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thanks: Invited contribution to the book : The Laplace Transform and its Applications edited by Nova Science Publishers, New-York.

Laplace Sum Rules in Quantum ChromoDynamics

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

We shortly review some applications of the (inverse) Laplace (LSR) transform sum rules in Quantum ChromoDynamics (QCD) for extracting the fundamental QCD parameters (coupling constant αs\alpha_{s}, quark and gluon condensates) and the hadron properties (masses and decay constants). Links of LSR to some other forms of QCD spectral sum rules are also discussed. As prototype examples, we discuss in detail the ρ\rho and π\pi meson sum rules.

Keywords : QCD spectral sum rules, QCD coupling αs\alpha_{s} quark masses and condensates,                     Hadron masses and couplings.

pacs:
11.55.Hx, 12.38.Lg, 13.20-Gd, 14.65.Dw, 14.65.Fy, 14.70.D

I Introduction

Different spectral sum rules based on dispersion relations called current algebra sum rules have been used before QCD FURLAN . Among these, there are the Weinberg WEIN and Das-Mathur-Okubo (DMO) DMO sum rules which assume the asymptotic realizations of chiral SU(2)LSU(2)RSU(2)_{L}\otimes SU(2)_{R} and SU(2)VSU(2)_{V} flavour symmetries to derive constraints on the vector and axial-vector mesons masses and couplings. One of the famous predictions from the Weinberg sum rules is the mass relation:

MA12Mρ,M_{A_{1}}\simeq\sqrt{2}M_{\rho}, (1)

which is reproduced within the errors by the data.

Within the advent of QCD, corrections to these sum rules have been studied FNR ; DMOQCD ; GMONARISON in 1979-80. At about the same time, Shifman-Vainshtein and Zakharov (hereafter referred as SVZ) SVZa ; ZAKA 111For reviews, see e.g. the books SNB1 ; SNB2 , the reviews in SNB3 ; RRY ; BERTa ; REV and the recent ones in Refs.SNREV22 ; SNREV21 ; SNbc15 ., have introduced the QCD spectral sum rules which are the improvement of the usual dispersion relation obeyed by e.g. the hadron two-point function:

ΠH(q2)=id4xeiqx0|𝒯𝒪H(x)(𝒪H(0))|0=t>dttq2iϵ1πImΠ(t)+,\Pi_{H}(q^{2})=i\int d^{4}x~{}e^{iqx}\langle 0|{\cal T}{\cal O}_{H}(x)\left({\cal O}_{H}(0)\right)^{\dagger}|0\rangle=\int_{t_{>}}^{\infty}\frac{dt}{t-q^{2}-i\epsilon}\frac{1}{\pi}{\rm Im}\Pi(t)+\cdots, (2)

where \cdots mean subtraction constants polynomial in the momentum q2Q2<0q^{2}\equiv-Q^{2}<0.

𝒪H(x){\cal O}_{H}(x) is a generic notation for a hadronic current:

– Quark bilinear local current ψ¯1Γ12ψ2\bar{\psi}_{1}\Gamma_{12}\psi_{2} for mesons. Γ12\Gamma_{12} is any Dirac matrices which specify the quantum numbers of the corresponding meson state (and its radial excitations),

– Quark trilinear local current ψ1ψ2ψ3\psi_{1}\psi_{2}\psi_{3} for baryons,

– Four-quark (ψ¯1Γ12ψ2)(ψ¯3Γ34ψ4)(\bar{\psi}_{1}\Gamma_{12}\psi_{2})(\bar{\psi}_{3}\Gamma_{34}\psi_{4}) or diquark anti-diquark (ψ¯1Γ12ψ¯2)(ψ3Γ34ψ4)(\bar{\psi}_{1}\Gamma_{12}\bar{\psi}_{2})(\psi_{3}\Gamma_{34}\psi_{4}) local current for molecules or tetraquark states,

– Pentaquark ψ1ψ2ψ3ψ4ψ5\psi_{1}\psi_{2}\psi_{3}\psi_{4}\psi_{5} states,

– Gluon local currents G2,G3G^{2},G^{3}\cdots for gluonia/glueball states,

– Quark-gluon local currents ψ¯1Gψ2,ψ¯1G2ψ2\bar{\psi}_{1}G\psi_{2},\bar{\psi}_{1}G^{2}\psi_{2}\cdots for hybrid states.

In the case of a ψ¯1ψ2\bar{\psi}_{1}\psi_{2} meson bound state built from a quark uu and the anti-quark d¯\bar{d}, the current reads:

𝒪H(x)=u¯Γd(x),{\cal O}_{H}(x)=\bar{u}\Gamma d(x), (3)

where Γ\Gamma denotes any Dirac matrices which specify the quantum number of the associated hadron. Γ=γu,γμγ5,γ5,1\Gamma=\gamma_{u},\gamma_{\mu}\gamma_{5},\gamma_{5},1 for the vector, axial-vector, pseudoscalar and scalar currents which correspond respectively to the ρ,A1,π\rho,A_{1},\pi and scalar quarkonium mesons.

II The SVZ Borel/Laplace sum rules (LSR)

Besides the Shifman-Vainshtein-Zakharov (SVZ) (see Fig. 1) theoretical improvement of the perturbative QCD expression within the Operator Product Expansion (OPE) where quark and gluon condensates of higher and higher dimensions are supposed to approximate the non-perturbative QCD contributions which we shall discuss in the next section, the phenomenological success of QCD (spectral) sum rules or SVZ sum rules also comes from the improvement of the usual dispersion relation which is the bridge between the high-energy QCD expression and the measurable spectral function at low energy. In the example of the light isovector (I=1I=1) vector current:

JHμ(x)=12[:ψ¯uγμψuψ¯dγμψd:].J^{\mu}_{H}(x)=\frac{1}{2}{[}:\bar{\psi}_{u}\gamma^{\mu}\psi_{u}-\bar{\psi}_{d}\gamma^{\mu}\psi_{d}:{]}. (4)

the spectral function is related to the e+ee^{+}e^{-}\to Hadrons total cross-section via the optical theorem:

Reeσ(e+eHadrons)σ(e+eμ+μ)=(32)8πImΠH(t).R_{ee}\equiv\frac{\sigma(e^{+}e^{-}\to\,{\rm Hadrons)}}{\sigma(e^{+}e^{-}\to\mu^{+}\mu^{-})}=\left(\frac{3}{2}\right)8\pi\,{\rm Im}\Pi_{H}(t). (5)
Refer to caption
Figure 1: Left to right : Arkady Vainshtein, SN, Valya Zakharov, Mikhael Shifman at the Munich conference (2006).

II.1 The form of the Laplace sum rules

This improvement has been achieved by working with large number nn of derivatives and large value of the momentum transfer Q2Q^{2} but taking their ratio τn/Q2\tau\equiv n/Q^{2} finite leading to the so-called SVZ Borel/Laplace or Exponential sum rules (LSR) and their ratios,222Non-relativistic version of this sum rule has been discussed by BELLa ; BERTa , while the inclusion of the PT αs\alpha_{s} correction to the QCD expression has shown that it has the property of an inverse Laplace transform in SNR SNR though the name LSR. :

0c(τ,μ)\displaystyle{\cal L}_{0}^{c}(\tau,\mu) \displaystyle\equiv limQ2,nn/Q2τ(Q2)n(n1)!nΠ(Q2)n=t>tc𝑑tetτ1πImΠH(t,μ),\displaystyle\lim_{\begin{tabular}[]{c}$Q^{2},n\to\infty$\\ $n/Q^{2}\equiv\tau$\end{tabular}}\frac{(-Q^{2})^{n}}{(n-1)!}\frac{\partial^{n}\Pi}{(\partial Q^{2})^{n}}=\int_{t>}^{t_{c}}dt~{}e^{-t\tau}\frac{1}{\pi}\mbox{Im}\Pi_{H}(t,\mu)~{}, (8)
10c(τ)\displaystyle{\cal R}^{c}_{10}(\tau) \displaystyle\equiv 1c0c=t>tc𝑑tetτtImΠH(t,μ)t>tc𝑑tetτImΠH(t,μ),\displaystyle\frac{{\cal L}^{c}_{1}}{{\cal L}^{c}_{0}}=\frac{\int_{t>}^{t_{c}}dt~{}e^{-t\tau}t\,\mbox{Im}\Pi_{H}(t,\mu)}{\int_{t>}^{t_{c}}dt~{}e^{-t\tau}\mbox{Im}\Pi_{H}(t,\mu)},~{}~{}~{}~{} (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}).

\diamond~{}Thanks to the exponential weight and for moderate values of τ\tau, the previous sum rule improvements enhance the low energy contribution to the spectral integral which is accessible experimentally.

II.2 The minimal duality ansatz (MDA)

In the often case where the data on the spectral function are not available, one usually parametrizes it via the minimal duality ansatz :

1π ImΠH(t)fH2MH2dδ(tMH2)+``QCD continuum"θ(ttc),\displaystyle\frac{1}{\pi}\mbox{ Im}\Pi_{H}(t)\simeq f^{2}_{H}M_{H}^{2d}\delta(t-M^{2}_{H})+``\mbox{QCD continuum}"\theta(t-t_{c}), (10)

in order to predict the masses and couplings of the lowest ground state and in some case the ones of its radial excitations. dd depends on the dimension of the current, fHf_{H} is the hadron decay constant normalized as fπ=f_{\pi}= 132 MeV. Its accuracy has been tested in various light and heavy quark channels e+eρ,J/ψ,Υ,e^{+}e^{-}\to\rho,J/\psi,\Upsilon,\dots where complete data are available SNB1 ; SNB2 and in the π\pi-pseudoscalar channel where an improved parametrization of the 3π3\pi channel within chiral perturbation theory has been used BIJNENS . Within a such parametrization, the ratio of sum rules is used to extract the mass of the lowest ground state as it is equal to its square.

II.3 Hadron masses from the ratio of moments

Within the MDA parametrization, the ratio of sum rules nc(τ){\cal R}_{n}^{c}(\tau) is used to extract the mass of the lowest ground state as it is equal to its square:

MH210c(τ).M_{H}^{2}\simeq{\cal R}^{c}_{10}(\tau). (11)

However, this analysis cannot be done blindly without studying / checking the moments 0,1{\cal L}_{0,1} which in some cases can violate positivity of the specral integral for some values of the sum rule variables (τ\tau) though their ratio can lead to a positive number identified with the hadron mass squared.

II.4 Hadron mass-splittings from the double ratio of sum rule (DRSR)  DRSR

The hadron HH and HH^{\prime} mass-splitting, like the one due to SU(3)SU(3) breakings, can be derived from the quantity:

rH/H10c(τ)|H10c(τ)|HMH2MH2,r_{H^{\prime}/H}\equiv\frac{{\cal R}_{10}^{c}(\tau^{\prime})|_{H^{\prime}}}{{\cal R}_{10}^{c}(\tau)|_{H}}\simeq\frac{M_{H^{\prime}}^{2}}{M_{H}^{2}}, (12)

provided that the optimal value: τ0τ0\tau^{\prime}_{0}\simeq\tau_{0}. A similar quantity can be used for the heavy quark moments.

III Link of LSR to some other sum rules

III.1 Local duality Finite Energy Sum Rules (FESR)

It has the form:

nc(tc,μ)=t>tc𝑑ttn1πImΠH(t,μ),{\cal F}^{c}_{n}(t_{c},\mu)=\int_{t>}^{t_{c}}dt\,t^{n}\frac{1}{\pi}\mbox{Im}~{}\Pi_{H}(t,\mu)~{}, (13)

where n0n\geq 0 is the degree of the sum rule. This sum rule has been used before QCD in Refs. LOGUNOV ; SAKURAI and within QCD in Refs. KRASNIKOV ; KATAEV ; LARIN .

This sum rule can be derived from LSR by using a small τ\tau-expansion and by matching for a given τ\tau its QCD and experimental side.

FESR can be used to fix the value of the QCD continuum threshold tct_{c} from its dual constraint with the mass and decay constant of the ground state FESR1 ; FESR2 . Contrary to LSR, FESR emphasizes the role of higher masses radial excitations to the integral. Therefore, it requires a good control of the high-energy part of the spectral function.

III.2 Gaussian Sum Rules

It has the form FESR1 ; FESR2 :

Gnc(s,σ,μ)=14πσt>tc𝑑te(t+s)24π1πImΠH(t,μ),{G}^{c}_{n}(s,\sigma,\mu)=\frac{1}{\sqrt{4\pi\sigma}}\int_{t>}^{t_{c}}dt~{}e^{-\frac{(t+s)^{2}}{4\pi}}\frac{1}{\pi}\mbox{Im}\Pi_{H}(t,\mu)~{}, (14)

for a Gaussian centered at ss with a finite width resolution 4πσ\sqrt{4\pi\sigma}. It has been also shown in Ref. FESR1 ; FESR2 that the LSR can be derived from the Gaussian sum rule using the ζ\zeta-prescription.

IV The SVZ - Operator Product Expansion (OPE)

\diamond~{}According to SVZ, the Right Hand Side (RHS) of the two-point function can be evaluated in QCD within the Operator Product Expansion (OPE) provided that Λ2Q2q2,mQ2\Lambda^{2}\ll Q^{2}\equiv-q^{2},m_{Q}^{2} where Λ(342±8)\Lambda\simeq(342\pm 8) MeV is the QCD scale for 3 flavours and mQm_{Q} is the heavy quark mass. In this way, it reads :

4π2ΠH(q2,mQ2,μ)=D=0,1,..C2D(q2,mQ2,μ)Q2DO2D(μ),4\pi^{2}\Pi_{H}(q^{2},m_{Q}^{2},\mu)=\sum_{D=0,1,..}\frac{C_{2D}(q^{2},m_{Q}^{2},\mu)}{Q^{2D}}\langle O_{2D}(\mu)\rangle~{}, (15)

where, in addition to the usual perturbative QCD contribution (unit operator), one has added the ones due to non-perturbative gauge invariant quark and gluon condensates O2D(μ)\langle O_{2D}(\mu)\rangle having a dimension 2D2D which have been assumed to parametrize approximately the not yet under good control QCD confinement. C2DC_{2D} are separated calculable Wilson coefficients in Perturbative (PT) QCD:

IV.1 The usual perturbative (PT) contribution

It corresponds to D=0D=0 while the quadratic quark mass corrections enter via D=1D=1.

IV.2 The quark and gluon condensates

They contribute through the OPE. Up to 2D=62D=6, they are successively the :

2D=42D=4 quark and gluon mψ¯ψm\langle\bar{\psi}\psi\rangle and αsG2\langle\alpha_{s}G^{2}\rangle,

2D=52D=5 mixed quark-gluon: ψ¯σμνλa2Gμνaψ\langle\bar{\psi}\sigma^{\mu\nu}\frac{\lambda_{a}}{2}G_{\mu\nu}^{a}\psi\rangle

2D=62D=6 four-quark and three-gluon: ψ¯Γ1ψψ¯Γ2ψ\langle\bar{\psi}\Gamma_{1}\psi\bar{\psi}\Gamma_{2}\psi\rangle and g3fabcGμρaGνb,ρGρc,ν\langle g^{3}f_{abc}G^{a}_{\mu\rho}G^{b,\rho}_{\nu}G^{c,\nu}_{\rho}\rangle.

– and so on.

IV.3 The 2D=42D=4 condensates

The quark condensate mψ¯ψm\langle\bar{\psi}\psi\rangle and the part of the trace of the energy-momentum transfer : θμμ|gmγψ¯ψ+(1/4)βGμνaGaμν\theta^{\mu}_{\mu}|_{g}\equiv m\gamma\langle\bar{\psi}\psi\rangle+(1/4)\beta\langle G^{a}_{\mu\nu}G_{a}^{\mu\nu}\rangle are known to be subtraction μ\mu-independent where γ,β\gamma,\,\beta are the quark mass anomalous dimension and Callan-Symanzik β\beta-function.

– The ψ¯ψ\langle\bar{\psi}\psi\rangle condensate can be deduced from the well-known Gell-Mann, Oakes, Renner relation GMOR :

(mu+md)ψ¯uψu+ψ¯dψd=mπ2fπ2,(m_{u}+m_{d})\langle\bar{\psi}_{u}\psi_{u}+\bar{\psi}_{d}\psi_{d}\rangle=-m_{\pi}^{2}f_{\pi}^{2}, (16)

once the running light quark mass is known (mπ,fπ=132m_{\pi},f_{\pi}=132 MeV are the pion mass and decay constant) or directly from light baryon sum rules DOSCHSN . With the value of the running u,du,d quark masses given in Table 2 in Ref. SNREV22 , one can deduce the value of ψ¯ψ\langle\bar{\psi}\psi\rangle in this Table 2.

– The original value of the 2D=42D=4 gluon condensate αsG2=0.04\langle\alpha_{s}G^{2}\rangle=0.04 GeV4 of SVZ SVZa ; RRY has been claimed BELLa ; BERTa from charmonium sum rules and Finite Energy Sum Rule (FESR) for e+eI=1e^{+}e^{-}\to I=1  Hadrons FESR1 ; FESR2 to be underestimated. Recent analysis from e+ee^{+}e^{-}\to Hadrons, τ\tau-decay and charmonium confirm these claims with the present updated average (see the different determinations in Table 1 of SNparam ) :

αsG2=(6.49±0.35)×102GeV4.\langle\alpha_{s}G^{2}\rangle=(6.49\pm 0.35)\times 10^{-2}~{}{\rm GeV}^{4}. (17)

IV.4 The 2D=52D=5 quark-gluon mixed condensate

It is usually parametrized as gψ¯Gψ=M02ψ¯ψg\langle\bar{\psi}G\psi\rangle=M_{0}^{2}\langle\bar{\psi}\psi\rangle. It mixes under renormalization and runs as (αs)1/(6β1)(\alpha_{s})^{1/(6\beta_{1})} in the chiral limit m=0m=0SNTARRACH . The scale :

M02=0.8(2)GeV2,M_{0}^{2}=0.8(2)~{}{\rm GeV}^{2}, (18)

has been phenomenologically estimated from light baryons IOFFE ; DOSCH ; PIVOm and heavy-light mesons SNhl sum rules.

IV.5 The 2D=62D=6 four-quark condensates

The renormalization of dimension-six condensates has been studied in SNTARRACH where it has been shown that these condensates mix under renormalization and then cannot be compatible with the vacuum saturation assumption used by SVZ. Its phenomenological estimate from τ\tau-like decays SNTAU , e+ee^{+}e^{-}\to Hadrons data LNT , τ\tau-decay SOLA , FESR  FESR1 ; FESR2 and baryon DOSCH sum rules, leads to the average :

ραsψ¯ψ25.8(9)104GeV6,\rho\alpha_{s}\langle\bar{\psi}\psi\rangle^{2}\simeq 5.8(9)10^{-4}\,{\rm GeV}^{6}, (19)

indicating a huge violation of the vacuum saturation or factorization:

αsψ¯ψ2|fac=1.0(9)×104GeV4,\alpha_{s}\langle\bar{\psi}\psi\rangle^{2}|_{fac}=1.0(9)\times 10^{-4}\,{\rm GeV}^{4}, (20)

by a factor ρ\rho about 5.8.

\diamond~{}Fixing the ratio αsG2/ραsψ¯ψ2=106(12)\langle\alpha_{s}G^{2}\rangle/\rho\alpha_{s}\langle\bar{\psi}\psi\rangle^{2}=106(12) GeV-2 as quoted in Ref. SND21 which reduces the analysis to a one-parameter fit, one deduces from LSR SNTAU :

αsG2=(6.1±0.7)102GeV6,\langle\alpha_{s}G^{2}\rangle=(6.1\pm 0.7)10^{-2}~{}{\rm GeV}^{6}, (21)

which shows the self-consistency of the previous numbers. Some other consistency tests can be found in SNTAU .

IV.6 The 2D=62D=6 g3fabcGaGbGcg^{3}f_{abc}\langle G^{a}G^{b}G^{c}\rangle condensate

It does not mix under renormalization and behaves as (αs)23/(6β1)(\alpha_{s})^{23/(6\,\beta_{1})}SNTARRACH , 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 number of quark flavours. The first improvement of the estimate of the g3fabcGaGbGcg^{3}f_{abc}\langle G^{a}G^{b}G^{c}\rangle condensate was the recent direct determination of the ratio of the dimension-six gluon condensate g3fabcG3\langle g^{3}f_{abc}G^{3}\rangle over the dimension-four one αsG2\langle\alpha_{s}G^{2}\rangle using heavy quark sum rules with the value SNcb1 :

ρGg3fabcG3/αsG2=(8.2±1.0)GeV2,\rho_{G}\equiv\langle g^{3}f_{abc}G^{3}\rangle/\langle\alpha_{s}G^{2}\rangle=(8.2\pm 1.0)~{}{\rm GeV}^{2}, (22)

which differs significantly from the instanton liquid model estimate NIKOL2 ; SHURYAK ; IOFFE2 . This result may question the validity of the instanton result. Earlier lattice results in pureYang-Mills found: ρG1.2\rho_{G}\approx 1.2 GeV2GIACO such that it is important to have new lattice results for this quantity. Note however, that the value given in Eq. 22 might also be an effective value of all unknown high-dimension condensates not taken into account in the analysis of  SNcb1 when requiring the fit of the data by the truncated OPE. We have seen in some examples SNREV21 ; SNREV22 that the effect of g3fabcG3\langle g^{3}f_{abc}G^{3}\rangle is a small correction at the stability region where the optimal results are extracted.

IV.7 Higher dimension condensates

Usually, the truncation of the OPE up to 2D=62D=6 provides enough information for extracting the masses and couplings of the ground state hadrons with a good accuracy. In many papers, some classes of higher dimension terms up to 2D=12 ! are added in the OPE. However, it is not clear if such term gives the dominant contributions compared to the omitted ones having the same dimension. The size of these high-dimension condensates is not also under a good control due to the eventual violation of the vacuum saturation used for their estimate.

IV.8 Beyond the SVZ-OPE

Different contributions beyond the standard SVZ-OPE (tachyonic gluon mass, small size instantons, duality violation) can be consulted in the recent reviews SNREV21 ; SNREV22 .

V The different terminologies of the SVZ sum rules

V.1 The origin of the name: Borel sum rule from the OPE

Applying the operator in Eq. 9 to the QCD expression in Eq. 15, the OPE of the 1st moment becomes:

0(τ,mq2,μ)=D=0,1,..C2D(τ,mq2,μ)τD(D)!O2D(μ),{\cal L}_{0}(\tau,m_{q}^{2},\mu)=\sum_{D=0,1,..}C_{2D}(\tau,m_{q}^{2},\mu)\frac{\tau^{D}}{(D)!}\langle O_{2D}(\mu)\rangle~{}, (23)

where the appearance of the (D)!(D)! factor in the OPE indicates the property of the Borel transform for the moment sum rule thus the name Borel sum rule. For this purpose, we recall that if we consider a function f(x)f(x), its Borel transform is:

f~(λ)=12πicic+ieλ/xf(x)xd(1/x),\tilde{f}(\lambda)=\frac{1}{2\pi\,i}\int_{c-i\infty}^{c+i\infty}e^{\lambda/x}f(x)\,x\,d(1/x), (24)

where the integration contour runs to the right of all the singularities of the function f(x)f(x). Then, the inverse Borel transform reads:

xf(x)=0f(x)eλ/x𝑑λ.xf(x)=\int_{0}^{\infty}f(x)\,e^{-\lambda/x}d\lambda. (25)

Therefore, if

f(x)=a0+a1x+a2x2++akxk+,f(x)=a_{0}+a_{1}x+a_{2}x^{2}+\cdots+a_{k}x^{k}+\cdots, (26)

then :

f~(λ)=a00!+a11!λ+a22!λ2++akk!λk+.\tilde{f}(\lambda)=\frac{a_{0}}{0!}+\frac{a_{1}}{1!}\lambda+\frac{a_{2}}{2!}\lambda^{2}+\cdots+\frac{a_{k}}{k!}\lambda^{k}+\cdots. (27)

The great advantage of this property is the improved convergence of the OPE for the Borel transform f~(λ)\tilde{f}(\lambda) compared to the one of the original two-point function f(x)f(x).

V.2 The origin of the name: Laplace sum rule (LSR) including αsn\alpha_{s}^{n} corrections

Refer to caption
Refer to caption
Figure 2: Left to right : SN, Eduardo de Rafael, Christine Kattner (soprano singer) @ QCD 2000 - Montpellier.

In Ref. SNR , S. Narison and E. de Rafael (referred hereafter as SNR)  333The main idea comes from Prof. E. de Rafael as I was a student in that time. have remarked that working with the renormalization group resummed QCD expression including radiative corrections, the sum rule has instead a Laplace transform property from which all QCD expressions can be derived.

The Laplace transform sum rule (LSR) can be derived from the dispersion relation (Hilbert transform) in Eq. 2 from the useful formulae (see e.g. the Appendix of  SNB1 ; SNB2 ) :

[1(Q2+m2)α]\displaystyle{\cal L}\Bigg{[}\frac{1}{(Q^{2}+m^{2})^{\alpha}}\Bigg{]} =\displaystyle= ταΓ(α)em2τ,\displaystyle\frac{\tau^{\alpha}}{\Gamma(\alpha)}e^{-m^{2}\tau},
[1(Q2)αlnQ2ν2]\displaystyle{\cal L}\Bigg{[}\frac{1}{(Q^{2})^{\alpha}}{\rm ln}\frac{Q^{2}}{\nu^{2}}\Bigg{]} =\displaystyle= ταΓ(α)[lnτν2+ψ(α)],\displaystyle\frac{\tau^{\alpha}}{\Gamma(\alpha)}\Big{[}-{\rm ln}\,\tau\nu^{2}+\psi(\alpha)\Big{]},
[1(Q2)αln2Q2ν2]\displaystyle{\cal L}\Bigg{[}\frac{1}{(Q^{2})^{\alpha}}{\rm ln}^{2}\frac{Q^{2}}{\nu^{2}}\Bigg{]} =\displaystyle= ταΓ(α)[ln2τν22ψ(α)lnτν2+ψ2(α)ψ(α)],\displaystyle\frac{\tau^{\alpha}}{\Gamma(\alpha)}\Big{[}{\rm ln}^{2}\,\tau\nu^{2}-2\psi(\alpha){\rm ln}\,\tau\nu^{2}+\psi^{2}(\alpha)-\psi^{\prime}(\alpha)\Big{]},
[1(x)α1(lnx)β]\displaystyle{\cal L}\Bigg{[}\frac{1}{(x)^{\alpha}}\frac{1}{({\rm ln}\,x)^{\beta}}\Bigg{]} =\displaystyle= yμ(y,β1,α1),\displaystyle y\,\mu(y,\beta-1,\alpha-1),
y0\displaystyle\stackrel{{\scriptstyle y\to 0}}{{\simeq}} yα+1Γ(α)1(lny)β[1+βψ(α)1lny+𝒪(1ln2y)]foryτΛ2\displaystyle\frac{y^{\alpha+1}}{\Gamma(\alpha)}\frac{1}{(-{\rm ln\,}y)^{\beta}}\Bigg{[}1+\beta\,\psi(\alpha)\frac{1}{{\rm ln\,}y}+{\cal O}\left(\frac{1}{{\rm ln^{2}}y}\right)\Bigg{]}~{}~{}{\rm for}~{}~{}~{}y\equiv\tau\Lambda^{2}
[lnlnxxα(lnx)β]\displaystyle{\cal L}\Bigg{[}\frac{{\rm ln\,ln}\,x}{x^{\alpha}({\rm ln}\,x)^{\beta}}\Bigg{]} y0\displaystyle\stackrel{{\scriptstyle y\to 0}}{{\simeq}} yα+1Γ(α)lnlny(lny)β[1+βψ(α)1lny+𝒪(1ln2y)]\displaystyle\frac{y^{\alpha+1}}{\Gamma(\alpha)}\frac{{\rm ln\,ln}\,y}{({\rm-ln}\,y)^{\beta}}\Bigg{[}1+\beta\,\psi(\alpha)\frac{1}{{\rm ln\,}y}+{\cal O}\left(\frac{1}{{\rm ln^{2}}y}\right)\Bigg{]} (28)

where {\cal L} is the (inverse) Laplace transform operator and :

ψ(z)\displaystyle\psi(z) \displaystyle\equiv ddzlnΓ(z),\displaystyle\frac{d}{dz}{\rm ln}\Gamma(z)~{},
μ(y,β,α)\displaystyle\mu(y,\beta,\alpha) \displaystyle\equiv 0𝑑xyα+xxβΓ(β+1)Γ(α+x+1),\displaystyle\int_{0}^{\infty}dx\,\frac{y^{\alpha+x}x^{\beta}}{\Gamma(\beta+1)\,\Gamma(\alpha+x+1)},
μ(y,β,α)\displaystyle\mu(y,-\beta,\alpha) =\displaystyle= (1)β1dβ1(dx)β1[yαxΓ(α+x+1)]x=0.\displaystyle(-1)^{\beta-1}\frac{d^{\beta-1}}{(dx)^{\beta-1}}\Bigg{[}\frac{y^{\alpha-x}}{\Gamma(\alpha+x+1)}\Bigg{]}_{x=0}. (29)

with the useful properties:

ψ(1)\displaystyle\psi(1) =\displaystyle= γe=0.5772(Eulerconstant),\displaystyle-\gamma_{e}=-0.5772...~{}~{}~{}~{}({\rm Euler~{}constant}),
μ(y,1,α)\displaystyle\mu(y,-1,\alpha) =\displaystyle= yαΓ(α+1),\displaystyle\frac{y^{\alpha}}{\Gamma(\alpha+1)},
μ(y,2,α)\displaystyle\mu(y,-2,\alpha) =\displaystyle= yαΓ(α+1)[lny+ψ(α+1)],\displaystyle\frac{y^{\alpha}}{\Gamma(\alpha+1)}{[}-{\rm ln}\,y+\psi(\alpha+1){]},
μ(y,3,α)\displaystyle\mu(y,-3,\alpha) =\displaystyle= yαΓ(α+1)[ln2y2ψ(α+1)lny+ψ2(α+1)ψ(α+1)].\displaystyle\frac{y^{\alpha}}{\Gamma(\alpha+1)}{[}-{\rm ln}^{2}\,y-2\psi(\alpha+1){\rm ln}\,y+\psi^{2}(\alpha+1)-\psi^{\prime}(\alpha+1){]}. (30)

In addition to previous formulae, the expression of the integral:

0tc𝑑ttnetτ=(n1)!τn(1ρn)withρn=etcτ(1+tcτ+(tcτ)nn!)\int_{0}^{t_{c}}dt\,t^{n}\,e^{-t\tau}=(n-1)!\,\tau^{-n}(1-\rho^{n})~{}~{}~{}~{}{\rm with~{}~{}~{}~{}}\rho^{n}=e^{-t_{c}\tau}\left(1+t_{c}\tau+\cdots\frac{(t_{c}\tau)^{n}}{n!}\right) (31)

is useful for the treatment of the QCD continuum contribution to the LSR from the QCD spectral function as parametrized in Eq. 10.

VI The QCD expressions of the prototype ρ\rho meson and pion LSR

We illustrate the derivation of the Laplace sum rule in the case of the vector and pseudoscalar (divergence of the axial-vector) currents:

Vμ(x)\displaystyle V_{\mu}(x) =\displaystyle= u¯(γμ)d(x),\displaystyle\bar{u}(\gamma_{\mu})d(x),
μAμ(x)\displaystyle\partial_{\mu}A^{\mu}(x) =\displaystyle= (mu+md)u¯(iγ5)d(x)\displaystyle(m_{u}+m_{d})\bar{u}(i\gamma_{5})d(x) (32)

and the corresponding two-point functions Π(q2)\Pi(q^{2}) and ψ5(q2)\psi_{5}(q^{2}) used in Ref. SNR for demonstrating (for the first time) the Laplace transform properties of the SVZ sum rule 444In these pedagogical examples, we shall limit to the perturbative QCD expression to order αs2\alpha_{s}^{2}. Analysis including higher order terms can be found in SNe23 ; SNLIGHT . :

(gμνq2qμqν)Π(q2)\displaystyle-(g_{\mu\nu}q^{2}-q_{\mu}q_{\nu})\Pi(q^{2}) =\displaystyle= id4xeiqx0|𝒯Vμ(x)Vν(0)|0,\displaystyle i\int d^{4}x\,e^{iqx}\langle 0|{\cal T}\,V_{\mu}(x)V^{\dagger}_{\nu}(0)|0\rangle,
ψ5(q2)\displaystyle\psi_{5}(q^{2}) =\displaystyle= id4xeiqx0|𝒯μAμ(x)(μAμ)(0)|0\displaystyle i\int d^{4}x\,e^{iqx}\langle 0|{\cal T}\,\partial^{\mu}A_{\mu}(x)\left(\partial^{\mu}A_{\mu}\right)^{\dagger}(0)|0\rangle (33)

VI.1 The ρ\rho meson channel

As the corresponding two-point correlator is once substracted, it is convenient to work with its first derivative:

χ(1)(Q2)(ddQ2)Π(Q2)=C0Q2+C2O2(Q2)2+2C4O4(Q2)3+3C6O6(Q2)4+\chi^{(1)}(Q^{2})\equiv\left(-\frac{d}{dQ^{2}}\right)\Pi(Q^{2})=\frac{C_{0}}{Q^{2}}+\frac{C_{2}\langle O_{2}\rangle}{(Q^{2})^{2}}+2\frac{C_{4}\langle O_{4}\rangle}{(Q^{2})^{3}}+3\frac{C_{6}\langle O_{6}\rangle}{(Q^{2})^{4}}+\cdots (34)

with (see e.g. SNB1 ; SNB2 ):

C0\displaystyle C_{0} =\displaystyle= 14π2[1+as+a¯s2R2+],\displaystyle\frac{1}{4\pi^{2}}\big{[}1+a_{s}+\bar{a}_{s}^{2}R_{2}+\cdots\big{]},
C2O2\displaystyle C_{2}\langle O_{2}\rangle =\displaystyle= 3(mu2+md2),\displaystyle 3(m_{u}^{2}+m_{d}^{2}),
C4O4\displaystyle C_{4}\langle O_{4}\rangle =\displaystyle= 4π2[muψ¯uψu+mdψ¯dψd]+π3αsG2+𝒪(mi4ln(mi2/q2),\displaystyle 4\pi^{2}\big{[}m_{u}\langle\bar{\psi}_{u}\psi_{u}\rangle+m_{d}\langle\bar{\psi}_{d}\psi_{d}\rangle\big{]}+\frac{\pi}{3}\langle\alpha_{s}G^{2}\rangle+{\cal O}(m^{4}_{i}\,{\rm ln}(m_{i}^{2}/q^{2}),
C6O6\displaystyle C_{6}\langle O_{6}\rangle =\displaystyle= 89681π3ραsψ¯qψq2,\displaystyle\frac{896}{81}\pi^{3}\rho\,\alpha_{s}\langle\bar{\psi}_{q}\psi_{q}\rangle^{2}, (35)

where R2=1.9860.115nfR_{2}=1.986-0.115\,n_{f} for nfn_{f} flavours. χ(1)(Q2)\chi^{(1)}(Q^{2}) is superconvergent and obeys the homogeneous Renormalization Group Equation (RGE):

(Q2Q2+β(αs)αsαsi[1+γ(αs)]xixi)χ(1)(Q2),\left(-Q^{2}\frac{\partial}{\partial Q^{2}}+\beta(\alpha_{s})\alpha_{s}\frac{\partial}{\partial\alpha_{s}}-\sum_{i}[1+\gamma(\alpha_{s})]x_{i}\frac{\partial}{\partial x_{i}}\right)\chi^{(1)}(Q^{2}), (36)

with the running parameters to order αs\alpha_{s} are (see e.g.FNR ; RUNDEC ; SNB1 ; SNB2 ):

as\displaystyle a_{s} \displaystyle\equiv α¯s(Q2)π=as(0)[1as(0)β2β1lnln(Q2/Λ2)]\displaystyle\frac{\bar{\alpha}_{s}(Q^{2})}{\pi}=a_{s}^{(0)}\Big{[}1-a_{s}^{(0)}\frac{\beta_{2}}{\beta_{1}}\,{\rm ln\,ln}(Q^{2}/\Lambda^{2})\Big{]}
m¯q(Q2)\displaystyle\bar{m}_{q}(Q^{2}) \displaystyle\equiv xiQ2m^q(β1as)γ1/β1)[1+β2β1(γ1β1γ2β2)as+2.707as2],\displaystyle x_{i}\sqrt{Q^{2}}\equiv\frac{\hat{m}_{q}}{(-\beta_{1}a_{s})^{\gamma_{1}/\beta_{1})}}\Big{[}1+\frac{\beta_{2}}{\beta_{1}}\left(\frac{\gamma_{1}}{\beta_{1}}-\frac{\gamma_{2}}{\beta_{2}}\right)a_{s}+2.707a_{s}^{2}\Big{]}, (37)

where:

as(0)=2β1ln(Q2/Λ2):Λ=(342±8)MeVfor3flavours.a_{s}^{(0)}=\frac{2}{-\beta_{1}\,{\rm ln}(Q^{2}/\Lambda^{2})}~{}~{}:~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}\Lambda=(342\pm 8)~{}{\rm MeV}~{}{\rm for~{}3~{}flavours}. (38)

β1,2\beta_{1,2} and γ1,2\gamma_{1,2} are respectively the 1st and 2nd coefficients of the β\beta function and mass anomalous dimension. For nfn_{f} quark flavours, they read:

β1=112+13nf,β2=514+1912nf,γ1=2,γ2=10112518nf.\beta_{1}=-\frac{11}{2}+\frac{1}{3}n_{f},~{}~{}~{}~{}~{}~{}\beta_{2}=-\frac{51}{4}+\frac{19}{12}n_{f},~{}~{}~{}~{}~{}~{}\gamma_{1}=2,~{}~{}~{}~{}~{}~{}\gamma_{2}=\frac{101}{12}-\frac{5}{18}n_{f}. (39)

Using the previous formulae of the Laplace transform into the QCD expressions of the corresponding two-point correlator, one can deduce the Laplace transform SNR ; SNB1 ; SNB2 :

0V\displaystyle{\cal L}^{V}_{0} \displaystyle\equiv 0etτ1πImΠV(t)=τ1(14π2){1+as(τ)+as2(τ)[R212β1γE+(β2/β1)lnln(τΛ2)]\displaystyle\int_{0}^{\infty}e^{-t\tau}\frac{1}{\pi}{\rm Im}\Pi_{V}(t)=\tau^{{}_{1}}\left(\frac{1}{4\pi^{2}}\right)\Bigg{\{}1+a_{s}(\tau)+a_{s}^{2}(\tau)\big{[}R_{2}-\frac{1}{2}\beta_{1}\gamma_{E}+(\beta_{2}/\beta_{1}){\rm ln\,ln}(\tau\Lambda^{2})\big{]} (40)
+4π2τ2[muψ¯uψu+mdψ¯dψd]+π3τ2αsG2+τ3(12)89681π3ραsψ¯qψq2},\displaystyle+4\pi^{2}\tau^{2}\big{[}m_{u}\langle\bar{\psi}_{u}\psi_{u}\rangle+m_{d}\langle\bar{\psi}_{d}\psi_{d}\rangle\big{]}+\frac{\pi}{3}\tau^{2}\langle\alpha_{s}G^{2}\rangle+\tau^{3}\left(\frac{1}{2}\right)\frac{896}{81}\pi^{3}\rho\,\alpha_{s}\langle\bar{\psi}_{q}\psi_{q}\rangle^{2}\Bigg{\}},

where the factor ρ=1\rho=1 if one uses the vacuum saturation assumption for the four-quark condensate.

VI.2 The pion channel

The corresponding two-point function behaves as (q2)2ln(q2/ν2)(q^{2})^{2}\,{\rm ln}(-q^{2}/\nu^{2})and is then twice substracted. Thererefore, its 2nd derivative ψ5(2)(q2)\psi_{5}^{(2)}(q^{2}) is superficially convergent and obeys the RGE in Eq. 36. Taking the Laplace transform of ψ5(2)\psi_{5}^{(2)}, one obtains: SNR ; SNB1 ; SNB2 555For an updated expression including higher order contributions, see e.g. SNLIGHT .:

0π\displaystyle{\cal L}_{0}^{\pi} =\displaystyle= 38π2(m^u+m^d)2(lnτΛ)2γ1/β1τ2{1[m¯u2+m¯d2+(m¯um¯d)2]τ\displaystyle\frac{3}{8\pi^{2}}\frac{(\hat{m}_{u}+\hat{m}_{d})^{2}}{\left(-\rm{ln}\,\sqrt{\tau}\Lambda\right)^{2\gamma_{1}/-\beta_{1}}}\tau^{-2}\Bigg{\{}1-\big{[}\bar{m}_{u}^{2}+\bar{m}_{d}^{2}+(\bar{m}_{u}-\bar{m}_{d})^{2}\big{]}\tau (41)
+as[113+2γE+2β1(γ2γ1β2β1)+2γ1β2β12ln(lnτΛ2)]]\displaystyle+\,a_{s}\Bigg{[}\frac{11}{3}+2\gamma_{E}+\frac{2}{-\beta_{1}}\left(\gamma_{2}-\gamma_{1}\frac{\beta_{2}}{\beta_{1}}\right)+2\gamma_{1}\frac{\beta_{2}}{\beta_{1}^{2}}\,{\rm ln\,\left(-ln\,\tau\Lambda^{2}\right)}\big{]}\Bigg{]}
83π2τ2[(mdmu2)ψ¯uψu+(mumd2)ψ¯dψd]+π3τ2αsG2\displaystyle-\,\frac{8}{3}\pi^{2}\tau^{2}\Bigg{[}\left(m_{d}-\frac{m_{u}}{2}\right)\langle\bar{\psi}_{u}\psi_{u}\rangle+\left(m_{u}-\frac{m_{d}}{2}\right)\langle\bar{\psi}_{d}\psi_{d}\rangle\Bigg{]}+\frac{\pi}{3}\tau^{2}\langle\alpha_{s}G^{2}\rangle
4π23τ3[mdψ¯uGψu+3227πραs(ψ¯uψu2+ψ¯dψd29ψ¯uψuψ¯dψd)]}.\displaystyle-\frac{4\pi^{2}}{3}\tau^{3}\Big{[}m_{d}\langle\bar{\psi}_{u}G\psi_{u}\rangle+\frac{32}{27}\pi\rho\alpha_{s}\left(\langle\bar{\psi}_{u}\psi_{u}\rangle^{2}+\langle\bar{\psi}_{d}\psi_{d}\rangle^{2}-9\langle\bar{\psi}_{u}\psi_{u}\rangle\langle\bar{\psi}_{d}\psi_{d}\rangle\right)\Big{]}~{}\Bigg{\}}.

VII Optimization procedure for the LSR

VII.1 The SVZ sum rule window

The second important step in the sum rule analysis is the extraction of the optimal result from the sum rule as, in principle, the Laplace sum rule (LSR) variable τ\tau, the degree of moments nn and the QCD continuum threshold tct_{c} are free external variables. In their original work, SVZ have adjusted the values of M21/τM^{2}\equiv 1/\tau and tct_{c} using some guessed %\% contributions, for finding the sum rule window where the QCD continuum contribution is less than some input number while the ground state one is bigger than some input number and where, in this sum rule window, the OPE is expected to converge. The arbitrariness values of these numbers have created some doubts for non-experts on the results from the sum rules, in addition to the ones on the eventual non-correctness of the non-trivial QCD-OPE expressions. Unfortunately, many sum rules practitioners continue to use this inaccurate SVZ criterion.

VII.2 τ\tau-stability from quantum mechanics and J/ΨJ/\Psi

Refer to caption
Figure 3: Behaviour of the ground state mass versus the time variable τ\tau for different truncation of the series from Ref. BELLa ; BERTa . The horizontal line is the exact solution. ω\omega is the harmonic oscillator frequency.
Refer to caption
Figure 4: Schematic behaviour of the J/ψJ/\psi mass versus the sum rule variable τN\tau_{N} from Ref. BELLa ; BERTa . The horizontal line is the experimental mass.

VII.3 Examples of τ\tau-stability from the Υ\Upsilon and BB mesons

Refer to caption
Figure 5: Behaviour of the ratio of moments 10b(m¯b2)\sqrt{{\cal R}^{b}_{10}}(\overline{m}_{b}^{2}) in GeV versus τ\tau in GeV-2 and for m¯b(m¯b)=4212\overline{m}_{b}(\overline{m}_{b})=4212 MeV from SNH12 . The black continuous (resp. short dashed) curves are the experimental contribution including (resp. without) the QCD continuum (it is about the MΥM_{\Upsilon}). The green (thick continuous) is the PT contribution including the D=4D=4 condensate to LO. The long dashed (red) curve is the contribution including the αs\alpha_{s} correction to the D=4D=4 contribution. The short dashed (blue) curve is the QCD expression including the D=6D=6 condensate and the dot-dashed (red-wine) is the QCD expression including the D=8D=8 contribution.
Refer to caption
Figure 6: Behaviour of fBf_{B} from Ref. SNFB12 versus the sum rule variable τ\tau for different values of the QCD continuum threshold tct_{c} and for a given μ=\mu= 3 GeV and m¯b(m¯b)=4177\overline{m}_{b}(\overline{m}_{b})=4177 MeV.

Hopefully, in the examples of harmonic oscillator in quantum mechanics and of the non-relativistic charmonium sum rules, Refs. BELLa ; BERTa have shown that the optimal information from the analysis for a truncated series is obtained at the minimum or inflexion point in τ\tau of the approximate theoretical curves (see Figs 3 and 4). This optimal criterion corresponds to the (principle of minimum sensitivity of the physical parameters on the external sum rule variable τ\tau) and where the exact solution is reached when one adds more and more terms in the approximate series.

In the case of hadrons, we illustrate in Figs. 5 and 6 the analysis for the Υ\Upsilon systems and for the BB meson decay constant using relativistic sum rules.

VII.4 tct_{c} and μ\mu-stabilities

Later on, we have extended this τ\tau-stability criterion to the continuum threshold variable tct_{c}666In many papers, the optimal value is extracted at the lowest value of tct_{c} ! but the result still increases with the tct_{c} changes. and to the arbitrary Perturbative (PT) subtraction point μ\mu777One can also use the RGE resummed solution which is equivalent to take μ2=1/τ\mu^{2}=1/\tau but in some case the value of τ\tau is relatively large such that the OPE is not well behaved. A such choice of μ\mu value is often outside the μ\mu-stability region.. The lowest value of tct_{c} corresponds to the beginning of τ\tau-stability while the tct_{c}-stability corresponds to a complete lowest ground state dominance in the spectral integral. In our analysis, we always consider the conservative optimal result inside this tct_{c}-region 888tc\sqrt{t_{c}} is often identified to the mass of the 1st radial excitation which is a crude approximation as the QCD continuum smears all higher state contributions to the spectral function..

VII.5 Ground state versus the QCD continuum

For some low value of (tc(t_{c} and large value of τ\tau, one can have some flat curves or some (apparent) minimum in τ\tau. Then, to check or/and to restrict the optimal region in this case, one also requests that the contribution of the ground state to e.g. the spectral integral (e.g. moment sum rule) is larger than the QCD continuum one. One can formulate this constraint in a more rigorous way as (see e.g. SNPC for some examples of applications) :

RP/Ct>tc𝑑tetτImΠ(t)tc𝑑tetτImΠ(t)1.R_{P/C}\equiv\frac{\int_{t>}^{t_{c}}dt\,e^{-t\tau}{\,\rm Im}\,\Pi(t)}{\int_{t_{c}}^{\infty}dt\,e^{-t\tau}{\,\rm Im}\,\Pi(t)}\geq 1. (42)

VIII Phenomenology of the ρ\rho-meson LSR

VIII.1 Lower bound on the ρ\rho-meson coupling from the lowest moment 0{\cal L}_{0}

We use the MDA parametrization of the spectral function and extract the ρ\rho-meson coupling 999Analysis using the complete e+eI=1e^{+}e^{-}\to I=1 Hadrons data can e.g. be found in Refs. LNT ; SNe23 . :

1πImΠρ(t)=Mρ22γρ2withΓρe+e=23α2πMρ2γρ2andγρexp=2.479(15)\frac{1}{\pi}\mbox{Im}\Pi_{\rho}(t)=\frac{M_{\rho}^{2}}{2\gamma_{\rho}^{2}}\,~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}{\rm with}\,~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}\Gamma_{\rho\to e^{+}e^{-}}=\frac{2}{3}\alpha^{2}\pi\frac{M_{\rho}}{2\gamma_{\rho}^{2}}\,~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}{\rm and}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}\gamma_{\rho}^{exp}=2.479(15) (43)

\diamond~{}Using positivity of the spectral integral and evaluating the LSR at τ=1/Mρ2\tau=1/M_{\rho}^{2}, SNR deduces the inequality to leading order of PT series 101010Notice that this inequality has been considered as an estimate in the original SVZ paper SVZa .:

γρ24π2e[1+𝒪(αs)π3αsG2Mρ4]γρ2.43.\gamma_{\rho}^{2}\geq\frac{4\pi}{2\,e}\Big{[}1+{\cal O}(\alpha_{s})-\frac{\pi}{3}\frac{\langle\alpha_{s}G^{2}\rangle}{M_{\rho}^{4}}\Big{]}\Longrightarrow\gamma_{\rho}\geq 2.43. (44)

We improve this bound by adding higher order terms in the PT series and including the contribution of the condensates up to dimension-six. We show the analysis in Fig.7 for different values of tct_{c} and τ\tau. The RP/CR_{P/C} condition is shown by the cyan curve where the lowest ground state dominates in the delimited right region. Optimal results are obtained for the sets (τ,tc)(\tau,t_{c}) from (0.5,1.5) to (1.1,3.0) in units of (GeV-2, GeV2). This leads to the improved lower bound at order αs2\alpha_{s}^{2} :

γρ1.83(13)tc(1)as(1)G2(1)ψ¯ψ2.\gamma_{\rho}\geq 1.83(13)_{t_{c}}(1)_{a_{s}}(1)_{G^{2}}(1)_{\bar{\psi}\psi^{2}}. (45)
Refer to caption
Figure 7: Lower bound of the γρ\gamma_{\rho} coupling versus the sum rule variable τ\tau for different values of the continuum threshold tct_{c}.
Refer to caption
Figure 8: τ\tau-behaviour of the lowest moment 0{\cal L}_{0} for different truncation of the OPE.

VIII.2 The lowest moment 0{\cal L}_{0} using the e+eI=1e^{+}e^{-}\to I=1 Hadrons data

It is informative to compare the QCD prediction of 0{\cal L}_{0} with the one where the complete e+eI=1e^{+}e^{-}\to I=1 Hadrons data is used to estimate the spectral integral. This analysis has been done recently in Ref. SNe23 which we show in Fig. 8

One can observe that there is a good agreement with the experimental e+ee^{+}e^{-} data. and the theory prediction using the previous sets of QCD parameters up to D=6,8D=6,8 condensates.

VIII.3 MρM_{\rho} from the lowest ratio of moments 10{\cal R}_{10}

\diamond~{}Within MDA, one expects that the ratio of moments provides the mass squared of the ρ\rho-meson ground state. We show the analysis versus τ\tau and for different values of tct_{c} in Fig. 9.

Refer to caption
Figure 9: MρM_{\rho} versus the sum rule variable τ\tau for different values of the continuum threshold tct_{c}.

The optimal results are obtained for the sets (τ,tc)(\tau,t_{c}) from (0.5,1.2) to (1.2,3.0) in units of (GeV-2, GeV2). We obtain:

Mρ848(109)tc(3)as(3)G2(13)ψ¯ψ2,M_{\rho}\simeq 848(109)_{t_{c}}(3)_{a_{s}}(3)_{G^{2}}(13)_{\bar{\psi}\psi^{2}}, (46)

where the error comes mainly from the value of tct_{c} which we have taken in the conservative range from the beginning of τ\tau stability until the tct_{c}-one.

\diamond~{}One can restrict this range of tct_{c} value using the constraint from the first moment of FESR. It reads FESR1 ; FESR2 :

Mρ22γρ2=tc4π2[1+as(tc)+as2(tc)[R2β12(β2/β1)lnln(tc/Λ2)]],\frac{M_{\rho}^{2}}{2\gamma_{\rho}^{2}}=\frac{t_{c}}{4\pi^{2}}\Big{[}1+a_{s}(t_{c})+a_{s}^{2}(t_{c})\big{[}R_{2}-\frac{\beta_{1}}{2}-(\beta_{2}/\beta_{1}){\rm ln\,ln}(tc/\Lambda^{2})\big{]}\Big{]}, (47)

from which we deduce:

tc1.962(24)tc(2)αsGeV2.t_{c}\simeq 1.962(24)_{t_{c}}(2)_{\alpha_{s}}~{}{\rm GeV}^{2}. (48)

\diamond~{}One should note that the low value of tct_{c} often chosen by many “QCD sum rules practitioners” to reproduce the value of the experimental mass or to extract the mass of the ground state does not coi ncide with the duality constraint from FESR. At the value of tct_{c} in Eq. 48, we obtain from the ratio of moments :

Mρ881MeV.M_{\rho}\simeq 881~{}{\rm MeV}. (49)

\diamond~{}From the previous analysis, the ratio of moments reproduces within 10% the experimental meson mass.

VIII.4 QCD condensates from 10{\cal R}_{10} using e+ee^{+}e^{-}\to Hadrons data

\diamond~{}The ratio of moments has the advantage to be less sensitive to αs\alpha_{s} correction than the moment 0{\cal L}_{0} as the PT correction starts to order αs2\alpha_{s}^{2}. It is then expected to be a good place for extracting the QCD condensates. This analysis has been initiated by Ref. LNT and revised recently in Ref. SNe23 . Using as input the value of the gluon condensate obtained from heavy quark sum rules SNparam ; SNREV22 ; SNREV21 given in Eq. 17, one obtains:

ραsψ¯ψ25.98(64)104GeV6,C8O8=(4.3±3.0)×102GeV8`,\rho\alpha_{s}\langle\bar{\psi}\psi\rangle^{2}\simeq 5.98(64)10^{-4}\,{\rm GeV}^{6},~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}~{}C_{8}\langle O_{8}\rangle=(4.3\pm 3.0)\times 10^{-2}\,{\rm GeV}^{8}`, (50)

where the value of the four-quark condensate is in good agreement with the one in Eq. 19.

\diamond~{}We show in Fig. 10 a comparison of the experimental expression of 10{\cal R}_{10} with the QCD prediction for different truncations of the OPE. One can notice a good agreement when the condensates up to dimension 6,8 are included.

Refer to caption
Figure 10: τ\tau-behaviour of the ratio of moments 10{\cal R}_{10} for different truncation of the OPE.

IX Sum of light quark masses from the pion LSR

IX.1 Lower bound on (m^u+m^d)(\hat{m}_{u}+\hat{m}_{d})

Using the pion sum rule, SNR has derived a lower bound on the RGI quark mass defined in Eq. 37 from the positivity of the spectral function and retaining the pion contribution. The results have been given for different values of the QCD scale Λ\Lambda. Given the present progress on the determination of Λ\Lambda, we show the new version of the figure given in Ref. SNR in Fig. 11 for different truncation of the PT series.

Refer to caption
Figure 11: τ\tau-behaviour of RGI (m^u+m^d)(\hat{m}_{u}+\hat{m}_{d}) lower bound for different truncation of the PT series.

We deduce the optimal lower bound at the maximum of the curves :

(m^u+m^d)\displaystyle(\hat{m}_{u}+\hat{m}_{d}) \displaystyle\geq 10.13(6)αs(22)G2(37)ψ¯ψ2MeV=10.13(44)MeV:NLO,\displaystyle 10.13(6)_{\alpha_{s}}(22)_{G^{2}}(37)_{\bar{\psi}\psi^{2}}~{}{\rm MeV}=10.13(44)~{}{\rm MeV}~{}~{}~{}:~{}~{}~{}~{}{\rm NLO}, (51)
\displaystyle\geq 7.92(26)αs(1)G2(8)ψ¯ψ2MeV=7.92(27)MeV:N4LO,\displaystyle 7.92(26)_{\alpha_{s}}(1)_{G^{2}}(8)_{\bar{\psi}\psi^{2}}~{}{\rm MeV}~{}~{}~{}=7.92(27)~{}{\rm MeV}~{}~{}~{}~{}:~{}~{}~{}~{}{\rm N4LO},

This bound can be improved by introducing the contribution of the next radial excitation π(1300)\pi(1300)SNLIGHT and/or some alternative approaches LELLOUCH .

IX.2 Estimate of (m^u+m^d)(\hat{m}_{u}+\hat{m}_{d})

One can transform the previous lower bound by introducing the π(1300)\pi(1300)\oplus QCD continuum for parametrizing the spectral function. Using the standard OPE, one obtains to order αs4\alpha_{s}^{4} for the RGI and running masses m¯q\overline{m}_{q} evaluated at 2 GeV SNLIGHT 111111Extension of the analysis to some other channels are discussed in this paper.:

(m^u+m^d)=9.76(88)MeV(m¯u+m¯d)(2)=8.08(61)MeV,(\hat{m}_{u}+\hat{m}_{d})=9.76(88)~{}{\rm MeV}~{}~{}~{}\to~{}~{}~{}(\overline{m}_{u}+\overline{m}_{d})(2)=8.08(61)~{}{\rm MeV}, (52)

where one can notice that the main uncertainties and the size of the central value come from the parametrization of the spectral function (radial excitations \oplus choice of the QCD continuum threshold tct_{c}). The error due to the way for truncating the PT series only affects slightly the total error (see e.g. KAHN ). These results agree with lattice calculations LATTLIGHT and from some other approaches quoted in PDG PDG .

X Some other applications of LSR

These applications have been already summarized in the recent short reviews SNREV21 ; SNREV22 where orginal references and some dedicated reviews can be found. They concern the :

\bullet~{}Light baryons qqqqqq^{\prime} ligth quark states

\bullet~{}Heavy quarks Q¯Q\bar{Q}Q sector.

\bullet~{}Heavy-light Q¯q\bar{Q}q states.

\bullet~{}So-called exotic states :

\diamond~{}Glueballs / gluonia gg,ggggg,ggg states.

\diamond~{}Hybrids q¯gq,\bar{q}gq,\cdots states.

\diamond~{}Light (q¯q¯)(qq)(\bar{q}\bar{q}^{\prime})(qq^{\prime}), heavy-light (q¯Q¯)(Qq)(\bar{q}\bar{Q})(Qq)\cdots , fully-heavy (Q¯Q¯)(QQ),(\bar{Q}\bar{Q})(QQ),\cdots four-quark states.

\diamond~{}Light (q¯q)(qq¯)(\bar{q}q^{\prime})(q\bar{q}^{\prime}), heavy-light (q¯Q)(Qq¯)(\bar{q}Q)(Q\bar{q})\cdots , fully-heavy (Q¯Q)(Q¯Q),(\bar{Q}Q)(\bar{Q}Q),\cdots molecule states.

We plan to develop these different parts in a more extended review on QCD spectral sum rules.

Concluding remarks

LSR and (in general) QCD spectral sum rules (QSSR) are useful tools to tackle within a good approximation the properties of hadrons and for extracting the fundamental parameters of the QCD Lagrangian. If properly done, QSSR is a serious alternative or/and a supplement to the lattice QCD numerical simulations.

References

  • (1) V. De Alfaro, S. Fubini, G. Furlan, C. Rossetti, Currents in hadron physics, North Holland Pub. Co. Amsterdam-London (1973).
  • (2) S. Weinberg, Phys. Rev. Lett. 18 (1967) 507.
  • (3) T. Das, V.S. Mathur, S. Okubo, Phys. Rev. Lett. 19 (1967) 470.
  • (4) E.G. Floratos, S. Narison and E. de Rafael, Nucl. Phys. B155 (1979) 155 and references quoted therein.
  • (5) S. Narison and E. de Rafael, Nucl. Phys B169 (1980) 253 and references quoted therein..
  • (6) S. Narison, Z. Phys. C 22 (1984) 161.
  • (7) M.A. Shifman, A.I. Vainshtein, V.I. Zakharov, Nucl. Phys. B147 (1979) 385; ibid, Nucl. Phys. B147 (1979) 448.
  • (8) V.I. Zakharov, Int. J. Mod .Phys. A14, (1999) 4865.
  • (9) S. Narison, QCD spectral sum rules, World Sci. Lect. Notes Phys. 26 (1989) 1.
  • (10) S. Narison, QCD as a theory of hadrons, Cambridge Monogr. Part. Phys. Nucl. Phys. Cosmol. 17. (2004) 1-778 [hep-ph/0205006].
  • (11) S. Narison, Phys. Rept. 84 (1982) 263; ibid, Riv. Nuovo Cim. 10N2 (1987) 1.
  • (12) L.J. Reinders, H.R. Rubinstein, S. Yazaki, Phys. Reports 127 (1985) 1.
  • (13) R.A. Bertlmann, Acta Phys. Austriaca 53, (1981) 305.
  • (14) M.A. Shifman, Prog. Theor. Phys. Suppl. 131 (1998)1; P. Colangelo and A. Khodjamirian, hep-ph/0010175; E. de Rafael, hep-ph/9802448; F.J. Yndurain, Monographs in Physics, Springer-Verlag, New York (1999).
  • (15) S. Narison,Nucl.Part. Phys. Proc.324-329 (2023) 94; ibid, 258-259 (2015) 189.
  • (16) S. Narison, Nucl. Part. Phys. Proc.312-317 (2021) 87; ibid, 300-302 (2018) 153.
  • (17) S. Narison, Nucl. Part. Phys. Proc. 309-311 (2020) 135; ibid 270-272 (2016) 143.
  • (18) J.S. Bell, R.A. Bertlmann, Nucl. Phys. B177, (1981) 218; ibid, Nucl. Phys. B187, (1981) 285.
  • (19) S. Narison, E. de Rafael, Phys. Lett. B103, (1981) 57.
  • (20) J. Bijnens, J. Prades, E. de Rafael, Phys. Lett. B348 (1995) 226.
  • (21) S. Narison, Phys. Lett. B210 (1988) 238; ibid, Phys. Lett. B337 (1994) 166.
  • (22) A.A. Logunov, L.D. Soloviev, A.N. Tavkhelidze, Phys. Lett. B24 (1967) 181.
  • (23) J.J. Sakurai, Phys. Lett. B46 (1973) 207.
  • (24) K.G. Chetyrkin, N.V. Krasnikov, A.N. Tavkhelidze, Phys. Lett. B76 (1978) 83.
  • (25) A.L. Kataev, N.V. Krasnikov, A.A. Pivovarov, Phys. Lett. B123 (1983) 93.
  • (26) S.G. Gorishnii, A.L. Kataev, S.A. Larin, Phys. Lett. B135 (1984) 457.
  • (27) R.A. Bertlmann, G. Launer and E. de Rafael, Nucl. Phys. B250, (1985) 61.
  • (28) R.A. Bertlmann, C.A. Dominguez, M. Loewe, M. Perrottet and E. de Rafael, Z. Phys. C39 (1988) 231.
  • (29) M. Gell-Mann, R.J. Oakes, B. Renner, Phys. Rev. 175 (1968) 2195.
  • (30) H.G. Dosch, S. Narison, Phys. Lett. B417 (1998) 173.
  • (31) S. Narison, Int. J. Mod. Phys. A33 (2018) no. 10, 185004; Addendum: Int. J. Mod. Phys. A33 (2018) no.10, 1850045.
  • (32) S. Narison, R. Tarrach, Phys. Lett. B125 (1983) 217.
  • (33) B.L. Ioffe, Prog. Part. Nucl. Phys. 56 (2006) 232; ibid, B188 (1981) 317; ibid, B191 (1981) 591.
  • (34) H.G. Dosch, Non-Perturbative Methods (Montpellier 1985); Y. Chung et al.Z. Phys. C25 (1984) 151; H.G. Dosch, M. Jamin, S. Narison, Phys. Lett. B220 (1989) 251.
  • (35) A.A. Ovchinnikov, A.A. Pivovarov, Yad. Fiz. 48 (1988) 1135.
  • (36) S. Narison, Phys. Lett. B605 (2005) 319.
  • (37) S. Narison, Phys. Lett. B673 (2009) 30.
  • (38) G. Launer, S. Narison, R. Tarrach, Z. Phys. C26 (1984) 433.
  • (39) C.A. Dominguez, J. Sola, Z. Phys. C40 (1988) 63.
  • (40) S. Narison, Phys. Lett. B300 (1993) 293; ibid B361 (1995) 121.
  • (41) S. Narison, Phys. Lett. B693 (2010) 559, erratum ibid, B705 (2011) 544; ibid, B706 (2012) 412; ibid, B707 (2012) 259.
  • (42) S.N. Nikolaev, A.V. Radyushkin, Phys. Lett. B124 (1983) 243.
  • (43) T. Schafer, E.V. Shuryak, Rev. Mod. Phys. 70 (1998) 323.
  • (44) B.L. Ioffe, A.V. Samsonov, Phys. At. Nucl. 63 (2000) 1448.
  • (45) A. Di Giacomo, Non-pertubative Methods, ed. Narison, World Scientific (1985); A. Di Giacomo, G.C. Rossi, Phys. Lett. B100 (1981) 481; M. D’Elia, A. Di Giacomo, E. Meggiolaro, Phys. Lett. B408 (1997) 315.
  • (46) S. Narison, arXiv : 2306.14639 [hep-ph] (2023).
  • (47) S. Narison, Phys. Lett. B707 (2012) 259.
  • (48) S. Narison, Phys. Lett. B718 (2013) 1321; ibid, Nucl. Phys. (Proc.Suppl.) 234 (2013) 187.
  • (49) R.M. Albuquerque, S. Narison, D. Rabetiarivony, arXiv : 2301.08199 (2023).
  • (50) S. Narison, Phys. Lett. B738 (2014) 346 and references therein.
  • (51) K.G. Chetyrkin, J.H. Kühn and M. Steinhauser,Comput. Phys. Comm 133 (2000) 43 and references therein.
  • (52) L. Lellouch, E. de Rafael, J. Taron, Phys.Lett. B414(1997)195; C.A. Dominguez, E. de Rafael, Annals Phys. 174 (1987) 372; J. Bijnens, J. Prades, E. de Rafael, Phys. Lett. B348 (1995), 226.
  • (53) S. Aoki et al., arXiv:1310.8555 [hep-lat] (2013).
  • (54) M.S.A. Alam Khan, arXiv: 2306.10266 [hep-ph] (2023).
  • (55) R.L. Workman et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2022 (2022) 083C01.