This paper was converted on www.awesomepapers.org from LaTeX by an anonymous user.
Want to know more? Visit the Converter page.

QCD condensates and αs\alpha_{s} from τ\tau-decay

Stephan Narison Laboratoire Univers et Particules de Montpellier (LUPM), CNRS-IN2P3,
Case 070, Place Eugène Bataillon, 34095 - Montpellier, France
and
Institute of High-Energy Physics of Madagascar (iHEPMAD)
University of Ankatso, Antananarivo 101, Madagascar
[email protected]
Abstract

We improve the determinations of the QCD condensates within the SVZ expansion in the axial-vector (A) channel using the ratio of Laplace sum rule (LSR) 10A(τ){\cal R}_{10}^{A}(\tau) within stability criteria and τ\tau-like higher moments n,A{\cal R}_{n,A} within stability for arbitrary τ\tau-mass squared s0s_{0}. We find the same violation of the factorization by a factor 6 of the four-quark condensate as from e+ee^{+}e^{-}\to Hadrons data. One can notice a systematic alternate sign and no exponential growth of the size of these condensates. Then, we extract αs\alpha_{s} from the lowest τ\tau-decay like moment. We obtain to order αs4\alpha_{s}^{4} the conservative value from the s0s_{0}-stability until Mτ2M_{\tau}^{2} : αs(Mτ)|A=0.3178(66)\alpha_{s}(M_{\tau})|_{A}=0.3178(66) (FO) and 0.3380 (44) (CI) leading to : αs(MZ)|A=0.1182(8)fit(3)evol.\alpha_{s}(M_{Z})|_{A}=0.1182(8)_{fit}(3)_{evol.} (FO) and 0.1206(5)fit(3)evol.0.1206(5)_{fit}(3)_{evol.} (CI). We extend the analysis to the channel and find: αs(Mτ)|VA=0.3135(83)\alpha_{s}(M_{\tau})|_{V-A}=0.3135(83) (FO) and 0.3322 (81) (CI) leading to : αs(MZ)|VA=0.1177(10)fit(3)evol.\alpha_{s}(M_{Z})|_{V-A}=0.1177(10)_{fit}(3)_{evol.} (FO) and 0.1200(9)fit(3)evol.0.1200(9)_{fit}(3)_{evol.} (CI). We observe that in different channels (e+ee^{+}e^{-}\to Hadrons,  A, V, V–A), the extraction of αs(Mτ)\alpha_{s}(M_{\tau}) at the observed τ\tau-mass leads to an overestimate of its value. Our determinations from these different channels lead to the mean : αs(Mτ)=0.3140(44)\alpha_{s}(M_{\tau})=0.3140(44) (FO) and 0.3346 (35) (CI) leading to : αs(MZ)=0.1178(6)fit(3)evol.\alpha_{s}(M_{Z})=0.1178(6)_{fit}(3)_{evol.} (FO) and 0.1202(4)fit(3)evol.0.1202(4)_{fit}(3)_{evol.} (CI). Comparisons with some other results are done.

keywords:
QCD spectral sum rules, QCD condensates, αs,τ\alpha_{s},\,\tau-decay, e+ee^{+}e^{-}\to Hadrons.

1 Introduction

In this paper, we pursue the determinations of the QCD condensates and αs\alpha_{s} done in [1, 2] for the e+ee^{+}e^{-}\to Hadrons and the vector (V) current to the case of axial-vector (A) and V–A currents. In so doing, we shall use the τ\tau sum rule variable stability criteria for the Laplace sum rule and the MτM_{\tau} stability for the τ\tau-like moment sum rule.

Definitions and normalizations of observables will be the same as in Ref. [1, 2] and will not be extensively discussed here.

2 The axial-vector (A) two-point function

\bullet~{}The two-point function

We shall be concerned with the two-point correlator :

ΠV(A)μν(q2)\displaystyle\Pi^{\mu\nu}_{V(A)}(q^{2}) =\displaystyle= id4xeiqx0|𝒯JV(A)μ(x)(JV(A)ν(0))|0\displaystyle i\int d^{4}x~{}e^{-iqx}\langle 0|{\cal T}{J^{\mu}_{V(A)}}(x)\left({J^{\nu}_{V(A)}}(0)\right)^{\dagger}|0\rangle (1)
=\displaystyle= (gμνq2qμqν)ΠV(A)(1)(q2)+qμqνΠV(A)(0)(q2)\displaystyle-(g^{\mu\nu}q^{2}-q^{\mu}q^{\nu})\Pi^{(1)}_{V(A)}(q^{2})+q^{\mu}q^{\nu}\Pi^{(0)}_{V(A)}(q^{2})

built from the T-product of the bilinear axial-vector current of u,du,d quark fields:

JV(A)μ(x)=:ψ¯uγμ(γ5)ψd:.J^{\mu}_{V(A)}(x)=:\bar{\psi}_{u}\gamma^{\mu}(\gamma_{5})\psi_{d}:. (2)

The upper indices (0) and (1) correspond to the spin of the associated hadrons. The two-point function obeys the dispersion relation:

ΠV(A)(q2)=t>dttq2iϵ1πImΠV(A)(t)+,\Pi_{V(A)}(q^{2})=\int_{t>}^{\infty}\frac{dt}{t-q^{2}-i\epsilon}\frac{1}{\pi}\,{\rm Im}\Pi_{V(A)}(t)+\cdots, (3)

where \cdots are subtraction constants polynomial in q2q^{2} and t>t> is the hadronic threshold.

\bullet~{}QCD expression of the two-point function

Within the SVZ-expansion [3], the two-point function can be expressed in terms of the sum of higher and higher quark and gluon condensates:

4π2ΠH(Q2,mq2,μ)=D=0,2,4,..CD,H(Q2,mq2,μ)OD,H(μ)(Q2)D/2D=0,2,4,..dD,H(Q2)D/2,4\pi^{2}\Pi_{H}(-Q^{2},m_{q}^{2},\mu)=\sum_{D=0,2,4,..}\frac{C_{D,H}(Q^{2},m_{q}^{2},\mu)\langle O_{D,H}(\mu)\rangle}{(Q^{2})^{D/2}}\equiv\sum_{D=0,2,4,..}\frac{d_{D,H}}{(Q^{2})^{D/2}}~{}, (4)

where HV(A)H\equiv V(A), μ\mu is the subtraction scale which separates the long (condensates) and short (Wilson coefficients) distance dynamics and mqm_{q} is the quark mass.

\diamond~{}In the chiral limit [4, 5]:

d2,A\displaystyle d_{2,A} =\displaystyle= d2,V=0,\displaystyle d_{2,V}=0,
d4,A\displaystyle d_{4,A} =\displaystyle= d4,V=π3αsG2(1+76as),\displaystyle d_{4,V}=\frac{\pi}{3}\langle\alpha_{s}G^{2}\rangle\left(1+\frac{7}{6}a_{s}\right),
d6,A\displaystyle d_{6,A} =\displaystyle= (117)d6,V=140881π3ραsψ¯ψ2,\displaystyle-\left(\frac{11}{7}\right)d_{6,V}=\frac{1408}{81}\pi^{3}\rho\alpha_{s}\langle\bar{\psi}\psi\rangle^{2},
d8,A\displaystyle d_{8,A} \displaystyle\approx d8,V39162παsG22\displaystyle d_{8,V}\approx-\frac{39}{162}\pi\langle\alpha_{s}G^{2}\rangle^{2} (5)

where ρ\rho measures the deviation from the factorization of the 4-quark condensates and the last equality for d8d_{8} is based on vacuum saturation estimate of some classes of computed dimension-8 diagrams.

\diamond~{}The perturbative expression of the spectral function is known to order αs4\alpha_{s}^{4}[6, 7]. It reads for 3 flavours:

4πImΠH(t)=1+as+1.6398as210.2839as3106.8798as4+𝒪(as5),4{\pi}\,{\rm Im}\Pi_{H}(t)=1+a_{s}+1.6398a_{s}^{2}-10.2839a_{s}^{3}-106.8798a_{s}^{4}+{\cal O}(a_{s}^{5}), (6)

where :

asαsπ=2β1Log(t/Λ2)+,a_{s}\equiv\frac{\alpha_{s}}{\pi}=\frac{2}{-\beta_{1}{\rm Log}(t/\Lambda^{2})}+\cdots, (7)

where β1=(1/2)(112nf/3)-\beta_{1}=(1/2)(11-2n_{f}/3) is the first coefficient of the β\beta-function and nfn_{f} is the number of quark flavours; \cdots stands for higher order terms which can e.g. be found in [8]. We shall use the value Λ=(342±8)\Lambda=(342\pm 8) MeV for nf=3n_{f}=3   from the PDG average [9].

\bullet~{}Spectral function from the data

We shall use the recent ALEPH data [10] in Fig. 1 for the spectral function a1(s)a_{1}(s).

Refer to caption
Figure 1: ALEPH data of the axial-vector spectral function.

Like in the case of the vector spectral function from e+ee^{+}e^{-}\to Hadrons [2], we subdivide the region from 3π3\pi threshold to Mτ2=3.16M_{\tau}^{2}=3.16 GeV2 into different subregions in ss (units in [GeV2]):

s=[0.4,0.8],[0.8,1.29],[1.29,1.42],[1.42,2.35],[2.35,3.16],s=[0.4,0.8],~{}[0.8,1.29],~{}[1.29,1.42],~{}[1.42,2.35],~{}[2.35,3.16], (8)

and fit the data with 3rd order polynomials using the optimized Mathematica program FindFit except for [1.29,1.42][1.29,1.42] where a 2nd order polynomial is used. We show the different fits in the Fig. 2.

Refer to caption
Refer to caption
Refer to caption
Refer to caption
Refer to caption
Figure 2: Fit of the data using a 2nd and 3rd order polynomial fits.

3 The ratio of Laplace sum rule (LSR) moments

Like in the case of vector channel, we shall use here the ratio of LSR moments [3, 11, 12]111For a recent review, see e.g. [13].:

10A(τ)1c0c=t>tc𝑑tetτt1πImΠH(t,μ2,mq2)t>tc𝑑tetτ1πImΠH(t,μ2,mq2),{\cal R}^{A}_{10}(\tau)\equiv\frac{{\cal L}^{c}_{1}}{{\cal L}^{c}_{0}}=\frac{\int_{t>}^{t_{c}}dt~{}e^{-t\tau}t\,\frac{1}{\pi}\,{\rm Im}\Pi_{H}(t,\mu^{2},m_{q}^{2})}{\int_{t>}^{t_{c}}dt~{}e^{-t\tau}\,\frac{1}{\pi}\,{\rm Im}\Pi_{H}(t,\mu^{2},m_{q}^{2})}, (9)

where τ\tau is the LSR variable, t>t> is the hadronic threshold. Here tct_{c} is the threshold of the “QCD continuum” which parametrizes, from the discontinuity of the Feynman diagrams, the spectral function ImΠH(t,mq2,μ2){\rm Im}\,\Pi_{H}(t,m_{q}^{2},\mu^{2}). mqm_{q} is the quark mass and μ\mu is an arbitrary subtraction point.

\bullet~{}QCD expression of the LSR moments

To order αs4\alpha_{s}^{4}, the perturbative (PT) expression of the lowest moment reads [1]:

0PT(τ)=32τ1[1+as+2.93856as2+6.2985as3+22.2233as4].{\cal L}^{PT}_{0}(\tau)=\frac{3}{2}\tau^{-1}\Big{[}1+a_{s}+2.93856\,a_{s}^{2}+6.2985\,a_{s}^{3}+22.2233\,a_{s}^{4}\Big{]}. (10)

Then, taking its derivative in τ\tau, one gets 1(τ){\cal L}_{1}(\tau) and then their ratio 10(τ){\cal R}_{10}(\tau).

From Eq. 4, one can deduce the non-perturbative contribution to the lowest LSR moment :

0NPT(τ)=32τ1DdD(D/21)!τD/2,{\cal L}^{NPT}_{0}(\tau)=\frac{3}{2}\tau^{-1}\sum_{D}\frac{d_{D}}{(D/2-1)!}\tau^{D/2}~{}, (11)

from which one can deduce 1NPT{\cal L}^{NPT}_{1} and 10A{\cal R}^{A}_{10}.

\bullet~{}d6,Ad_{6,A} and d8,Ad_{8,A} from 10A{\cal R}^{A}_{10}

We show in Fig. 3a) the τ\tau behaviour of the phenomenological side of 10A{\cal R}^{A}_{10} (experiment \oplus QCD continuum beyond the threshold tct_{c}) for values of tct_{c} around the physical τ\tau-lepton mass squared where the effect of tct_{c} is negligible.

a)                                                                      b)
Refer to caption
Refer to caption

Figure 3: a): R10AR^{A}_{10} versus the LSR variable τ\tau; b): d6,Ad_{6,A} and d8,Ad_{8,A} from the 10A{\cal R}^{A}_{10}

For determining d6,Ad_{6,A} and d8,Ad_{8,A}, we use as input the more precise value of αsG2\langle\alpha_{s}G^{2}\rangle from the heavy quark mass-splittings and some other sum rules [14, 15]:

αsG2=(6.39±0.35)×102GeV4,\langle\alpha_{s}G^{2}\rangle=(6.39\pm 0.35)\times 10^{-2}\,{\rm GeV^{4}}, (12)

and perform a two-parameter fit (d6,A,d8,A)(d_{6,A},d_{8,A}) by confronting the phenomenological and QCD side of R10AR^{A}_{10} for different values of τ\tau. The QCD coupling αs\alpha_{s} is evaluated at the LSR sum rule scale τ\tau where we use Λ=(342±8)\Lambda=(342\pm 8) MeV for nf=3n_{f}=3 flavours deduced from the PDG world average [9]. The results of the analysis are shown in Fig. 3. There is an inflexion point around τ2.5\tau\simeq 2.5 GeV-2 at which we extract the optimal values of the condensates. One should note that at this scale the OPE converges quite well in the vector channel [1]. Then, we may expect that for the axial-vector the same feature occurs. We obtain the optimal result:

d6,A=(33.5±3.0±2.7)×102GeV6d8,A=(47.2±2.8±3.2)×102GeV8d_{6,A}=(33.5\pm 3.0\pm 2.7)\times 10^{-2}\,{\rm GeV^{6}}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}d_{8,A}=-(47.2\pm 2.8\pm 3.2)\times 10^{-2}\,{\rm GeV^{8}} (13)

where the 1st error comes from the fitting procedure and the 2nd one from the localization of τ(2.5±0.1)\tau\simeq(2.5\pm 0.1) GeV-2.

Refer to caption
Figure 4: αsG2\langle\alpha_{s}G^{2}\rangle versus the LSR variable τ\tau.

\bullet~{}αsG2\langle\alpha_{s}G^{2}\rangle from 10A{\cal R}^{A}_{10}

We use the previous values of d6,Ad_{6,A} and d8,Ad_{8,A} into 10A{\cal R}^{A}_{10} and we re-extract αsG2\langle\alpha_{s}G^{2}\rangle using a one-parameter fit. The analysis is shown in Fig. 4. We obtain:

αsG2=(6.9±1.5)×102GeV4,\langle\alpha_{s}G^{2}\rangle=(6.9\pm 1.5)\times 10^{-2}\,{\rm GeV}^{4}, (14)

in good agreement with the one in Eq. 12 used previously as input. This result also indicates the sef-consistency of the set of condensates entering in the analysis.

4 BNP τ\tau-decay like moments

As emphasized by BNP in Ref. [4, 5], it is more convenient to express the moment in terms of the combination of Spin (1+0) and Spin 0 spectral functions in order to avoid some eventual pole from Π(0)\Pi^{(0)} at s=0s=0:

n,H=6πi|s|=M02𝑑x(1x)2xn((1+2x)ΠH(1+0)(x)2xΠH(0)(x)){\cal R}_{n,H}=6\pi\,i\,\int_{|s|=M_{0}^{2}}dx\,(1-x)^{2}\,x^{n}\left((1+2x)\,\Pi^{(1+0)}_{H}(x)-2x\Pi^{(0)}_{H}(x)\right) (15)

with xs/M02x\equiv s/M^{2}_{0}, HV,AH\equiv V,A. nn indicates the degree of moment. The lowest moment 0,A{\cal R}_{0,A} corresponds to the physical τ\tau-decay process [5, 4].

\bullet~{}The lowest moment 0,A{\cal R}_{0,A} from the data

Refer to caption
Figure 5: Lowest moment R0,AR_{0,A} versus the hypothetical τ\tau-mass squared s0s_{0}.

Using previous fits of the data, we show in Fig. 5 the behaviour of the lowest moment 0/A{\cal R}_{0/A} versus an hypothetical τ\tau-lepton mass squared s0M02s_{0}\equiv M^{2}_{0}. At the observed mass value: Mτ=1.777M_{\tau}=1.777 GeV, one obtains:

0,A=1.698(14).{\cal R}_{0,A}=1.698(14). (16)

It reproduces with high accuracy the ALEPH value [10] :

0,A|Aleph=1.694(10),{\cal R}_{0,A}|_{\rm Aleph}=1.694(10), (17)

which is an important self-consistency test of our fitting procedure.

\bullet~{}The lowest BNP moment 0,A{\cal R}_{0,A}

The QCD expression of 0,A{\cal R}_{0,A} including the dimension six (d6,A)(d_{6,A}) and eight (d8,A)(d_{8,A}) condensates within the SVZ expansion [3] can be deduced from [4]. To simplify for the reader, we give its expression, in the chiral limit 222We use the complete expression including quark masses and αs\alpha_{s} corrections in the numerical analysis.:

0,A=Nc2|Vud|2Sew{1+δew+δA(0)+D=1,2,δA(2D)].{\cal R}_{0,A}=\frac{N_{c}}{2}|V_{ud}|^{2}\,S_{ew}\Big{\{}1+\delta^{\prime}_{ew}+\delta^{(0)}_{A}+\sum_{D=1,2,\dots}\delta_{A}^{(2D)}\Big{]}. (18)

where the electroweak factors and corrections are :

Vud=0.97418,Sew=1.019,δew=0.0010.V_{ud}=0.97418,~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}S_{ew}=1.019,~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}\delta^{\prime}_{ew}=0.0010. (19)

The QCD corrections copied from BNP are:

\diamond~{}Perturbative corrections to order αs4\alpha_{s}^{4}:

δA(0)|FO\displaystyle\delta^{(0)}_{A}|_{FO} =\displaystyle= as+5.2023as2+26.366as3+127.079as4,\displaystyle a_{s}+5.2023\,a_{s}^{2}+26.366\,a_{s}^{3}+127.079\,a_{s}^{4},
δA(0)|CI\displaystyle\delta^{(0)}_{A}|_{CI} =\displaystyle= 1.364as+2.54as2+9.71as3+64.29as4,\displaystyle 1.364\,a_{s}+2.54\,a_{s}^{2}+9.71\,a_{s}^{3}+64.29\,a_{s}^{4}, (20)

for fixed order (FO) [4] and contour improved (CI)  [16].

Observing that the PT series grows geometrically [17] from the calculated coefficients in different channels, we estimate the as5a_{s}^{5} coefficient to be [1] :

δ5FO±552as5,δ5CI±228as5,\delta_{5}^{FO}\approx\pm 552\,a_{s}^{5},~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}\delta_{5}^{CI}\approx\pm 228\,a_{s}^{5}~{}, (21)

which one can consider either to be the error due to the unknown higher order terms of the series or (more optimistically) to be the estimate of the uncalculated αs5\alpha_{s}^{5} coefficient.

\diamond~{}Power corrections up to d8,Ad_{8,A}:

They read:

δA(2)\displaystyle\delta^{(2)}_{A} =\displaystyle= 8(1+163as)(mu2+md2)M024(1+253as)(mumd)M02,δA(2)|tach=2×1.05asλ2M02,\displaystyle-8(1+\frac{16}{3}a_{s})\frac{(m_{u}^{2}+m_{d}^{2})}{M_{0}^{2}}-4(1+\frac{25}{3}a_{s})\frac{(m_{u}m_{d})}{M_{0}^{2}},\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\delta^{(2)}_{A}|_{tach}=-2\times 1.05\frac{\,a_{s}\lambda^{2}}{M_{0}^{2}},
δA(4)\displaystyle\delta^{(4)}_{A} =\displaystyle= 11π4as2αsG2M04+32π2(1+6316as2)(mu+md)ψ¯uψuM048π2kmkψ¯kψkM04+𝒪(mq4)\displaystyle\frac{11\pi}{4}a_{s}^{2}\frac{\langle\alpha_{s}G^{2}\rangle}{M_{0}^{4}}+32\pi^{2}\left(1+\frac{63}{16}a_{s}^{2}\right)\frac{(m_{u}+m_{d})\langle\bar{\psi}_{u}\psi_{u}\rangle}{M_{0}^{4}}-8\pi^{2}\sum_{k}\frac{m_{k}\langle\bar{\psi}_{k}\psi_{k}\rangle}{M_{0}^{4}}+{\cal O}(m_{q}^{4})
δA(6)\displaystyle\delta^{(6)}_{A} =\displaystyle= 6d6,AM06,δA(8)=4d8,AM08,\displaystyle-6\frac{d_{6,A}}{M_{0}^{6}},\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\delta_{A}^{(8)}=-4\frac{d_{8,A}}{M_{0}^{8}}, (22)

where s0M02s_{0}\equiv M_{0}^{2} while d6,Ad_{6,A} and d8,Ad_{8,A} have been defined in Eqs. 5 . We have assumed ψ¯uψu=ψ¯dψd\langle\bar{\psi}_{u}\psi_{u}\rangle=\langle\bar{\psi}_{d}\psi_{d}\rangle. We shall not include the D=2D=2 contribution due to an eventual tachyonic gluon mass within the standard OPE. Using duality [17], this term can be included in the estimate of the non-calculated higher order terms of the PT series discussed previously. Instanton contributions are expected to have higher dimensions and their contributions can be safely neglected [1].

\bullet~{}d6,Ad_{6,A} and d8,Ad_{8,A} condensates from 0,A{\cal R}_{0,A}

a)                                                                      b)
Refer to caption
Refer to caption

Figure 6: a): |d6,A||d_{6,A}| (lowest curve) and |d8,A||d_{8,A}| (highest curve) versus M02M^{2}_{0}; b): similar to a) but for |d8,A||d_{8,A}| and |d10,A||d_{10,A}|.

We confront the experimental and QCD sides of 0,A{\cal R}_{0,A} for different values of s0s_{0}. Like in the case of the ratio of Laplace sum rules, we use a two-parameter fit (d6,A,d8,Ad_{6,A},d_{8,A}) to extract the values of these condensates using as input the values of the d4d_{4} condensates and light quark masses. We consider the PT series up to order αs4\alpha_{s}^{4} and evaluate αs\alpha_{s} at the hypothetical τ\tau-mass squared s0=M02s_{0}=M_{0}^{2}. We use Λ=(342±8)\Lambda=(342\pm 8) MeV for nf=3n_{f}=3 flavours from the PDG world average [9]. The results versus s0s_{0} are shown in Fig. 6a).

We consider as a reliable value the one from s0=1.93s_{0}=1.93 GeV2 beyond the peak of the A1A_{1} meson. We notice a stability (minimum) around 3 GeV2 just below the physical τ\tau mass which we consider as our optimal value:

d6,A\displaystyle d_{6,A} =\displaystyle= (36.2±0.5)×102GeV6d8,A=(55.2±0.9)×102GeV8(FO)\displaystyle(36.2\pm 0.5)\times 10^{-2}\,{\rm GeV^{6}}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}d_{8,A}=-(55.2\pm 0.9)\times 10^{-2}\,{\rm GeV^{8}}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}{\rm(FO)}
d6,A\displaystyle d_{6,A} =\displaystyle= (33.1±0.5)×102GeV6d8,A=(50.6±0.8)×102GeV8(CI)\displaystyle(33.1\pm 0.5)\times 10^{-2}\,{\rm GeV^{6}}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}d_{8,A}=-(50.6\pm 0.8)\times 10^{-2}\,{\rm GeV^{8}}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}{\rm(CI)} (23)

One can notice from the analysis that the absolute values of the condensates are slightly higher for FO than for CI. To be conservative, we take the arithmetic average of the FO and CI values and add as a systematic the largest distance between the mean and the individual value :

d6,A=(34.6±1.8)×102GeV6d8,A=(52.9±2.4)×102GeV8.d_{6,A}=(34.6\pm 1.8)\times 10^{-2}\,{\rm GeV^{6}}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}d_{8,A}=-(52.9\pm 2.4)\times 10^{-2}\,{\rm GeV^{8}}. (24)

5 d8,Ad_{8,A} and d10,Ad_{10,A} from 1,A{\cal R}_{1,A}

The expression of 1,A{\cal R}_{1,A} is similar to 1,V{\cal R}_{1,V} given in Eq. 20 of Ref. [1]. Using a two-parameter fit (d8,A,d10,Ad_{8,A},d_{10,A}) of 1,A{\cal R}_{1,A} for different s0s_{0}, we show the result of the analysis in Fig. 6b) using FO PT series. One obtains:

d8,A=(51.4±11.0)×102GeV6d10,A=(70.1±21.6)×102GeV8.d_{8,A}=-(51.4\pm 11.0)\times 10^{-2}\,{\rm GeV^{6}}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}d_{10,A}=(70.1\pm 21.6)\times 10^{-2}\,{\rm GeV^{8}}. (25)

The results are stable versus s0s_{0} but less accurate than in the case of 0,A{\cal R}_{0,A} such that one cannot differentiate a FO from CI truncation of the PT series. Then, for higher moments, we shall only consider FO PT series.

6 Final values of d6,Ad_{6,A} and d8,Ad_{8,A}

As a final value of d6,Ad_{6,A}, we take the mean of the values in Eqs. 13 and 24. We obtain:

d6,A=(34.4±1.7)×102GeV6,d_{6,A}=(34.4\pm 1.7)\times 10^{-2}\,{\rm GeV}^{6}, (26)

while for d8,Ad_{8,A}, we take the mean of the values obtained in Eqs.  13, 24 and 25. We obtain:

d8,A=(51.51±2.08)×102GeV8.d_{8,A}=-(51.51\pm 2.08)\times 10^{-2}\,{\rm GeV}^{8}. (27)

\diamond~{}We notice that the relation :

d6,A(11/7)d6,V,d_{6,A}\simeq-(11/7)\,d_{6,V}, (28)

is quite well satisfied within the errors. This result also suggests a violation of the four-quark condensate vacuum saturation (see Eq. 5) similar to the one found from e+ee^{+}e^{-}\to Hadrons data [1, 2] :

ραsψ¯ψ2=(6.38±0.30)×104GeV6ρ(6.38±0.30).\rho\alpha_{s}\langle\bar{\psi}\psi\rangle^{2}=(6.38\pm 0.30)\times 10^{-4}\,{\rm GeV}^{6}~{}~{}~{}~{}\longrightarrow~{}~{}~{}~{}\rho\simeq(6.38\pm 0.30). (29)

\bullet~{}Determination of αs(Mτ)\alpha_{s}(M_{\tau})

We use the previous values of d6,Ad_{6,A} and d8,Ad_{8,A} together with the one of αsG2\langle\alpha_{s}G^{2}\rangle in Eq.12 as inputs in the lowest BNP moment 0,A{\cal R}_{0,A} in order to determine αs(Mτ)\alpha_{s}(M_{\tau}). We show in Fig. 7, the behaviour of αs(Mτ)\alpha_{s}(M_{\tau}) versus an hypothetical τ\tau mass squared M02s0M_{0}^{2}\equiv s_{0}. One can notice an inflexion point in the region 2.50.15+0.102.5^{+0.10}_{-0.15} GeV2 at which we extract the optimal result. The conservative result from s0=2.1s_{0}=2.1 GeV2 to Mτ2M_{\tau}^{2} (see Fig. 7) is :

αs(Mτ)|A\displaystyle\alpha_{s}(M_{\tau})|_{A} =\displaystyle= 0.3178(10)(65)αs(MZ)|A=0.1182(8)(3)evol(FO)\displaystyle 0.3178(10)(65)~{}~{}~{}~{}~{}~{}~{}\longrightarrow~{}~{}~{}~{}~{}~{}~{}\alpha_{s}(M_{Z})|_{A}=0.1182(8)(3)_{evol}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}{\rm(FO)} (30)
=\displaystyle= 0.3380(10)(43)αs(MZ)|A=0.1206(5)(3)evol(CI).\displaystyle 0.3380(10)(43)~{}~{}~{}~{}~{}~{}~{}~{}\longrightarrow~{}~{}~{}~{}~{}~{}~{}\alpha_{s}(M_{Z})|_{A}=0.1206(5)(3)_{evol}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}{\rm(CI)}.

The 1st error in αs(Mτ)|A\alpha_{s}(M_{\tau})|_{A} comes from the fitting procedure. The 2nd one comes from an estimate of the αs5\alpha_{s}^{5} contribution from Ref. [1]. At the scale s0=s_{0}=2.5 GeV2 the sum of non-perturbative contributions to the moment normalized to the parton model is:

δNP,A(7.9±1.1)×102.\delta_{NP,A}\simeq-(7.9\pm 1.1)\times 10^{-2}. (31)

One can notice that extracting αs(Mτ)|A\alpha_{s}(M_{\tau})|_{A} at the observed τ\tau-mass tends to overestimate the result:

αs(Mτ)|A=0.3352(40)FO,0.3592(47)CI.\alpha_{s}(M_{\tau})|_{A}=0.3352(40)~{}~{}~{}{\rm FO},~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}0.3592(47)~{}~{}~{}{\rm CI}. (32)

These values extracted at MτM_{\tau} agree with the ones from Ref. [18] obtained at the same scale. The same feature has been observed in the case of e+ee^{+}e^{-}\to Hadrons.

Refer to caption
Figure 7: αs(Mτ)\alpha_{s}(M_{\tau}) versus the hypothetical τ\tau-mass squared s0s_{0}.

\bullet~{}Comparison with previous results

Channel d6d_{6} d8-d_{8} αs(Mτ)\alpha_{s}(M_{\tau}) FO αs(Mτ)\alpha_{s}(M_{\tau}) CI Refs.
e+ee^{+}e^{-} (26.3±3.7)-(26.3\pm 3.7) (18.2±0.6)-(18.2\pm 0.6) 0.3081(86) 0.3260(78) [1]
V 0.3129(79) 0.3291(70) [1]
A 34.4±1.734.4\pm 1.7 51.5±2.151.5\pm 2.1 0.3157(65) 0.3368(45) This work
A 43.4±13.843.4\pm 13.8 59.2±19.759.2\pm 19.7 0.3390(180)0.3390(180) 0.3640(230)0.3640(230) [18]
A 19.7±1.019.7\pm 1.0 27±1.227\pm 1.2 0.3350(120) [10]
A 9.6±3.39.6\pm 3.3 9.0±5.09.0\pm 5.0 0.3230(160) 0.3470(230) [20]
Table 1: Values of the QCD condensates from some other τ\tau-moments at Fixed Order (FO) PT series and of αs(Mτ)\alpha_{s}(M_{\tau}) for FO and Contour Improved (CI) PT series.

We compare our results with the ones from e+ee^{+}e^{-} and τ\tau-decay Vector channel [1] and with the results obtained by different authors in the Axial-Vector channel:

\diamond~{}Our values of d6,Ad_{6,A} and d8,Ad_{8,A} are in good agreement within the errors with the ones of Ref. [18] but about two times larger than the ones of Ref.[10].

\diamond~{}The value of d8,Ad_{8,A} suggests that the assumption in Eq. 5:

d8,Ad8,Vd_{8,A}\approx d_{8,V} (33)

is not satisfied by the fitted values given in Table 1.

7 High-dimension condensates

To determine the high-dimension condensates, we use the analogue of the moments given Eq. 19 of Ref. [1] for the vector channel.

\bullet~{}d10,Ad_{10,A} and d12,Ad_{12,A} condensates from 2,A{\cal R}_{2,A}

We use a two-parameter fit to extract (d10,A,d12,A)(d_{10,A},d_{12,A}) from 2,A{\cal R}_{2,A}, (d12,A,d14,A)(d_{12,A},d_{14,A}) from 3,A{\cal R}_{3,A}. The s0s_{0} behaviour of the results is given in Fig. 8.

a)                                                                      b)
Refer to caption
Refer to caption

Figure 8: a): |d10,A||d_{10,A}| (lowest curve) and |d12,A||d_{12,A}| (highest curve) versus M02M^{2}_{0}; b): similar to a) but for |d12,A||d_{12,A}| and |d14,A||d_{14,A}|.

We deduce from 2,A{\cal R}_{2,A}:

d10,A=(53.9±0.7)×102GeV10,d12,A=(65.±1.)×102GeV12d_{10,A}=(53.9\pm 0.7)\times 10^{-2}\,{\rm GeV}^{10},~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}d_{12,A}=-(65.\pm 1.)\times 10^{-2}\,{\rm GeV}^{12} (34)

inside the stability region 1.93 GeV2 to Mτ2M_{\tau}^{2}. We take as a final value of d10,Ad_{10,A} the mean from 1,A{\cal R}_{1,A} in Eq. 25 and the one from 2,A{\cal R}_{2,A} in Eq. 34:

d10,A=(53.9±0.7)×102GeV10.d_{10,A}=(53.9\pm 0.7)\times 10^{-2}\,{\rm GeV}^{10}. (35)

\bullet~{}d2n,Ad_{2n,A} and d2(n+1),Ad_{2(n+1),A} condensates

We do the same procedure as previously for higher dimension condensates n6n\geq 6. The s0s_{0} behaviours of the condensates are shown in Figs. 9,  10. The results are summarized in Table 2.

a)                                                                      b)
Refer to caption
Refer to caption

Figure 9: a): |d14,A||d_{14,A}| (lowest curve) and |d16,A||d_{16,A}| (highest curve) versus M02M^{2}_{0}; b): similar to a) but for |d16,A||d_{16,A}| and |d18,A||d_{18,A}|.
Refer to caption
Figure 10: |d18,A||d_{18,A}| (lowest curve) and |d12,A||d_{12,A}| (highest curve) versus M02M^{2}_{0}.

\diamond~{}One can notice that the condensates in the A channel has alternate sign.

\diamond~{}Their size is almost constant and more accurate than previous determinations in the literaure. There is not also any sign of an exponential growth. This feature in the Euclidian region does not favour a sizeable duality violation in the time-like region [19].

d6,A\color[rgb]{.1,.5,0.3}d_{6,A} d8,A\color[rgb]{.1,.5,0.3}-d_{8,A} d10,A\color[rgb]{.1,.5,0.3}d_{10,A} d12,A\color[rgb]{.1,.5,0.3}-d_{12,A} d14,A\color[rgb]{.1,.5,0.3}d_{14,A} d16,A\color[rgb]{.1,.5,0.3}-d_{16,A} d18,A\color[rgb]{.1,.5,0.3}d_{18,A} d20,A\color[rgb]{.1,.5,0.3}-d_{20,A} Refs.
34.4±1.734.4\pm 1.7 51.5±2.151.5\pm 2.1 53.9±0.753.9\pm 0.7 63.3±1.863.3\pm 1.8 77.0±6.077.0\pm 6.0 93.1±4.093.1\pm 4.0 104.3±7.7104.3\pm 7.7 119.7±8.2119.7\pm 8.2 This work
43.4±13.843.4\pm 13.8 59.2±19.759.2\pm 19.7 63.2±33.663.2\pm 33.6 43.4±31.643.4\pm 31.6 [18]
19.7±1.019.7\pm 1.0 27±1.227\pm 1.2 [10]
9.6±3.39.6\pm 3.3 9.0±5.09.0\pm 5.0 [20]
Table 2: Values of the QCD condensates of dimension DD in units of 10210^{-2} GeVD from this work and some other estimates.

8 The V–A channel

\bullet~{}The two-point function

Its corresponds to the V–A quark current:

JVAμ(x)=:ψ¯uγμ(1γ5)ψd:.J^{\mu}_{V-A}(x)=:\bar{\psi}_{u}\gamma^{\mu}(1-\gamma_{5})\psi_{d}:. (36)

In the chiral limit, the QCD expression of the corresponding two-point function is similar to the one in Eq. 5 where:

d6,VA\displaystyle d_{6,V-A} =\displaystyle= 12(d6,V+d6,A)=12(47)d6,V\displaystyle\frac{1}{2}\left(d_{6,V}+d_{6,A}\right)=-\frac{1}{2}\left(\frac{4}{7}\right)d_{6,V}
=\displaystyle= 51227π3ραsψ¯ψ2=(37.5±1.9)×102GeV6,\displaystyle\frac{512}{27}\pi^{3}\rho\alpha_{s}\langle\bar{\psi}\psi\rangle^{2}=(37.5\pm 1.9)\times 10^{-2}\,{\rm GeV}^{6},
d8,VA\displaystyle d_{8,V-A} =\displaystyle= 12(d8,V+d8,A)(14.5±2.2)×102GeV8\displaystyle\frac{1}{2}\left(d_{8,V}+d_{8,A}\right)\simeq-(14.5\pm 2.2)\times 10^{-2}\,{\rm GeV}^{8} (37)

\bullet~{}Data handling of the spectral function

The spectral function has been measured by ALEPH [10] which we show in Fig.,̇11.

Refer to caption
Figure 11: V–A spectral function measured by ALEPH.

In order to fit the data, we proceed like in the case of the axial-vector channel by subdividing the region into 5 subregions :

[4mπ2,0.585],[0.585,0.85],[0.85,1.45],[1.45,1.975],[1.975,Mτ2],[4m_{\pi}^{2},0.585],~{}[0.585,0.85],~{}[0.85,1.45],~{}[1.45,1.975],~{}[1.975,M_{\tau}^{2}], (38)

in units of GeV2. We use 3rd order polynomials. The results of the fits are given in Fig. 12.

Refer to caption
Refer to caption
Refer to caption
Refer to caption
Refer to caption
Figure 12: Fit of the data using a 2nd and 3rd order polynomial fits.

\bullet~{}The lowest BNP moment 0,VA{\cal R}_{0,V-A}

In the chiral limit their expression is similar to the previous ones for the axial-vector current modulo an overall factor 2 and the change into the condensates contributions dD,VAd_{D,V-A} of dimension DD. We show the s0s_{0} behaviour of the moment in Fig.13.

Refer to caption
Figure 13: s0s_{0} behaviour of the experimental moment 0,VA{\cal R}_{0,V--A}.

For s0=Mτ2s_{0}=M_{\tau}^{2}, we obtain :

0,VA=3.484±0.022{\cal R}_{0,V-A}=3.484\pm 0.022 (39)

to be compared with the ALEPH data [10]:

0,VA|Aleph=3.475±0.011,{\cal R}_{0,V-A}|_{Aleph}=3.475\pm 0.011, (40)

where our error is larger which may due to the fact that we have separately fitted the upper and lower values of the data.

\bullet~{}The d6,VAd_{6,V-A} and d8,VAd_{8,V-A} condensates

We shall use the values of the corresponding condensates from the e+ee^{+}e^{-}\to Hadrons in Ref. [1, 2] and the ones from the axial-vector channel obtained in the previous section. They read:

d6,VA\displaystyle d_{6,V-A} \displaystyle\equiv 12(d6,V+d6,A)=+(3.6±0.5)×102GeV6,\displaystyle\frac{1}{2}\left(d_{6,V}+d_{6,A}\right)=+(3.6\pm 0.5)\times 10^{-2}\,{\rm GeV}^{6},
d8,VA\displaystyle d_{8,V-A} \displaystyle\equiv 12(d8,V+d8,A)=(14.5±2.2)×102GeV8,\displaystyle\frac{1}{2}\left(d_{8,V}+d_{8,A}\right)=-(14.5\pm 2.2)\times 10^{-2}\,{\rm GeV}^{8}, (41)

where the error is the largest relative % error from each channel. We note (as can be found in Ref. [4]) that for 0,VA(s0){\cal R}_{0,V-A}(s_{0}), the contribution of αsG2\langle\alpha_{s}G^{2}\rangle is αs\alpha_{s} suppressed while the one of d6,VAd_{6,V-A} is smaller than in the individual V and A channels. Then, we expect that V–A is a golden channel for extracting αs\alpha_{s}.

\bullet~{}αs\alpha_{s} from 0,VA(s0){\cal R}_{0,V-A}(s_{0})

Refer to caption
Figure 14: αs(Mτ)\alpha_{s}(M_{\tau}) versus an hypothetical τ\tau-mass squared s0s_{0}. The upper curves corresponds to CI perturbative series and the lower ones to FO. The horizontal lines come from a least-square fit of the data in the optimal region s0(2.32.9)s_{0}\simeq(2.3\sim 2.9) GeV2.

Using the value of αsG2\langle\alpha_{s}G^{2}\rangle in Eq. 12 and the previous values of d6,VAd_{6,V-A} and d8,VAd_{8,V-A} in Eq, 41, we extract the value of αs(Mτ)\alpha_{s}(M_{\tau}) as a function of s0s_{0} (see Fig. 14) from 0,VA(s0){\cal R}_{0,V-A}(s_{0}). We notice a stable result in the region s0(2.52.6)s_{0}\simeq(2.5\sim 2.6) GeV2 though not quite convincing. The, we consider as a conservative value the one obtained from a least-square fit of the values inside the region [2,5,Mτ2][2,5,M_{\tau}^{2}]. The optimal result corresponds s0=2.8s_{0}=2.8 GeV2 (see Fig. 14):

αs(Mτ)|VA\displaystyle\alpha_{s}(M_{\tau})|_{V-A} =\displaystyle= 0.3135(51)(65)αs(MZ)|VA=0.1177(10)(3)evol(FO)\displaystyle 0.3135(51)(65)~{}~{}~{}~{}~{}~{}~{}\longrightarrow~{}~{}~{}~{}~{}~{}~{}\alpha_{s}(M_{Z})|_{V-A}=0.1177(10)(3)_{evol}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}{\rm(FO)} (42)
=\displaystyle= 0.3322(69)(43)αs(MZ)|VA=0.1200(9)(3)evol(CI).\displaystyle 0.3322(69)(43)~{}~{}~{}~{}~{}~{}~{}~{}\longrightarrow~{}~{}~{}~{}~{}~{}~{}\alpha_{s}(M_{Z})|_{V-A}=0.1200(9)(3)_{evol}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}{\rm(CI)}.

The 1st error in αs(Mτ)|VA\alpha_{s}(M_{\tau})|_{V-A} comes from the fitting procedure. The 2nd one from an estimate of the αs5\alpha_{s}^{5} contribution from Ref. [1]. At this scale the sum of non-perturbative contributions to the moment normalized to the parton model is:

δNP,VA+(2.7±1.1)×104,\delta_{NP,V-A}\simeq+(2.7\pm 1.1)\times 10^{-4}, (43)

which is completely negligible. One can notice from Fig. 14 that extracting αs(Mτ)|VA\alpha_{s}(M_{\tau})|_{V-A} at the observed MτM_{\tau}-mass tends to overestimate its value :

αs(Mτ)|VA=0.3227(69)(65)FO,0.3423(92)(43)CI.\alpha_{s}(M_{\tau})|_{V-A}=0.3227(69)(65)~{}~{}~{}{\rm FO},~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}0.3423(92)(43)~{}~{}~{}{\rm CI}. (44)

\bullet~{}Comparison with some previous results

d6,VAd_{6,V-A} d8,VA-d_{8,V-A} αs(Mτ)\alpha_{s}(M_{\tau}) FO αs(Mτ)\alpha_{s}(M_{\tau}) CI s0s_{0} [GeV]2 Refs.
3.6±0.53.6\pm 0.5 14.5±2.214.5\pm 2.2 0.3135(83) 0.3322(81) 2.5 Mτ2\to M_{\tau}^{2} This work
3.6±0.53.6\pm 0.5 14.5±2.214.5\pm 2.2 0.3227(95) 0.3423(102) Mτ2M_{\tau}^{2} This work
5.13.1+5.55.1^{+5.5}_{-3.1} 3.2±2.23.2\pm 2.2 0.31700.0050+0.01000.3170^{+0.0100}_{-0.0050} 0.33600.0090+0.01100.3360^{+0.0110}_{-0.0090} Mτ2(D10)M_{\tau}^{2}\,(D\leq 10) Table 7  [18]
2416+2424^{+24}_{-16} 3232+2532^{+25}_{-32} 0.32900.0110+0.01200.3290^{+0.0120}_{-0.0110} 0.34900.0140+0.01600.3490^{+0.0160}_{-0.0140} Mτ2(D12)M_{\tau}^{2}\,(D\leq 12) Table 8  [18]
2.4±0.82.4\pm 0.8 3.2±0.83.2\pm 0.8 0.3410(78)0.3410(78) Mτ2M_{\tau}^{2} [10]
1.5±4.81.5\pm 4.8 3.7±9.03.7\pm 9.0 0.3240(145) 0.3480(212)0.3480(212) Mτ2M_{\tau}^{2} [20]
Table 3: Values of the QCD condensates from 0,e+e{\cal R}_{0,e^{+}e^{-}} and 0,A{\cal R}_{0,A} at Fixed Order (FO) PT series and of αs(Mτ)\alpha_{s}(M_{\tau}) for FO and Contour Improved (CI) PT series. The condensates are in units of 10210^{-2} GeVD.

In Table 3, we compare our results with some other determinations [10, 18, 20]333Some estimates including renormalon within a large β\beta approximation [ resp. duality violation] effects can be e.g. found in Refs. [21] [resp. [22]]. obtained at the scale s0=Mτ2s_{0}=M_{\tau}^{2}.

\diamond~{}There is a quite good agreement for d6,VAd_{6,V-A} but not for d8,VAd_{8,V-A} from different determinations.

\diamond~{}The central values of the condensates given in Table 7 of Ref. [18] using a truncation of the OPE up to D=10D=10 are systematically smaller than the ones in their Table 8 using the OPE up to D=12D=12 though they agree within the errors.

\diamond~{}Extracting αs\alpha_{s} at MτM_{\tau}, there is a good agreement among different determinations where the values are slightly higher than the ones from the optimal region given in the first row  (see Fig. 14).

9 Mean value of αs\alpha_{s} from e+ee^{+}e^{-}\to Hadrons and A, V–A τ\tau-decays

Using the result from e+ee^{+}e^{-}\to Hadrons and from the A and V–A τ\tau-decay channels, we deduce the mean:

αs(Mτ)\displaystyle\alpha_{s}(M_{\tau}) =\displaystyle= 0.3140(44)(FO)αs(MZ)=1178(6)fit(3)evol.,\displaystyle 0.3140(44)\,{\rm(FO)}~{}~{}~{}~{}~{}~{}~{}~{}\longrightarrow~{}~{}~{}~{}~{}~{}~{}\alpha_{s}(M_{Z})=1178(6)_{fit}(3)_{evol.}, (45)
=\displaystyle= 0.3346(35)(CI)αs(MZ)=0.1202(4)fit(3)evol.\displaystyle 0.3346(35)\,{\rm(CI)}~{}~{}~{}~{}~{}~{}~{}~{}\longrightarrow~{}~{}~{}~{}~{}~{}~{}\alpha_{s}(M_{Z})=0.1202(4)_{fit}(3)_{evol.}

10 Summary

\bullet~{}We have improved the determinations of the QCD condensates in the axial-vector channel using a ratio of LSR and higher BNP-like moments. Our results are summarized in Table 2. We observe alternate signs, an almost constant value of their size. The absence of an exponential behaviour in the Euclidian region may not favour a duality violation in the time-like region [19].

\bullet~{}We have used as inputs the value of αsG2\langle\alpha_{s}G^{2}\rangle better determinaed from the heavy quark channels and the ones of the previous condensates d6,Ad_{6,A} and d8,Ad_{8,A} to extract αs(Mτ)\alpha_{s}(M_{\tau}) from the lowest BNP-moment 0,A(s0){\cal R}_{0,A}(s_{0}). Our conservative result in Eq. 30 is obtained from s02.1s_{0}\simeq 2.1 GeV2 to Mτ2M_{\tau}^{2} where we notice from Fig. 7 that extracting αs(Mτ)\alpha_{s}(M_{\tau}) at the observed τ\tau-mass leads to an overestimate of its value.

\bullet~{}We combine the previous values of the d6,Ad_{6,A} and d8,Ad_{8,A} with the ones of the d6,Vd_{6,V} and d8,Vd_{8,V} from e+ee^{+}e^{-}\to Hadrons [1, 2] into the lowest moment 0,VA(s0){\cal R}_{0,V-A}(s_{0}) in the V–A channel. Then, we extract the conservative value of αs(Mτ)\alpha_{s}(M_{\tau}) given in Eq. 44 at s0=[2.5s_{0}=[2.5 GeV2Mτ2{}^{2}\to M_{\tau}^{2}]. Like in the case of the e+ee^{+}e^{-}\to Hadrons and axial-vector channel, we also notice that extracting αs(Mτ)\alpha_{s}(M_{\tau}) at MτM_{\tau} leads to an overestimate.

\bullet~{}We have not considered some eventual effects beyond the SVZ-expansion as:

\diamond~{}According to Ref. [17], the effect a tachyonic gluon mass [23] for parametrizing phenomenologically the UV renormalon effect is equivalent by duality to the contribution of the uncalculated higher order PT terms. We assume that these terms are well approximated by the estimate of the αs5\alpha_{s}^{5} term done in the paper using the observation that the coefficients of the calculated PT terms behave as a geometric sum.

\diamond~{}The observation that the calculated PT terms behave as a geometric sum and that no signal of alternate sign of these PT terms do not (a priori) favour the motivation of a large β\beta-approximation for the estimate of the UV renormalon.

\diamond~{}The non-observation of an exponential behaviour of the non-perturbative condensate effects in the Euclidian region may indicate that Duality Violation in the time-like region [22] may not be sizeable [19].

\diamond~{}Instanton effects act as high-dimension operators and their effects have been shown to be negligible in the vector channel [1]. We expect similar features for the A and V–A channels.

Acknowledgement

I thank Toni Pich for a careful reading of the manuscript and the 2nd referee for some constructive comments.

References

  • [1] S. Narison, Nucl. Phys. A 1046 (2024) 122873, Nucl. Phys. A1050 (2024) 122915 (erratum),
    S. Narison, QCD24 (8-12 july 2024, Montpellier-FR), Nucl. Part. Phys. Proc.. 347 (2024) 105.
  • [2] S. Narison, Nucl. Phys. A 1039 (2023) 122744;
    S. Narison, QCD23 (10-14 july 2023, Montpellier-FR), Nucl. Part. Phys. Proc. 343 (2024).
  • [3] M.A. Shifman, A.I. Vainshtein, V.I. Zakharov, Nucl. Phys. B147 (1979) 385;
    M.A. Shifman, A.I. Vainshtein, V.I. Zakharov, Nucl. Phys. B147 (1979) 448.
  • [4] E. Braaten, S. Narison, A. Pich, Nucl. Phys. B373 (1992) 581.
  • [5] E. Braaten, Phys. Rev. Lett. 60 (1988) 606; E. Braaten, Phys. Rev. D39 (1989) 1458;
    S. Narison, A. Pich, Phys. Lett. B211 (1988) 183.
  • [6] S.G. Gorishny, A.L. Kataev, S.A. Larin, Phys. Lett. B259 (1991) 144; L.R. Surguladze, M.A. Samuel, Phys. Rev. Lett. 66 (1991) 560.
  • [7] P. A. Baikov, K.G. Chetyrkin.J.H. Kühn, Phys.Rev.Lett. 101(2008) 012002.
  • [8] S. Narison, QCD as a theory of hadrons, Cambridge Monogr. Part. Phys. Nucl. Phys. Cosmol. 17. (2004) 1-778 [hep-ph/0205006].
  • [9] R.L. Workman et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2022 (2022) 083C01.
  • [10] The ALEPH collaboration: M. Davier, A. Hoecker, B. Malaescu, C. Yuan, Z. Zhang, Eur. Phys. J. C74 (2014) 2803; http://aleph.web.lal.in2p3.fr/tau/specfun13.html.
  • [11] S. Narison and E. de Rafael, Phys. Lett. B 103, (1981) 57.
  • [12] J.S. Bell and R.A. Bertlmann, Nucl. Phys. B187, (1981) 285.
  • [13] For a recent review, see e.g. S. Narison, The Laplace Transform and its Applications, ed. V. Martinez-Lucaes, Nova Science Pub., New-York - 2024 (arXiv: 2309.00258 [hep-ph]).
  • [14] S. Narison, Int. J. Mod. Phys. A33 (2018) no. 10, 185004; Addendum: Int. J. Mod. Phys. A33 (2018) no.10, 1850045.
  • [15] S. Narison, Phys. Lett. B693 (2010) 559, erratum ibid, B705 (2011) 544; ibid, B706 (2012) 412; ibid, B707 (2012) 259.
  • [16] F. Le Diberder, A. Pich, Phys. Lett. B286 (1992) 147; B289 (1992) 165.
  • [17] S. Narison, V.I. Zakharov, Phys. Lett. B679 (2009) 355.
  • [18] A. Pich, A. Rodríguez-Sánchez, Phys.Rev. D94 (2016) 3, 034027; Mod.Phys.Lett. A31 (2016) 30, 1630032; Nucl. Part. Phys. Proc.287-288 (2017) 81.
  • [19] M. Shifman, Nucl. Phys. Proc. Suppl. B207-208 (2010) 298; ibid arXiv: hep-ph/0009131; B. Blok, M. Shifman, Da-Xin Zhang, Phys. Rev. D 57 (1998) 2691; Phys. Rev. D 59 (1999) 019901 (erratum).
  • [20] The OPAL collaboration: K. Ackerstaff et al., Euro. Phys. J. C7 (1999) 571.
  • [21] C. Ayala, G. Cvetic, D. Teca, J.Phys. G 50 (2023) n0.n^{0}. 4, 045004;
    M. Beneke, D. Boito, M. Jamin, JHEP 01 (2013) 125.
  • [22] D. Boito, M. Golterman, K. Maltman, S. Peris, Phys. Rev. D 95 (2017) non^{o}. 3, 034024
  • [23] K.G. Chetyrkin, S. Narison, V. I. Zakharov, Nucl. Phys. B550(1999) 353.