photon-jet correlations at rhic
DESCRIPTION
Photon-Jet Correlations at RHIC. Saskia Mioduszewski Texas A&M University. 18 July, 2007. Outline. What can be learned from g -jet measurements? How to measure? Current Status of Measurement at RHIC. Dominant. g. q. γ. q. g. γ. q. g. q. Bremsstrahlung. Why g -jet?. q. - PowerPoint PPT PresentationTRANSCRIPT
Outline
• What can be learned from What can be learned from -jet -jet measurements?measurements?
• How to measure?How to measure?
• Current Status of Measurement at RHICCurrent Status of Measurement at RHIC
Why -jet?q
qg
γ q
q g
γ
Compton Annihilation
q
q
q
q
g
g
g
γγ
Bremsstrahlung
“Golden Probe” of energy loss - calibrated probe of jet energy - X.-N. Wang et al.
Gluon jet vs. quark jet energy loss – compare -jet to 0-jet (in -jet, the jet will mostly be from quarks) - need to understand the surface bias to interpret data !
Dominant
What can be learned?
• Ultimate goal is to understand energy loss mechanism
• Complementary to single particle spectra and di-jets
• No surface bias for trigger particle, different surface bias for -jet coincidence
Single-Particle Spectra – What have we learned?
Hadrons are suppressed by factor ~5, Photons are not
Single-Particle Spectra – What have we learned?
Hadrons are suppressed by factor ~5, Photons are not
PHENIX, Phys. Rev. Lett. 96, 202301 (2006)
PHENIX 0 Spectrum
Fractional “effective” energy loss Sloss ~ 20% in most central Au+Au collisions
PHENIX preliminary
pedestal and flow subtracted
4 < pT,trig< 6 GeV/c, 2< pT,assoc< pT,trig
Di-Jets through Hadron-Hadron Correlations
“Disappearance of away-side jet” in central Au+Au collisions
0-5%
Escaping Jet“Near Side”
Lost Jet“Far Side”
STAR, PRL 90 (2003) 082302
“Reappearance of away-side jet”
With increasing trigger pT, away-side jet correlation reappears
STAR, Phys. Rev. Lett. 97 (2006) 162301
Higher pT Jet“Near Side”
“Punch-through” Jet?
“Reappearance of away-side jet”
With increasing trigger pT, away-side jet correlation reappears
STAR, Phys. Rev. Lett. 97 (2006) 162301
Tangential emission?
Surface Bias of Di-Jets?
8 < pT,trig< 15 , 4< pT,assoc< 6 GeV/c
8 < pT,trig< 15 GeV/c
STAR, Phys. Rev. Lett. 97 (2006) 162301Renk and Eskola, hep-ph/0610059
BDMPS-style energy loss + evolving bulk system
What can be learned?
• Di-jets suffer surface bias of trigger jet, punch-through of away-side (or only tangential emission)
• -Jet trigger photon has no bias, but existence of away-side jet creates a (different) bias
Measurement of % transmission as a function of true jet energy
q
Challenging Measurement
• Trigger photon measured with electro-magnetic calorimeter
• Large background from hadronic decays (0, )
• Background sources of photons (hadronic decays) suppressed in central Au+Au collisions
PHENIX, Phys. Rev. Lett. 94, 232301 (2005)
Challenging Measurement
• Trigger photon measured with electro-magnetic calorimeter
• Large background from hadronic decays (0, )
• Background signal is di-jet (0-jet)
• Subtract from inclusive signal
• Need large-statistics data set for -jet measurement
Statistical measurement of -jet yields
• Measure inclusive -jet correlation function
• Measure 0-jet (-jet) correlation function
• Construct resulting decay-jet correlation
taking into account decay kinematics
• Subtract decay-jet from inclusive-jet
Result is direct-jet
PHENIX -jet in p+p
PHENIX Preliminary PHENIX Preliminary
J.Jin, QM 2006
Comparison to PYTHIA – verification of method
Direct -h YieldsRun 5 p+p @ 200 GeV
5-7 X 1-2 GeV/c 7-9 X 1-2 GeV/c
5-7 X 2-5 GeV/c 7-9 X 2-5 GeV/c 9-12 X 2-5 GeV/c
9-12 X 1-2 GeV/c
• Signature small near-side correlation signal apparent
• Yield sensitive to contribution at the near-side
• New corrected results consistent with QM result within systematic error
• Still room for some fragmentation contribution
M. Nguyen, APS 07
Cu+Cudirect-h+/- vs. -h+/- jet yields
per-trigger jet pair yields: systematic from R
systematic from subtraction method
A. Adare, WWND 2007
Distinguishing direct photons from 0
pT (GeV/c)
Op
enin
g a
ng
le (
rad
ian
s)
Opening angle of 0 as a function of pT
• Segmentation of calorimeter towers in STAR () = (0.05,0.05) 2 decay photons hit same tower starting pT ~ 5 or 6 GeV/c
• Segmentation in PHENIX ~ 0.01 radians
Distinguishing direct photons from 0
• Reject clusters that look like 2 close photons (from 0 decay) from shower shape
• Retain sample of correlations that are direct-jet “rich”
• Estimate remaining contamination from 0-jet
• Measure and subtract 0-jet away-side yield
Distinguishing single photons from 2 decay photons in STAR
Shower-max detector
()~(0.007,0.007)
A. Hamed, Collective Dynamics 2007
STAR -jet in p+pSubhasis Chattopadhyay, QM 2006
-- Improved 0/ separation using shower profile in SMD
0
0 bin
mixed bin
photon bin
STAR -jet in p+p
Subhasis Chattopadhyay, QM 2006
EEtttrigger trigger from 8.5GeV/c to 10.5 GeVfrom 8.5GeV/c to 10.5 GeV
Comparison to HIJING p+p –
verification of method
Next Steps
• Do similar analysis for Au+Au collisions as was done in p+p and d+Au
• Challenge within large-multiplicity background
• Run-7 results coming soon
• Results must be interpreted together with di-jet results and/or within model to take surface bias into account
Summary
• Di-Jets’ surface bias results indicate jets are either transmitted with negligible energy loss or absorbed completely
• Photon-Jet Measurement will complement the di-jet for more complete probe
• A significant (statistically and systematically) -jet Measurement in Au+Au is needed
• Need a great deal of statistics!• Stay tuned for the results from Run-7….
Increase in statistics over Run-4 Au+Au > factor of 10