Title: Rapidity Asymmetry in d A Collisions
1Jet Tomography of Hot Dense Matter
Jet
Xin-Nian Wang LBNL, June 25, 2003
2Equation of States
F. Karsch 2001
QGP
Hadrons
Quarks(2x3x2x2)
Gluons(2x8)
3Medium Response Function
4Computed Tomography (CT)
Calibrated source
Jet Tomography Using Parton Jets
5Jets Beams of quarks and gluons
6EM Radiation
EM field carried by a fast moving electron
EM Radiation by scattering Interference between
initial and final state radiation
7Electron Tomography
Classical radiation of a point charge (Jackson,
p671)
8Two Limits
9LPM Effect
10Radiation in QCD Colors Make the Difference
k
11DIS off Nuclei
12Parton energy loss A twisted story
13HERMES data
in Au nuclei
14Expanding Medium
(GVW, GOW,Wiedemann)
15Single spectra in AA collisions
16Nuclear Modification Factor
17Single hadron suppression
Talks by Hwa, Bass, Greco, Molnar
18Di-hadron Spectra
19Suppression of away-side jet
Df
20Azimuthal Anisotropy
dihadron
Single hadron
21Azimuthal anisotropy II
Talk by R. Lacey, S Voloshin
22Partonic Energy Loss at RHIC
From RHIC data of AuAu Collisions
Initial Density about 30 times of that in a Cold
Au Nucleus
23Energy Loss Is Partonic!
Could it be caused by hadronic absorption or
rescattering?
NO!
24Parton Energy Loss 2
- (2) Centrality dependence
25Parton energy loss (3)
26Parton Energy Loss (4)
early
late
Geometrical anisotropy is an early phenomenon!
27Parton Energy Loss (4)
- (5) Same-side jet profile
Same-side jet cone remains the same as in pp
collision
PHENIX sees the same
Hadron rescattering will change the correlation
Between leading and sub-leading hadrons
28Measuring Parton Energy Loss
29Partonic energy loss (6) SPS
30Summary
- Discovery of Jet Quenching proves that a strongly
interacting dense matter is formed Opaque to
jets - Jet quenching is caused by partonic energy loss
- Dense matter at RHIC is 30 times higher than cold
nuclei - Collective behavior Hydrodyamic limit (talks by
Csernai,Huovinen, Nonaka) - It has to be QGP within QCD
- Jet tomography become useful and power tool for
studying properties of dense matter
31Hard Probes Collaboration
http//www-hpc.lbl.gov/
Hard Processes in pp, pA and AA
- Jet and high pt hadron
- Quarkonium
- Heavy Quarks
- Direct Photons
- DY
32Parton Shadowing in Nuclei
33Energy Dependence
Thermal absorption important at lower E
Detailed balance
Enke Wang XNW PRL87(01)142301
34Medium Modified Fragmentation