Upload
others
View
7
Download
0
Embed Size (px)
Citation preview
V. Hedberg Weak Interactions 1
Weakinteractions
V. Hedberg Weak Interactions 2
Gauge invariant theories.
The equation y=x2 is symmetric or invariant under the transformation A, i.e. it looks
The electroweak theoryy
x
y´
x´
y=x2 y´=x´2A
y´=yx´=-x
the same before and after the transformation.
Gauge invariant theories the main equations do not change a gauge transformation is performed.
Requiring gauge invarianiance deduce the various interactions.
when
V. Hedberg Weak Interactions 3
What is a gauge transformation ?
The electroweak theory
Different gauge transformations different interactions.
Non-relativistic electromagnetism
The equation of motion: for a free non-relativistic particle:
The free particle Schroedinger equation
i x t t
------------------- 12m------- x t
2–=
Goal: modify this equation to describes particles that
Example:
interact electromagnetically.
V. Hedberg Weak Interactions 4
The electroweak theoryAssumption: the new equation is invariant under a
U(1) phase transformation:
x t ' x t eiq x t x t =were is an arbirary continous function. x t
Failure: the transformed wavefunction is not a solution to the Schroedinger equation.
' x t
The Gauge principle Gauge principle: to keep the invariance condition satisfied it is necessary to add a minimal field to the Schroedinger equation
an interaction will have to be introduced.
V. Hedberg Weak Interactions 5
The electroweak theoryThe electroweak theoryIntroduce interaction: require that the Schroedinger equationis also invariant under a gauge transformation of type
A A' A +=
V V' V t
------–=
i x t t
------------------- 12m------- p qA– qV+ x t =
Invariance: U(1) phase transformation + gauge transformation
where A and V are the vector and scalar potenials of the electro-magnetic field in which a particle with a charge q is moving.
The equation for a non-relativistic particle with charge q moving in an electromagnetic field.
new equation
V. Hedberg Weak Interactions 6
The electroweak theory
Weak isospin charge I3 Weak hypercharge YW
w
massless gauge particles W+,W-,W0, B0
The gauge particles interact with massless fermions.
The electro weak theory by Glashow, Weinberg and Salam.
The EW or GWS model is a quantum field theory for both weakinteractions and electromagnetic interactions.
Electric charge QQ = I3 + YW/2 w
Gauge invariance
V. Hedberg Weak Interactions 7
The Higgs field generates mass to gauge bosons and fermions.
W+ and W- weak radioactive decay
not observed experimentally
the electromagnetic interaction gauge boson for the weak neutral current interaction
B0 Wcos W0 Wsin+=
Z0 B0 Wsin– W0 Wcos+=
the weak mixing angle
The electroweak theory
W0 and B0
Photon gauge boson for Z0
W a parameter (not predicted).
V. Hedberg Weak Interactions 8
Only W-exchange
The electroweak theory divergent processes
e+
e-
W-
W+
e+
e- W-
W+
e
Divergent integrals
The Z0-boson new diagrams cancel out the divergencies
e+
e-Z0
W-
W+
e+
e- Z0
Z0
e-
e+
e- Z0
e-
Divergent integrals
Non-divergent integrals
Non-divergent integrals
infinities
V. Hedberg Weak Interactions 9
Coupling constants in EW e, gW and gZ
The electroweak theory
The coupling constants are not independent(in order for all the infinities to cancel out)
8 gW Wsin gZ Wcos= =
The weak mixing angle (Weinberg angle) WcosMWMZ----------=
The unification condition.
e/ g Wsin g Wcos=e = ´ 8 8g= gW g´= gZ
Alternatives
“Strength parameters”
= e2
4QED: s=
gs24QCD:137
1 91 EW: 850
1Z= gZ
2
42501W=
gW2
4
V. Hedberg Weak Interactions 10
e- e
W-
e-
e
e e-
W- W+ W-
The electroweak theoryThe strength parameters contribution of different processes (diagrams) to the cross-section.
Example: muon-scattering on electrons
Diagrams with increasing complexity can contribute:
Second order diagram Sixth order diagram
gW
gW
gW gW gW
gW gW gW
Second order diagram cross section is proportional to
+ e- + e
aW2
aW6Sixth order diagram cross section is proportional to
V. Hedberg Weak Interactions 11
e- e
W+
gW
gW
GFMW
e-
e
The electroweak theory Point-like interactions and low-energy measurements
Fermi’s theory of weak interactions four-fermion point-like interactions (without W and Z exchange).
W bosons are heavy charged current interactions can be approximated by a zero-range interaction at low energy
Fermi coupling constant (GF)
GF2
--------gW
2
MW2
----------4WMW
2----------------= =Relationship between gW and GF:
The strength of the zero-range interactionsnext slide
V. Hedberg Weak Interactions 12
GF2
--------gW
2
MW2
----------= em
2------------------- gW Wsin= MW
2gW
2 2
GF----------------
em
2GF 2
Wsin-----------------------------------= =
MZ2
em
2GF 2
W 2
Wsincos-------------------------------------------------------=
and gives
WcosMWMZ----------= and MW
2em
2GF 2
Wsin-----------------------------------= gives
A bit of algebra:
GZ2
-------gZ
2
MZ2
--------= GZGF--------
2gZ2
2gW2
---------------MW
2
MZ2
----------
2 2
Wcos----------------------
2 2
Wsin------------------------------------------------
2W
2Wsin=cos= =which gives
The electroweak theoryThe unification condition
Definition Weinberg angle
GZ neutral current coupling constant in the low energy approximationzero-range
V. Hedberg Weak Interactions 13
The electroweak theory
2
Wsin 0 277 0,014=
Measurement of the weak mixing angle predict the masses of the W and Z:
MW 78,3 2,4 GeV/c2=
MZ; 89,0 2,0 GeV/c2=
GZ/GF=sin2(W) Measurements of weak interaction rates at low energyGZ and GF
Discovery at CERN of W and Z at predicted massesconfirmation that the electroweak theory is correct.
V. Hedberg Weak Interactions 14
Modern estimation of the Weinberg angle (from many experiments)
The electroweak theory
2Wsin 0,2255 0,0021=
This value and the previous formulas give:
MZ; 89,0 GeV/c2=
MW 78,5 GeV/c2=while direct measurements give
MZ; 91,2 GeV/c2=
MW 80,4 GeV/c2=
The difference is caused by higher-order diagrams(not taken into account in the low-energy formulas)
e-e
W-
W-
W-
Z0
e-e
W-
W-
b t
V. Hedberg Weak Interactions 15
The electroweak theory
e-e
W-
W-
W-
Z0
e-e
W-
W-
b t
Higher-order corrections with top-quarksmeasurement of electroweak processespredict the top-quark mass
mt 170 30 GeV/c2=
The directly measured mass of the top quark at Fermilab bythe CDF experiment gave a value
mt 176 5 GeV/c2=
Perfect agreement with the low-energy prediction !
V. Hedberg Weak Interactions 16
The W and Z bosons The force carriers in weak interactions are spin-1 bosons (as in QED and QCD) that couple to quarks and leptons.
All observed low-energy weak processes charged current reactions mediated by W+ or W- bosons.
The Electroweak Theory predicted that neutral current reactions caused by the Z0 boson should exist.
the intermediate vector bosonsW+ , W- and Z0
that are the force carriers of weak interactions
have a very short range ( order of 2 x 10-3 fm ).( mW=80.4 GeV and MZ=91.2 GeV ) weak interactions W+, W- and Z0 bosons are very massive particles
(e.g. -decay)
V. Hedberg Weak Interactions 17
Accelerator: The Proton Synchrotron (PS) at CERN
Discovery of the neutral current
The PS accelerator: Length = 628 m, Number of magnets = 277, Proton beam energy = 28 GeV Neutrino beams:
Step 2. Charged pions and kaons decay +++e++e++Step 1. Intense proton beam hits a target
V. Hedberg Weak Interactions 18
Discovery of the neutral current Neutral current events was first observed by the Gargamelle experiment at CERN in 1973.
Magnet coils
N2 liquidpropane
Compressor-decompressor
system
Flash lights
Plastic membranes
Filmcameras
Step 1. The liquid propane is at a temperature below its boiling point.
Step 2. When the enters the propane, its pressure is lowered to make it superheated.Step 3. Charged tracks ionize the propane and these ions create bubbles in the liquid.Step 4. The bubble tracks are photographed by film cameras.
V. Hedberg Weak Interactions 19
Discovery of the neutral current Elastic and inelastic neutral current reactions possible.
nucleon
hadrons
Main background neutron - nucleon interactions.
V. Hedberg Weak Interactions 20
Discovery of the neutral current
e-
e+
e-e-
e+
Bremsstrahlung
Conversion
One of the first neutral current reactions seen by the Gargamelle experiment.
V. Hedberg Weak Interactions 21
The discovery of the W and Z bosons
Dipole magnet
Quadrupol magnet
Cavity
The accelerator: The Super Proton Synchrotron
The SPS accelerator: Length = 6.9 km, Number of magnets = 960, Fixed target = 400 450 GeV
pp-collider = 540 630 900 GeV
The W and Z were discovered by the UA1 and UA2 experiments.
V. Hedberg Weak Interactions 22
SPS(CERN)
Length: 7 km (960 magnets)Experiments: UA1, UA2
e
q
q
qg
g
g
hadrons
p
450 GeV
q
q
qg
g
gp
hadrons
g
450 GeV
The discovery of the W and Z bosonsLEP(CERN)
Length: 27 km (4184 magnets)Experiments: DELPHI, OPAL, ALEPH, L3
ee- ee+
46 GeV104 GeV
46 GeV104 GeV
hadrons
hadrons
Z0q
q-
The energy of the quarks and gluons carry only a fraction of the proton
To produce W- ans Z-bosons with a mass of 80-90 GeV a collider with a beam energy of 270 GeV was needed.
The beam energy was later increased to 450 GeV.
energy.
V. Hedberg Weak Interactions 23
The discovery of the W and Z bosons
Gargamelle
ATLASUA1
DELPHI
V. Hedberg Weak Interactions 24
The discovery of the W and Z bosonsThe experiment: UA1
Tracking detector: Central wire chamber with 0.7 T dipole magnet.Electromagnetic calorimeter: Lead/scintillator sandwichHadronic calorimeter: Iron/Scintillator sandwichMuon detector: 8 planes of drift chambers.
V. Hedberg Weak Interactions 25
The discovery of the W and Z bosonsProduction of W and Z bosons
u + d W+ d + u W-
u + u Z0 d + d Z0
p
p
q
qW Z0
The W and Z bosons are in proton colliders produced byquark-antiquark annihilations:
The lifetime of both the W and the Z is about 3 x 10-25 sthey cannot be seen directly in the experiments.
V. Hedberg Weak Interactions 26
The discovery of the W and Z bosonsThe decay of W and Z bosons
p + p W-+ X l- + l
p + p W++ X q´ + q
p + p W-+ X q´ + q
p + p Z0+ X q + q
p + p Z0+ X l+ + l-
p + p W++ X l+ + l
hadronic decays leptonic decays
Cannot be found amongall other hadrons produced.
The decays to leptonsare easy to identify
V. Hedberg Weak Interactions 27
The discovery of the W and Z bosonsAnalysis of W-events in UA1
The analysis searched for events with a charged lepton + neutrino
A high momentum electron is indicated by the arrow.
V. Hedberg Weak Interactions 28
The discovery of the W and Z bosonsTransverse momentum
The transverse momentum and energyof a particle: PT = P sin()
ET = E sin()
ET = PT if the mass of the particle issmall since E2=P2+m2
where is the angle to the beam.
The total momentum is zero of all the particles in a collision.
Neutrinos are not detectableif the total momentum = 0the event has missing momentum
pPT
PL
(or missing energy).
V. Hedberg Weak Interactions 29
The discovery of the W and Z bosonsAnalysis of W-events in UA1
The analysis was looking for events with a charged lepton and The main selection criteria in the UA1 W-analysis was:i) A charged electron or muon with a large momentum (>10 GeV/c)ii) This lepton should be emitted at a wide angle to the beam (>5o)iii) There should be large missing transverse momentum in the event
The expected distribution of thetransverse energy of the selectedelectrons was compared with themeasured distribution.
MW 83 5 2 8 GeV= W 6 5 GeV
From the first 148 electron and 47muon events it was estimated that:
Wjet-jet
Transverse Energy (GeV)Eve
nts
10
20
20 30 40 50
MeasuredDistribution
BackgroundSubtractedDistribution
SimulatedDistributionMW=83.5 GeV
V. Hedberg Weak Interactions 30
The discovery of the W and Z bosonsAnalysis of Z-events in UA1
The analysis was looking for a pair of charged leptons.
e-
e+
V. Hedberg Weak Interactions 31
The discovery of the W and Z bosonsInvariant mass
= 2 E1E2 ( 1 - cos )if m=0
E1
E2
Zmz
me
mz2
mz2 = ( P1 + P2 )2 ( 4-vectors )
E1me
E2 me
me
The invariant mass of a particle thatdecays to two other particles:
V. Hedberg Weak Interactions 32
The discovery of the W and Z bosonsAnalysis of Z-events in UA1
Main search criteria require pair of electrons or muons with a large transverse energy.
The mass distributionof pairs of electronswhere each electron has ET>8 GeV.
MZ 93 0 1 4 GeV=
Z 8 1 GeV
20 40 60 80 100Mass (GeV)
4
8
Even
ts
jet-jetbackground
Z0
candidates
The first 18 electron pairsand 10 muon pairs in UA1
V. Hedberg Weak Interactions 33
Precision studies of the W and Z bosonsThe accelerator: The Large Electron Positron Collider
Electrons-positrons collisions in four experiments.
Z mass maximum288 superconducting cavities.
Collision energy: 91 GeV 209 GeV
V. Hedberg Weak Interactions 34
Precision studies of the W and Z bosons
Cavity
Dipole magnet
Quadrupol magnet
V. Hedberg Weak Interactions 35
TEVATRON(FERMILAB)
Length: 6 km (990 magnets)Experiments: CDF, D0
e
q
q
qg
g
g
hadrons
p
1000 GeV
q
q
qg
g
gp
hadrons
g
1000 GeV
LHC (CERN)
Length: 27 km (1232 + 386 magnets)Experiments: ATLAS, CMS, LHCb, ALICE
e
q
q
qg
g
g
hadrons
p
7000 GeV
q
q
qg
g
gp
hadrons
g
7000 GeV
LEP(CERN)
Length: 27 km (4184 magnets)Experiments: DELPHI, OPAL, ALEPH, L3
ee- ee+
46 GeV104 GeV
46 GeV104 GeV
hadrons
hadrons
Z0q
q-
HERA (DESY)
Length: 6 km (1650 magnets)Experiments: H1, ZEUS
e
ee+
30 GeV
ee+q
q
qg
g
g
hadrons
p
920 GeV
Precision studies of the W and Z bosons
V. Hedberg Weak Interactions 36
Precision studies of the W and Z bosonsDifferences between proton and electron colliders.
Synchrotron radiation:Total energy loss is proportional to 1/mass4
1/radiusTotal energy loss is proportional to 4Ebeam Total energy loss is proportional to
Energy loss in an electron accelerator is 1013 times larger.
LEP: 344 cavities, accelerating voltage=3630 MV, energy=104 GeV LHC: 16 cavities, accelerating voltage = 16 MV, energy=7000 GeV
Beam momentumLength of bending field
Magnetic bending field LEP: 0.12 Tesla bending fieldLHC: 8.38 Tesla bending field } factor 70
V. Hedberg Weak Interactions 37
Precision studies of the W and Z bosonsThe accelerator: The Large Electron Positron ColliderIn an electron-positron collider it is important to know the collision energy with a high accuracy. It took many years tounderstand the factors that influenced the collision energy in LEP.
Days
ΔE (
MeV
)
Energy calibrations
Horizontal Orbit (XARC)
Lake level fit
-20
-10
0
120 140 160 180 200 220 240
Geological shiftsDuring 1993 the LEP energy was observed to change with time.
Part of the change was due to
which caused small geologicalshifts of the accelerator.
Rainfalls and the water table
affected the LEP energy.
the water level in lake Geneva
in the Jura mountains also
V. Hedberg Weak Interactions 38
Precision studies of the W and Z bosonsΔ
E [
MeV
]
November 11th, 1992
Δ E
[M
eV]
August 29th, 1993
Daytime
October 11th, 1993
-5
0
5
23:00 3:00 7:00 11:00 15:00 19:00 23:00 3:00
-5
0
5
11:0
0
13:0
0
15:0
0
17:0
0
19:0
0
21:0
0
23:0
0
18:0
0
20:0
0
22:0
0
24:0
0
2:00
4:00
6:00
8:00
Tides
Earth tides caused by the moon will produce small distortions of the earth’s crust.
This can affect the accelerator so that the electrons orbit change.
An orbit change of 1 mm would change the energy with about 10 MeV.
V. Hedberg Weak Interactions 39
Vacuum Chamber Current Correlation
LEP
SPS
CERN
airpor
t
Belleg
arde
Lau
sann
e
La Versoix
Lac de
Geneve
Meyrin
Zimeysa
Cornavin
IP1
IP2
IP3
IP4IP5
IP6
IP7
IP8
1 km
1
Vol
tage
on
rails
[V]
RAIL
TGV
Gen
eve
Mey
rin
Zim
eysa
17.11.1995
Vol
tage
on
beam
pipe
[V]
LEP beam pipe
Time
Ben
ding
B f
ield
[Gau
ss]
LEP NMR
-7
0
-0.024
-0.02
-0.016
-0.012
746.28
746.30
746.32
746.34
746.36
16:50 16:55
Beampipe current
LEP Lake
Trains
River
Geneva
The trains from Geneva to Francecaused parasitic currents on the LEP beampipe.These currents (1 A) affected the magnetic field in the LEP magnetsand this changed the energy.
Precision studies of the W and Z bosons
V. Hedberg Weak Interactions 40
Precision studies of the W and Z bosonsThe DELPHI Experiment
DELPHIVertex Detector
Inner Detector
Time Projection Chamber
Small Angle Tile Calorimeter
Very Small Angle Tagger
Beam Pipe
Quadrupole
Barrel RICH
Outer Detector
High Density Projection Chamber
Superconducting Coil
Scintillators
Barrel Hadron Calorimeter
Barrel Muon ChambersForward Chamber A
Forward RICH
Forward Chamber B
Forward EM Calorimeter
Forward Hadron Calorimeter
Forward Hodoscope
Forward Muon Chambers
Surround Muon Chambers
The DELPHI ExperimentTracking detector:Time projectionchamber
Electromagneticcalorimeter:Lead absorber
Magnet
Hadronic calorimeterIron absorber
Muon detectors
V. Hedberg Weak Interactions 41
The DELPHI Experiment
Precision studies of the W and Z bosons
The DELPHI cavern The Time Projection chamber
V. Hedberg Weak Interactions 42
Precision studies of the W and Z bosons
TPC
Cerenkov
Electromag.calorimeter
Magnet
Hadroniccalorimeter
Muonspectrometer
Studies of the Z-boson
e
e-
+
e+
e Zo-
From the number of produced electronpair events one can calculate the crosssection for the following process:
Crosssection
Collision energy
V. Hedberg Weak Interactions 43
TPCCherenkov
Electromag.calorimeter
Magne t
Hadroniccalorimeter
Muonspectrometer
Precision studies of the W and Z bosonsStudies of the Z-boson
From the number of produced muonpair events one can calculate the crosssection for the following process:
Crosssection
Collision energy
-
+
e+
e Zo-
V. Hedberg Weak Interactions 44
TPCCherenkov
Electromag.calorimeter
Magne t
Hadroniccalorimeter
Precision studies of the W and Z bosonsStudies of the Z-boson
From the number of produced taupair events one can calculate the crosssection for the following process:
Crosssection
Collision energy
+
e+
e Zo-
-
Muonspectrometer
V. Hedberg Weak Interactions 45
The number of neutrino families
(pb)
Center of mass energy (GeV)
e
e-
+
e+
e Zo-
-
+
-
+
q
qBranching ratio ( B ):
}0.10 0.20 0.70
Decay width ( ): 0.25 GeV 0.50 GeV 1.74 GeV
B---= Bxx
xxZ---------=
where the lifetime is given by
BZZ-------
Bhad Bll B+ +
had ll + +--------------------------------------------= =
Bhadhad-------------
Bllll-------
B---------- 3 25–10 s= = = =
1GeV 1– 6 582 25–10 s=Note:
The total decay width Z isthe sum of the partial decaywidths.
V. Hedberg Weak Interactions 46
The number of neutrino families
MZ
Z
: The total Z0 decay rateZ Z(Z0 X)
: The decay rate to final state XMZ : The mass of the Z0
where
B Z0 e+e- B Z0 X Z0 e+e-
Z-----------------------------------
Z0 X Z
---------------------------The height of the peak isproportional to the branching ratios:
It was possible to determine the partial decay widths of the Z0
by fitting Breit-Wigners to the measured distributions at LEP.
Collision energy - ECM
If Ecm=MZ:
e+e- 12MZ
2
ECM2
------------------ Z ee Z
ECM2
MZ2–
2
MZ2Z
2+
---------------------------------------------------------------=
e+e- 12
MCM2
--------------- Z ee Z
Z2
----------------------------------------------------------------=
Z0
V. Hedberg Weak Interactions 47
The number of neutrino familiesThe fitted parameters of the Z0 peak gave the following result:MZ 91,187 0,007 GeV/c2=
Z 2,490 0,007 GeV=
Z0 hadrons 1,741 0,006 GeV= Z0 l+l- 0,0838 0,0003 GeV=
However, the leptonic and hadronic decays account for only 80%of all the Z0 decays.
The remaining decays are those to neutrinos that cannot bemeasured directly by the experiment
Z Z0 hadrons 3 Z0 l+l- ++= N Z0 ll
From the measured values of the decay widths one gets
N Z0 ll 0,498 0,009 GeV=
V. Hedberg Weak Interactions 48
The number of neutrino families
5
10
15
20
25
30
35
88 89 90 91 92 93 94 95
N=2
N=3
N=4
DELPHI
Energy, GeV
N 2,994 0,011=
The decay rate of the Z0 to neutrinos can be calculated:which together with
gives Z0 ll 0,166 GeV= N Z0 ll
0,498 GeV=
Z0 to There are no explicit restrictionson the number of generations in the standard model.
The study of the Z0 peak at LEPshows that there are onlythree types of light neutrinos(with a mass less than MZ.)
hadrons
V. Hedberg Weak Interactions 49
Precision studies of the W and Z bosonsStudies of the W-boson
e+ e-
A WW-event with 4 jets
The W bosons were produced in pairs at LEP.
e+
e-
e+
e Zo-
e
W+
W-
/
W+
W-
The signature for WW-events was:
qq qq llqq l
V. Hedberg Weak Interactions 50
Precision studies of the W and Z bosonsStudies of the W-boson
0
50
100
150
200
250
50 60 70 80 90 100
DATA
WW
(Mw = 80.35)
ZZ
QCD
W mass [ GeV/c2 ]
even
ts /
2 G
eV/c
2
Step 1. Select WW-pair events Step 2. Calculate the W-mass
qq qq
W
2= ( )PP +q q
_
W
2= 2 E E ( 1 - cos )q
_
if m = 0q
( 4-vectors )2
q
The mass distribution of jet-pairs
V. Hedberg Weak Interactions 51
W and Z reactions
�l l+
W�
gW
- q q’
W�
Vqq’gW
�l
Z0
l+�l l-
Z0
gZ gZ
�l
Z0
l+�l l-
Z0
Z0
gZ
Z0
Leptonic reactions Hadronic reactions
Charge
Neutral
currentreactions
currentreactions
V. Hedberg Weak Interactions 52
Charged current reactions
Purely leptonic processes:
Charged current reactions are reactions mediated by thecharged W-bosons.
Purely hadronic processes:
Semileptonic reactions:
W-
e-
e
- e- + e +
+ p
n p + e- + e
du
sud u
ud
W-
p
du
dsu d
uu
W-
p
ddu
udu
e-
e
W-
n
p
V. Hedberg Weak Interactions 53
Leptonic charged current reactions
+ + ...
e-
e-
e-
e-
e-
e+
l l-
W
l l+
W
All the electromagnetic interactions eight basic interactions:
Leptonic weak interaction described by basic vertices:
The basic vertex forelectron-photon interactions.
The two basic vertices for W-leptoninteractions..
V. Hedberg Weak Interactions 54
l
W+
l+
l
W-
l-
l+
W+
l
W-
l+
l
l
l+
W+
W-
l-
l
l-
W+
l
l
W-
l+
l l- + W+
W+ l l-
l+ W+ + l
W-+ l+ l
l+ + l W+
W- l- + l
vacuum l- + l + W+ l+ + l + W- vacuum
Eight basic charged current reactions from two basic W vertices:
Leptonic charged current reactions
V. Hedberg Weak Interactions 55
Weak interactions conserve lepton numbers: Le , L , L .
Feynman diagrams:1) at each vertex, there is one arrow pointing in and one out2) the lepton indices “l” are the same on both lines.
+ + ...
W
e-
e-
W+W-
e-
+ + ...
e
W
e-
e
e-
W+W-
e-
e
Allowed:
Forbidden:
Leptonic charged current reactions
V. Hedberg Weak Interactions 56
Leptonic charged current reactionsThe weak strength parameter: W
W is the same at all leptonic vertices (do not depend on leptontype).
Example: The decay rate of W to e+
W e WMW W 80 GeVEstimation from theory
W e 0,2 GeVMeasurement
W=0.003
The electromagnetic strength parameter: em=0.007
V. Hedberg Weak Interactions 57
Leptonic charged current reactionsWhy is the weak interaction so weak if W and em is ofa similar size ?
Compare the decay of charged and neutral pions:
u
u
{Electromagnetic decay
Lifetime = 8 x 10 s-17
-W-
du
Weak decay
{Lifetime = 3000000000 x 10 s
-17
(Lifetime of a real W = 0.00000003 x 10 s)-17
CONCLUSION: The apparent weakness of the weak interactionsis due to the very large W and Z masses.
V. Hedberg Weak Interactions 58
W and Z reactions
�l l+
W�
gW
- q q’
W�
Vqq’gW
�l
Z0
l+�l l-
Z0
gZ gZ
�l
Z0
l+�l l-
Z0
Z0
gZ
Z0
Leptonic reactions Hadronic reactions
Charge
Neutral
currentreactions
currentreactions
V. Hedberg Weak Interactions 59
Hadronic charged current reactionsIn weak hadronic interactions, constituent quarks emit or absorb W or Z bosons.
ddu
udu
e-
e
gWW-
gudn
p
du
sud u
ud
W-
p
du
dsu d
uu
W-
p
Examples:
Neutron -decay.
The dominant quark diagrams for decay
V. Hedberg Weak Interactions 60
Hadronic charged current reactionsASSUMPTION: Lepton-quark symmetry i.e. correspondinggenerations of quarks and leptons have identical weakinteractions.
- c
s
e
e- u
d
- t
b
u d
W
u d
W
c s
W W
gud gcsc s
gud gcsl l-
W
l l+
W
gW gW
The W-quark vertices for the first two generations, assuming lepton-quark symmetry.
The W-lepton vertices.
Interactions will then only take place within a family !
V. Hedberg Weak Interactions 61
Hadronic charged current reactionsExperimental tests of the assumption of lepton-quark symmetry.
Some weak reactions should be allowed and some should beforbidden if lepton-quark symmetry is true:
du
K- su
-W-
du Allowed
-W-
su
Not AllowedK-
{
{Different families
Measurements of these decays give: Branching ratio = 0.9999 = 2.6 x 10-8 sK- Branching ratio = 0.6343 = 1.2x 10-8 s
CONCLUSION: Quarks from different generations canparticipate in charged current interactions !
V. Hedberg Weak Interactions 62
Hadronic charged current reactionsCabibbo introduced the concept of quark mixing in order to explain the kaon decays.
Quark mixing scheme d- and s-quarks participate in weak interactions via the linear combinations:
d' d C s Csin+cos=
s' d C s Ccos+sin–=where C is called the Cabibbo angle.
The quark-lepton symmetry applies to doublets like
ud'
and cs'
+
u
W
d’gW
u
W
d u
W
sgud gus
gud=gWcosC gus=gWsinC
The ud’W vertex can beinterpreted as a sum ofthe udW and usW vertices:
V. Hedberg Weak Interactions 63
Hadronic charged current reactionsWith the quark mixing hypothesis, more W-quark vertices:
u d
W
u d
W
c s
W W
gcsc s
gud gcs
u s
W
u s
W
c d
W W
gus gcdc dgus gcd
gW CcosgW Ccosgud
gW CcosgW Ccos
g– W Csing– W CsingW CsingW Csin
gud gcs gW Ccos= =
gus g– cd gW Csin= =
Within a generation:
Between generations:
V. Hedberg Weak Interactions 64
Measurements of the Cabibbo angle.
Hadronic charged current reactions
The Cabibbo angle has to be measured.
Comparing the decay rates of with K-
K- -
- - ------------------------------------
gus2
gud2
--------- 2
Ctan= gives the result C 12,7 0,1=
gW Ccos 0 98gW=gW Csin 0 22gW=
The coupling constants within and between generations:
V. Hedberg Weak Interactions 65
Charmed particle decays.
Hadronic charged current reactions
c
s
W+
gW Ccos
gW
c
d
W+
gW Csin
ll
ll
gW
Particles with charm quarks almost always give a strange particlein the final state because other decays are Cabibbo supressed:
gcd2
gcs2
--------- 2
Ctan 120------= =
The supression factor is given by:
C 12 6=if
The charmed quark couplings gcd and gcs have been measuredin neutrino scattering experiments with the result: C 12 1=
V. Hedberg Weak Interactions 66
Two generation quark mixing can be written in matrix form:
Weak interactions and the third generation
d's'
Ccos Csin
Csin– Ccos
ds
=
This means that the following weak transitions are favoured:
C
s
u
d
And that the following weak transitions are surpressed:
C
s
u
d
While charge conservation forbids the following charged current
C
s
u
d
Charge = 2/3
Charge = -1/3
ud'
and cs'
with transitions within
transitions:
V. Hedberg Weak Interactions 67
Weak interactions and the third generationWeak interactions and the third generationThe existence of the c-quark was predicted from lepton-quarksymmetry before it was discovered in experiments in 1974.
After the discovery of the lepton and the b-quark, the sixthquark was predicted to complete the symmetry the top quark was discovered in 1994
d's'b'
Vud Vus Vub
Vcd Vcs VcbVtd Vts Vtb
dsb
=
The third generation gives rise to the Cabibbo-Kobayashi-Maskawa (CKM) matrix V:
The relation between the matrix elements in the CKM-matrix and the coupling constants are given by g = gWV where=u,c,t and =d,s,b .
V. Hedberg Weak Interactions 68
Weak interactions and the third generation
If the mixing between the b and t quarks with lighter quarkscan be neglected the CKM-matrix is reduced to:
Vud Vus VubVcd Vcs VcbVtd Vts Vtb
Ccos Csin 0
Csin– Ccos 0
0 0 1
If Vub, Vcb, Vtd and Vts are not small The two-generation mixing model would not work
Weak transitions can now take place between:
u d’ = Vudd+Vuss+Vubb c s’ = Vcdd+Vcss+Vcbb t b’ = Vtdd+Vtss+Vtbb
V. Hedberg Weak Interactions 69
Weak interactions and the third generation
Vub=Vcb=Vtd=Vts=0 t-quark decay only to b-quarks
b-quark is stable(since it cannot decay to u- or c-quarks)
Semileptonic decays of b-quarks to u- and c-quarks
The observed decay rate isproportional to the squared
are observed in experiments !
Not true
couplings: gub
2 Vub2gW
2=
W-l
b
l-
gub
u
gW
VubgW
b - quarks
V. Hedberg Weak Interactions 70
Weak interactions and the third generationb - quarks
The most precise measurements at present give
Vub 0 004 and Vcb 0 04
This means that the CKM-matrix becomes
Vud Vus VubVcd Vcs VcbVtd Vts Vtb
Ccos Csin 0 004
Csin– Ccos 0 04
1
0 0
0 98 0 22 0 0040 22– 0 98 0 04
1
0 0
V. Hedberg Weak Interactions 71
Weak interactions and the third generationThe top quark
The top quark is much heavier than even the W-bosons and itcan decay by
t
d
W+
t
s
W+
t
b
W+
gtd 0 gts 0 gts= gW
Since gtd and gts are close to zero, the only significant decaymode of the t-quarks is
t W+ + b
with a rate proportional to W gW2 4= 0 0042
Estimation of the decay width of the top ( Wmt 1 GeV )suggests a very short lifetime
t 4 25–10 s
V. Hedberg Weak Interactions 72
W, Z, top 3-4x10-13ps 0 Beampipe Not possible0 ( ) 0.0008 ps 0.025m Beampipe Not possibleCharm: D0/D /Ds 0.4-1 ps 150-350m Beampipe MicrovertexBottom: B0/B /Bs/ 1.5 ps 450m Beampipe MicrovertexKs ( ) 80 ps 2.7cm Tracker Tracker
KKL ( ) ( ee)
Particle Lifetime Decay Decay Decay Length Place Measurement
0.3 ps 90m Beampipe Microvertex
+-
+-+-
+- 10,000 ps 3.7m Tracker Not possible30,000 ps 7.8m No decay Not possible50,000 ps 16 m No decay Not possible2,000,000 ps 659 m No decay Not possible
Compare particles decay length
Weak interactions and the third generation
V. Hedberg Weak Interactions 73
The discovery of the top quarkThe accelerator: The Tevatron
CDF
Tevatron Main injector
p 150 GeV900 GeV
Tevatron: pp-collider 4.5 T 6.3 km 1800 GeV
Type Bending field Length Collision energy
pp-collider 1.8 T 6.9 km 900 GeV SPS:pp-collider 8.4 T 27 km 14000 GeV LHC:
Superconducting magnets
V. Hedberg Weak Interactions 74
The Tevatron
Old main ring
The discovery of the top quarkThe accelerator: The Tevatron
The Tevatron accelerator was put under the old main ring which was used as a pre-accelerator (it has since been removed).
One of thesuperconductingdipole bendingmagnets.
A cross sectionof a dipolemagnet showingthe coilstructure.
V. Hedberg Weak Interactions 75
V. Hedberg Weak Interactions 108 Had. Calorimeter
Muon system
Drift chamber
Electromagn. Calorimeter
=0=1
The discovery of the top quarkThe experiment: The Collider Detector at Fermilab
Solenoidmagnet
Silicon Vertex Detector
Lead/Scintillator Iron/Scintillator
V. Hedberg Weak Interactions 76
The discovery of the top quarkThe experiment: CDF
V. Hedberg Weak Interactions 77
The discovery of the top quark
Production of top-quarks
In proton-antiproton colliders, pairs of top quarks are mostlyproduced by the quark-antiquark annihilation process:
q + q g t + t
t
t
g
q
q
p
p
V. Hedberg Weak Interactions 78
The discovery of the top quarkThe decay of top-quarks
The most likely decay
p + p t + t + X
W+ + b
W- + b
l+ + lq + q{
l- + lq + q{
of a top quark is to ab quark and to a W.
W+l
t
l+
W- q
t
q
b
b
The W can decay to leptons or hadrons the final stateis a complex mixof jets and leptons.
V. Hedberg Weak Interactions 79
The discovery of the top quark
Expected Signal
Expected Background
Mt 176 5 GeV=
After a selection of likely top event
mass distribution of the top-candidates.had been made, one could plot the
The resulting distribution hada large background componentbut one could neverthelessextract a top mass:
V. Hedberg Weak Interactions 80
W and Z reactions
�l l+
W�
gW
- q q’
W�
Vqq’gW
�l
Z0
l+�l l-
Z0
gZ gZ
�l
Z0
l+�l l-
Z0
Z0
gZ
Z0
Leptonic reactions Hadronic reactions
Charge
Neutral
currentreactions
currentreactions
V. Hedberg Weak Interactions 81
Neutral current reactions
l l-
W
l l+
W
q q’
W
gW Ccos
gW CsingW gW
l
Z0
l+l l-
Z0
Z0
gZ gZ gZ
The basic vertices with W bosons have:- Conserved lepton numbers- Not conserved quark flavour (quark mixing)
The basic vertices with Z bosons have:- Conserved lepton numbers- Conserved quark flavour (no quark mixing)
The basic W vertices The basic Z vertices
V. Hedberg Weak Interactions 82
Neutral current reactionsIn processes in which a photon can be exchanged, a Z0 bosoncan be exchanged as well:
l
Z0
l+l l-
Z0
Z0
gZ gZ gZ
Example: e+e- has two dominant contributions
e+
e-
e+
e-Z0
V. Hedberg Weak Interactions 83
Neutral current reactionsEstimation of the cross-section for the photon- and
2
ECM2
---------------- Z GZ2ECM
2 where Ecm is the collision energy.
The photon exchange process will dominate at low energies.
At Ecm=Mz this low-energy approximation fails andthe Z0 peak is described by the Breit-Wigner formula:
ECM M2
ECM2
------------- CECM
2 M2–
2M2
2+
----------------------------------------------------------= where M is the mass of the resonanceand its decay width.
Z-exchange process in e+e- collisions at low energy:
V. Hedberg Weak Interactions 84
Neutral current reactionse+
e-
e+
e-Z0
2
E2------- Z GZ
2E2
(pb)
Z
MZ
ee 12MZ
2
ECM2
------------------ Z0 ee Z0
ECM2 MZ
2–
2MZ
2Z
2+
-------------------------------------------------------------=
Center of mass energy (GeV)
V. Hedberg Weak Interactions 85
Test of flavour conservationThat flavour is conserved at a Z0 vertex can be verified byexperiments.
Example: measurement of the decay rate of charged kaons
W+
su
uu
K+
Z0
lsu
du
K+
l
K+ K+ l + l
K+ + l l+ + l
K+ 0 + + + ----------------------------------------------------------- 10 7–
The measured upper limit on the ratio of the decay rate ofthese two processes was
until experiment E787 came along .....
V. Hedberg Weak Interactions 86
Test of flavour conservationThe BNL experiment E787 was a fixed target experiment thatused a K+ beam created by 24 GeV protons from the AGS.
AGSE787
The 800 m long AGS
AGS
BoosterLinac
g-2 muonstorage ring
Tandem
Experimental Area
Van de Graaff
AGS to RHIC
has 240 magnets.
V. Hedberg Weak Interactions 87
C
SC
ck
rel
Veto
ITarget
B4
o
EndcapT
ge
mTarget
Scintillating fibers DriftchamberMaterial
to slow down Kaons
0.8 GeV K+ beam
CsI Calorimeterto veto on photons
Tracking
Scintillators
Calorimeterto veto on photons
+
Test of flavour conservation
The Kaons were stopped in a target made of scintillating fibersand the decay of the K+ at rest was then studied.
The momentum, energy and range of the particle from thedecay was measured.
f
50 c(b)
TTarget
CalorimeterScintillators
Driftchambers
E787 K+ l + l
V. Hedberg Weak Interactions 88
Test of flavour conservation
Target
Scintillating fibers
Drift chamber hits Scintillators
After many years of running two candidate events for K+ l + l were found.
The result from these two events were:
K+ + l l+ + l
K+ 0 + + + ----------------------------------------------------------- 1 6 10–
100 033
--------------------------- 5 9–10==
V. Hedberg Weak Interactions 89
Test of flavour conservationThe events could, however, be explained by second-ordercharged current reactions rather than neutral current processes:
s
uu
dK+ +π
l
νν ν
l
νν
l
ν
s
uu
du c t+π+K
s
uu
dK +π+
w w w w w w
Due to the t-d vertex in the third diagram above, it was alsopossible to set limits on the Vtd element in the Cabibbo-Kobayashi-Maskawa matrix:
0 007 Vtd 0 030
V. Hedberg Weak Interactions 90
The Higgs bosonGenerally, experimental data agrees extremly well with thepredictions of the gauge invariant electroweak theory.
Gauge invariance the gauge bosons have zero mass.True for photons in QED and gluons in QCD but not for W and Z.
A new scalar field called the Higgs field is introduced to generate mass to the W and Z bosons as well as fermion masses.
Associated with the field is a new particle called the Higgs boson.
particles but do not predict its mass.The theory predicts how the Higgs boson couples to other
V. Hedberg Weak Interactions 91
The Higgs bosonThe Higgs field has the unusual characteristic of having anon-zero value 0 in vacuum (i.e. the field is not zero in itsgroundstate).
0
Since the vacuum expectation value is not zero, the vacuum issupposed to be populated with massive Higgs bosons and when a gauge field interacts with the Higgs field it acquires mass.
V. Hedberg Weak Interactions 92
The Higgs bosonFrom the interaction with the Higgs field, the W and Z bosons require masses with the ratio given by
WcosMWMZ----------=
H0 gHff
f
f
gHff2 2GFmf
2=
In the same way, fermions acquire mass by interacting withthe Higgs bosons.
The coupling constant for this process depends on the fermionmass:
The existance of the Higgs boson has not been experimentallyverified despite many years of searches.
V. Hedberg Weak Interactions 93
Search for the Higgs boson at LEPThe LEP project had two phases:
LEP 1: The collision energy was equal to the mass of the Z0.LEP 2: The collision energy was increased gradually during several
years by adding superconducting cavities until it reached its maximum energy (209 GeV).
In this case the Higgs particle would be lighter than the Z0
Higgs search at LEP 1
Z0 H0 + l+ + l-
Z0 H0 + l + l
e+
e
H0
Zo
bb
ee
-
Zo
*
V. Hedberg Weak Interactions 94
Search for the Higgs boson at LEPThe predicted branching ratio for Higgs production is low
3 6–10
Z0 H0l+l- tot
----------------------------------------- 10 4–
but millions of Z0s were produced in the LEP experiments andso the experiments were still sensitive to a Higgs signal.
0
2
4
6
8
10
12
14
16
0 10 20 30 40 50 60 70 800
2
4
6
8
10
12
14
16
0 10 20 30 40 50 60 70 80
Mass of hadrons (GeV)
Even
ts Data
Background The DELPHI experiment lookedat one million Z0 events and selected those that containedboth leptons and hadrons.
No signal was observed and oneconcluded that mH > 56 GeV.
V. Hedberg Weak Interactions 95
Higgs search at LEP 2
Search for the Higgs boson at LEP
At LEP 2 one expects the main Higgs production to happen byso-called Higgs strahlung:
e+
e
H0
Zo
bb WW gg cc
qq ee
74% 8% 8% 6% 4%
70% 20% 3% 3% 3%
-
Zo*
Most of the Higgs events would
Two of these should be coming
have 4 jets in the final state.
from b-quarks.
e+ + e- H0 + Z0
Example of a Higgs candidate in DELPHI
V. Hedberg Weak Interactions 96
Search for the Higgs boson at LEPDuring the last year of operation of LEP 2, the ALEPH experiment recorded a couple of events which could be due to the decays of a Higgs boson with a mass of about 115 GeV.
The other experimentsat LEP did not see a signaland when all data was addedtogether there was nodiscovery.
The DELPHI experiment puta limit on the Higgs mass of:
MH 114 GeV/c2
DELPHI, L3ALEPH, OPAL
V. Hedberg Weak Interactions 97
Search for the Higgs boson at LEPThe measurement of many electroweak parameters at LEP (andother places) makes it possible to make a global fit with theHiggs mass as a free parameter.
Fit without using the result of directsearches:
Fit using the limits from direct searches;
mH = 80+30 GeV < 154 GeV-23mH = 120+15 GeV < 144 GeV-5
V. Hedberg Weak Interactions 98
Search for the Higgs boson at LHC
ATLAS
CMS
LHCb
ALICE
CERN
Experiments
ATLAS: Proton-proton collisions
CMS:Proton-protoncollisions
ALICE:Atom-atomcollisions
LHCb:Proton-protoncollisions giving b quarks
CERN
The Large Hadron Collider (LHC)The 27 km long proton-proton collider has a 14 TeV collision energy (1150 TeV for lead-lead collisions).
V. Hedberg Weak Interactions 99
Search for the Higgs boson at LHCThe 1232 dipole magnets produce a8.3 Tesla magnetic field which areused to bend the proton trajectory.
The current in the super-conducting magnet coils is 11800 Ampere.
The protons are travelling in 2808bunches that each contain 1011
protons.
pp
V. Hedberg Weak Interactions 100
Search for the Higgs boson at LHCIn addition to the dipole bending magnets there are some 386quadrupole magnets used to focus the protons beams.
Cavities with strong high-frequency electric fields are used toprovide the energy to the beams. The LHC has 2x8 cavities thatgive 16 MV at 400 MHz.
V. Hedberg Weak Interactions 101
Search for the Higgs boson at LHC The ATLAS experiment
ATLAS is the worlds largest particle physics experiment.
Muon detector Hadron calorimeter
Electromagnetic calorimeter
Tracking detectors
Length: 44 m Diameter: 22 mWeight: 6000 tonnes
The collaboration:3000 physicists>160 universities34 countries
V. Hedberg Weak Interactions 102
Search for the Higgs boson at LHC Higgs boson production
LEP limit
WW, ZZ fusion
W,Z bremsstrahlung
tt fusion
gg fusion gg fusion
WW, ZZ fusion
V. Hedberg Weak Interactions 103
Search for the Higgs boson at LHC Higgs boson decay
10%
40%
1%
0.1%100 200 300 400 500 700 1000
Higgs mass (GeV)
Bra
nch
ing
rati
o
bbWW
ZZt t
γγ
4%
has to select decays that arebackground
The background is huge and one
are visible above the
The cleanest process is if the Higgs has a large enough mass so that itcan decay to two Z0 that then decay to leptons.
There is 109-1010 inelastic interactions for every Higgs bosonthat is produced. At low mass most decay to bb and at highmass most decay to WW and ZZ.
(bb is for example hopeless).
V. Hedberg Weak Interactions 104
Search for the Higgs boson at LHC
[GeV]4lm200 220 240 260 280 300 320 340 360 380 400
Even
ts/(5
GeV
)
0
10
20
30
40
50
[GeV]4lm200 220 240 260 280 300 320 340 360 380 400
Even
ts/(5
GeV
)
0
10
20
30
40
504l→ZZ*→H
ZZZbbtt
-1 L=30 fb∫ATLAS
e e
H
Z Z
e+ e- �+ �-
p p
Short lifetime
Short lifetime
Long lifetime
Computer simulations of collisions in which Higgs bosons are detected by finding four leptons show a very clear signal if the Higgs mass is 300 GeV.
Higgs signal
background
Mass of the 4 leptons
V. Hedberg Weak Interactions 105
[GeV]4lm100 110 120 130 140 150 160 170 180 190 200
Even
ts/(2
.5 G
eV)
02468
101214161820
[GeV]4lm100 110 120 130 140 150 160 170 180 190 200
Even
ts/(2
.5 G
eV)
02468
101214161820 4l→ZZ*→H
ZZZbbtt
-1 L=30 fb∫ATLAS
Search for the Higgs boson at LHC It is possible to use the 4-lepton channel also if mH < 2mZ, but then the Higgs decays to one real andone virtual Z0.
Higgs signalif mH=130 GeV
2mz
At a Higgs mass close to the LEP limit, the branching ratio for H0 ZZ leptons is very small and one is also considering using H0 but this process also has a minute branching ratio:
Br = 1-2 x 10-3
H0
W+
W+
W-
H0
t
t
t Production diagrams:
V. Hedberg Weak Interactions 106
1
10
10 2
102
103
mH (GeV)
Sig
nal s
igni
fican
ce H → γ γ ttH (H → bb) H → ZZ(*) → 4 l
H → ZZ → llνν H → WW → lνjj
H → WW(*) → lνlν
Total significance
5 σ
∫ L dt = 30 fb-1
(no K-factors)
ATLAS
Higgs mass
DiscoveryLimit
ZZ
WW WW
One can estimate the signal significance for different search channels:
Search for the Higgs boson at LHC