1 Introduction to Deep Inelastic Scattering (DIS) Rik Yoshida Argonne National Laboratory CTEQ...
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Transcript of 1 Introduction to Deep Inelastic Scattering (DIS) Rik Yoshida Argonne National Laboratory CTEQ...
1
Introduction to Deep Inelastic Scattering (DIS)
Rik YoshidaArgonne National Laboratory
CTEQ summer school 07May 30, 2007
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Some preliminary remarks• This is not a historical review
– for a very nice historical review see EnricoTassi’s lectures from 2003:
• http:://www-zeus.desy.de/~tassi/cteq2003.ppt• Nor a review of experimental status
• Enrico’s second lecture (same place)• Max Klein’s DIS lecture from CTEQ 2006
• Nor a theoretical discussion– Morning lectures from George Sterman
• Aim: to leave you with some intuitive feeling for what is happening in Deep Inelastic Scattering (DIS). Going to stick to electron- (positron-) proton DIS
3
Partons in the protonFeynman’s parton model: the nucleon is made up of point-like constituents (later identified with quarks and gluons)which behave incoherently.The probability f(x) for the parton f to carry the fractionx of the proton momentum is an intrinsic property of thenucleon and is process independent.
If I were thinking about an experiment where wecollide protons with protons at, say, 14 TeV: then this is great! Because:
-Protons are just a “beam of partons” (incoherent)-The f(x)s, the “beam parameters”, could be measured in some other process. (process independent)
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Quarks and Gluons as partons
∫x[u(x)+u(x)+d(x)+d(x)+s(x)+s(x)+….]dx = 1
u(x) : up quark distributionu(x) : up anti-quark distributionetc.
Momentum has to add up to 1 (“momentum sum rule”)
Quantum numbers of the nucleon has to be right
∫[u(x)-u(x)]dx=2 ∫[d(x)-d(x)]dx=1
∫[s(x)-s(x)+……]dx=0
So for a proton:
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DIS kinematicsep collision proton in “∞” momentum frame
√s = ep cms energyQ2=-q2= 4-momentum transfer squared (or virtuality of the “photon”)
No transversemomentum
x = fractional longitudinal momentum carried by the struck parton
0 ≤ x ≤ 1
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DIS kinematicsep collision
Q2=-q2=-(k-k’)2=2EeE’e(1+cosθe)
x =Q2/2P•q = Ee E’e (1+cosθe)EP 2Ee-E’e(1-cosθe)
Initial electron energyFinal electron energy
Initial proton energy
Electron scattering angle
Everything we need can be reconstructed from themeasurement of E’e and θe. (in principle)
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Deep Inelastic Scattering experiments
Fixed target DIS at SLAC, FNAL and CERN completed ~ 10-20 years agoHERA collider: H1 and ZEUS experiments 1992 – 2007 (will complete July 2, 2007)
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e-p Neutral Current (NC) cross-section:
d2σ 2πα2
dxdQ2 xQ4 [Y+F2(x,Q2)-y2 FL(x,Q2)+Y-xF3(x,Q2)]=
y=Q2/xs 0 ≤ y ≤ 1 “inelasticity” Y±=1±(1-y)
Has to do withZ0 exchange:small for Q<<MZ
Has to do withlong. photon. Only large at largest y
We’ll come backto these
d2σ 2πα2
dxdQ2 xQ4= Y+F2(x,Q2)
So for now:
F2 = x∑(q + q) eq + Z-exchangequark charge
quark and anti-quark distributions
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The partons are point-like and incoherentthen Q2 shouldn’t matter. Bjorken scaling: F2 has no Q2 dependence.
IF, proton was made of 3 quarks each with 1/3 of proton’smomentum:
F2 = x∑(q(x) + q(x)) eq
no anti-quark!
F2
1/3 x
q(x)=δ(x-1/3)
or with some smearing
Let’s look at some data
2
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Proton Structure Function F2
F2
Seems to be….NOT
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So what does this mean..?
QCD, of course:
quarks radiate gluons
q
q
gluons can produce qq pairs
gluons can radiate gluons!
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r≈ hc/Q = 0.2fm/Q[GeV]
rγ*(Q2)
Virtuality (4-momentum transfer) Q gives the distancescale r at which the proton is probed.
~1.6 fm (McAllister & Hofstadter ’56)
CERN, FNAL fixed target DIS: rmin≈ 1/100 proton dia.HERA ep collider DIS: rmin≈ 1/1000 proton dia.
e
e’Proton
HERA: Ee=27.5 GeV, EP=920 GeV
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Higher the resolution (i.e. higher the Q2) more branchingsto lower x we “see”.
So what do we expect F2 as a function of x ata fixed Q2 to look like?
F2
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1/3
1/3
1/3
F2(x)
F2(x)
F2(x)
x
x
x
Three quarks with 1/3 of total proton momentum each.
Three quarks with some momentumsmearing.
The three quarks radiate partons at low x.
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Proton Structure Function F2
How this change with Q2 happens quantitatively described by the:
Dokshitzer-Gribov-Lipatov-Altarelli-Parisi (DGLAP) equations
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DGLAP equations are easy to “understand” intuitively
First we have the four “splitting functions”
z z z z
1-z 1-z 1-z 1-z
Pab(z) : the probability that parton a will radiate a parton b with the fraction z of the original momentum carried by a.
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= αs [qf × Pqq + g × Pgq]
Now DGLAP equations (schematically)
dqf(x,Q2)d ln Q2
convolution
strong coupling constant
Change of quark distribution q with Q2 is given by the probability that q and g radiate q.
dg(x,Q2)= αs [∑qf × Pqg + g × Pgg]d ln Q2
Same for gluons:
o o
o o
18
DGLAP fit (or QCD fit) extracts the partondistributions from measurements. (Lectures by Jeff Owens next week)
Here’s a 1 min description: Step 1: parametrise the parton momentum desity f(x) at some Q2. e.g.
uv(x) u-valence dv(x) d-valence g(x) gluon S(x) sum of all “sea” (i.e. non valence) quarks
Step 2: find the parameters by fitting to DIS (andother) data using DGLAP equations to evolve f(x) inQ2.
“The orginal three quarks”
f(x)=p1xp2(1-x)p3(1+p4√x+p5x)
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Sea PDF
x
xS
At x<<1/3, quarks and (antiquarks) are all “sea”.Since F2 = eq ∑x(q + q), xS is very much like F2
Fractionaluncertainty
2
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Gluon PDF
x
xg
Gluons, on the other hand, are determined fromthe scaling violations dF2/dlnQ2 via the DGLAP equations.
Uncertainties are larger.Scaling violations couple αs and gluon g
Fit with αs alsoa free param.
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So far:
F2 ~ ∑(q+q) ≈ S (sea quarks) measured directly in NC DIS
Scaling violations
dF2/dlnQ2 ~ αs•g Scaling violations gives gluons (times αs). DGLAP equations.
What about valence quarks?
∑(q-q) = uv + dv can we determine them separately?
Can we decouple αs and g ?
22
Return to Neutral Current (NC) cross-section:
d2σ(e±p) 2πα2
dxdQ2 xQ4 [Y+F2(x,Q2) Y-xF3(x,Q2)]=Y±=1±(1-y)
±
Now write out the e+p and e-p separately
xF3 = ∑(q(x,Q2)-q(x,Q2)) xBq ~The valence quarks!
Bq = -2eqaqaeχZ+ 4vqaqveaeχZ2
χZ= ( ) Keeps xF3 small if Q<MZ1 Q2
sin2θW MZ+Q22
(keep ignoring FL for now..)
Bq = -2eqaqaeχZ+ 4vqaqveaeχZ2
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Return to Neutral Current (NC) cross-section:
d2σ(e±p) 2πα2
dxdQ2 xQ4 [Y+F2(x,Q2) Y-xF3(x,Q2)]=Y±=1±(1-y)
±
Now write out the e+p and e-p separately
xF3 = ∑(q(x,Q2)-q(x,Q2)) xBq ~The valence quarks!
Bq = -2eqaqaeχZ+ 4vqaqveaeχZ2
(keep ignoring FL for now..)
Bq = -2eqaqaeχZ+ 4vqaqveaeχZ2
eq: electric charge of a quarkaqvq: axial-vector and vector couplings of a quarkaeve: axial-vector and vector couplings of an electron
γ-Z interference Z-exchange
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Return to Neutral Current (NC) cross-section:
d2σ(e±p) 2πα2
dxdQ2 xQ4 [Y+F2(x,Q2) Y-xF3(x,Q2)]=Y±=1±(1-y)
±
Now write out the e+p and e-p separately
xF3 = ∑(q(x,Q2)-q(x,Q2)) xBq ~The valence quarks!
(keep ignoring FL for now..)
Let’s look at the “reduced NC cross-section”
σNC± = F2(x,Q2) (Y-/Y+)•xF3(x,Q2)±
Note the change of sign from e+p to e-p
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σNC±
xMeasurements are at relatively high x
Reduced Neutral Current Cross-section
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Recent (Spring 07) preliminary result from HERA
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Charged Current Cross-Sections
dσCC(e±p) GF MW dxdQ2 2πx MW+Q2= [ ]2σCC±
2
2 2
Skip a few steps….
σCC+ = x [u + c + (1 - y)2(d + s)] ~ d
σCC- = x [u + c + (1 – y)2(d + s)] ~ ucharm
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σCC±
Reduced Charged-Current Cross-Section
x
σCC+ ~ d σCC- ~ u
Now let’s look at the valence quarks from the QCD fits
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Valence PDFs
x
xf
The momenta from valence quarks are producinggluons and sea quarks at low x
30
Jet production in DIS (HERA)
Sensitive to αs
Sensitive to gluon ~10-3 < x < ~10-2Sensitive to quarks
~10-2 < x < ~10-1complementaryto gluon from F2
Same range as NC and CC
σjet ~ αs•f(x)
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No ET in Breit Frame
Jet production cross-section used in QCD fit
Jet measurements in Breit frame
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Gluon distributions
x xUsing only HERA (ZEUS)data including NC,CC and jets
Using HERA (ZEUS) F2 dataand FNAL, CERN fixed tgt
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Finally…
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Proton Structure Function F2
F2
Now we understand what is happening here.
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Some remarks about DGLAP equations:
But now parton densities must be “evolved” in Q2.
What does this mean?
The “incoherence” of the original parton modelis preserved. i.e. a parton doesn’t know anythingabout its neighbor.
never happens
The “process independent” partons also survive.
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A parton at x at Q2 is a source of partons atx’ < x at Q’2 > Q2.
x
Q2
Q’2
x’
In fact, any parton atx > x’ at Q2 is a source.
To know the parton densityat x’, Q’2 it’s necessary(and sufficient) toknow the parton densityin the range: x’ ≤ x ≤ 1at some lower Q2.
1
measured
known
unkn
own
What does this mean for the LHC?
If you know the partons in range x’ ≤ x ≤ 1 at some Q2,then you know the partons in the range x’ ≤ x ≤ 1 for allQ’2 > Q2.
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Fixed targetDIS
HERA DIS
Tevatron jets
~safe Q2
“known”
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2 4
parton1(x1) + parton2(x2) State with mass M
LHC (or hadron-hadron) parton kinematics
x1= (M/√s) exp (y) x2= (M/√s) exp (-y)
y= ln( )1 E+PZ2 E-PZ
rapidity:
pseudo-rapidity:
η=-ln tan(θ/2)
angle wrt beam
39
2 4
So if I want to predict Z or W productioncross-section at LHC at some rapidity y, say, -4:
q,q(x1=10-4,Q2=MW,Z) q,q(x2=0.3,Q2=MW,Z)
need
2 2
and
σ(ppW,Z+X) ~ q,q(x1,MW,Z) × q,q(x2,MW,Z) × σ(qqW,Z)22
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xf(x)
xS(x)xg(x) “measured”
“mea
sure
d”“evolved”xg(x)xS(x)
Evolving PDFs up to MW,Z scale
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-6 6
σ(ar
b. sc
ale)
η
Z production at LHC
Uncertainty ~5%
A. Cooper-Sarkar (HERA-LHC workshop 2007)
Jet production at LHCExamples of predictions for LHC using partons from DIS
42
Final remarks I• We’ve just gone through an informal tour of QCD-improved
parton model and its application to data from ep Deep Inelastic Scattering.
• Some health warnings:– Most of what I talked about is a leading-order picture. In
practice, most things are done at least to next-to-leading order. At NLO, the interpretation of the results are not as straight-forward.
– Many people worry about whether we are not missing something fundamentally with the picture of DGLAP equations.
• Much of the data are at very low x: DGLAP is a lnQ2 approximation. Why aren’t ln(1/x) terms important…or are they? BFKL equations.
• The density of the partons, especially that of the gluons is getting very high. When and where should we worry about “shadowing”, “gluon recombination” etc.
• The idea of incoherence of partons may be breaking down in some kinematic regions: phenomenon of “hard diffraction” is difficult to understand in terms of partons without correlations to each other.
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Final remarks II• There are many other DIS physics topics I did not cover
here.• Electoweak physics• Heavy quark production• Diffraction, Vector Meson production, low Q2 physics• Beyond the SM searches.• Polarized DIS• …
• I hope I have refreshed your memory about some familiar DIS physics, and got you ready for the rest of the school.
• Thanks to the organizers for their kind invitation. Thanks to Claire Gwenlan for preparing some of the plots animation for me.
– You can find the animated gifs in:• http://www.hep.anl.gov/ryoshida/animated_proton.htm
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Extras (FL)
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FL=(Q2/4π2α) σL
Longitudinal cross-section
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QCD predicts a relationshipbetween scaling violationsand FL through the gluondensity.
increasing y
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You can determineFL from a NLO DGLAPfit to NC cross-section.
x
Indeed, we also only determineF2 the same way, in principle:
We measure this only
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C. Diaconu: DIS 07 conference April 07
HERA measurement of FL on-going nowNormally 920 GeV