Jet Tomography of Hot Dense Matter Jet XinNian

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Jet Tomography of Hot & Dense Matter Jet Xin-Nian Wang LBNL, June 25, 2003

Jet Tomography of Hot & Dense Matter Jet Xin-Nian Wang LBNL, June 25, 2003

Equation of States F. Karsch ‘ 2001 Hadrons: QGP: Quarks(2 x 3 x 2

Equation of States F. Karsch ‘ 2001 Hadrons: QGP: Quarks(2 x 3 x 2 x 2) Gluons(2 x 8)

Medium Response Function Dynamic System: Photon or dilepton emission J/Y suppression QCD Response: (talks

Medium Response Function Dynamic System: Photon or dilepton emission J/Y suppression QCD Response: (talks by Averbeck, Sinha, Fries, Granier de Cassagnac) Quark scattering

Computed Tomography (CT) Calibrated source Absorption properties Computer assisted correction Image Jet Tomography: Using

Computed Tomography (CT) Calibrated source Absorption properties Computer assisted correction Image Jet Tomography: Using Parton Jets

Jets: Beams of quarks and gluons Au+Au Jet Tomography Talks by Jacobs, Bathe

Jets: Beams of quarks and gluons Au+Au Jet Tomography Talks by Jacobs, Bathe

EM Radiation EM field carried by a fast moving electron v Final rad. EM

EM Radiation EM field carried by a fast moving electron v Final rad. EM Radiation by scattering: Interference between initial and final state radiation Initial rad.

Electron Tomography Classical radiation of a point charge (Jackson, p 671) i j Formation

Electron Tomography Classical radiation of a point charge (Jackson, p 671) i j Formation time

Two Limits Factorization Limit: Bethe Heitler Limit: Like a single scattering

Two Limits Factorization Limit: Bethe Heitler Limit: Like a single scattering

LPM Effect Ncoh radiation like from a single scattering Ncoh Landau Pomeranchuck Migdal Ncoh

LPM Effect Ncoh radiation like from a single scattering Ncoh Landau Pomeranchuck Migdal Ncoh

Radiation in QCD: Colors Make the Difference pi a pf c k k pi

Radiation in QCD: Colors Make the Difference pi a pf c k k pi pf QED y 0 QCD Gluon multiple scattering (BDMP’ 96) 0 y

DIS off Nuclei e- Frag. Func.

DIS off Nuclei e- Frag. Func.

Parton energy loss: A twisted story e- Modified frag. function Parton Energy Loss

Parton energy loss: A twisted story e- Modified frag. function Parton Energy Loss

HERMES data in Au nuclei

HERMES data in Au nuclei

Expanding Medium (GVW, GOW, Wiedemann) Energy loss in a static medium with density

Expanding Medium (GVW, GOW, Wiedemann) Energy loss in a static medium with density

Single spectra in A+A collisions p. QCD Parton Model

Single spectra in A+A collisions p. QCD Parton Model

Nuclear Modification Factor Initial state effect: Shadowing & pt broadening: XNW, PRC 61(00)064910 Fai,

Nuclear Modification Factor Initial state effect: Shadowing & pt broadening: XNW, PRC 61(00)064910 Fai, Papp, and Levai (02) Vitev & Gyulassy (02) Vitev (03) LP model Alberto Accardi (01) Color dipole model Kopeliovich et al (02) p. A

Single hadron suppression Talks by: Hwa, Bass, Greco, Molnar

Single hadron suppression Talks by: Hwa, Bass, Greco, Molnar

Di-hadron Spectra Hadron-trigger fragmentation function:

Di-hadron Spectra Hadron-trigger fragmentation function:

Suppression of away-side jet Df

Suppression of away-side jet Df

Azimuthal Anisotropy dihadron Single hadron

Azimuthal Anisotropy dihadron Single hadron

Azimuthal anisotropy II Talk by R. Lacey, S Voloshin

Azimuthal anisotropy II Talk by R. Lacey, S Voloshin

Partonic Energy Loss at RHIC From RHIC data of Au+Au Collisions Ge. V for

Partonic Energy Loss at RHIC From RHIC data of Au+Au Collisions Ge. V for E=10 Ge. V Initial Density about 30 times of that in a Cold Au Nucleus Consistent with estimate of initial condition Talks by Venugopalan, Bickley

Energy Loss Is Partonic! Could it be caused by hadronic absorption or rescattering? (1)

Energy Loss Is Partonic! Could it be caused by hadronic absorption or rescattering? (1) Hadron formation time: NO! h Uncertainty principle:

Parton Energy Loss: 2 (2) Centrality dependence:

Parton Energy Loss: 2 (2) Centrality dependence:

Parton energy loss: (3) PT Dependence:

Parton energy loss: (3) PT Dependence:

Parton Energy Loss: (4) • Large v 2 early late Geometrical anisotropy is an

Parton Energy Loss: (4) • Large v 2 early late Geometrical anisotropy is an early phenomenon!

Parton Energy Loss: (4) (5) Same-side jet profile Same-side jet cone remains the same

Parton 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

Measuring Parton Energy Loss p. Ttrig ET

Measuring Parton Energy Loss p. Ttrig ET

Partonic energy loss: (6) SPS

Partonic energy loss: (6) SPS

Summary • Discovery of Jet Quenching proves that a strongly interacting dense matter is

Summary • 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

Hard Probes Collaboration http: //www-hpc. lbl. gov/ Hard Processes in p+p, p+A and A+A

Hard Probes Collaboration http: //www-hpc. lbl. gov/ Hard Processes in p+p, p+A and A+A • • • Jet and high pt hadron Quarkonium Heavy Quarks Direct Photons DY

Parton Shadowing in Nuclei shadowing EMC

Parton Shadowing in Nuclei shadowing EMC

Energy Dependence Thermal absorption important at lower E Detailed balance Enke Wang & XNW

Energy Dependence Thermal absorption important at lower E Detailed balance Enke Wang & XNW PRL 87(01)142301

Medium Modified Fragmentation

Medium Modified Fragmentation