W and Z production at the Tevatron

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So what are gluons?
The force carrier of QCD
What is the evidence for colour?
What is the evidence for gluons?
ATLAS 2010
A M Cooper-Sarkar
Jan 2011
Gemma (Trigger representative for ATLAS Higgs group
Sinead (VBF convenor for LHC cross-section working group)
Elias (Editor of ATLAS Z →τ τ documentation
QED (electrons
and photons)
QCD (quarks
and gluons)
q
e+
e-
q
e+
e-
γ
q
And here are some
pictures of quarks,
gluons, electrons
and photons from
LEP @ CERN
1989-2000
e+ e- annihilation.
Illustrating that
partons behave
similarly to the pointlike electron and
photon
q
You don’t see the quark or gluon emerge instead you see a jet: a
“blast” of particles, all going in roughly the same direction.
QCD is a locally gauge invariant field theory like QED
For QED this means
Where q is the charge and θ is a space-time dependent
phase. The QED Lagrangian is
U(1)
with
and
The interaction between the fermions and the field is in
the covaraint derviative
The quark part of theQCD Lagrangian is
With
where taij
are hermitian matrices = λaij /2.
This describes the qqg interaction
For QCD
Where g is the strong charge and t.θ is the product of
the colour group generators with a vector of space-time Where quarks now have colour indices
phase functions in colour space.
i=1,2,3 (R,G,B) as well as flavour indices
SU(3)
f.
The group generators t satisfy
The gluon fields A have a=1-8 flavour
indices......
Where fabc are SU(3) structure constants.
f123=1, f147=f246=f257=f345=1/2,f156=f367=1/2,f458=f678=√3/2
The Gell-Mann λ matrices are given by
The colour exchange in q q g
diagram can be thought of like this
SO the gluon has colour red- antigreen:
r-gbar
Obviously
r-bbar, g-rbar, g-bbar, b-gbar, b-rbar
and the combinations
(r-rbar - g-gbar)/√2,
(r-rbar + g-gbar – 2b-bar)/√6
and
are also possible
(r-rbar + b-bar + g-gbar)/√3
In the mathematics of SU(3) this is 3 * 3 = 8 + 1
And the last combination is the singlet– which is not coloured at all,
hence eight coloured gluons
(Think of SU(2) 2*2=3+1 -triplets and singlets- in atomic physics if this puzzles you)
The second part of the QCD Lagrangian is purely gluonic
Where
The difference from QED is the A A term which is what makes gluons interact with gluons
(NON-Abelian) with both a g-g-g vertex and a g-g-g-g vertex
The colour flow is more
complex for these vertices ~
twice as strong as for q-q-g
This extra term is also what makes QCD gauge invariant under local SU(3) transformation
Perturbative QCD involves an order by order expansion in a small coupling
αS = g2 /4π << 1 and calculations are made using Feynman diagrams. The rules for the
vertices have already been shown.
The main complication in comparison to QED is the need for colour factors.
After squaring an amplitude and summing over colours of incoming and outgoing
particles the colour factors often appear in one or other of the following combinations:
Where the final diagram gives the Fierz indentity- a mathematical formulation of
the colour flow.
See page 38/39 Devenish and Cooper-Sarkar for a simple colour factor
calculation
To go to QCD e4 must be replaced
And the colour factor from the loop insertion CF=4/3
Consider QED Compton scattering with
one virtual photon
And using the Golden rule to got to the crosssection via the phase space factors
The QCD analogue is QCDC and the kinematic
invariants are
A further important process is Boson-Gluon
Fusion BGF
The amplitudes for the two QED diagrams are
Adding squaring and taking care of spins
Devenish and Cooper-Sarkar p40-43
which, similarly, has the cross-section
Contributions to the perturbative expansion of
scattering amplitudes beyond the leading order
are often divergent, e.g for QED
For many loops the effect of summing the
‘leading logs’ can be accounted for by
redefining the coupling
We must remove the dependence on Λ and
α0 by defining the coupling at some scale μ2
and writing its value at all other scales Q2 in
terms of this (‘renomalisation’ )
The loops are divergent beacuse of unrestricted
integration over momentum in these loops
We have to renormalize the theory. This is done
by making constants of the theory like the
coupling α become dependent on the scale of
the process. It is sucessful if this takes care of
ALL the infinities to all orders.
Thus for Q2>μ2 the coupling increases
And indeed the 1/137 you are used to at low
energies becomes 1/125 at the scale of MZ2
This can be understood qualitatively in terms
of charge screening
For one loop the fermion propagator
becomes
What of QCD?
where
Λ is a high momentum cut-off and α0 is the bare
e.m. charge
What of QCD?
There is another type of loop diagram.
Both contributions diverge logarithmically but with
opposite sign
The QCD coupling is renormalised as
Where
at leading order.
Note the quark loop gives 1/6π for each flavour
of fermion (nf) – this is like the 1/3π of QED bar a
convetional factor of 2. The new feacture is the
33/12π of the gluon loop which swaps the sign
Gives us anti-screening
Or ASMYPTOTIC FREEDOM
The coupling decreases as the scale goes up
At high energies we may make perturbative
caluclations
At low- energies we can’t and we have
CONFINEMENT
Let us apply some of this to the parton model
and the γ*p cross-section is
=
Now let’s add these diagrams
The hard cross section here is just the
QCDC diagrams so
The convolution of a probability of finding a parton
in the proton with a hard scattering cross-section.
The γ*quark interaction cross-section is
Where
where
So if c=cosθ
so
gives the QPM parton model result
There are singularities at c=1, z=1.
z=1 is an infra-red singluarity that is
cancelled by other terms
c=1 corresponds to the gluon being
emitted collinearly. The residue at the
pole is
Do the integration in terms of the gluon (or quark
transverse momentum in the CMS
Gives
Redefine the parton density
Where
Where
But the pt integral also needs a lower cut-off to
regulate it so
Essentially gluon radiation introduces non zero
pt and integrating over it gives log terms.
Define
The next step is to ‘renormalise’ the parton
density by choosing a factorisation scale
at which to define the parton density
Thus the bare parton density becomes a
renormalised parton density which depends on
the scale at which it is observed. The collinear
singularity is absorbed into the parton density
As the probability for a quark to split into a quark
and a gluon
then
and
Where the log term is dominant.
if Q2=μ2 is the factorisation scale then
NOW add this term to the QPM result
The renormalised parton density qi(x,μ2) cannot
be calculated perturbatively (soft non perturbative
physics has been absorbed into it) but we do
know how it evolves with scale
And introducing an infra-red cut-off and a bare
gluon density gives
where
Except that we still have to add on the BGF
processes
Is the probaibility for a gluon to split into a qqbar pair
Regularising the cut-off in this extra
contribution to F2 gives us an extra
contribution to qi(x,μ2) such that its evolution
with scale is given by
where the extra term depends o a
renormalised gluon denisty. The expression
for F2 then remains as
Writing the angular integral in terms of pt
Probable end lecture 2
So F2(x,Q2) = Σi ei2(xq(x,Q2) + xq(x,Q2))
in LO QCD
And the theory predicts the rate at which the parton distributions (both quarks and
gluons) evolve with Q2- (the energy scale of the probe) -BUT it does not predict
their starting shape
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