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2
Outline of lectures
I. QCD in p+p collisions
II. Energy loss in Heavy Ion Collisions at high-pT
III. Intermediate pT
Extracting medium parameters
IV. Jet reconstructionOutlook to LHC
3
Part I: perturbative QCD in p+p collisions
• A few words on experiments
• What do we know/understand in p+p– Jet production– Direct photons– Hadron production– Heavy flavour
• Experimental notes: luminosity and triggering
4
Particle Data Group topical reviews http://pdg.lbl.gov/2004/reviews/contents_sports.html
QCD and jets: CTEQ web page and summer school lectures http://www.phys.psu.edu/~cteq/
Handbook of Perturbative QCD, Rev. Mod. Phys. 67, 157–248 (1995)http://www.phys.psu.edu/~cteq/handbook/v1.1/handbook.ps.gz
QCD and Collider Physics, R. K. Ellis, W. J. Sterling, D.R. Webber, Cambridge University Press (1996)
An Introduction to Quantum Field Theory, M. Peskin and D. Schroeder, Addison Wesley (1995)
Introduction to High Energy Physics, D. E. Perkins, Cambridge University Press, Fourth Edition (2000)
General QCD references
5
Heavy Ion references
RHIC overviews:P. Jacobs and X. N. Wang, Prog. Part. Nucl. Phys. 54, 443 (2005)B. Mueller and J. Nagle, Ann. Rev. Nucl. Part. Sci. 56, 93 (2006)
RHIC experimental white papersBRAHMS: nucl-ex/0410020PHENIX: nucl-ex/0410003PHOBOS: nucl-ex/0410022STAR: nucl-ex/0501009
LHC Yellow Reports
6
Experimental facilities: accelerators
Centre-of-mass energies √s:SPS < 20 GeVRHIC 200 - 500 GeVTevaTron 1.9 TeVLHC 5.5 - 14 TeV
Note also:SppS 630 GeV
7
Example detector for DIS
Here: forward electromagnetic calorimeters to measure scattered electron in Deeply Inelastic Scattering
Detectors are designed for specific measurements
8
STAR and PHENIX at RHIC
PHENIXSTAR
Large acceptance at mid-rapidity:TPC tracking(coarse) EMCalSome forward Calorimeters
General purpose detector
Central tracking/calo arms(partial coverage, finely segmented calo)Forward muon arms
Focus on rare probes(electrons/photons)
STAR
(PHOBOS, BRAHMS even more specialised)
PHENIX
9
Barrel: tracking + secondary vertices + PID– Charged particles || < 0.9– Excellent momentum resolution up to 100 GeV/c
(p/p < 6%)– Tracking down to 100 MeV/c– Excellent Particle ID and heavy flavor tagging
EMCal for jet reconstruction– Pb-scintillator, 13k towers– = 107, || < 0.7– Energy resolution ~10%/√E
– Trigger capabilities
PHOS: small acceptance, High granularity EMCal
– High resolution PbWO4 crystals– || < 0.12, 220 < < 320– Energy resolution: E/E = 3%/E
Hard probes in ALICE
Forward muon arm
‘STAR+PHENIX in one’ at LHC
10
QCD and quark parton model
S. Bethke, J Phys G 26, R27
Running coupling:s grows with decreasing Q2
Asy
mpt
otic
free
dom
At low energies, quarks are confined in hadrons
Confinement, asymptotic freedom are unique to QCD
At high energies, quarks and gluons are manifest
gqqee
Theory only cleanly describes certaint limits
Study ‘emergent phenomena’ in QCD
11
Perturbative QCD: a controlled approximation
c
chbbaa
abcdba
T
hpp
z
Dcdab
td
dQxfQxfdxdxK
pdyd
d
0
/222
)(ˆ
),(),(
Parton density functionNon-perturbative: distribution of partons in protonExtracted from fits to DIS (ep) dataRelatively well-known
Matrix elementPerturbative componentCalculated at NLO (s
2) or betterOften need resummed logs (e.g. FONLL)
Fragmentation functionNon-perturbativeMeasured/extracted from e+e-
Convolution: most observables integrate over x, Q2
12
Perturbative QCD processes
• Hadron production• Heavy flavours• Jet production
– e+e- → jets – p(bar)+p → jets
• Direct photon production
Measurem
ent difficulty
The
ory
diff
icul
ty
13
Resolved kinematics inDeep Inelastic Scattering
small x
large x
x = partonic momentum fraction
DIS: Measured electron momentum fixes kinematics
),(2
),(2
14 2
22
2
2
4
2
2
2
QxFy
QxFy
yxQdxdQ
dL
eXep
14
Differential kinematics in p+pExample: 0-pairs to probe low-x
p+p simulation
hep-ex/0502040
Forward pion
Second pion
Resulting x-range
Need at least two hadrons to fix kinematics in p+p
211
ees
px T
16
Testing QCD at high energy
small x
large x
x = partonic momentum fraction
Dominant ‘theory’ uncertainty: PDFs
Theory matches data over many orders of magnitude
Universality: PDFs from DIS used to calculate jet-production
Note: can ignore fragmentation effects
CDF, PRD75, 092006
DIS to measure PDFs
17
Testing QCD at RHIC with jets
Jets also measured at RHIC
However: signficant uncertainties in energy scale, both ‘theory’ and
experiment
STAR, hep-ex/0608030
Note: kinematic range up to 50 GeV
NLO pQCD also works at RHIC
18
Direct photon basics
Production processes– Direct (LO): Compton and
annihilation – Fragmentation (NLO)
direct
fragment
Gordon and Vogelsang, PRD48, 3136 (1993)
Small Rate: Yields
Fragmentation:
20
Direct photons: comparison to theoryP. Aurenche et al, PRD73:094007
Good agreement theory-experiment From low energy (√s=20 GeV at CERN) to highest energies (1.96 TeV TevaTron)
Exception: E706, fixed target FNAL deviates from trend: exp problem?
21
(fragment) / (inclusive)
Experimental access to fragmentation • Two Methods in p+p 200GeV
– Isolation cut ( 0.1*E > Econe(R=0.5) ): identifies non-fragmentation photons– Photons associated with high-pT hadron: fragmentation
PHENIX, PRL98, 012002 (2007)
R E Triggering leadinghadron
Look at associatedphotons
(Isolated)/(all direct)
Only ~10% of show significant associated hadronic activity
22
QCD NLO resources
• PHOX family (Aurenche et al)http://wwwlapp.in2p3.fr/lapth/PHOX_FAMILY/main.html
• MC@NLO (Frixione and Webber)http://www.hep.phy.cam.ac.uk/theory/webber/MCatNLO/
You can use these codes yourself to generate the theory curves!
And more: test your ideas on how to measure isolated photons or di-jets or...
23
0 at lower energies
0 production at lower energies (ISR, fixed target FNAL) not
well described
Good description at RHIC energies
Soft jets at lower √s not well controlled?
C. Bourelly and J. Soffer, hep-ph/0311110
24
Light hadron production at RHIC
NLO calculations: W. Vogelsang
Star, PRL 91, 172302Brahms, nucl-ex/0403005
0 and charged hadrons at RHIC in good agreement with NLO pQCD
PRL 91, 241803
25
Baryon production in p+p @ √s=200 GeV
Albino, Kniehl, Kramer, Nucl Phys B725, 181
Several sets of fragmentation functions (from e+e-) give large differences for baryon production at RHIC
Need to keep track of uncertainties in FF
26
Uncertainty analysis of Fragmentation functionHirai, Kumano, Nagai, Sudo, PRD75:094009
z=pT,h / 2√s z=pT,h / Ejet
Full uncertainty analysis being pursuedUncertainties increase at small and large z
27
Global analysis of FFproton anti-protonpions
De Florian, Sassot, Stratmann, PRD 76:074033, PRD75:114010
... or do a global fit, including p+p dataUniversality still holds
28
Hadron spectraAKK S. Albino, B. A. Kniehl and G. Kramer, Nucl. Phys. B 725 (2005) 181
KKP B. A. Kniehl, G. Kramer and B. PotterNucl. Phys. B 597 (2001) 337
DSS D. de Florian, R. Sassot, and M. Stratmann, Phys.Rev.D75 (2007) 114010 Kretzer S. Kretzer, Phys. Rev. D 62
(2000) 054001
New data up to pT~14 GeVLatest FF fits describe data reasonably well
Extra lesson: don’t ‘just take something’ if you want to do serious physics
29
~factor 2
D0
Non-Photonic Electrons
hep-ex/0609010
CD
F,
PR
L 91
, 24
1804
(2
003)
Theoretical Uncertainty Band
Non-photonic electrons measure charm+bottom
Reasonable agreement with theoryNote: large scale uncertainties
30
Charm from non-photonic electrons
• PHENIX electrons from heavy-flavor decays agree with FONLL pQCD calculation
• STAR electrons, D mesons, muons disagree with FONLL
hep-ex/0609010
Theoretical Uncertainty Band
31
Summary: QCD in p+p collisions
• Testing universality of PDFs, FFs• Jets, photons mainly depends on PDFs: works well• Baryon fragmentation uncertain
– Hadron spectra agree with theory, if you take right FF
• Heavy flavour – Large discrepancy between RHIC experiments– Theory also large uncertainty?
Spectra measurements integrate over large ranges in x, Q2
Di-hadron measurements can be used to select low-x
32
Intermezzo: Luminosity and all that
100 x 100 GeV pp RUN-6 integrated Luminosity (final)
0
5
10
15
20
25
30
35
40
45
50
12-F
eb
4-M
ar
24-M
ar
13-A
pr
3-M
ay
23-M
ay
12-J
un
delivere
d lu
min
osit
y (
pb
-1)
PHENIX pb-1
STAR pb-1
Inte
gra
ted
de
liv
ere
d l
um
ino
sit
y (
pb
-1)
2006 pp @ s = 200 GeV
Improved Collision Luminosity 2006-8
10
50
40
30
20
0
Run7 RHIC AuAu Integrated Luminosity for Physics(singles corrected)
0
500
1000
1500
2000
2500
3000
3500
25-Mar
1-Ap
r
8-Ap
r
15-Ap
r
22-Ap
r
29-Ap
r
6-May
13-May
20-May
27-May
3-Jun
10-Jun
17-Jun
24-Jun
date
Inte
gra
ted
Lu
min
os
ity
[m
b^
-1]
STAR
PHENIX
Lmax
Lmin
MONOp
LARP
Time during runIn
teg
rate
d d
eli
ve
red
lu
min
os
ity
(mb
-1)
2007 Au+Au @ sNN = 200 GeV
Simple question: what do these plots mean?(in practical terms)
L = 45 pb-1 inel = 42 mb
45 1012* 42 10-3 = 1.9 1012 collisions!
L=3200 mb-1 hadr = 7b
2.2 1010 collisions
From S. Vigdor, QM2008:
33
Event rates
L = 45 pb-1 inel = 42 mb
45 1012* 42 10-3 = 1.9 1012 collisions
L=3200 mb-1 hadr = 7b
2.2 1010 collisions
Examples from RHIC
p+p Au+Au
Note <Ncoll> ~ 200
Interaction rate 500-1000 kHz
Interaction rate 5-20 kHz
Recording rates: STAR 100 Hz, PHENIX 5 kHz (?)
Need to trigger, i.e. select ‘interesting’ events
Rate reduction: 1000-10000 for p+p, 10-100 for Au+Au
34
High-pT triggers
Fast detectors (measure up to a few MHz)– Obvious choice: (EM) calorimeter
For example: Keep all events with a photon > 7 GeV, rate few Hz at RHIC
Two strategies:– Small fiducial, trigger photons– Larger fiducial, trigger 0, ‘jet’ energy
Very suitable for high-pT/hard physics
Trigger sees all 1012 events
36
0 in p+p, d+Au
M. Russcher
2005 p+p
STAR gearing up , 0 in p+p, d+Au
Good agreement with NLO pQCD and PHENIX
PHENIX, B. Sahlmüller
RdA centrality dependence
Measures Cronin, initial state effects
nucl-ex/0610036
38
fiber optic links
mwave links
Plan to Implement and Test Stochastic Cooling of Heavy Ion Beams at RHIC
(submitted to DOE 12/31/07) Test combined effect of long. &
transverse stochastic cooling for one beam in 2009 run.
If results follow detailed simula-tions, full implementation by 2011.
Simulations long. + trans. stochastic cooling + 56 MHz SRF for both beam goes ~2/3 way (with present bunch intensity) to RHIC-II projected L at order of magnitude less cost, ~5 years quicker than e-cooling.
“RHIC-II” goal
Simulated effects of beam cooling for full-energy Au+Au
Present intensity, no cooling
Present intensity, full stochastic
Present intensity,
e-cooling
Intensity x 1.5, full stochastic
Intensity x 1.5, e-cooling
39
What Are Jets ?
Colored partons from the hard scatter evolve via soft quark and gluon radiation and hadronization process to form a “spray” of roughly collinear colorless hadrons → JETS
The hadrons in a jet have small transverse momenta relative to their parent parton’s direction and the sum of their longitudinal momenta roughly gives the parent parton momentum Keep in mind that there are particles in a jet originating from other partons in the event
Jets manifest themselves as localized clusters of energy
Jet
outgoing parton
Fragmentation process
Hard scatter
colorless states - hadrons -
R ( ) ( ) 2 2coneR
Jets are the experim
ental signatures of q
uarks and gluons
They are expected to re
flect k
inematics and to
pology of parto
ns
Really, je
ts are what je
t algorit
hm defines th
em to be!
40
Probing differential kinematicsExample: 0-pairs to for low-x
FMS plots
hep-ex/0502040p+p simulation d+Au simulation
Sensitive down to xg ~ 10-3 (few 10-4 in CGC scenario)
Measure gluon density at low x in cold nuclear matter Can distinguish shadowing (suppression of yields) and CGC (‘monojets’)
FMS group
41
Direct at high-pT
T. Isobe
p+p year-5
RHIC is accumulating p+p stats
0-10% Au+Au
Nuclear effects + E-loss (frag )
Quark- in-medium conversions
No enhancement in Au+AuAgrees with NLO pQCD
42
Particle Ratios
• Ratios extended to 15 GeV/c• The effect of the jet trigger on the ratios is negligible (comparison
between Pythia minimum bias and Pythia jet triggered data)
43
π and p Spectra
• Spectra compared to NLO pQCD calculations
AKK S. Albino, B. A. Kniehl and G. Kramer, Nucl. Phys. B 725 (2005) 181
KKP B. A. Kniehl, G. Kramer and B. PotterNucl. Phys. B 597 (2001) 337
DSS D. de Florian, R. Sassot, and M. Stratmann, Phys.Rev.D75 (2007) 114010 Kretzer S. Kretzer, Phys. Rev. D 62 (2000) 054001