Electroweak Theory and Higgs Physics Preliminary Version
Transcript of Electroweak Theory and Higgs Physics Preliminary Version
Electroweak Theory
and Higgs Physics
Preliminary Version
Chris QuiggFermilab Theory Group
Fermilab Academic Lectures · 1 – 17 November 2005
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 1bis
A Decade of Discovery Past . . . Electroweak theory → law of nature
[Z, e+e−, pp, νN , (g − 2)µ, . . . ]
Higgs-boson influence observed in the vacuum
[EW experiments]
Neutrino flavor oscillations: νµ → ντ ,νe → νµ/ντ [ν, νatm, reactors]
Understanding QCD
[heavy flavor, Z0, pp, νN , ep, ions, lattice]
Discovery of top quark [pp]
Direct CP violation in K → ππ [fixed-target]
B-meson decays violate CP [e+e− → BB]
Flat universe dominated by dark matter, energy
[SN Ia, CMB, LSS]
Detection of ντ interactions [fixed-target]
Quarks & leptons structureless at TeV scale
[mainly colliders]
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 2bis
A Decade of Discovery Past . . . Electroweak theory → law of nature
[Z, e+e−, pp, νN , (g − 2)µ, . . . ]
Higgs-boson influence observed in the vacuum
[EW experiments]
Neutrino flavor oscillations: νµ → ντ ,νe → νµ/ντ [ν, νatm, reactors]
Understanding QCD
[heavy flavor, Z0, pp, νN , ep, ions, lattice]
Discovery of top quark [pp]
Direct CP violation in K → ππ [fixed-target]
B-meson decays violate CP [e+e− → BB]
Flat universe dominated by dark matter, energy
[SN Ia, CMB, LSS]
Detection of ντ interactions [fixed-target]
Quarks & leptons structureless at TeV scale
[mainly colliders]
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 2bis
Goal: Understanding the Everyday
Why are there atoms?
Why chemistry?
Why stable structures?
What makes life possible?
What would the world be likewithout a (Higgs) mechanism to hideelectroweak symmetry and givemasses to the quarks and leptons?Consider the effects of all theSU(3)c ⊗ SU(2)L ⊗ U(1)Y gaugesymmetries.
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 3bis
Goal: Understanding the Everyday
Why are there atoms?
Why chemistry?
Why stable structures?
What makes life possible?
What would the world be like,without a (Higgs) mechanism to hideelectroweak symmetry and givemasses to the quarks and leptons?Consider the effects of all theSU(3)c ⊗ SU(2)L ⊗ U(1)Y gaugesymmetries.
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 3bis
Searching for the mechanism ofelectroweak symmetry breaking,we seek to understand
why the world is the way it is.
This is one of the deepestquestions humans have everpursued, and
it is coming within the reach ofparticle physics.
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 4bis
Tevatron Collider is running now,
breaking new ground in sensitivity
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 5bis
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 6bis
Tevatron Collider in a Nutshell
980-GeV protons, antiprotons
(2π km)
frequency of revolution ≈ 45 000 s−1
392 ns between crossings
(36 ⊗ 36 bunches)
collision rate = L · σinelastic ≈ 107 s−1
c ≈ 109 km/h; vp ≈ c − 495 km/h
Record Linit = 1.64 × 1032 cm−2 s−1
[CERN ISR: pp, 1.4]
Maximum p at Low β: 1.661 × 1012
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 7bis
The LHC will operate soon, breaking
new ground in energy and sensitivity
30 June 200530 June30 June30 June 200520052005Gigi Rolandi - CERNGigi RolandiGigi RolandiGigi Rolandi - CERN - CERN - CERN
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 8bis
LHC in a nutshell
7-TeV protons on protons (27 km);
vp ≈ c − 10 km/h
Novel two-in-one dipoles (≈ 9 teslas)
Startup: 43 ⊗ 43 → 156 ⊗ 156
bunches, L ≈ 6 × 1031 cm−2 s−1
Early: 936 bunches,
L∼> 5 × 1032 cm−2 s−1 [75 ns]
Next phase: 2808 bunches,
L → 2 × 1033 cm−2 s−1
25 ns bunch spacing
Eventual: L∼> 1034 cm−2 s−1:
100 fb−1/year
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 9bis
Tentative Outline . . .
Preliminaries
Current state of particle physics
A few words about QCD
Sources of mass
Antecedents of the electroweak theory
What led to EW theory
What EW theory needs to explain
Some consequences of the Fermi theory
µ decay
νe scattering
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 10bis
. . . Outline . . .
SU(2)L ⊗ U(1)Y theory
Gauge theories
Spontaneous symmetry breaking
Consequences: W±, Z0/NC, H, mf?
Measuring sin2 θW in νe scattering
GIM / CKM
Phenomena at tree level and beyond
Z0 pole
W mass and width
Atomic parity violation
Vacuum energy problem
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 11bis
. . . Outline
The Higgs boson and the 1-TeV scale
Why the Higgs boson must exist
Higgs properties, constraints
How well can we anticipate MH?
Higgs searches
The problems of mass
The EW scale and beyond
Hierarchy problem
Why is the EW scale so small?
Why is the Planck scale so large?
Outlook
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 12bis
General References
C. Quigg, “Nature’s Greatest Puzzles,”
hep-ph/0502070
C. Quigg, “The Electroweak Theory,”
hep-ph/0204104 (TASI 2000 Lectures)
C. Quigg, Gauge Theories of the Strong, Weak,
and Electromagnetic Interactions
I. J. R. Aitchison & A. J. G. Hey, Gauge Theories
in Particle Physics
R. N. Cahn & G. Goldhaber, Experimental
Foundations of Particle Physics
G. Altarelli & M. Grunewald, “Precision
Electroweak Tests of the SM,” hep-ph/0404165
F. Teubert, “Electroweak Physics,” ICHEP04
S. de Jong, “Tests of the Electroweak Sector of
the Standard Model,” EPS HEPP 2005
Problem sets: http://lutece.fnal.gov/TASI/default.html
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 13bis
Our picture of matter
Pointlike constituents (r < 10−18 m)
(
u
d
)
L
(
c
s
)
L
(
t
b
)
L
(
νe
e−
)
L
(
νµ
µ−
)
L
(
ντ
τ−
)
L
Few fundamental forces, derived from
gauge symmetries
SU(3)c ⊗ SU(2)L ⊗ U(1)Y
Electroweak symmetry breaking
Higgs mechanism?
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 14bis
uL
dL
cL
sL
tL
bL
eL
µL
τLνe
νµ
ντ
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 15bis
uR
dR
cR
sR
tR
bR
eR
µR
τR
uL
dL
cL
sL
tL
bL
eL
µL
τLνe
νµ
ντ
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 16bis
uR
dR
cR
sR
tR
bR
eR
µR
τR
uL
dL
cL
sL
tL
bL
eL
µL
τLνe
νµ
ντ
νe
νµ
ντ
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 16bis
uR
dR
cR
sR
tR
bR
eR
µR
τR
uL
dL
cL
sL
tL
bL
eL
µL
τLν1
ν2
ν3
ν1
ν2
ν3
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 16ter
Elementarity Are quarks and leptons structureless?
Symmetry Electroweak symmetry breaking and the 1-TeV scale
Origin of gauge symmetries
Meaning of discrete symmetries
Unity Coupling constant unification
Unification of quarks and leptons
(neutrality of atoms ⇒ new forces!);
of constituents and force particles
Incorporation of gravity
Identity Fermion masses and mixings; CP violation; ν oscillations
What makes an electron an e and a top quark a t?
Topography What is the fabric of space and time?
. . . the origin of space and time?
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 17bis
Elementarity
The World’s Most Powerful Microscopes
nanonanophysics
CDF dijet event (√
s = 1.96 TeV):
ET = 1.364 TeV
qq → jet + jet
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 18bis
Elementarity
If the Lagrangian has the form ±g2
2Λ2 ψLγµψLψLγµψL (with g2/4π set
equal to 1), then we define Λ ≡ Λ±
LL. For the full definitions and for other
forms, see the Note in the Listings on Searches for Quark and Lepton Compos-iteness in the full Review and the original literature.
Λ+
LL(e e e e) > 8.3 TeV, CL = 95%
Λ−
LL(e e e e) > 10.3 TeV, CL = 95%
Λ+
LL(e eµµ) > 8.5 TeV, CL = 95%
Λ−
LL(e eµµ) > 6.3 TeV, CL = 95%
Λ+
LL(e e τ τ) > 5.4 TeV, CL = 95%
Λ−
LL(e e τ τ) > 6.5 TeV, CL = 95%
Λ+LL
(````) > 9.0 TeV, CL = 95%
Λ−
LL(````) > 7.8 TeV, CL = 95%
Λ+
LL(e e uu) > 23.3 TeV, CL = 95%
Λ−
LL(e e uu) > 12.5 TeV, CL = 95%
Λ+
LL(e e d d) > 11.1 TeV, CL = 95%
Λ−
LL(e e d d) > 26.4 TeV, CL = 95%
Λ+
LL(e e c c) > 1.0 TeV, CL = 95%
Λ−
LL(e e c c) > 2.1 TeV, CL = 95%
Λ+LL
(e e bb) > 5.6 TeV, CL = 95%
Λ−
LL(e e bb) > 4.9 TeV, CL = 95%
Λ+LL
(µµqq) > 2.9 TeV, CL = 95%
Λ−
LL(µµqq) > 4.2 TeV, CL = 95%
Λ(`ν `ν) > 3.10 TeV, CL = 90%Λ(e ν qq) > 2.81 TeV, CL = 95%
Λ+
LL(qqqq) > 2.7 TeV, CL = 95%
Λ−
LL(qqqq) > 2.4 TeV, CL = 95%
Λ+
LL(ν ν qq) > 5.0 TeV, CL = 95%
Λ−
LL(ν ν qq) > 5.4 TeV, CL = 95%
HTTP://PDG.LBL.GOV Page 3 Created: 6/14/2004 20:00
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 19bis
Two views of Symmetry
1. Indistinguishability
One object transformed into another
Familiar (and useful!) from
Global Symmetries: isospin, SU(3)f , . . .
Spacetime Symmetries
Gauge Symmetries
“EQUIVALENCE”
Idealize more perfect worlds, the better
to understand our diverse, changing world
Unbroken unified theory: perfect world of
equivalent forces, interchangeable massless
particles . . .Perfectly boring?
Symmetry ⇔ Disorder
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 20bis
A Perfect World
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 21bis
Two views of Symmetry
2. Unobservable
Goodness of a symmetry means
something cannot be measured
e.g., vanishing asymmetry
Un observable Transformation Conserved
Absolute position ~r → ~r + ~∆ ~p
Absolute time t → t + δ E
Absolute orientation r → r′ ~L
Absolute velocity ~v → ~v + ~w
Absolute right ~r → −~r P
Absolute future t → −t T
Absolute charge Q → −Q C
Absolute phase...
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 22bis
Unity
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 23bis
QCD is part of the standard model
. . . a remarkably simple, successful, and rich theory
Wilczek, hep-ph/9907340
Perturbative QCD
• Exists, thanks to asymptotic freedom
• Describes many phenomena in quantitative
detail:
Q2-evolution of structure functions
Jet production in pp collisions
Many decays, event shapes, . . .
• We can measure the running of αs
(engineering value for unification)
Nonperturbative (lattice) QCD
• Predicts the hadron spectrum
• Gives our best information on quark masses,
etc. El-Khadra & Luke, hep-ph/0208114
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 24bis
F2(x,Q2) in νFe interactions (NuTeV)
0.1
1
1 10 100 1000
F 2(x
,Q2 )
Q2 (GeV/c)2
x=0.015 (X3)
x=0.045 (X1.8)
x=0.080 (X1.3)
x=0.125x=0.175x=0.225
x=0.275
x=0.35
x=0.45
x=0.55
x=0.65
x=0.75NuTeVCCFR
CDHSWNuTeV fit
hep-ex/0509010
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 25bis
F2(x,Q2) in `N interactions (ZEUS)
ZEUS
0
1
2
3
4
5
1 10 102
103
104
105
F2 em
-log
10(x
)
Q2(GeV2)
ZEUS NLO QCD fit
tot. error
ZEUS 96/97
BCDMS
E665
NMC
x=6.32E-5 x=0.000102x=0.000161
x=0.000253
x=0.0004x=0.0005
x=0.000632x=0.0008
x=0.0013
x=0.0021
x=0.0032
x=0.005
x=0.008
x=0.013
x=0.021
x=0.032
x=0.05
x=0.08
x=0.13
x=0.18
x=0.25
x=0.4
x=0.65
ZEUS, hep-ex/0208023.
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 26bis
Inclusive jet cross section at√s = 1.96 TeV (CDF-II)
(GeV/c)Tp0 100 200 300 400 500 600 700
[n
b/(
GeV
/c)]
T
/dyd
pσ2
d
10-8
10-7
10-6
10-5
10-4
10-3
10-2
10-1
1
10
CDF Run II Preliminary
/2)JetT=pµNLO pQCD EKS CTEQ 6.1M, (
=1.3 Sep
=0.75, Rmerge=0.7, fconeMidpoint R0.1<|y|<0.7
-1 L = 385 pb∫
Total systematic uncertainty
Data corrected to parton level
NLO pQCD
CDF Run II Preliminary
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 27bis
Running αs(Q)
Comprehensive survey: W. de Boer, hep-ex/0407021
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 28bis
jets & shapes 161 GeV
jets & shapes 172 GeV
0.08 0.10 0.12 0.14
(((( ))))s Z
-decays [LEP]
xF [ -DIS]F [e-, µ-DIS]
decays
(Z --> had.) [LEP]
e e [ ]+had
_e e [jets & shapes 35 GeV]+ _
(pp --> jets)
pp --> bb X
0
QQ + lattice QCD
DIS [GLS-SR]
2
3
pp, pp --> X
DIS [Bj-SR]
e e [jets & shapes 58 GeV]+ _
jets & shapes 133 GeV
e e [jets & shapes 22 GeV]+ _
e e [jets & shapes 44 GeV]+ _
e e [ ]+had
_
jets & shapes 183 GeV
DIS [pol. strct. fctn.]
jets & shapes 189 GeV
e e [scaling. viol.]+ _
jets & shapes 91.2 GeV
e e F+ _2
e e [jets & shapes 14 GeV]+ _
e e [4-jet rate]+ _
jets & shapes 195 GeVjets & shapes 201 GeVjets & shapes 206 GeV
DIS [ep –> jets]
hep-ex/0407021
2
4
6
8
1 0
1 2
1 1 0 100
1/α
s
Q [GeV]
NM
C
G–
LS
CL
EO
PE
P
τ
TR
ISTA
N
LE
PU
A2
La
ttic
e
e+e
–
e+e
– e
ven
t sh
ap
es
LEP2
PDG
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 29bis
Quenched hadron spectrum
0.4
0.6
0.8
1.0
1.2
1.4
1.6
1.8
m [
Ge
V]
GF11 infinite volume K input
CPPACS K input
CPPACS φ inputK
K*
φ
N
Λ
Σ
Ξ
∆
Σ*
Ξ*
Ω
S. Aoki, et al. (CP–PACS), Phys. Rev. Lett. 84, 238 (2000)
(No dynamical fermions)
2 + 1 dynamical flavors: A. Ukawa, Beijing QCD 2005,
http://www.phy.pku.edu.cn/˜qcd/transparency/20-plen-m/Ukawa.pdf.
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 30bis
The Origins of Mass
(masses of nuclei “understood”)
p, [π], ρ understood: QCD
confinement energy is the source
“Mass without mass”
Wilczek, Phys. Today (November 1999)
We understand the visible mass of the Universe
. . . without the Higgs mechanism
W,Z electroweak symmetry breaking
M2W = 1
2g2v2 = πα/GF
√2 sin2 θW
M2Z = M2
W /cos2 θW
q, `∓ EWSB + Yukawa couplings
ν` EWSB + Yukawa couplings; new physics?
All fermion masses ⇔ physics beyond standard model
H ?? fifth force ??
Chris Quigg Electroweak Theory · Fermilab Academic Lectures 2005 31bis