Transcript Document

The STAR experiment
-jet Measurements
Table of Contents:
Motivation
STAR QM2005 && QM2006
Experimental setup
Data and Analysis Method
Transverse Shower Profile
Results and Interpretation
Summary
Quark Matter 2008, February 4-10, Jaipur, India
Texas A&M group
Ahmed M. Hamed
Jaipur 02-08-08
Energy loss
Motivation
Inclusive particle spectra at mid-rapidity:
Heavy quarks suppress as much as light quarks in the medium.
No observation confirms the expected color factors effect in energy
loss .
•Parton Distribution Function
•Fragmentation Function
•Intrinsic KT
• Hard-Scattering
•Shadowing
•Partonic energy loss
Forms of energy loss, s(T)?
D0h/a(Z)->Dh/a(z,E)
Jet-like azimuthal correlations
Motivation
Charged-Charged hadrons correlation
Similar near side yield for jet-like yield per trigger in pp/AuAu
The away-side in AuAu is strongly suppressed compared to pp and dAu.
4 < pT,trig< 6 GeV/c, 2< pT,assoc< pT,trig
0-5%
STAR, PRL 90 (2003) 082302
STAR PRL 97 (2006) 162301
How Neutral-Charged correlation looks like?
Motivation
direct component
Direct photons
fragmentation component
Bremsstrahlung
No near side in gamma-jet correlation
This contribution is negligible
oGamma-charged hadrons correlation.
 Calibrated probe of the QGP – at LO.
 No Surface Bias
 Hard process

Possible discriminator for quark/gluon jet at LO.
How about neutral pions?
Motivation
In AuAu 0 –spectra are suppressed by a factor of ~5 relative to
the scaled p+p collisions.
The away-side in di-jet production is more suppressed.
Direct photons and 0 yields are similar in AuAu at
~10GeV
Background sources of direct photons suppressed in medium.
What are the expectations from previous measurements?
STAR QM2005
AuAu@200GeV, Thomas Dietel
Pythia
Simulation shows
no associated
particles in the
near-side of -jet
correlations.
Run2004
( 30 ub-1 ) of AuAu@200GeV
Suppression in both near- and away-side yield in central bin compared to peripheral bin.
Correlations of charged particle show no modification of the associated near-side yield.
Need /0 discrimination.
STAR QM2006
pp@200GeV, S. Chattopadhyay
Shower shape analysis is used for /0 discrimination.
Reduction in near angle peak towards photon Bin.
Effect is more prominent for larger Ettrigger .
Away-side yield is reduced.
What about AuAu?
pp2005?
Experimental setup
Tracker detectors(slow),
Trigger detectors(fast),
and Calorimeters(fast).
Measurements of hadrons
production over a large
solid angle.
STAR BEMC can probe for
further higher transverse
energy.
STAR Detector
Experimental setup
STAR BEMC
-plane
Electromagnetic transverse
shower characteristics
High energy core.
Low energy halo.
STAR BSMD can distinguish between /0 up to pt~26GeV/c
Data and analysis method
Run2007
Online:
Trigger on cluster of one or two towers with
Et>7.54GeV
oData in Run2007( ~590 ub-1 )
Offline:
Photon candidates “trigger particles”
Trigger particle as of Et>8GeV in one or two adjacent
towers.
Trigger particle as of E>0.5GeV in one of BSMD
strips.
Charged
particles veto as
op>3GeV o<0.025 <0.025
of:
Tracks “associated particles”
Number of fit points
Number of fit
points/number of possible points
>20.
>0.52
Pt>3GeV/c
Correlate photon candidates “triggers” with associated tracks
Correct for tracking efficiency Subtract elliptic flow
Use Transverse Shower Profile for /0 identification.
Extract -jet away side yield
Systematic study of:
track veto cut, /0 identification, etc..
Transverse Shower Profile
Transverse shower profile figure is here
Results and interpretation
Neutral-Charged hadrons correlation
oNear side is suppressed in central bins compared to peripheral bins due to the
increase of /0 ratio .
oSuppression in near side increases with trigger energy.
Results and interpretation
Et trigger effect
o(enriched sample)-jet correlation near-side is suppressed compared to 0-jet near-side.
o0-jet correlation near-side increases with Et of the trigger particle
o(enriched sample)-jet correlation near-side shows no dependence on Et
of the trigger particle
Results and interpretation
Et trigger effect
o(enriched sample)-jet correlation near-side is suppressed compared to 0-jet near-side.
o0-jet correlation near-side increases with Et of the trigger particle
o(enriched sample)-jet correlation near-side shows no dependence on trigger particle Et.
o(enriched sample)-jet away-side is suppressed compared to 0-jet away-side at
same centrality and Et.
Results and interpretation
Medium effect
oClear away-side suppression in the medium.
o(enriched sample)-jet correlation near-side shows no centrality dependence.
Results and interpretation
Extraction of 0 and -rich yields
1. Fit with 2-guassian and polynomial
2. Near-side yield=||<0.63, Away-side yield=|-|<0.63
Results and interpretation
Comparison of 0 associated yields with charge associated yields in pp and dAu respectively
Two different data sets: pp2006 and dAu2003
Complete different analysis techniques
oGood agreement in the away- and near- side yields of the associated particles.
Results and interpretation
Comparison of 0 associated yields with charge associated yields in AuAu
oGood agreement with previous STAR published analysis
Results and interpretation
Comparison of 0 associated yields with charge associated yields in AuAu
oGood agreement with previous STAR published analysis in the common pt_assoc. bins.
Results and interpretation Et dependence of 0 and -rich sample
oNear-side yield of -rich sample shows no
Et dependence.
oNear-side yield of 0 shows slight increase with
trigger Et.
Results and interpretation
Extraction of corrected  away-side yields
1. R=(-rich-hadron yields/pi0-hadron yields)near-side
2. f= (pi0-hadron yields)away-side *R.
3. -corrected yields=[(-rich-hadron yields)away-side-f]/(1-R)
oGood match with STAR results at QM2006 in the region of overlap.
Results and interpretation
corrected  away-side yields in AuAu
o away-side yield is smaller than 0 away-side yield.
o away-side yield is harder than 0 away-side yield.
Results and interpretation
 IAA
Summary