high p t hadron collider physics
DESCRIPTION
High P T Hadron Collider Physics. Outline 1 - The Standard Model and EWSB 2 - Collider Physics 3 - Tevatron Physics QCD b and t Production EW Production and D-Y. Backup Text. Units. Tools Needed. (will use both during lecture demonstrations). - PowerPoint PPT PresentationTRANSCRIPT
FNAL Academic Lectures - May, 2006 1
High PHigh PTT Hadron Collider Physics Hadron Collider PhysicsHigh PHigh PTT Hadron Collider Physics Hadron Collider Physics
Outline
• 1 - The Standard Model and EWSB
• 2 - Collider Physics
• 3 - Tevatron Physics• QCD• b and t Production• EW Production and D-Y
FNAL Academic Lectures - May, 2006 2
Backup TextBackup TextBackup TextBackup Text
FNAL Academic Lectures - May, 2006 3
UnitsUnitsUnitsUnits
Recall that coupling constants indicate the strength of the interaction and characterize a
particular force. For example, electromagnetism has a coupling constant which is the electron
charge, e and a “fine structure” constant ce 4/2 that is dimensionless. The
electromagnetic potential energy is rereVrU /)()( 2 and V(r) is the electromagnetic
potential. The dimensions of e2 are then energy times length, 2[ ] [ ( ) ]e U r r , the same as those of
c . Thus, in the units we adopt, 1c , e is also dimensionless. With ~ 1/137, we find e ~
0.303. Coupling constants for the two other forces, the strong and the weak, will be indicated by
gi, and the corresponding fine structure constants by i with i = s, W.
The units for cross section, , which we will use are barns (1 barn = 10-24 cm2). Note that 2 2( ) 0.4c GeV mb where 27 21 10mb cm . The units used in COMPHEP are pb = 10-12 b for
cross section and GeV for energy units. As an example, at a center of mass, C.M., energy, s ,
of 1 TeV = 1000 GeV, in the absence of dynamics and coupling constants, a cross section scale
of s/1~ ~ 400 pb is expected simply by dimensional arguments.
FNAL Academic Lectures - May, 2006 4
Tools NeededTools NeededTools NeededTools NeededWe will extensively use a single computational tool, COMPHEP. The aim was to expand a
slightly formal academic presentation to a more interactive mode for the student, giving “hands
on” experience. The plan was that the student would work the examples and then be fully
enabled to do problems on her own. COMPHEP runs on the Windows platform, which was why
it was chosen since the aim was to provide maximum applicability of the tool. A LINUX version
is also available for students using that operating system
The COMPHEP program is freeware. We have taken the approach of first working through the
algebra. That way, the reader can make a “back of the envelope” calculation of the desired quantity.
Then she can use COMPHEP for a more detailed examination of the question. The use and description
of COMPHEP is explained in detail. A web address where the executable code (zipped) and a users
manual are available. The author has also posted these items: http://uscms.fnal.gov/uscms/dgreen.
Freeware to unzip files can be found at http://www.winzip.com/ and http://www.pkware.com/.
(will use both during lecture demonstrations)
( Google them all – also Ghostview and Acrobat reader )
FNAL Academic Lectures - May, 2006 5
COMPHEP – Models and ParticlesCOMPHEP – Models and ParticlesCOMPHEP – Models and ParticlesCOMPHEP – Models and Particles
Can edit the couplings – e.g. ggH
Use SM Feynman gauge
Watch for LOCK
FNAL Academic Lectures - May, 2006 6
COMPHEP - ProcessCOMPHEP - ProcessCOMPHEP - ProcessCOMPHEP - Process
1-> 2,3
1-> 2,3,4
1,2 ->3,4
1,2 ->3,4,5
1,2-> 3,4,5,6 (slow)
*x options
No 2 -> 1
FNAL Academic Lectures - May, 2006 7
COMPHEP –Simpson, BRCOMPHEP –Simpson, BRCOMPHEP –Simpson, BRCOMPHEP –Simpson, BR
Find simple 2->2. Graphs (with menu)
Results can be written in .txt files
Several PDF, p and pbar,
Check stability of results
FNAL Academic Lectures - May, 2006 8
COMPHEP - CutsCOMPHEP - CutsCOMPHEP - CutsCOMPHEP - Cuts
May be needed to avoid poles or to simulate experimental cuts, e.g. rapidtiy or mass or Pt.
FNAL Academic Lectures - May, 2006 9
COMPHEP - CutsCOMPHEP - CutsCOMPHEP - CutsCOMPHEP - Cuts
FNAL Academic Lectures - May, 2006 10
COMPHEP - VegasCOMPHEP - VegasCOMPHEP - VegasCOMPHEP - Vegas
Full matrix element calculation – interference. Watch chisq approach 1. Setup plots, draw them and write them.
FNAL Academic Lectures - May, 2006 11
COMPHEP - DecaysCOMPHEP - DecaysCOMPHEP - DecaysCOMPHEP - Decays
Strictly tree level. Does not do “loops” or “box” diagrams.
Explore this very useful tool. If there are problems bring them to the class and we’ll try to fix them.
FNAL Academic Lectures - May, 2006 12
1 - The SM and EWSB1 - The SM and EWSB1 - The SM and EWSB1 - The SM and EWSB
• 1.1 The Energy Frontier
• 1.2 The Particles of the SM
• 1.3 Gauge Boson Masses and Couplings
• 1.4 Electroweak Unification
• 1.5 The Higgs Mechanism for Bosons and Fermions
• 1.6 Higgs Interactions and Decays
FNAL Academic Lectures - May, 2006 13
Higgs boson
t quark
b quark
s quark
ISR
Tevatron
SPEAR
SppS
TRISTAN
LEPII
CESR
Prin-Stan
Accelerators
electron
hadron
W, Z bosons
c quark
LHC
PEP
SLC
1960 1970 1980 1990 2000
Starting Year2010
10-1
100
101
102
103
104
Con
stit
uent
CM
Ene
rgy
(GeV
)
Historically HEP has advanced with machines that increase the available C.M. energy. The LHC is designed to cover the allowed Higgs mass range. Colliders give maximum C.M. energy.
The Energy The Energy FrontierFrontier
FNAL Academic Lectures - May, 2006 14
The Standard Model of Elementary The Standard Model of Elementary Particle PhysicsParticle Physics
The Standard Model of Elementary The Standard Model of Elementary Particle PhysicsParticle Physics
• Matter consists of half integral spin fermions. The strongly interacting fermions are called quarks. The fermions with electroweak interactions are called leptons. The uncharged leptons are called neutrinos.
• The forces are carried by integral spin bosons. The strong force is carried by 8 gluons (g), the electromagnetic force by the photon (), and the weak interaction by the W+ Zo and W-. The g and are massless, while the W and Z have ~ 80 and 91 GeV mass respectively.
J = 1 g,, W+,Zo,W- Force Carriers
J = 1/2
u
d
c
s
t
b
e
e
Q/e=
2/3
-1/3
1
0
Quarks
Leptons
J = 0 H
FNAL Academic Lectures - May, 2006 15
Gravity – Hail and FarewellGravity – Hail and FarewellGravity – Hail and FarewellGravity – Hail and Farewell
UG(r) = GNM2/r, depends on mass in comparison to the electrical energy UEM(r) = e2/r. The
quantity GN is Newton’s gravitational constant. The fine structure constants of the forces
appearing in the SM, such as electromagnetism, where 137/1~4/2 ce , are dimensionless
and mass independent. The gravitational analogue, 2 / 4Gr NG M c , is not.
Ignore gravity. However, gravity is a precursor gauge theory which is non-Abelian. The gauge quanta are “charged” non-linearity. The gravity field carries energy, or mass. Therefore, “gravity gravitates”. This is also true of the strong force (gluons are colored) and the weak force (W,Z carry weak charge). The photon is the only gauge boson which is uncharged.
FNAL Academic Lectures - May, 2006 16
How do the Z and W acquire mass and not How do the Z and W acquire mass and not the photon?the photon?
How do the Z and W acquire mass and not How do the Z and W acquire mass and not the photon?the photon?
Gravity - Physics is the same in any local general coordinate system --> metric tensor or spin 2 massless graviton coupled universally to mass = GN.
Electromagnetism - Physics is the same regardless of wave function phase assigned at each local point --> massless, spin = 1, photon field with universal coupling = e
These are “gauge theories” where local invariance implies massless quanta and specifies a universal ( GN, e ) coupling of the field to matter.
Strong interactions are mediated by massless “gluons” universally coupled to the “color charge” of quarks = gs.
Weak interactions are mediated by massive W+,Z,W- universally coupled to quarks and leptons. gWsinW = e. How does this “spontaneous electroweak symmetry breaking” occur? (Higgs mechanism)
FNAL Academic Lectures - May, 2006 17
Lepton Colliders - LEPLepton Colliders - LEPLepton Colliders - LEPLepton Colliders - LEP
Z peak
L and R leptons have different couplings to the Z. There is Z-photon interference which leads to a F/B asymmetry. A way to measure the Weinberg angle. gW measured from muon decay.
FNAL Academic Lectures - May, 2006 18
Field TheoryField TheoryField TheoryField Theory
2 2 2,E P M P P M
2( ) M
To describe quantum fields we will use for fermion (J = ½) fields, for scalar (J = 0)
fields, and for vector (J = 1) gauge fields in this text. For masses, m is used for fermions and
M for bosons.
2
( )( ) ( )( )
~ ( ) ,I
D D
g g
P
by AeP
ieAD
ggggggg, ZWWWW , WWWWZZWWZWWWW ,,,
Classical Special Relativity
Lagrangian density, P is an operator
Classical gauge replacement
Quantum gauge replacement
FNAL Academic Lectures - May, 2006 19
WW in e+e- CollisionsWW in e+e- CollisionsWW in e+e- CollisionsWW in e+e- Collisions
Test of self-coupling of vector bosons. There are s channel Z and photon diagrams, and t channel neutrino exchange. Test of VVV couplings.
In COMPHEP play with the Breit-Wigner option as s dependence of the cross section depends crucially on the W width – i.e. technique to measure W width..
FNAL Academic Lectures - May, 2006 20
Simpson –Angular DistSimpson –Angular DistSimpson –Angular DistSimpson –Angular Dist
Cross section without neutrino exchange in the t channel. Note divergent C.M. energy dependence – voilates unitarity.
FNAL Academic Lectures - May, 2006 21
WW Cross Section at LEPWW Cross Section at LEPWW Cross Section at LEPWW Cross Section at LEP
COMPHEP point shown. Proof that the WWZ triple gauge boson coupling is needed and that there are interfering amplitudes that themselves violate initarity.
FNAL Academic Lectures - May, 2006 22
WWWW at LEP at LEPWWWW at LEP at LEP
Probe of quartic couplings.
LEP data confirms SM
WWAA, WWZA
Cross section in COMPHEP with all final state bosons having Pt > 5 GeV is 0.36 pb
FNAL Academic Lectures - May, 2006 23
ZZ at LEPZZ at LEPZZ at LEPZZ at LEP
SM has only the single Feynman diagram. There are no relevant triple or quartic couplings – in the SM. Use the data to set limits on couplings beyond the SM.
FNAL Academic Lectures - May, 2006 24
e+e- Cross Sectionse+e- Cross Sectionse+e- Cross Sectionse+e- Cross Sections
WW, ZZ, and WW are seen at LEPII. At even higher C.M. energies, WWZ and ZZZ are produced - indicating triple and quartic V couplings. New channels open up at the proposed ILC.
Try a few (red dots) processes yourself…..
FNAL Academic Lectures - May, 2006 25
ILC Process - ExampleILC Process - ExampleILC Process - ExampleILC Process - Example
Cross section ~ 1 fb at 500 GeV in COMPHEP. Approximate agreement with full calculation.
FNAL Academic Lectures - May, 2006 26
The Higgs Boson PostulatedThe Higgs Boson PostulatedThe Higgs Boson PostulatedThe Higgs Boson Postulated
422 ||||)( V
2/22
~ ( ) ( )V
4~)( V
Potential Lagrangian density
Minimum at a non-zero vev “cosmological term”
This is Landau-Ginzberg superconductivity – much too simple?
FNAL Academic Lectures - May, 2006 27
How the W and Z get their MassHow the W and Z get their MassHow the W and Z get their MassHow the W and Z get their Mass
Covariant derivative contains gauge fields W,Z. Suppose an additional scaler field exists and has a vacuum expectation value. Quartic couplings give mass to the W and Z, as required by the data [ V(r) ~e(exp(-r/)/r) - weak at large r, strength e at small r].
2 2 2 2 2 22 1 2
( )( ) ( )( )
0~
( )( ) ~ / 2 ( ) / 2 (0)W W Z Z
D D
D D g g g e
WWZ
W
MggM
gM
M
cos/2/
2/
0
22
21
2
FNAL Academic Lectures - May, 2006 28
Numerical W, Z Mass PredictionNumerical W, Z Mass PredictionNumerical W, Z Mass PredictionNumerical W, Z Mass Prediction
The masses for the W and Z are specified by the coupling constants. G comes from beta decays or muon decay.
2 2 5 2
2
/ 2 / 8 , 10
/ / 2
2 / 4 , 174
W W
W W
G g M G GeV
M g
G GeV
2
2
sin ~ 0.231, ~ 28.7 , sin 0.481
~ 1/137, / sin ~ 1/ 31.6, ~ 0.63
oW W W
W W Wg
/ 2 ~ 80
/ cos ~ 91W W
Z W W
M g GeV
M M GeV
FNAL Academic Lectures - May, 2006 29
Higgs Decays to BosonsHiggs Decays to BosonsHiggs Decays to BosonsHiggs Decays to Bosons
Field excitations ==> interactions with gauge bosons VVH, VVHH, VVV, VVVV
2( ) / ~ ( /16)( / )H W H WH WW M M M
Higgs couples to mass. Photons and gluons are massless to preserve gauge symmetry unbroken. Thus there is no direct gluon or photon coupling.
2 2 2 2 22 1 2
0
( )( ) ( ) / 2 ( )( ) / 2
H
H W W H Z ZD D g g g
Using the Higgs potential, V(), expanding about the minimum at , and
identifying the mass term in as 2H H HM , we find that the mass is,
.2462 GeVM H Since is an arbitrary dimensionless coupling, there is no
prediction for the Higgs mass in the SM.
, ~ gW2 <>[ W W H ] ~ gWMW [ W W H ].
FNAL Academic Lectures - May, 2006 30
ZZH Coupling and ILC ProductionZZH Coupling and ILC ProductionZZH Coupling and ILC ProductionZZH Coupling and ILC Production
ILC at 500 GeV C.M. Higgs production by off shell Z production followed by H radiation, Z* ->Z+H.
FNAL Academic Lectures - May, 2006 31
Higgs Coupling to FermionsHiggs Coupling to FermionsHiggs Coupling to FermionsHiggs Coupling to Fermions
~ [ ]f L Rg
],[][~ ff mg
2/)/(
]/2[
WfWf
WWfff
Mmgg
gMggm
•The fermions are left handed weak doublets and right handed singlets. A mass term in the Lagrangian, is then not a weak singlet as is required.
•A Higgs weak doublet is needed, with Yukawa coupling,
Yukawa
Mass from Dirac Lagrangian density
Fermion weak coupling constant
( )m
( )L R R Lm
FNAL Academic Lectures - May, 2006 32
Higgs Decay to FermionsHiggs Decay to FermionsHiggs Decay to FermionsHiggs Decay to Fermions
• The threshold factor is for P wave, 2l+1 since scalar decay into fermion pairs occurs in P wave due to the intrinsic parity of fermion pairs.
• The Higgs is poorly coupled to normal (light) matter
• gt ~ gW (mt/ MW)/2 ~ 1.0, so top is strongly coupled to the Higgs.
2 3( ) / ~ (3 /8)( / )H W f WH qq M m M
FNAL Academic Lectures - May, 2006 33
The Higgs Decay WidthThe Higgs Decay WidthThe Higgs Decay WidthThe Higgs Decay Width
The Higgs decay width, scales as MH
3. Thus at low mass, the detector defines the effective resonant width and hence the time needed to discover a resonant enhancement. At high masses, the weak interactions become strong and /M ~ 1.
FNAL Academic Lectures - May, 2006 34
Higgs Width - WW + ZZHiggs Width - WW + ZZHiggs Width - WW + ZZHiggs Width - WW + ZZ
Higgs decays to V V have widths ~ M3
Try this as a
COMPHEP
example
FNAL Academic Lectures - May, 2006 35
Higgs Width Below ZZ ThresholdHiggs Width Below ZZ ThresholdHiggs Width Below ZZ ThresholdHiggs Width Below ZZ Threshold
Below ZZ threshold, decays can occur in the tails of the Breit Wigner Z resonance, with ~ 2.5 GeV, M ~ 91 GeV. This compares to the width to the heaviest quark, b at a Higgs mass of ~ 150 GeV. Means that W*W is an LHC strategy.
FNAL Academic Lectures - May, 2006 36
Early LHC Data TakingEarly LHC Data TakingEarly LHC Data TakingEarly LHC Data Taking
• We have seen that the Higgs couples to mass. Thus, the cross section for production from gluons or u, d quarks is expected to be small.
• Therefore, it is a good strategy to prepare for LHC discoveries by establishing credibility. The SM predictions , extrapolated from the Tevatron, should first be validated by the LHC experimenters.
FNAL Academic Lectures - May, 2006 37
Vector Bosons and Forces Vector Bosons and Forces Vector Bosons and Forces Vector Bosons and Forces
The 4 forces appear to be of much different strength and range. We will see that this view is largely a misperception.