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Appendix C
Radiative Corrections

Before measurements of observable quantities can be made in the framework of the SM, the effects of many secondary effects due to the electromagnetic, weak and strong interactions must be included. Such effects are called radiative corrections and naturally divide into three areas for the general process e+e-® Z0® f[`(f)]) as follows: This appendix presents an overview of the sources of radiative corrections in the framework of the Standard Model with an emphasis on the electroweak component (GSW) of the radiative corrections since this specifically applies to the analysis presented in this thesis. Since the physical input parameters a, MZ0, MW±, MH, mf for the SM are clearest in the on-shell scheme where sin2qW = 1-[(MW2)/(MZ2)], this scheme will be used in discussing radiative corrections.

QED Corrections

The QED Corrections are dependent on the details of the experimental setup but independent of the detailed structure of the underlying non-electromagnetic part of the theory. In fact, the only global parameters needed are MZ, GZ, vf, af and mf, without restriction to the SM. The corrections have coupling strengths which are determined by the low energy a with the associated O(a) diagrams shown in Figure C.1. The corrections are gauge invariant and renormalizable. At LEP, a realistic treatment of the QED corrections require higher order contributions than simply O(a). In general, the practical methods of dealing with higher order QED effects are broken down into four basic areas: i) soft photon resummation in the O(a) result, ii) explicit 2-loop calculations, iii) the structure function approach, and iv) the multi-photon radiation according to the method of Yennie, Frautschi, and Suura (YFS) [63]. The interested reader is referred to references [63] for an excellent discussion of these higher order QED contributions.


Graphic: images/feyndiagqed.gif

Figure C.1: The Feynman Diagrams for O(a) QED Corrections to e+e-® f[`(f)]


Weak Corrections

The Weak Corrections dependent on the detailed internal structure of the theory, e.g. dependence on the non-Abelian structure and the Higgs sector of the SM, but are independent of the experimental setup. In particular, they depend on the unknown parameters MH, mt and therefore include all the components necessary for the renormalizability of the SM. Due to the complex structure of the corrections, a detailed treatment of the corrections is required. The radiative corrections associated with the weak interaction involve corrections to the vector boson propagators g and Z0 shown in Figure C.2 [105], corrections to the vertex and corrections due to the box diagrams with two massive boson exchanged as shown in Figure C.3 [104], . In calculating the weak corrections, it is instructive to consider each of the above corrections separately.


Graphic: images/propcorr.gif

Figure C.2: Propagator Corrections to e+e-® f[`(f)]


Graphic: images/vertcorr.gif

Figure C.3: Vertex Corrections and Box Contributions to e+e-® f[`(f)]


Propagator Corrections

The propagator corrections involve all particles in the SM including the conjectured Higgs boson and top quark, thus depending on MH and mt. The propagator corrections are implemented in the e+e- amplitude in terms of three 1PI self-energy functions [105]
Pgg(s)
=
^
S
 

gg 
(s)

s
PgZ(s)
=
^
S
 

gZ 
(s)

s
and
PZ(s)
labeleq:selfenergyfun
(C.1)
The renormalized self-energies are expressed in terms of the non-renormalized ones as follows [100] [101]:
^
S
 

gg 
(s)
=
Sgg(s)- sSgg¢(0)
^
S
 

gZ 
(s)
=
SgZ(s)- SgZ(0)+ s ì
í
î
 2SgZ(0)

MZ2
-  cos(qW)

sW
æ
è
 dMZ2

MZ2
-  dMW2

MW2
ö
ø
ü
ý
þ
^
S
 

ZZ 
(s)
=
SZZ(s)- dMZ2 +dZ2Z (s-MZ2)
^
S
 

WW 
(s)
=
SWW(s)- dMW2 +dZ2W (s-MW2)
(C.2)
with
dZ2Z
=
-Sgg¢(0)-2  cos2(qW)-sin2qW

sinqWcos(qW)
 SgZ(0)

MZ2
+  cos2(qW)-sin2qW

sin2qW
æ
è
 dMZ2

MZ2
 dMW2

MW2
ö
ø
dZ2W
=
-Sgg¢(0)-2  cos(qW)

sW
 SgZ(0)

MZ2
+  cos2(qW)

sin2qW
æ
è
 dMZ2

MZ2
 dMW2

MW2
ö
ø
dMW2
=
Re ( SWW(MW2))
dMZ2
=
Re æ
ç
ç
è
SZZ(MZ2)-
^
S
 

gZ 
(MZ2)2

MZ2+
^
S
 

gg 
(MZ2)
ö
÷
÷
ø
(C.3)
with the corrected propagators containing the renormalized 1-particle irreducible (1PI) one-loop self-energies expressed by [105]:
^
D
 

W 
(s)
=
 1

s-MW2 +
^
S
 

WW 
(s)
^
D
 

Z 
(s)
=
 1

s-MZ2 +
^
S
 

ZZ 
(s)-
^
S
 

gZ 
(s)2

s+
^
S
 

gg 
(s)
^
D
 

g 
(s)
=
 1

s +
^
S
 

gg 
(s)-
^
S
 

gZ 
(s)2

s-MZ2+
^
S
 

ZZ 
(s)
^
D
 

gZ 
(s)
=
^
S
 

gZ 
(s)

[s+
^
S
 

gg 
(s)][s-MZ2 +
^
S
 

ZZ 
(s)] -
^
S
 

gZ 
(s)2
(C.4)
The leading terms of the quantity PZ(s) are of the form:
PZ(s)
=
-Da+  cos2(qW)-sin2qW

sin2qW
D

r
 
+ ···
(C.5)
where
Da
=
-Re( Pgg(MZ2)),
D

r
 
=
 a

4p
·  3

4sin2qWcos2(qW)
æ
è
 mt

MZ
ö
ø
2

 
(C.6)
where D[`(r)] is identified as the ``r parameter''  [107].

The O(a2) corrected Z0 width, DGZ, is given by,
DGZ
=

å
f 
NCf  2

3
aMZ [ vf Re( FVZf (MZ2 )) +af Re( FAZf (MZ2 ))]
+

å
f 
NCf  a

3
MZ(vf2+af2) ·dQED
+

å
f=q 
NCf  a

3
MZ(vf2+af2) ·dQCD
+

å
f 
G(Z® Hf

f
 
)
(C.7)
together with
dQED
=
 3a

4p
Qf2
dQCD
=
 as(MZ2)

p
+ 1.405 æ
è
 as(MZ2)

p
ö
ø
2

 
(C.8)
and G(Z® Hf[`(f)]) [108]. Taking into account the mass dependence of the QCD corrections in the partial width for Z®b[`(b)] increases GZ by 2 MeV with as(MZ2)=0.11±0.01 [103]. The uncertainty from as induces an uncertainty in the total width of about ±6 GeV. The quantities are universal and can be applied to t-channel exchanges as well.

Photon Exchange

The diagonal g propagator diagram has the following form:



Graphic: images/gexchng.gif
 

=
Qe Qf  e2

1+Pgg(s)
 1

s
»
Qe Qf  e2(s)

s
(C.9)


where the real part Re(Pgg(s)) has been absorbed by defining a running electric charge
e2(s) =  e2

1+Re( Pgg(s))
.

Z0 Boson Exchange

The diagonal Z0 propagator diagram has the following form:



Graphic: images/zexchng.gif
 

=
 e2

4sin2qWcos2(qW)
·  1

1+PZ(s)
·  J(e) ·J(f)

s-MZ2 + i  Im( SZ(s))

1+PZ(s)
(C.10)

where
SZ(s)
=
^
S
 

ZZ 
(s)-
^
S
 

gZ 
(s)2

s+
^
S
 

gg 
(s)
    Re( SZ(s)) = (s-MZ2)PZ(s)
(C.11)
and the initial (e) and final (f) current matrix elements are given by


J(e)
=

v
 

e 
[gm (I3e - 2sin2qWQe ) -gmg)5 I3e ] ue
J(f)
=

v
 

f 
[gm (I3f - 2sin2qWQf ) -gmg)5 I3f ] uf
(C.12)

g -Z0 Mixing

The gZ mixing diagram beyond the tree level has following form:



Graphic: images/gzmixing.gif
 

=
gm(vf-afg5 ) + gmQf  PgZ(s)

1+Pgg(s)
=
 1

2sinqWcos(qW)
ì
í
î
gm é
ë
I3f -2Qf æ
è
sin2qW- sinqWcos(qW)  PgZ(s)

1+Pgg(s)
ö
ø
ù
û
-I3f gmg5 ü
ý
þ
(C.13)


The redefinition of a universal effective mixing angle, sin2 [`(q)]W, gives
sin2

q
 

W 
=
sin2 qW- cos(qW)sinqWRe æ
è
 PgZ(s)

1+Pgg(s)
ö
ø
=
sin2qW+cos2(qW)D

r
 
+ ···
(C.14)
with the fermionic currents expressed in terms of sin2 [`(q)]W,

J
 
(e,f)
 
=
gm(I3e,f - 2Qe,f sin2

q
 

W 
) -I3e,f gmg5.
(C.15)
If the variation of sin2qW is incorporated into the previous formalism, one obtains,
MW2sin2qW = MZ2cos2(qW)sin2qW =  A

1-Dr
(C.16)
where
A =  pa

Ö2Gm
= ( 37.2802 ±0.0003 GeV )2
(C.17)
The leading behavior of Dr can be determined by eliminating the combination e2/ sin2qWcos2(qW) in Equation (C.10) with the help of Equation (C.16),
Dr
=
Da-  cos2(qW)

sin2qW
D

r
 
+ ···
(C.18)
and PZ from Equation (C.5) gives,
 e2

4sin2qWcos2(qW)
·  1

1+PZ(s)
=
Ö2GmMZ2  1-Dr

1+PZ(s)
=
Ö2GmMZ2 [ 1+D

r
 
+ ···
(C.19)
A new quantity, [`(Dr)], is usually defined to relate sin2 [`(q)]W directly to the Z0 mass:
MZ2cos2(qWb)sin2qWb
=
 A

1-

Dr
 
(C.20)
where the leading terms are given by

Dr
 
=
Da- D

r
 
+ ···
(C.21)
where in the light fermion part Da is identical to Dr.

Vertex Corrections

The vertex corrections refer to the gff and Z0ff 3-point functions in one-loop order after renormalization with the self-energy contributions to the external legs included. In contrast to the propagator corrections The vertex corrections, unlike the propagator corrections, are not universal, depending in general on the fermion species. For this reason, the vertex corrections must be listed separately for n, e, u, d type fermions (the b quark is exceptional due to the virtual top contributions in the vertex). Of the vertex correction diagrams shown in Figure C.3, only (a)-(c) have non-negligible contributions for f ¹ b, while (d)-(g) are negligible due to the small Yukawa couplings.


Graphic: images/vertcorrselfnrg.gif

Figure C.4: The Vertex Correction and Fermion Self-energy Interactions


The corrected vertices are given in terms of the weak form factors, FV,AZ,f and FV,Ag,f for the Zff and gff vertices as follows [24],
GmZff
=
iegm(vf -afg5) [ 1+Qf2 FQED(s) ] +iegm [ FVZf(s) -FAZf(s)g5 ]
Gmgff
=
-ieQf gm [ 1+Qf2 FQED(s) ] -iegm [ FVgf(s) -FAgf(s)g5 ]
(C.22)
The QED contribution from g exchange is, for Ös >> mf2, contained in the single form factor
FQED
=
 a

4p
-2log  s

l2
æ
è
log  s

mf2
-1 ö
ø
+ log  s

mf2
+log2  s

mf2
+ 4 æ
è
 p2

3
-1 ö
ø
+2pi æ
è
log  s

l2
-  3

2
ö
ø
(C.23)
where the weak form factors for the neutral current vertices are of the form, neutrinos:
FVZn
=
FAZn
(C.24)
charged fermions:
FVZf
=
 a

4p
[ vf (vf2 + 3af2) l2(s,MZ) + FLf ]
FAZf
=
 a

4p
[af (3vf2 + af2) l2(s,MZ) + FLf ]
(C.25)
with
FLl
=
 1

8sin3qWcos(qW)
l2(s,MW) -  3cos(qW)

4sin3qW
l3(s,MW)
FLu
=
-
1-  2

3
sin2qW

8sin3qWcos(qW)
l2(s,MW) -  3cos(qW)

4sin3qW
l3(s,MW)
FLd
=
1-  4

3
sin2qW

8sin3qWcos(qW)
l2(s,MW) -  3cos(qW)

4sin3qW
l3(s,MW)
(C.26)
and the weak form factors for the electromagnetic vertices are of the form,
FVgf
=
 a

4p
[Qf (vf2 +af2 ) l2(s,MZ) + GLf ]
FAgf
=
 a

4p
[Qf 2vf af l2(s,MZ) + GLf ]
(C.27)
with
GLl
=
-  3

4sin2qW
l3(s,MW)
GLu
=
-  1

12sin2qW
l3(s,MW) +  3

4sin2qW
l3(s,MW)
GLd
=
 1

6sin2qW
l3(s,MW) +  3

4sin2qW
l3(s,MW) .
(C.28)
The lengthy expressions for the functions l2, l3, FLb, and FLb are not listed here but referred to for the readers information  [100] [104]. The infrared divergence are cancelled when the virtual QED corrections are combined with the corresponding real photon corrections. Since FQED without real bremsstrahlung is physically meaningless, it is treated in the more specific discussion of the various measurable quantities and skipped here.

The values for the leptonic and hadronic form factors for Ös =MZ2 are listed in Table C.1 along with the Born coupling constants ve, ae. In addition to the contributions from the 2-point functions, the effective coupling constants near the Z peak are determined by
vf + Re( FVZf (MZ2) )      af + Re( FAZf (MZ2) )
(C.29)
These effective coupling constants allow an easy estimate of the quantitative effects in various measurable quantities. In general, the vertex corrections contribute a correction to the width and cross-section of the Z0from O(1%) to 4% (in the b case). Table C.2 lists the effects of the vertex corrections on the Born cross-section for the processes dG/G(Z®e+e-) and dG/G(Z®b[`(b)]).


mt FVZe(MZ2) FAZe(MZ2) vl al
(GeV) l l
50 0.0019 0.0018 -0.0647 -0.6005
100 0.0020 0.0019 -0.0778 -0.6056
150 0.0021 0.0020 -0.0927 -0.6115
200 0.0021 0.0020 -0.1100 -0.6191
250 0.0022 0.0022 -0.1244 -0.6247
Table C.1: Leptonic and Hadronic Weak Form Factors
Here MZ =93 GeV and MH = 100 GeV.


mt dG/G(Z®e+e-) dG/G(Z®b[`(b)])
(GeV) % %
50 -0.67 -0.70
100 -0.69 -1.01
150 -0.72 -1.81
200 -0.75 -2.95
250 -0.78 -3.80
Table C.2: Effects of Vertex Corrections
Here MZ =93 GeV and MH = 100 GeV.


Box Corrections

The electroweak box diagrams include the two gauge boson diagrams as well as the QED box diagrams. The contribution of the QED boxes is smaller than that of the gauge boson boxes due to the cancellations between real and virtual photon contributions to the phase space. The weak box diagrams consist of the Z0Z0 and W±W± exchange diagrams
Graphic: images/zwexchng.gif

with contributions to the weak amplitude typically of the from
=
e2  JNC,CC(e) ·JNC,CC(f)

s
·  a

2p
[ I(s,t,MZ) -,+ ±I(s,u,MZ) ]
e2  JNC,CC(e)5 ·JNC,CC(f)5

s
·  a

2p
[ +,- ±I5 (s,t,MZ) + I5(s,u,MZ) ]
(C.30)
where
JNC(e,f)
=

v
 

e,f 
gm (ve,f2 +ae,f2 -2ve,f ae,f g5 ) ue,f
JNC(e,f)5
=

v
 

e 
gmg5 (ve,f2 +ae,f-2ve,f ae,f g5 ) ue,f
JCC(e,f)
=
 1

4sin2qW

v
 

e,f 
gm(1-g5 ) ue,f
(C.31)
The contribution of the gauge boson box diagrams near the Z0 peak is of the order the a/p to the photon exchange amplitude. The contribution to the differential cross-section at Ös = MZ2 is smaller than 0.02%. This is because these box diagrams are non-resonant and their contribution to the Z0 cross-section is suppressed by the large resonance factor.

Improved Born Approximation

As an example of the implementation of radiative effects in the Standard Model, the cumulative effects of the QED, Weak, and QCD radiative corrections are presented for the general process e+e-® Z0® f[`(f)]. The approach requires correcting the Born approximation for the process by including effective values of parameters defining the coupling strengths and normalizations. It is sufficient to include the leading light fermion and heavy top contributions along with the structure suggested from the consideration of higher orders in the leading terms. The contributions from the propagators, vertices and boxes are incorporated through the coupling strengths defined in terms of the original Born parameters as follows,
 e2

s
®
 e2(s)

s
a
®
a(MZ2) =  a

1-Da
= 1.064a
MZGZ0
®
 s

MZ2
·MZGZ
sin2qW
®
sin2

q
 

W 
   (in J(e) and J(f)) =  1

2
æ
ç
è
1-   æ
Ö

1-  4A

rMZ2 (1-Da)
 
ö
÷
ø
(C.32)
where the r parameter serves as the normalization of the Z0 amplitude and is given by
r
=
 1

1-Dr
    Dr = 3  Gmmt2

8p2Ö2
(C.33)
and the effective mixing angle parameter, A, is
A
=
 pa

Ö2GF
º (37.2802±0.0003 GeV)2
(C.34)
Using these effective parameters, the improved Born invariant amplitude for e+e-® Z0® f[`(f)] near the Z0 resonance is given by

M
 

Born 
=
Qe Qf  4pa(MZ2)

s
Jem(e) ·Jem(f) +Ö2GmMZ2r

J
 
(e)
em 
·

J
 
(f)
em 

s-MZ2+i  s

MZ2
MZGZ
(C.35)
where the matrix elements of the electromagnetic current are
Jem(e) =

v
 

e 
gmue and Jem(f) =

u
 

f 
gmvf
(C.36)
or redefined in terms of the effective parameters as
Jefff
=
( Ö2GmMZ2rf)[ 1/2]

f
 
gm[I3f (1-g5 ) -2Qf sin2qf] f
(C.37)
The total Z0 width obtained by including the radiative corrections is given by
GZ
=

å
f 
GZ(Z®f

f
 
)
=
NfC  MZ

12p
Ö2GFMZ2r
Ö
 

1-4mf
 
é
ë
(If3-2Qfsin2
-
q
 

W 
)2(1+2mf) + (1-4mf) ù
û
(C.38)
The improved Born approximation yields values which agree with experimental results to within 1%, except for the G(Z0® b[`(b)]). In the case of G(Z0® b[`(b)]), non-leading terms in the vertex corrections, which are numerically more significant than in the self-energies, give rise to the deviations from the correct results. Notice that the improved Born approximation does not contain any information about the Higgs mass.

More involved treatment of G(Z0® b[`(b)]) as well as other processes with similar maladies yield closer agreement to experimental results. In the case of the G(Z0® b[`(b)]), Additional corrections from the vertex corrections for the G(Z0® b[`(b)]) involving the top quark leads to the modification of the improved Born approximation parameters r®rb and k® kb where
r
®
r æ
è
1-  4

3
Dr ö
ø
º rb
sin2

q
 

W 
®
sin2

q
 

W 
æ
è
1+  2

3
Dr ö
ø
º sin2

q
 

W 
·kb .
(C.39)
The single Z0b[`(b)] vertex in the Born amplitude is renormalized by replacing r with
r
®

Ö
 

rrb
 
(C.40)
With this parameterization, G(Z0® b[`(b)]) is determined to be 362 MeV, which agrees with the complete order calculations to within 1% citebib:omicronalphares.


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