QFT II Problem Set 12.
FS 2019 Prof. M. Grazzini https://www.physik.uzh.ch/en/teaching/PHY552/FS2019.html Due by: 27/5/2019
Exercise 1. Renormalization in QCD at one loop: The gluon Propagators
In this exercise series we will learn how to compute the UV divergent diagrams at one loop in QCD and how to renormalize these. For this we will absorb these divergencies into the physical quantities and write the bare Lagrangian parameters in terms of renomalized ones such as masses and coupling constants. The divergent diagrams include the corrections to the propagators and the corrections to the vertices. In this exercise we will look at the gluon propagator only.
There are three self energy diagrams for gluon at one loop as shown in Figure 1.
Figure 1: One loop gluon self energy
(a) Let Πµν express the one loop gluon self energy. Write down an expression for each diagram contributing to Πµν, i.e. Πµν1 , Πµν2 and Πµν3 by applying Feynman rules.
(b) Compute the gluonic contribution, i.e. Πµν3 in d-dimensions.
• First work out the numerator and write Πµν3 as:
Πµν3 = g2 2 Ncδcd
Z ddk (2π)d
Aµν
k2(p+k)2 (1) wherek and pare the loop and external momentas respectively.
Keeping the tensor structure apply Feynman parametrization and make the necessary shifting of the loop momentum. Note that the terms linear in the loop momentum are odd and therefore vanishes:
Z ddk (2π)d
kµ
(k2−∆)2 = 0 (2)
This means you can make the replacement:
kµkν = k2
d gµν+ terms linear in k which vanish (3) You should find:
Πµν3 = g2 2 Ncδcd
Z dx
Z ddk (2π)d
gµν
2 +4d−6d
k2+ 2∆ + 5p2
+Mµν
(k2−∆2)2 (4)
where
Mµν = pµpν
p2 ∆(4d−6) +p2(d−6)
, ∆ =−p2x(1−x) (5) 1
• Now make the Wick rotation to perform the loop integration in the Euclidean space.
Note that:
Z ddk (2π)d
k2
(k2+ ∆)2 = (2−)∆
−1 ∆−(4π)Γ() (6) Z ddk
(2π)d 1
(k2+ ∆)2 = ∆−(4π)Γ() (7)
• Finally you need to perform the integration over the Feynman parameter x. Your result should be
Πµν3 = ig2
2 NCδcdp2
gµν(19−12) +pµpν
p2 (−22 + 14)
(8) Γ() (4π)(−p2)− B(2−,2−)
1− (9)
whereB(2−,2−) is the Beta function:
B(2−,2−) = Z 1
0
dx x1−(1−x)1− (10) (c) Now compute the ghost contribution Πµν2 following the same steps before. (Do not forget
the minus sign for the fermion and the ghost loop!) You should find:
Πµν2 = 1 2
g2NCδcd
16π2 (4π)(−p2)−Γ()
gµνp2+ 2(1−)pµpν B(2−,2−)
1− (11)
(d) Show that the sum of Πµν2 and Πµν3 can be brought to the form:
Πµν(p) = p2gµν−pµpν
Π(p2) (12) wherep is the momentum of the external gluon. This implies that:
Πµνpµ= 0. (13)
which is a consequence of the Ward identity in QCD and tells that the gluons are trans- verse. It is important to notice that individually the second and third diagrams cannot be brought to this form. This means to express a physical gluon propagator we need the ghost contribution!
(e) Now compute the fermionic contribution Πµν1 . Take the fermions running in the loop massless so that you can write:
Πµν1 =− g2 4π2
δab
2 nfΓ() (4π)
gµνp2−pµpν
(−p2)−B(2−,2−) (14) (f) We define the renomalized wave function for the gluon field as:
A=Z31/2AR (15)
which leads to renormalised propagator at leading order:
Dabµν = δab(−igµν)
Z3p2 (16)
2
Then up to second order in perturbation theory the gluon propagator is:
Sabµν(p) = δab(−igµν)
Z3p2 + δac(−igµσ)
Z3p2 Πcdστ(p)δdb(−igτ ν)
Z3p2 (17)
Using the transversality:
Πcdστ(p) =δcd
−gστ +pσpτ p2
Π(p2) (18)
Now using this and expressing Sabµν(p) as a geometric sum we have:
Sabµν(p) = δab(−igµν)
Z3p2+ Π(p2) (19)
Now combine your results for Π(p2) from part iv) to determineZ3 so that the divergences cancel:
Z3= 1− αs 4π 1
2 3nf− 5
3NC
+ finite (20)
Exercise 2. 1-loop renormalised QCD coupling constant
To renormalise QCD one re-scales the fields and parameters in such a way that the Lagrangian can be written: LR+Lc.t, where LR has the form of the original ‘bare’ Lagrangian L0, but with each term replaced by it’s corresponding renormalised one, andLc.tcontains the respective counter-terms. In particular, under the re-scaling:
Aaµ=Z
1 2
3AaµR ψ=Z
1 2
2ψR g=ZggR
the bare quark-quark-gluon vertex is transformed:
gψγ¯ µTaψAaµ−→ gRµεψ¯RtaAaµRγµψR ZgZ2Z
1 2
3
| {z }
≡Z1F
,
where as usual theµε was introduced to render the coupling dimensionless in dimensional reg- ularisation.
(a) Using the definition Zi = 1 +δZi for i= 2,3,1F, expand the renormalisation factors to O(g2R) and show that
g=
1−δZ2−1
2δZ3+δZ1F
gR µε.
(b) Then, with
Z3 = 1−gR
4π 2
2 3nf −5
3Nc
1
ε+ finite
+O g4R
, (21)
Z2 = 1−gR
4π 2
CF
1
ε+ finite
+O gR4
, (22)
Z1F = 1−gR 4π
2
[Nc+CF] 1
ε+ finite
+O gR4
, (23)
3
whereCF = (Nc2−1)/2Nc, show that this has the explicit form g=
1− g2R 16π2
11
6 NC −1
3nf 1
ε+ finite
gR µε, up to higher orders ingR.
Exercise 3. The 1-loop Beta function in QCD
The Beta function β(gR) in renormalised QCD determines how the coupling parameter gR(µ) depends on the renormalisation scale µvia the following differential equation:
∂gR
∂lnµ =µ∂gR
∂µ =β(gR) (24)
where the derivatives are taken withg held constant.
(a) With this definition use the result of Exercise 2 part (b) to show that:
β =− 11
3 NC−2 3nf
gR3
16π2 +O(gR5) (b) By defining a scale ΛQCD via the condition:
µ→ΛlimQCD 1 g2R(µ) = 0
solve equation 24 explicitly and show thatαS(µ) :=g2R/4π satisfies:
αS(µ) = 4π
11
3 NC−23nf ln
µ2 Λ2QCD
(c) Classify all the different possible behaviours ofαS(µ) as a function of NC and nf. What is the form ofαS(µ) in the case of QCD? Why is this so significant?
Exercise 4. Renormalization invariance of the β-function In terms of the α=g2/4π the β-function is defined by
∂α
∂lnµ2 =β(α) and has the following expansion:
β(α) =−α
β0
α 4π
+β1
α 4π
2
+O α3
.
Show that the first two coefficients of the expansion are renormalization scheme invariant, i.e.
β0A=β0B, β1A=β1B, for any two schemesA and B.
Hint. You may start from the fact thatαB =αA 1 +O αA . 4