Standard Model precision measurements Misure di precisione del modello standard
Lesson 1: Measurements at Z pole
Stefano Lacaprara
INFN Padova
Dottorato di ricerca in fisica
Universit` a di Padova, Dipartimento di Fisica e Astronomia Padova, 5 March 2019
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 1/56
Outline
1 Introduction
2 Z-pole observables
3 Asymmetries
4 W mass and width
5 Top mass
6 Higgs mass and features
7 Global ElectroWeak fit
Introduction I
Stefano Lacaprara
I email: Stefano.Lacaprara@pd.infn.it
I tel: 049 9677100
I studio: st 137, Physics Dept. main building, 1 st floor SM precision measurements 5 lessons, ×2 hours each ; G.Simi will follow covering flavour physics (5x2h)
A.Palano (Bari) will follow covering new exotic states (tetra-penta quark) and Dalitz plot analysis methods in b-physics (6h)
All the slides available on moodle at
https://elearning.unipd.it/dfa/course/view.php?id=756
I All of you are subscribed to the course on moodle.
We will also record the class and put the registraton on moodle.
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 3/56
Introduction II
Final test: mandatory as per PhD school rules.
A short seminar ( ≈ 20 0 ) on one of the topics covered during the course, including discussion with us about topics related to the presentation and the course in general.
I a list of possible topics will be provided, also topic suggest by students are fine (check with us in advance)
I the topic should not be the main theme of your PhD work.
Where to start?
“Begin at the beginning and go on till you come to the end; then stop.” L.Carrol
Starting from the end, instead: Global SM fit, aka the success of SM.
Fit vs indirect vs meas :
3
− −
2−
1 0 1 2 3 tot O) /σ
−
indirect (O2) Z s(M α
2) Z (5)(M αhad
∆ mt
b R0 c R0 0,b AFB
0,c AFB
Ab Ac (Tevt.) lept Θeff sin2
FB) lept(Q Θeff sin2
(SLD) Al
(LEP) Al
0,l AFB
lep R0
0 had σ
ΓZ MZ ΓW MW MH
Global EW fit Indirect determination Measurement G
fitter
SMMar ’18
Pulls:
3
− −2 −1 0 1 2 3
σ
meas meas) / O−
(Ofit 2) (MZ αs2) (MZ (5) αhad
∆ mt
b R0
c R0 Ab Ac 0,b AFB
0,c AFB (Tevt.) lept eff 2Θ sin
FB) lept(Q Θeff sin2
(SLD) Al
(LEP) Al
0,l AFB
lep R0
0 had σ
ΓZ MZ ΓW MW MH
1.3 -0.2 0.5 -0.7 0.0 0.6 0.0 2.4 0.8 0.1 -0.7 -2.1 0.1 -0.9 -1.0 -1.5 -0.2 0.3 0.1 -1.5 G
fitter
SM 0.0Mar ’18
Higgs mass prediction and measurement
60 70 80 90 100 110 120 130 140
[GeV]
MH 0
0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 2χ∆
σ 1
σ 2 SM fit
measurement SM fit w/o MH
LHC combination [PRL 114, 191803 (2015)]
G fitter
SMMar ’18
Will cover (some) of the experimental aspect of SM precision measurements
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 5/56
Input to global EWK fit
(in parenthesis the order followed in these lessons)
3
− − 2 − 1 0 1 2 3
tot
O) / σ
−
indirect
(O
2) (MZ
α
s2) (MZ (5)
α
had∆
mtb R0 c R0 0,b AFB
0,c AFB
Ab Ac (Tevt.) lept
Θ
eff sin2) FB lept(Q
Θ
eff sin2(SLD) Al
(LEP) Al
0,l AFB
lep R0
0
σ
hadΓ
Z MZΓ
W MW MHGlobal EW fit Indirect determination Measurement
G fitter
SMMar ’18
Higgs mass (5)
I LHC
W mass and width (3)
I LEP2, Tevatron, LHC Z-pole observables (1,2)
I LEP1, SLD
I M Z , Γ Z I σ had 0
I sin 2 θ lept eff (2)
I Asymmetries (2)
I BR R lep,b,c 0 = Γ had /Γ ``,b ¯ b,c ¯ c top mass (4)
I Tevatron, LHC other:
I α s (M Z 2 ), ∆α had (M Z 2 )
Input to global EWK fit
(in parenthesis the order followed in these lessons)
Higgs mass (5)
I LHC
W mass and width (3)
I LEP2, Tevatron, LHC Z-pole observables (1,2)
I LEP1, SLD
I M Z , Γ Z I σ had 0
I sin 2 θ lept eff (2)
I Asymmetries (2)
I BR R lep,b,c 0 = Γ had /Γ ``,b ¯ b,c ¯ c top mass (4)
I Tevatron, LHC
other:
I α s (M Z 2 ), ∆α had (M Z 2 )
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 6/56
Outline
1 Introduction
2 Z-pole observables Standard Model Z lineshape
3 Asymmetries
4 W mass and width
5 Top mass
6 Higgs mass and features
7 Stefano Lacaprara (INFN Padova) Global ElectroWeak fit Fit SM Padova 5/03/2019 7/56
Standard model lagrangian
− 1 2
∂
νg
aµ∂
νg
µa− g
sf
abc∂
µg
aνg
µbg
νc− 1 4
g
s2f
abcf
adeg
µbg
νcg
µdg
νe+ 1 2
ig
s2( ¯ q
σiγ
µq
σj)g
µa+ ¯ G
a∂
2G
a+ g
sf
abc∂
µG ¯
aG
bg
µc− ∂
νW
µ+∂
νW
µ−− M
2W
µ+W
µ−− 1 2
∂
νZ
µ0∂
νZ
µ0− 1 2c
w2M
2Z
µ0Z
µ0−
1
2 ∂
µA
ν∂
µA
ν− 1
2 ∂
µH∂
µH − 1
2 m
2hH
2− ∂
µφ
+∂
µφ
−− M
2φ
+φ
−− 1
2 ∂
µφ
0∂
µφ
0− 1
2c
w2Mφ
0φ
0− β
h[ 2M
2g
2+ 2M
g H + 1
2 (H
2+ φ
0φ
0+ 2φ
+φ
−)] + 2M
4g
2α
h− igc
w[∂
νZ
µ0(W
µ+W
ν−− W
ν+W
µ−) − Z
ν0(W
µ+∂
νW
µ−− W
µ−∂
νW
µ+) + Z
µ0(W
ν+∂
νW
µ−− W
ν−∂
νW
µ+)] − igs
w[∂
νA
µ(W
µ+W
ν−− W
ν+W
µ−) − A
ν(W
µ+∂
νW
µ−− W
µ−∂
νW
µ+) + A
µ(W
ν+∂
νW
µ−− W
ν−∂
νW
µ+)] − 1
2 g
2W
µ+W
µ−W
ν+W
ν−+ 1
2 g
2W
µ+W
ν−W
µ+W
ν−+ g
2c
w2(Z
µ0W
µ+Z
ν0W
ν−− Z
µ0Z
µ0W
ν+W
ν−) + g
2s
2w(A
µW
µ+A
νW
ν−− A
µA
µW
ν+W
ν−) + g
2s
wc
w[A
µZ
ν0(W
µ+W
ν−− W
ν+W
µ−) − 2A
µZ
µ0W
ν+W
ν−] − g α[H
3+ Hφ
0φ
0+ 2Hφ
+φ
−] − 1
8 g
2α
h[H
4+ (φ
0)
4+ 4(φ
+φ
−)
2+ 4(φ
0)
2φ
+φ
−+ 4H
2φ
+φ
−+ 2(φ
0)
2H
2] − gMW
µ+W
µ−H − 1 2 g M
c
2wZ
µ0Z
µ0H − 1
2 ig [W
µ+(φ
0∂
µφ
−− φ
−∂
µφ
0) −
W
µ−(φ
0∂
µφ
+− φ
+∂
µφ
0)] + 1 2
g [W
µ+(H∂
µφ
−− φ
−∂
µH) − W
µ−(H∂
µφ
+− φ
+∂
µH)] + 1 2
g 1 c
w(Z
0µ(H∂
µφ
0− φ
0∂
µH) − ig s
2wc
wMZ
µ0(W
µ+φ
−− W
µ−φ
+) + igs
wMA
µ(W
µ+φ
−− W
µ−φ
+) −
ig 1 − 2c
2w2c
wZ
0µ(φ
+∂
µφ
−− φ
−∂
µφ
+) + igs
wA
µ(φ
+∂
µφ
−− φ
−∂
µφ
+) − 1
4 g
2W
µ+W
µ−[H
2+ (φ
0)
2+ 2φ
+φ
−] − 1 4 g
21
c
2wZ
µ0Z
0µ[H
2+ (φ
0)
2+ 2(2s
w2− 1)
2φ
+φ
−] − 1 2 g
2s
w2c
wZ
µ0φ
0(W
µ+φ
−+
W
µ−φ
+) − 1 2 ig
2s
w2c
wZ
µ0H(W
µ+φ
−− W
µ−φ
+) + 1
2 g
2s
wA
µφ
0(W
µ+φ
−+ W
µ−φ
+) + 1
2 ig
2s
wA
µH(W
µ+φ
−− W
µ−φ
+) − g
2s
wc
w(2c
2w− 1)Z
µ0A
µφ
+φ
−− g
1s
w2A
µA
µφ
+φ
−− ¯ e
λ(γ∂ + m
λe)e
λ−
¯
ν
λγ∂ν
λ− ¯ u
jλ(γ∂ + m
λu)u
jλ− ¯ d
jλ(γ∂ + m
λd)d
λj+ igs
wA
µ[−(¯ e
λγ
µe
λ) + 2
3 ( ¯ u
λjγ
µu
λj) − 1
3 ( ¯ d
jλγ
µd
jλ)] + ig 4c
wZ
µ0[( ¯ ν
λγ
µ(1 + γ
5)ν
λ) + (¯ e
λγ
µ(4s
2w− 1 − γ
5)e
λ) + ( ¯ u
λjγ
µ( 4 3 s
2w− 1 − γ
5)u
jλ) + ( ¯ d
jλγ
µ(1 − 8
3 s
2w− γ
5)d
jλ)] + ig 2 √
2 W
µ+[( ¯ ν
λγ
µ(1 + γ
5)e
λ) + ( ¯ u
λjγ
µ(1 + γ
5)C
λκd
jκ)] + ig 2 √
2 W
µ−[(¯ e
λγ
µ(1 + γ
5)ν
λ) + ( ¯ d
κjC
λκ†γ
µ(1 + γ
5)u
λj)] + ig 2 √ 2
m
λeM [−φ
+( ¯ ν
λ(1 − γ
5)e
λ) + φ
−(¯ e
λ(1 + γ
5)ν
λ)] − g
2 m
λeM
[H(¯ e
λe
λ) + i φ
0(¯ e
λγ
5e
λ)] + ig 2M √
2
φ
+[−m
κd( ¯ u
λjC
λκ(1 − γ
5)d
jκ) + m
λu( ¯ u
jλC
λκ(1 + γ
5)d
jκ] + ig 2M √
2
φ
−[m
λd( ¯ d
jλC
λκ†(1 + γ
5)u
κj) − m
κu( ¯ d
λjC
λκ†(1 −
γ
5)u
κj] − g 2
m
λuM H( ¯ u
λju
λj) − g
2 m
λdM H( ¯ d
λjd
jλ) + ig 2
m
λuM φ
0( ¯ u
λjγ
5u
λj) − ig 2
m
dλM φ
0( ¯ d
λjγ
5d
λj) + ¯ X
+(∂
2− M
2)X
++ ¯ X
−(∂
2− M
2)X
−+ ¯ X
0(∂
2− M
2c
2w)X
0+ ¯ Y ∂
2Y + igc
wW
µ+(∂
µX ¯
0X
−−
∂
µX ¯
+X
0) + igs
wW
µ+(∂
µY X ¯
−− ∂
µX ¯
+Y ) + igc
wW
µ−(∂
µX ¯
−X
0− ∂
µX ¯
0X
+) + igs
wW
µ−(∂
µX ¯
−Y − ∂
µY X ¯
+) + igc
wZ
0µ(∂
µX ¯
+X
+− ∂
µX ¯
−X
−) + igs
wA
µ(∂
µX ¯
+X
+− ∂
µX ¯
−X
−) − 1
2
gM[ ¯ X
+X
+H + ¯ X
−X
−H + 1 c
w2X ¯
0X
0H] + 1 − 2c
w22c
wigM[ ¯ X
+X
0φ
+− ¯ X
−X
0φ
−] + 1 2c
wigM[ ¯ X
0X
−φ
+− ¯ X
0X
+φ
−] + igMs
w[ ¯ X
0X
−φ
+− ¯ X
0X
+φ
−] + 1 2
igM[ ¯ X
+X
+φ
0− ¯ X
−X
−φ
0]
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 8/56
Standard model lagrangian
− 1
2 ∂
νg
µa∂
νg
µa− g
sf
abc∂
µg
νag
µbg
νc− 1
4 g
s2f
abcf
adeg
µbg
νcg
dµg
eν+ 1
2 ig
s2( ¯ q
σiγ
µq
jσ)g
aµ+ ¯ G
a∂
2G
a+ g
sf
abc∂
µG ¯
aG
bg
µc− ∂
νW
µ+∂
νW
µ−− M
2W
µ+W
µ−− 1
2 ∂
νZ
µ0∂
νZ
0µ− 1 2c
2wM
2Z
µ0Z
µ0− 1
2 ∂
µA
ν∂
µA
ν− 1 2 ∂
µH∂
µH − 1
2 m
2hH
2− ∂
µφ
+∂
µφ
−− M
2φ
+φ
−− 1
2 ∂
µφ
0∂
µφ
0− 1
2c
w2Mφ
0φ
0− β
h[ 2M
2g
2+ 2M
g H + 1
2 (H
2+ φ
0φ
0+ 2φ
+φ
−)] + 2M
4g
2α
h− igc
w[∂
νZ
0µ(W
µ+W
ν−− W
ν+W
µ−) − Z
ν0(W
µ+∂
νW
µ−− W
µ−∂
νW
µ+) + Z
0µ(W
ν+∂
νW
µ−− W
ν−∂
νW
µ+)] − igs
w[∂
νA
µ(W
µ+W
ν−− W
ν+W
µ−) − A
ν(W
µ+∂
νW
µ−− W
µ−∂
νW
µ+) + A
µ(W
ν+∂
νW
µ−− W
ν−∂
νW
µ+)] − 1
2 g
2W
µ+W
µ−W
ν+W
ν−+ 1
2 g
2W
µ+W
ν−W
µ+W
ν−+ g
2c
w2(Z
µ0W
µ+Z
ν0W
ν−− Z
µ0Z
µ0W
ν+W
ν−) + g
2s
w2(A
µW
µ+A
νW
ν−− A
µA
µW
ν+W
ν−) + g
2s
wc
w[A
µZ
ν0(W
µ+W
ν−− W
ν+W
µ−) − 2A
µZ
µ0W
ν+W
ν−] − g α[H
3+ Hφ
0φ
0+ 2Hφ
+φ
−] − 1
8 g
2α
h[H
4+ (φ
0)
4+ 4(φ
+φ
−)
2+ 4(φ
0)
2φ
+φ
−+ 4H
2φ
+φ
−+ 2(φ
0)
2H
2] − gMW
µ+W
µ−H − 1 2 g M
c
2wZ
µ0Z
0µH − 1
2 ig [W
µ+(φ
0∂
µφ
−− φ
−∂
µφ
0) −
W
µ−(φ
0∂
µφ
+− φ
+∂
µφ
0)] + 1
2 g [W
µ+(H∂
µφ
−− φ
−∂
µH) − W
µ−(H∂
µφ
+− φ
+∂
µH)] + 1 2 g 1
c
w(Z
µ0(H∂
µφ
0− φ
0∂
µH) − ig s
w2c
wMZ
µ0(W
µ+φ
−− W
µ−φ
+) + igs
wMA
µ(W
µ+φ
−− W
µ−φ
+) −
ig 1 − 2c
w22c
wZ
µ0(φ
+∂
µφ
−− φ
−∂
µφ
+) + igs
wA
µ(φ
+∂
µφ
−− φ
−∂
µφ
+) − 1
4 g
2W
µ+W
µ−[H
2+ (φ
0)
2+ 2φ
+φ
−] − 1 4 g
21
c
w2Z
0µZ
µ0[H
2+ (φ
0)
2+ 2(2s
2w− 1)
2φ
+φ
−] − 1 2 g
2s
w2c
wZ
0µφ
0(W
µ+φ
−+
W
µ−φ
+) − 1 2 ig
2s
2wc
wZ
µ0H(W
µ+φ
−− W
µ−φ
+) + 1
2 g
2s
wA
µφ
0(W
µ+φ
−+ W
µ−φ
+) + 1
2 ig
2s
wA
µH(W
µ+φ
−− W
µ−φ
+) − g
2s
wc
w(2c
w2− 1)Z
µ0A
µφ
+φ
−− g
1s
w2A
µA
µφ
+φ
−− ¯ e
λ(γ∂ + m
λe)e
λ−
¯
ν
λγ∂ν
λ− ¯ u
λj(γ∂ + m
λu)u
jλ− ¯ d
jλ(γ∂ + m
λd)d
jλ+ igs
wA
µ[−(¯ e
λγ
µe
λ) + 2
3 ( ¯ u
λjγ
µu
λj) − 1
3 ( ¯ d
jλγ
µd
jλ)] + ig 4c
wZ
µ0[( ¯ ν
λγ
µ(1 + γ
5)ν
λ) + (¯ e
λγ
µ(4s
w2− 1 − γ
5)e
λ) + ( ¯ u
λjγ
µ( 4 3 s
w2− 1 −
γ
5)u
λj) + ( ¯ d
λjγ
µ(1 − 8
3 s
2w− γ
5)d
jλ)] + ig 2 √
2 W
µ+[( ¯ ν
λγ
µ(1 + γ
5)e
λ) + ( ¯ u
λjγ
µ(1 + γ
5)C
λκd
jκ)] + ig 2 √
2 W
µ−[(¯ e
λγ
µ(1 + γ
5)ν
λ) + ( ¯ d
jκC
λκ†γ
µ(1 + γ
5)u
λj)] + ig 2 √ 2
m
λeM [−φ
+( ¯ ν
λ(1 −
γ
5)e
λ) + φ
−(¯ e
λ(1 + γ
5)ν
λ)] − g 2
m
λeM [H(¯ e
λe
λ) + i φ
0(¯ e
λγ
5e
λ)] + ig 2M √
2 φ
+[−m
κd( ¯ u
jλC
λκ(1 − γ
5)d
jκ) + m
uλ( ¯ u
jλC
λκ(1 + γ
5)d
jκ] + ig 2M √
2 φ
−[m
λd( ¯ d
jλC
λκ†(1 + γ
5)u
jκ) − m
uκ( ¯ d
jλC
λκ†(1 −
γ
5)u
κj] − g 2
m
λuM H( ¯ u
λju
jλ) − g
2 m
dλM H( ¯ d
jλd
jλ) + ig 2
m
λuM φ
0( ¯ u
jλγ
5u
λj) − ig 2
m
λdM φ
0( ¯ d
λjγ
5d
jλ) + ¯ X
+(∂
2− M
2)X
++ ¯ X
−(∂
2− M
2)X
−+ ¯ X
0(∂
2− M
2c
2w)X
0+ ¯ Y ∂
2Y + igc
wW
µ+(∂
µX ¯
0X
−−
∂
µX ¯
+X
0) + igs
wW
µ+(∂
µY X ¯
−− ∂
µX ¯
+Y ) + igc
wW
µ−(∂
µX ¯
−X
0− ∂
µX ¯
0X
+) + igs
wW
µ−(∂
µX ¯
−Y − ∂
µY X ¯
+) + igc
wZ
µ0(∂
µX ¯
+X
+− ∂
µX ¯
−X
−) + igs
wA
µ(∂
µX ¯
+X
+− ∂
µX ¯
−X
−) − 1
2 gM[ ¯ X
+X
+H + ¯ X
−X
−H + 1 c
w2X ¯
0X
0H] + 1 − 2c
2w2c
wigM[ ¯ X
+X
0φ
+− ¯ X
−X
0φ
−] + 1 2c
wigM[ ¯ X
0X
−φ
+− ¯ X
0X
+φ
−] + igMs
w[ ¯ X
0X
−φ
+− ¯ X
0X
+φ
−] + 1
2 igM[ ¯ X
+X
+φ
0− ¯ X
−X
−φ
0]
Just kidding
latex from T.Gutierrez, who also noted a sign error somewhere
Standard model lagrangian [1]
L = − 1
4 W µν · W µν − 1
4 B µν B µν
W ± , Z, γ kinetic energies and self-interactions
+¯ Lγ µ
i ∂ µ − g 1
2 τ · W µ − g 0 Y 2 B µ
L + ¯ Rγ µ
i ∂ µ − g 0 Y 2 B µ
R
lepton and quark kinetic energies and interactions with W ± , Z, γ
+
i ∂ µ − g 1
2 τ · W µ − g 0 Y 2 B µ
φ
2
− V (φ)
W ± , Z, γ, and Higgs masses and couplings
−G i (¯ LφR + ¯ Rφ ∗† L).
lepton and quark masses and coupling to Higgs
gauge fermions Higgs Yukawa
(flavour physics in L and R via CKM (q) and PMNS ν in fermions part)
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 9/56
SM free parameters
masses after spontaneous symmetry breaking:
Free parameters: g , g 0 , V (φ) = aφ 2 + bφ 4 , G i higgs boson
I ν = r −a
2b minimum of Higgs potential (vacuum expectation value)
I m H = 2 √ a vector bosons
I A µ = g 0 W µ 3 + gB µ
p g 2 + g 02 , m A = 0;
I W µ ± = W µ 1 ∓ W µ 2
√ 2 , m W = νg 2 ;
I Z µ = gW µ 3 − g 0 B µ
p g 2 + g 02 , m Z = ν p g 2 + g 02
2 ;
fermions (excluding ν 0 s)
I m fermions = G i ν
√ 2
Free parameters and boson masses
Excluding the fermion and Higgs masses
g , g 0 , ν OR
electron charge e = gg 0
p g 2 + g 02 Millikan experiment Weinberg angle sin θ W = g 0
p g 2 + g 02 pν, p ¯ ν scattering or σ(e pol − d ) asymmetry Fermi constant G F = 1
ν 2 √
2 µ lifetime
Notable SM relations M W 2 = e 2
4G F
√ 2 sin 2 θ W
= πα
√ 2G F sin 2 θ W
M Z = M W
cos θ W
ρ 0 = M W 2 M Z 2 cos 2 θ W
= 1 Depends only on Higgs sector
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 11/56
W and Z discovery
Well before LEP
sin θ W = 0.23 ± 10%, α = 1/137.035 . . ., G F = 1.16639(1) · 10 −5 GeV −2 o Prediction: M W = 82 ± 6 GeV and M Z = 92 ± 5 GeV
Need a new collider: build Sp ¯ pS and discover W and Z: UA1[2, 3]/UA2[4, 5]
Fermions-vector bosons couplings
γ
ff
f¯
−ieQ f γ µ
Zf
f¯
−i g cos θ W γ µ 1
2
c V f − c A f γ 5
W f
f¯′
−i g
√ 2 γ µ 1
2 1 − γ 5 Where Q, c V f =
T (3) − 2Q sin 2 θ W
, and c A f = T (3) depends on fermion type:
fermion Q f T (3) c A f c V f
(ν e , ν µ , ν τ ) L 0 1/2 1/2 1/2 = 0.50 (e, µ, τ ) L -1 -1/2 -1/2 −1/2 + 2 sin 2 θ W = 0.03 (e, µ, τ ) R -1 0 0 +2 sin 2 θ W = 0.47 (u, c, t) L 2/3 1/2 1/2 1/2 + 4/3 sin 2 θ W = 0.19 (u, c, t) R 2/3 0 0 4/3 sin 2 θ W = 0.31 (d , s, b) L -1/3 -1/2 -1/2 −1/2 + 2/3 sin 2 θ W = 0.34 (d , s, b) R -1/3 0 0 2/3 sin 2 θ W = 0.16
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 13/56
Radiative corrections
Correction to propagator
Vertex corrections
Are absorbed using effective (complex) coupling g V /Af and θ W eff
sin 2 θ W eff = (1 + ∆κ f ) sin 2 θ W
g Vf = p
(1 + ∆ρ f ) T 3 − 2Q sin 2 θ W eff g Af = p
(1 + ∆ρ f ) T 3
∆ρ = 3G F M W 2 8 √
2π 2
M t 2
M W 2 − tan 2 θ W
ln M H 2
M W 2 − 5 6
+ . . .
∆κ = 3G F M W 2 8 √
2π 2
cotan 2 θ W
M t 2 M W 2 − 10
9
ln M H 2
M W 2 − 5 6
+ . . . (extra M f 2
M W 2 for f = b)
Strong dependence on M top , weak on M H , small dependence to flavour, with exception to b quarks
Radiative corrections (II)
Changes to SM relation due to radiative corrections (a different way to write the notable SM relations) cos 2 θ eff (f ) sin 2 θ (f ) eff = πα(0)
√ 2M Z 2 G F
1 1 − ∆r (f ) where:
∆r (f ) = ∆α + ∆r w (f ) and ∆α(s) = ∆α eµτ (s) + ∆α top (s) + ∆α (5) had (s) As before, absorb radiative correction using running α(s) = α(0)
1 − ∆α(s) α(q 2 = 0) = 1/137.035 999 76(50) → α(M Z 2 ) = 1/128.945
∆r w (f ) is weak correction, flavour dependent ∆r w (f ) = −∆ρ + . . . ρ = 1 + ∆ρ
And now the experimental part. . . mostly from [6]
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 15/56
Cross sections for Z and W boson production
CLEO@CESR [7]
I Cornell
DORIS@DESY [8](Υ) PETRA@DESY[9](gluon), BABAR@PEP-II [10], BELLE@KEKB [11], TOPAZ@TRISTAN [12]
I discovery of α em ( √ s)
I KEK
SLD@SLC
I Stanford
LEP and LEP II
Tristan today at KEK
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 17/56
cos θ is the angle between e − and µ − On resonance √
s = M Z : γ/Z vanish ( ∼ 0.2% at √
s = M Z ± 3GeV ), γ ∼ 1%, Z dominates
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 18/56
cos θ is the angle between e − and µ − (1 + cos 2 θ) terms contribute to σ tot
(cos θ) terms introduce asymmetries forward-backward
if e + e − → q ¯ q: cos θ difficult to know (q vs ¯ q harder than ` vs ¯ `) Additional color term ×N c
and QCD final state radiative correction ×(1 + δ QCD ), see later
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 18/56
Cross section for e + e − → e + e −
At tree level, two diagrams:
e
−e
−e
−e
−e
+e
+e
+e
+γ/Z γ/Z
t − channel s− channel
s-channel
I same as e + e − → f ¯ f ;
I dominates at large angle;
t-channel
I Bhabha scattering a
I largely dominates at small scattering angle
F σ ≈ 1/θ 3 : close to colliding e − beam
I very well known QED process;
I Used to measure LEP luminosity with large angle luminometer
a Bhabha Homi Jehangir, indian theoretical phys. (Bombay 1909 - m. Bianco 1966)
ISR/FSR
ISR
Emission of γ from initial state. Important effect (radiative return to Z peak).
σ(s) = Z 1
0
dz · H QED tot (z, s) · σ ew (zs) FSR
both QED and QCD (only for quarks) change partial and total width
Γ h = Σ f Γ f 0 (1 + δ f QED )(1 + δ f QCD ) δ f QED ≈ 3αQ f 2
4π ∼ 0.17%, δ f QCD ≈ α s (M Z 2 )
π ∼ 3.8%
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 20/56
ISR impact on Z line-shape
Note the huge importance of ISR radiative (QED) corrections!
Decrease σ by 30% and shift peak position by ∼ 100 MeV
σ tot had is measured
value reported and used for electroweak fit, is σ had 0 , where QED correction are evaluated
pseudo-observable
Same also for R f 0 , Γ 0 Z , A 0 FB , . . .
Measurement at the Z line-shape
Considering only hadronic final states:
σ(s) = 12π Γ e Γ had
M Z 2
s
(s − M z 2 ) 2 + M Z 2 Γ 2 Z (neglecting the –small– γ contribution) At peak: σ 0 = 12π
M Z 2 Γ e Γ had
Γ Z
,
where: Γ had = Σ q6=t Γ q ¯ q and Γ Z = Γ ee + Γ µµ + Γ τ τ + Γ had + Γ inv
We can measure 6+1 parameters:
Z mass M Z from peak position;
Z total width Γ Z from peak width;
hadronic pole cross-section σ 0 from peak height;
Width ratios R 0 ` = R 0 e,µ,τ = Γ had /Γ ee,µµ,τ τ from exclusive peak height;
Width ratios R 0 b = Γ bb /Γ had as above;
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 22/56
Example of Z → ee event: OPAL
Very clean environment
Electron ID via tracks and ECAL clusters: E /p = 1 (B = 0.5T )
Example of Z → qqg ALEPH
Good example of FSR (QCD): slightly more complex events, larger hadron multiplicity, jet reco (E/HCAL) very good tracker B = 1.5T ,
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 24/56
Example of Z → µµ for L3
Even clearer environment: outer tracking detector for µ ID.
L3 had all detectors inside solenoid (0.5T ), excellent ECAL (BGO)
Z → ττ example for DELPHI
τ → 3hν τ three prong, and τ → hν τ one prong decays DELPHI had RICH (PID)
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 26/56
Event selection and classification
Event selection is quite easy thanks to the very clean environment:
E ch (sum of tracks momenta) vs charged multiplicity.
L3 hadron selection
OPAL lepton selection
channel had ee µµ τ τ
efficiency % 99 − 95 98 − 97 98 − 95 70 − 90
background % 0.5 1 1 1 − 3
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 28/56
γγ cross section at LEP
LEP not so clean as one might imagine.
Gamma-Gamma interaction produce a lot of interaction in addition to Z production.
The scattered electrons escape in the beam pipe, undetected.
At Z peak, x-section is ~150nb (vs ~30nb for ee->Z), but it is reduced to ~6nb via pt and
cuts
Statistics collected at LEP
In 1990, 91, 93, and 95 a total of 7 + 20 pb −1 lumi collected off-peak Actual L collected by each
experiment ∼ 10 − 15% less
Number of events ×1 · 10 3
Total per experiment:
4M Z → q ¯ q 0.5M Z → ` + ` −
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 30/56
Cross section measurement
σ tot = (N sel − N bg )
sel L Background and efficiency from MC.
Key issue is luminosity L measurement
e + e − → e + e − via t-channel dominates at low θ.
Collect Bhabha events with very forward calorimenters 25 to 60 mrad from beam.
x-section goes as 1/θ 3 : difficult to define the geometrical acceptance of forward calorimeters.
I common systematic uncert: . 0.05%,
I from theory ∼ 0.05%.
at LHC 2.6%, at BelleII 0.7%
Hadronic cross section vs √ s
Off-peak measurements M Z ± 2 GeV are crucial for Γ Z
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 32/56
Hadronic and leptonic cross-section vs √ s
M Z from peak position
I ee → ee(γ) also t-channel and inteference
Γ Z from peak width in hadronic final state (larger stats)
Width ratios R from exclusive cross-sections.
I σ had ,e,µ,τ 0 ∝ Γ e Γ had ,e,µ,τ
For M Z critical is the determination of √
s for LEP.
LEP √
s: resonant depolarization [13]
Electron with momentum p in uniform vertical magnetic field B
E ∼ p = eBR = e 2π BL B is not uniform, LEP ring not a circle
E beam = e 2π
I
B · d`
Dipole B field is vertical.
Electron spin aligns with B
Sokolov-Ternov theo., patent in ’73!.
Due to spin-B interaction: E > E ↑↓ .
spin flip due to synchrotron radiation, but flip rate is not symmetric.
Pol trans ∝
1 − e −t/τ
, with τ 10h
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 34/56
LEP √
s: resonant depolarization
spin precess in B field, with a ν proportinal to B (Larmor precession)
I number of precessions per turn:
ν s = g e − 2 2
e 2πm e
I
B · d` = g e − 2 2
E beam
m e I ν s is proportional to E Beam
apply an additional, radial B field, oscillating with freq ν
I if ν = ν s , the spin is rotated until it becomes horizontal
I about 10 4 turns (1s) to rotate by 90 deg
I stochastic sync. rad.: horizonal pol is unstable → destroyed.
LEP √
s: resonant depolarization
External freq is: f dep = (k ± [ν]) · f rev
where f rev = 11.25 kHz is that of LEP, k is an integer;
[ν] = ν scan is the non-integer part of the ν of the bending field;
a freq scan is performed, ν scan is moved slowly
then the polarization is measured (Compton scattering), then repeat for different bunches
Process is slow, and can be done only at the end of a fill
precision (limited to ν scan step) is
≈ 100 keV Ultimate LEP √
s resolution ≈ 2.2 MeV.
Why?
At LEP start, exp. σ( √
s) ∼ 10 MeV
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 36/56
Tidal movement of earth at LEP [14]
Tidal movement of earth at LEP [14]
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 37/56
Tidal movement of earth at LEP [14]
Tidal movement of earth at LEP [14]
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 37/56
Tidal movement of earth at LEP [14]
Tidal movement of earth at LEP [14]
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 37/56
Tidal movement of earth at LEP [14]
Tidal movement of earth at LEP [14]
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 37/56
Tidal movement of earth move the dipole magnets.
Typical displacement 1mm (in 27km), giving a 10 MeV peak-to-peak change.
Other ground distortion from Geneva lake level, heavy rain . . .
Vagabond electric currents from trains.
Final M Z syst from √
s about 1.7 MeV
Results
M Z = 91.1875 ± 0.0021 GeV (23ppm)
±1.7 MeV LEP √ s scale
±0.3 MeV QED corr (ISR)
±0.1 MeV fit parametrization
±0.05 MeV L
±0.05 MeV α had
Contribution γ − Z interference
Γ Z = 2.4952 ± 0.0023 GeV
±1.2 MeV from QED corr (ISR)
±0.2 MeV from QED corr (FSR)
±0.1 MeV from fit parametrization
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 39/56
Lepton universality
Partial width: R 0 ` = Γ had /Γ `
R e 0 =20.804 ± 0.050 R µ 0 =20.785 ± 0.033 R τ 0 =20.764 ± 0.045
R τ 0 expected to be smaller due to m τ > m µ m e
Assuming lepton universality:
R ` 0 =20.767 ± 0.25
σ 0 had =41.541 ± 0.037 nb
Number of neutrino families
With lepton universality:
Γ Z =2495.2 ± 2.3 MeV Γ had =1744.4.8 ± 2.0 MeV
Γ ` =83.895 ± 0.086 MeV Γ inv =499.0 ± 1.5 MeV
Γ SM inv = 501.7 ± 0.2 +0.1 −0.9 (m H ) MeV
Γ x inv = −2.7 +1.8 −1.5 MeV N ν = 2.9840 ± 0.0082 δN ν ≈ 10.5 δn had
n had ⊕ 3.0 δn lep
n lep ⊕ 7.5 δ L L
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 41/56
R b,c
It is not possible, in general, to distinguish quark flavour, with the exception of b and c-quarks, using different techniques:
Useing two features: long b (and c) lifetime and exclusive b and c decays.
lifetime tagging;
I cτ for b is ∼ 450µm (in lab ×γ)
I cτ for c is ∼ 150µm (in lab ×γ)
I detect displaced secondary vertex via impact parameter or decay length measurements exclusive decays:
I leptonic decay;
I decay with D mesons;
Correction to R b,c from QCD (gluon radiation from final state quarks), in addition to QED correction
and LEP energy scale.
lifetime tagging
Heavy hadrons have long lifetime and large boost at LEP
Impact Parameter (d 0 ):
I d 0 is the distance of closest approach from the primary vertex of the extrapolated track;
I the resolution depends on the track reconstruction and primay vertex knowledge;
I silicon microvertex close to beam pipe for resolution, PV depends on accelerator (SLC better than LEP);
I a signed quantity wrt the jet dir.
F badly measured track can intercept the “wrong-side” of the beam-spot;
I d 0 sign = d 0 /σ(d 0 );
Decay length (L)
I Signed as well
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 43/56
lifetime tagging
d 0 significance L significance and NN
b ↔ c separation via M vtx
Resolution
δ IP ∼ 16 − 100µm (Rφ/Z ) , δ b ∼ 300µm
b-tagging performance
Lepton tagging
A lepton inside a jet is a stong indication of a b or c flavour.
To distinguish from b to ¯ b use semileptonic decay of b quarks.
b → ` − ; ≈ 10%
c → ` + ; ≈ 13%
b → c → ` + cascade decay ;
Distinguish between direct and cascade decay using lepton p T and p lower purity and efficiency wrt lifetime tagger
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 45/56
D-Meson Tags
Tagging via reconstruction of charmed meson and barions in jet:
direct evidence of a jet originated by an heavy quark.
low B ∼ O(%)
b → c fragmentation is small
distinguish c from b decay by charmed mesons momentum;
I D 0 → K − π +
I D + → K − π + π +
I D s → K + K − π +
I Λ + c → pK − π +
I D ∗+ → π + D 0
F slow π + , no need for PID
R q for b and c
Single-tag (one b/c) or double-tag methods (both sides: allows to extract tag ε from data)
charm R c beauty R b
Dotted line is systematic uncertainties
Contribution from SLD (next lesson): smaller interaction region, better b-tagging, smaller uncertainties
Stefano Lacaprara (INFN Padova) Fit SM Padova 5/03/2019 47/56
Input to global EWK fit
(in parenthesis the order followed in these lessons)
3
− − 2 − 1 0 1 2 3
tot
O) / σ
−
indirect
(O
2) (MZ
α
s2) (MZ (5)
α
had∆
mtb R0 c R0 0,b AFB
0,c AFB
Ab Ac (Tevt.) lept
Θ
eff sin2) FB lept(Q
Θ
eff sin2(SLD) Al
(LEP) Al
0,l AFB
lep R0
0
σ
hadΓ
Z MZΓ
W MW MHGlobal EW fit Indirect determination Measurement
G fitter
SMMar ’18