the choice of the bottom-quark MS¯ mass, Δm¯b(m¯b)=±0.007 GeV, we obtain

    ΔMb|Conv.Δm¯b(m¯b)=(0.007+0.008)(GeV),

    (14)

    ΔMb|PMCΔm¯b(m¯b)=(0.005+0.007)(GeV).

    (15)

    This indicates that the bottom-quark OS mass could depend almost linearly on its MS¯ mass, since the uncertainty is at the same order of O(Δm¯b(m¯b)).

    In summary, we have determined the bottom-quark OS mass using the four-loop MS¯-on-shell relation in conjunction with the newly suggested PMC approach, which determines the correct magnitudes of the αs and the MS¯-running mass simultaneously by using the β-function and γm-function of the pQCD series. Taking the bottom-quark MS¯ mass m¯b(m¯b)=4.183±0.007 GeV as an input, we have derived a precise bottom-quark OS mass:

    Mb|Conv.=5.0620.525+0.533(GeV),

    (16)

    Mb|PMC=5.3720.075+0.091(GeV),

    (17)

    where the uncertainties stem from the mean square of those originating from ΔMb|Highorder, ΔMb|Δαs(MZ), and ΔMb|Conv.Δm¯b(m¯b), respectively. It is important to note that the conventional prediction still exhibits renormalization scale uncertainty, which arises from varying μr within the range μr[m¯b(m¯b)/2,2m¯b(m¯b)].

    The accuracy of the pQCD predictions within the framework of the MS¯ running mass scheme is critically dependent on the precise determination of αs and m¯q. With the implementation of the PMC approach, the accurate values of the effective αs and m¯q can be ascertained. This results in a more convergent pQCD series, thereby reducing uncertainties and promoting the attainment of a reliable and precise pQCD prediction.

  • [1]
    Tarrach R 1981 Nucl. Phys. B 183 384

    Google Scholar

    [2]
    't Hooft G 1973 Nucl. Phys. B 61 455

    Google Scholar

    [3]
    Bardeen W A, Buras A J, Duke D W and Muta T 1978 Phys. Rev. D 18 3998

    Google Scholar

    [4]
    Beneke M and Braun V M 1995 Phys. Lett. B 348 513

    Google Scholar

    [5]
    Neubert M 1995 Phys. Rev. D 51 5924

    Google Scholar

    [6]
    Beneke M 1999 Phys. Rep. 317 1

    Google Scholar

    [7]
    Gray N, Broadhurst D J, Grafe W and Schilcher K 1990 Z. Phys. C 48 673

    Google Scholar

    [8]
    Chetyrkin K G and Steinhauser M 2000 Nucl. Phys. B 573 617

    Google Scholar

    [9]
    Melnikov K and Ritbergen T V 2000 Phys. Lett. B 482 99

    Google Scholar

    [10]
    Jegerlehner F, Kalmykov M Y and Veretin O 2003 Nucl. Phys. B 658 49

    Google Scholar

    [11]
    Jegerlehner F and Kalmykov M Y 2003 Acta Phys. Polon. B 34 5335

    Google Scholar

    [12]
    Faisst M, Kühn J H and Veretin O 2004 Phys. Lett. B 589 35

    Google Scholar

    [13]
    Marquard P, Mihaila L, Piclum J H and Steinhauser M 2007 Nucl. Phys. B 773 1

    Google Scholar

    [14]
    Marquard P, Smirnov A V, Smirnov V A and Steinhauser M 2015 Phys. Rev. Lett. 114 142002

    Google Scholar

    [15]
    Marquard P, Smirnov A V, Smirnov V A, Steinhauser M and Wellmann D 2016 Phys. Rev. D 94 074025

    Google Scholar

    [16]
    Alam Khan M S A 2023 Phys. Rev. D 108 074029

    Google Scholar

    [17]
    Kataev A L and Molokoedov V S 2018 JETP Lett. 108 777

    Google Scholar

    [18]
    Kataev A L and Molokoedov V S 2019 Theor. Math. Phys. 200 1374

    Google Scholar

    [19]
    Kataev A L and Molokoedov V S 2020 Eur. Phys. J. C 80 1160

    Google Scholar

    [20]
    Politzer H D 1973 Phys. Rev. Lett. 30 1346

    Google Scholar

    [21]
    Gross D J and Wilczek F 1973 Phys. Rev. Lett. 30 1343

    Google Scholar

    [22]
    Politzer H D 1974 Phys. Rep. 14 129

    Google Scholar

    [23]
    Gross D J and Wilczek F 1973 Phys. Rev. D 8 3633

    Google Scholar

    [24]
    Chetyrkin K G 2005 Nucl. Phys. B 710 499

    Google Scholar

    [25]
    Baikov P A, Chetyrkin K G and Kühn J H 2017 Phys. Rev. Lett. 118 082002

    Google Scholar

    [26]
    Vermaseren J A M, Larin S A and van Ritbergen T 1997 Phys. Lett. B 405 327

    Google Scholar

    [27]
    Chetyrkin K G 1997 Phys. Lett. B 404 161

    Google Scholar

    [28]
    Baikov P A, Chetyrkin K G and Kühn J H 2014 J. High Energy Phys. 10 76

    Google Scholar

    [29]
    Wu X G, Brodsky S J and Mojaza M 2013 Prog. Part. Nucl. Phys. 72 44

    Google Scholar

    [30]
    Wu X G, Ma Y, Wang S Q, Fu H B, Ma H H, Brodsky S J and Mojaza M 2015 Rept. Prog. Phys. 78 126201

    Google Scholar

    [31]
    Navas S, [Particle Data Group] et al. 2024 Phys. Rev. D 110 030001

    Google Scholar

    [32]
    Brodsky S J and Wu X G 2012 Phys. Rev. D 85 034038

    Google Scholar

    [33]
    Brodsky S J and Di Giustino L 2012 Phys. Rev. D 86 085026

    Google Scholar

    [34]
    Brodsky S J and Wu X G 2012 Phys. Rev. Lett. 109 042002

    Google Scholar

    [35]
    Mojaza M, Brodsky S J and Wu X G 2013 Phys. Rev. Lett. 110 192001

    Google Scholar

    [36]
    Brodsky S J, Mojaza M and Wu X G 2014 Phys. Rev. D 89 014027

    Google Scholar

    [37]
    Shen J M, Wu X G, Du B L and Brodsky S J 2017 Phys. Rev. D 95 094006

    Google Scholar

    [38]
    Du B L, Wu X G, Shen J M and Brodsky S J 2019 Eur. Phys. J. C 79 182

    Google Scholar

    [39]
    Wu X G, Shen J M, Du B L, Huang X D, Wang S Q and Brodsky S J 2019 Prog. Part. Nucl. Phys. 108 103706

    Google Scholar

    [40]
    Di Giustino L, Brodsky S J, Ratcliffe P G, Wu X G and Wang S Q 2024 Prog. Part. Nucl. Phys. 135 104092

    Google Scholar

    [41]
    Huang X D, Wu X G, Zheng X C, Yan J, Wu Z F and Ma H H 2024 Chin. Phys. C 48 053113

    Google Scholar

    [42]
    Basdevant J L 1972 Fortsch. Phys. 20 283

    Google Scholar

    [43]
    Samuel M A, Li G and Steinfelds E 1994 Phys. Lett. B 323 188

    Google Scholar

    [44]
    Samuel M A, Ellis J and Karliner M 1995 Phys. Rev. Lett. 74 4380

    Google Scholar

    [45]
    Herren F and Steinhauser M 2018 Comput. Phys. Commun. 224 333

    Google Scholar

    [46]
    Gell-Mann M and Low F E 1954 Phys. Rev. 95 1300

    Google Scholar

    [47]
    Shen J M, Qin B H, Yan J, Wang S Q and Wu X G 2023 J. High Energy Phys. 2023 109

    Google Scholar

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