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It has been mentioned above that in the calculation of virtual corrections to LO diagrams UV divergencies are encountered. These are associated with the large-momentum limit of the emerging loop integrals. In a renormalizable quantum field theory like QCD, such divergencies can be removed at any order in the perturbative expansion by adding a finite number of terms to the original, unrenormalized Lagrangian. This amounts to a redefinition of the gluon, ghost, and quark fields, and the parameters of the theory, i.e., the coupling gs, quark masses (if appropriate), and gauge-fixing parameter η inLQCD:

Aaµ → Z31/2Aa, χa → Z˜31/2χar ,

ψ → Z21/2ψr , gs → ZggS,r, m → Zmmr ,

η → Z3ηr, (2.17)

where Z3,Z˜3, Z2, Zg, Zm are the gluon-, ghost-, and quark-field, coupling-constant, and mass renormalization constants. The subscript r labels the renormalized fields and pa-rameters. Color and flavor indices have been suppressed for simplicity. The gauge-fixing parameter η is associated with the same renormalization constant Z3 as the gluon fields in order to preserve the form of the gauge-fixing term in LQCD. Also the other renormal-ization constants are related to each other via so-called Slavnov-Taylor identities [58, 59]

reflecting the gauge-symmetry of the Lagrangian.

So far we have only renamed the fields and parameters entering the Lagrangian. The ultimate goal of this procedure, however, is to obtain a priori unrenormalized – so-called bare – Greens functions Gb, e.g., two-point functions such as quark or gluon propagators, from the rewritten LQCD in a form that all UV singularities can be reshuffled into the multiplicative renormalization constants Zi,

Gb=ZiGr. (2.18)

2.3 Renormalization 15

The remaining – UV finite – piecesGrare then interpreted as the “physical” Greens func-tions of the renormalized fields. If it is possible to follow this procedure, the Lagrangian is said to be renormalizable. In a fixed order perturbative calculation a multiplicative renormalization of the form (2.18) amounts to a subtraction of divergencies. For instance, considering the Greens function of Eq. (2.18) atO(αs), we find after writingZi andGb as series in αs

Gr=Zi1Gb '(1−αsCi) (Gb,0sGb,1) , (2.19) with coefficients Ci and Gb,1 which still contain singularities, while the lowest-order con-tributionGb,0 is finite. Expanding Eq. (2.19) and disregarding terms of O(α2s) we obtain Gr =Gb,0s[Gb,1−CiGb,0] +O(α2s). (2.20) The Ci in theO(αs) contribution of Eq. (2.20) serves to cancel the pole terms of Gb,1. It is therefore often referred to as “counter term”. We will illustrate the concept sketched here by an explicit example in Sec. 2.3.1

The renormalization procedure contains a certain amount of arbitrariness. In order to obtain finite and therewith physically meaningful quantities, clearly all divergencies have to be removed. However, there exists no physical constraint restricting the subtractions to infinities only. Any number of finite terms can be subtracted along with the UV poles as well. Therefore, a certain prescription has to be chosen for the calculation of renormalized quantities. Depending on this rule one encounters different renormalization schemes. Ap-plying dimensional regularization for isolating any kind of singularities suggests to simply subtract any UV poles of the form 1/ε from the unrenormalized Greens functions and reshuffle them into the associated renormalization constants. This method is known as Minimal Subtraction (MS) and was developed by ’t Hooft in the early seventies [60]. On the other hand, any poles in εusually show up in the combination

1

ε+ ln 4π−γE , (2.21)

where γE is the Euler-Mascheroni constant. Thus, it is more natural to subtract this expression rather than simply the 1/ε poles. In practice, this is done by a replacement of the regularization scale,

µ2d → µ˜2d = µ2d eγE

4π , (2.22)

and the subtraction of 1/ε-poles only rather than the full expression (2.21). It can be easily seen that performing a series expansion for the factor ¡

˜ µ2d¢ε

, which always enters along with the dimensionless coupling, produces exactly the terms of Eq. (2.21) asε→0. This renormalization prescription, the so-called Modified Minimal Subtraction (MS) scheme [61]

is the most commonly used in pQCD and will be applied throughout this work.

In practice, the renormalization of the sum of all virtual corrections to a massless cross section can also be achieved by the replacement of the bare couplingαbs according to

αbs

see, e.g., [62], with

Sε= exp{ε[ln 4π−γE]} and β0 = 11

3 CA−2

3Nf , (2.24) where CA= 3 and µr is an arbitrary scale introduced via the renormalization procedure.

Observables computed at different scales are related to each other via renormalization group equations [60, 63]. These are based on the physical requirement that any observable must be independent of unphysical scales, which are only an artifact of the renormalization procedure as discussed in (2.12). If the behavior of a quantity under the renormalization group equations is known its variation in a change of the scale from an initial value µ0 to any other value µis determined up to terms beyond the order in αs considered.

E.g., at NLO the running of the strong couplingαs2) is controlled by the renormal-ization group equation

µ∂αs

∂µ =−β0

2π α2s− β1

2 αs3+O(α4s), (2.25) where β1 = 51−19Nf/3 and Nf is the number of flavors. Solving this equation one obtains [64]

αs(µ)' 4π β0ln (µ22)

"

1−2β1 β02

ln£

ln(µ22)¤ ln(µ22)

#

. (2.26)

Here the mass parameter Λ encodes the constant of integration in a convenient way. It is a fundamental parameter of QCD and has to be determined from experiment. Λ also depends on the choice of renormalization scheme. Of course, results obtained in one specific renormalization scheme can be transformed to another one by performing an additional finite renormalization.

2.3.1 Example: Quark Selfenergy

To illustrate the concepts and methods introduced so far by an instructive example let us calculate the selfenergy S(p) of a quark at O(αs) in n dimensions and renormalize it in the MS scheme. A generalization of the methods encountered in this simple task to more complicated cases will be presented in Chap. 3.

The bare or unrenormalized selfenergy Silb(p) of a quark with momentum p, a loop momentum k, and color indices i, l,

p, i (p−k), j p, l k, a

= Silb (p), (2.27)

2.3 Renormalization 17

is calculated with the help of the Feynman rules of App. A. For the computation of the color factor we use the identity

X

a,j

TijaTjla =CFδil, (2.28) withCF = 4/3. The dimensionless coupling constantgsis replaced according to Eq. (2.16) by ˜gs=gsµ˜εd. Doing so we obtain

with a loop integration that diverges in four dimensions as k→ ∞. Inn <4 dimensions, however, it has a well-defined meaning and can be calculated in a straightforward manner.

With a projection onto the scalar integral B˜0 = 1

both integrals, resulting from a decomposition of the integrand in (2.29), can be calculated.

Making furthermore use of the expansion

Γ(1 +ε)∼eγEε (2.31)

This unrenormalized expression for the quark selfenergy obviously diverges as ε→0. To get a physically sensible, renormalized result Σ(p2), we have to subtract solely the singular term,

This renormalization prescription has to be slightly modified for external on-shell quarks. Starting from the unrenormalized selfenergy (2.34), only a counter term 1/2ε rather than 1/εis subtracted for external legs since these lines are renormalized with the square root of the respective renormalization constant, √

Zi, rather than Zi as internal propagators, cf. Eqs. (2.19) and (2.20),

Σ(p2) =−αs

Then,ε is analytically continued to negative values,ε→ε˜=−ε, giving Σ(p2) =−αs

Now the quark can safely be put onto the mass-shell. Setting p2 = 0 we obtain Σ(p2 = 0) =−αs

4π 1

2ε . (2.39)

The UV divergence has transformed into an IR pole by the renormalization procedure. As mentioned above, such singularities cancel if all contributions to a physically well-defined observable are added.