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Title: Frdric FLEURET


1
Recent RHIC results on photon, dilepton and heavy
quarks
  • Frédéric FLEURET
  • LLR - École polytechnique, France
  • X Whorkshop on High Energy Physics
    Phenomenology
  • PHENIX collaboration

2
Deconfined matter Quark Gluon Plasma
  • The phase diagram

Big Bang
  • high temperature (1012 K)
  • 10-6 s. Plasma ? confined matter

Core of Neutron stars
  • Star collapse
  • High density of matter
  • (5 to 10 times standard nuclear density)
  • Confined matter ? plasma

3
History of experimental facilites
  • QGP experiment history

BNL - AGS 4 GeV
CERN - SPS 20 GeV
Fixed target Experiments
BNL - RHIC 200 GeV
CERN - LHC 5.5 TeV
Collider Experiments
4
Experimental facility RHIC-BNL-NY
BRAHMS
PHOBOS
species and (PHENIX) luminosity
RHIC
PHENIX
STAR
2 independent rings with 3.9 km
circumference Anything from pp (up to 500 GeV)
to AuAu (up to 200 GeV per nucleon pair)
5
Experimental facility PHENIX STAR
  • PHENIX
  • Beam counters
  • Central rapidity ylt0.35
  • Tracking (DC, PC)
  • EM calorimeter
  • TOF
  • RICH
  • Muon spectrometers 1.2ltylt2.2
  • Measures everything
  • STAR
  • Large TPC
  • Silicon vertex tracker
  • EM calorimeter
  • Time of flight
  • Track 2000 charges particles in hlt1

6
Centrality and Nuclear Modification Factor
  • Npart number of interacting nucleons
  • Ncoll number of binary nucleon-nucleon
    collisions
  • small impact parameter b ? large Npart, large
    Ncoll
  • large impact parameter ?b ? small Npart, small
    Ncoll
  • Centrality
  • Nuclear Modification Factor

Soft interactions Nparticipants Hard
interactions Ncollisions
For hard probes, if no nuclear effects, RAA 1
7
The smoking gun _at_ RHIC
  • Jet quenching

p-p
Suppression in central AuAu due to high density
medium
  • back-to-back di-hadron correlations
  • very similar in pp and dAu
  • strongly suppressed in central AuAu collisions
    at 200 GeV

7
8
Electromagnetic radiations
  • Why studying electromagnetic radiations ?
  • electromagnetic probes do not interact strongly
  • Suffer little or no final state interaction
  • Give access to the hot and dense phase of the
    reaction
  • Carry information of the system at the time of
    their production

Freeze-out
photons
hadronisation
thermalisation
Formation phase (pre-equilibrium)
9
Electromagnetic radiations
  • I) photons
  • Testing pQCD
  • Thermal photons
  • II) Low Mass Region
  • Vector mesons in medium
  • III) Intermediate Mass Region
  • Thermal dileptons
  • Heavy quarks continuum open charm
  • IV) High Mass Region
  • Heavy quarks resonances

10
Photons
  • pQCD photons
  • Thermal photons

11
Sources of photons
  • In pp collisions
  • Direct photons
  • Compton scattering
  • q g ? q g
  • qq annihilation
  • q q ? g g
  • Bremsstrahlung
  • Fragmentation photons
  • Final state hadron decay (background)

12
Sources of photons
  • In AA collisions
  • High pT photons (pTgt 6 GeV) non thermal
  • Initial parton-parton scattering as in pp
  • not affected by Hot and Dense Matter ? test the
    theoretical description of AA collisions with
    pQCD
  • Low pT photons (pT lt 3 GeV) thermal
  • Come from the thermalized medium
  • Carry information about the initial temperature
    of the Quark Gluon Plasma
  • Thermal photons are created in the QGP as well as
    in the hadron gas over the entire lifetime of
    these phases ? test hydro models
  • Low and intermediate pT photons (up to 6 GeV)
  • Interaction of the quarks and gluons from the
    hard scattering processes with the QGP
  • qhard gQGP ? q g
  • g get a large fraction of the momentum of qhard

13
pQCD photons (High pT) in pp collisions
  • Phenix year-3 and year-5 data set
  • Reference for AuAu
  • Measured pp yield compatible with NLO pQCD
    calculations (tends to be higher by 20)

Phys. Rev. Lett. 98, 012002 (2007)
Phenix Run 3
Run 5
Phenix Run 5
14
pQCD photons (High pT) in dAu
  • Phenix
  • Consistent with NLO pQCD calculation
  • Star
  • gdir gincl gdecay
  • Plot R 1 gdir/gdecay
  • Cancel systematic uncertainties
  • Signal consistent with pQCD NLO calculation

15
pQCD photons (high pT) in AuAu
  • PHENIX Run 2
  • Computing RAA.vs.Npart
  • p0 are quenched
  • Direct g are not
  • PHENIX Run 4
  • Reach up to 18 GeV/c (12 GeV for Run 2)
  • Qualitatively well described by NLO pQCD
    calculations

16
pQCD photons (High pT) in AuAu
  • AuAu run 4 compared with pp
  • Computing RAA
  • consistent with Ncoll scaling below 10 GeV
  • Small decrease observed at very high pT
  • interpretation
  • F. Arleo JHEP 0609 (2006) 015
  • High-pT suppression due to isospin effect, in
    addition to jet quenching and shadowing.

shadowing
shadowing energy loss
isospin
17
Thermal photons (low pT)
  • Central AuAu run 4
  • Excess over pQCD observed at pTlt 4
  • ? Well described including hydrodynamical
    predictions for thermal photons (QGP HG)
  • D. dEnterria and D. Perressounko (Eur. Phys.
    J. C46, 451 464 (2006))
  • Initial temperature T0 590 MeV at t0
    2R/g 0.15 fm/c
  • Precision dAu data required to confirm

PHENIX preliminary
18
Dileptons
  • Vector mesons in medium
  • (Low Mass Region)
  • Thermal dileptons
  • (Intermediate Mass Region)

19
Vector meson in medium (Low Mass Region)
  • Chiral Symmetry Restoration
  • Adding mass term in QCD lagrangian brokes chiral
    symetry
  • Lattice QCD predicts that it is restored at Tc
    150 200 MeV
  • Experimentally expect mass drop and broadening of
    the r-meson
  • At SPS-CERN (20 GeV), low mass excess observed
    by CERES in PbAu and confirmed by NA60 in InIn.

Phys. Rev. Lett 96, 162302 (2006)
Nucl. Phys. A774, 43 (2006)
20
Thermal radiations (Intermediate Mass Region)
  • QGP thermal radiation
  • Expect thermal radiation from hot medium ?
    initial temperature of the QGP
  • Experimentally, should be accessible in the
    Intermediate Mass Region
  • At SPS CERN (20 GeV)
  • Intermediate mass excess observed by NA50 in
    PbPb
  • NA60 in InIn ? not coming from D decays ?
    prompt dileptons

Excess compared to the expected Drell-Yan yield
Excess over open charm and Drell-Yan
21
LMR and IMR at RHIC
  • AuAu 200 GeV (run 4)
  • Measured by PHENIX
  • Measures di-electrons
  • 8.108 Min Bias events
  • large background at low mass (S/B 1/200 _at_ 0.5
    GeV)
  • Background subtracted by event mixing technique
  • checking background subtraction (converter
    run)
  • use a subset of data (5.107 events) taken with
    additional material around the beam pipe
  • increase background by a factor 2.5
  • Results agree within statistical errors

22
LMR and IMR at RHIC
  • AuAu 200 GeV (run 4)
  • Cocktail plot
  • low mass region
  • Data below 150 MeV/c² well described by the
    cocktail
  • Enhancement observed in 150 lt mee lt 750 MeV
  • intermediate mass region
  • Absence of excess with cc correlated PYTHIA
    distribution
  • But medium effect should randomize the cc
    correlation ? room for thermal radiation

23
Low Mass Region at RHIC
  • AuAu 200 GeV (run4)
  • Centrality dependence
  • ? (Yield/(Npart/2)) .vs. Npart
  • Low Mass Region
  • 0 lt mee lt 100 MeV/c²
  • dominated by p0 decays
  • ? follows expected yield
  • 150 lt mee lt 750 MeV/c²
  • excess increases with Npart
  • ? consistent with in-medium enhancement from
    scattering processes like pp or qq annihilation

24
Intermediate Mass Region at RHIC
  • AuAu 200 GeV (run4)
  • Centrality dependence
  • ? (Yield/Ncoll) .vs. Npart
  • Intermediate Mass Region
  • 1.2 lt mee lt 2.8 GeV/c²
  • ? Consistent with the expectations based on
    PYTHIA

25
Closer look at heavy quarks
l-
Direct reconstruction Difficult without measure
of vertex (ct 120 mm)
K
c
K-
Indirect reconstruction Measure contribution of
semileptonic decays from Heavy flavor to lepton
spectra
p
26
Heavy flavour in pp
  • Precise measurements made by both PHENIX and STAR
  • Difference observed between PHENIX and STAR
  • PHENIX is a factor 2 larger than FONLL
    calculations (but agrees within uncertainties)
  • STAR is a factor gt 2 larger than PHENIX

PRL98, 192301 (2007)
PRL97, 252002 (2006)
27
Heavy flavour cross section
  • Comparison between STAR and PHENIX
  • Same discrepancy observed in AuAu
  • PHENIX is a factor 2 larger than FONLL
    calculations
  • STAR is a factor gt 2 larger than PHENIX

28
Heavy flavour RAA
STAR PRL98, 192301 (2007) PHENIX PRL98,
172301 (2007)
  • RAA comparison
  • Consistent RAA observed between PHENIX and STAR
  • The difference observed in pp and AuAu yields
    is cancelled out in the ratio.
  • At large pT suppression similar to that of light
    hadrons

29
Elliptic flow v2
  • Within a strongly interacting medium
  • Initial spatial anisotropy converted into
    momentum anisotropy
  • Efficicency of conversion depends on the
    properties of the medium
  • v2 2nd fourier coefficient of momentum
    anisotropy
  • Flow

reaction plane
v2gt0 ? flow in the reaction plane v2lt0 ? flow out
of the reaction plane
30
Charm flows
  • Large v2 observed
  • Armesto et al. pQCD calculation with radiative
    energy loss (curve I) ? strongly coupled medium.
  • Van Hees et al. heavy quark transport
    calculation including elastic scattering (curve
    II) ? diffusion coefficient consistent with
    estimates obtained in the light quark sector.
  • Moore and Teaney (curve III) ? diffusion
    coefficient similar to II.
  • Large energy loss and flow in AuAu ? strong
    evidence for the coupling of heavy quarks in the
    medium

PHENIX PRL98, 172301 (2007)
31
Quarkonia
  • J/Y cross section
  • J/Y CNM effects
  • (Cold Nuclear Matter)
  • J/Y HDM effects
  • (Hot and Dense Matter)
  • Other quarkonia

32
Quarkonia
  • Theoretical context

Matsui and Satz first proposed the study of
quarkonia as a signature of Quark Gluon Plasma
(QGP) Phys. Lett. B 178 (1986) 416
  •  if high energy heavy ion collisions lead to the
    formation of a hot quark-gluon plasma, then color
    screening prevents cc binding in the deconfined
    interior of the interaction region / it is
    concluded that J/Y suppression in nuclear
    collisions should provide an unambigous signature
    of quark-gluon plasma formation 

33
Quarkonia
NA50, Eur. Phys. Journal C39 (2005) 335
  • Experimental context
  • J/y production in pA and AA collisions has been
    studied at SPS starting 1986.
  • NA38, NA50, NA60
  • Anomalous suppression observed in PbPb (NA50)
    and InIn (NA60) central collisions (high energy
    density, high temperature).
  • Different models (with or without QGP) describe
    the data
  • At RHIC, vs up to 200 GeV, 10 x bigger than SPS
    vs

central
peripheral
Mid-central
34
J/Y at RHIC
  • Production
  • Main production process gluon fusion
  • Feed-down
  • 60 from direct production
  • 30 cc ? J/y g
  • 10 y ? J/y X
  • In nuclear matter
  • Initial state effects
  • Nuclear shadowing (Cold Nuclear Matter Effect)
  • Final state effects
  • Absorption in nuclear matter (Cold Nuclear Matter
    Effect)
  • Anomalous suppression (Hot and Dense Matter
    Effect ?)
  • Experimentally
  • At RHIC vs up to 200 GeV (lt20 GeV at SPS)
  • J/y is mainly measured by the PHENIX experiment
  • Measure J/y in pp used as a reference
  • Measure J/y in dAu to study Cold Nuclear
    Effects
  • Measure J/y in AuAu and CuCu to study anomalous
    suppression.

35
J/Y production in pp
  • To be used as a reference for AA
  • spp in agreement with Color Octet Model

PRL 98, 232002 (2007)
PRL98,232002(2007)
J/Y is a hard process ? expect in AA collisions
(sJ/Y)AA ? ltNcollgt?(sJ/Y)pp
In the following, well use
(if no nuclear effect RAA1)
36
Cold Nuclear Matter (CNM) effects
Projectile
  • Absorption by nuclear matter
  • After its production, charmonium can interact
    with nucleons from projectile and target
  • Introducing L, the  length  of nuclear matter
    seen by the J/Y
  • J/Y survival probability
  • At SPS
  • Expect some absorption at RHIC

L
Target
J/y
J/y normal nuclear absorption curve
Eskola, Kolhinen, Vogt Nucl. Phys. A696 (2001)
  • Shadowing
  • Nuclear shadowing is an initial-state effect on
    the parton distributions.
  • Gluon distribution function can be different when
    comparing proton and nucleus.
  • Expect some (anti) shadowing at RHIC

x is the momentum fraction of the nucleon that
a parton (quark or gluon) carries.
37
CNM effects _at_ RHIC J/Y in dAu
South
Central
North
  • PHENIX data compatible with
  • Weak gluon shadowing
  • Small absorption mb
  • Need more precise dAu data

arXiv0711.3917
central
peripheral
mid-central
X1 gt X2(0.003)
X1 lt X2(0.09)
X1 X2(0.02)
J/? South y lt 0
J/? North y gt 0
J/? Central y 0
38
AuAu and CuCu _at_ RHIC
  • Suppresssion at RHIC
  • ? Similar suppression in AuAu and CuCu at same
    centrality
  • ? larger suppression observed at forward
    rapidity in AuAu

AuAu PHENIX Final PRL98, 232301 (2007) CuCu
PHENIX Preliminary nucl-ex/0510051
39
AA results - comparison SPS .vs. RHIC
  • Including CNM effects
  • Lack of precision on CNM effects at RHIC
  • ? cant discriminate between
  • Same anomalous suppression at SPS and RHIC
  • Different anomalous suppression at SPS and RHIC
  • ? need more precise measurement of CNM effects at
    RHIC ? need more dAu data
  • Comparison with SPS results
  • ? Suppression at RHIC ? suppression at SPS (at
    mid-rapidity).
  • ? But cold nuclear matter effects may be
    different.

40
Interpretations
  • Models including anomalous suppression only
  • Which reproduce SPS data,
  • Predict too much suppression
  • Color screening CNM (1 mb)
  • Comovers CNM (1 3 mb)
  • Direct production CNM
  • Rapidity dependence
  • Predict more suppression at central rapidity
  • Comover density is higher in central region
  • Does not reproduce the data
  • Data show more suppression at forward rapidity
    than at central rapidity

PRL98, 232301 (2007)
41
Interpretations
  • Models including anomalous suppression only
  • Which reproduce SPS data,
  • Predict too much suppression
  • Color screening CNM (1 mb)
  • Comovers CNM (1 3 mb)
  • Direct production CNM
  • Adding recombination
  • Recombination cc -gt J/Y g
  • NJ/Y ? Ncc²
  • Compensate direct suppression
  • Need better open charm measurement to better
    constraint recombination
  • Measure J/Y flow to check recombination

PRL98, 232301 (2007)
PRL 92, 212301 (2004)
Eur. Phys. J C43, 97 (2005)
PRL97, 232301 (2006)
PRC 69, 054903 (2004)
NPA789, 334 (2007)
42
Futur quarkonia measurements
  • Measuring other quarkonia would help to
    understand J/Y cc, Y, U

PHENIX Run 5 200GeV pp
43
Conclusions
  • Electromagnetic radiations provide a large
    physics potential
  • Photon
  • Test of pQCD and initial state effects in AA
    collisions
  • Evidence for thermal radiation at low pT
  • Dileptons
  • Enhancement in mass range 150 lt mee (MeV/c²) lt
    750 ? vector meson modification in medium
  • Heavy quarks
  • Heavy quarks suppression at large pT and heavy
    quarks flow ? coupling of heavy quarks in the
    medium
  • Quarkonia
  • J/Y suppression similar to SPS results
  • Need to better constraint Cold Nuclear Matter
    effects
  • Recombination at play ?
  • Futur
  • run 7 AuAu data taken in 2007 ? currently
    analysing
  • run 8 dAu data ? currently taking data
  • other high-luminosity runs detector upgrades
  • Quark matter 2008
  • February 4 10, 2008, Jaipur

44
Backup slides
45
Sources of photons
  • C. Gale, Nuc. Phys. A 785 (2007)
  • N-N compton and annihilation photons
  • Jet-th jet-thermal photons
  • Jet-bremss. jet-bremsstrahlung photons
  • Jet-fragmentation g from the fragmentation of
    the escaping jets
  • th-th g from the thermal radiation of the
    cooling system
  • In AA collisions
  • Decay photons From p0, h, w,
  • Direct photons
  • Compton and annihilation
  • Jet-thermal, jet-brehmsstrahlung
  • Fragmentation
  • Thermal radiation of the cooling system

46
pQCD photons (High pT) in AuAu
  • AuAu run 4 compared with pp
  • Computing RAA
  • consistent with Ncoll below 10 GeV
  • Small decrease observed at very high pT
  • F. Arleo
  • JHEP 0609 (2006) 015
  • High-pT suppression due to isospin effect, in
    addition to jet-quenching and shadowing.

47
Thermal photons (low pT)
  • Low pT photons (pT lt 3 GeV) thermal
  • Come from the thermalized medium
  • Carry information about the initial temperature
    of the QGP
  • Thermal photons are created in the QGP as well as
    in the hadron gas over the entire lifetime of
    these phases ? test hydro models

Stefan Bathe
47
48
Low Mass Region NA60
  • Phys. Rev. Lett 96, 162302 (2006)

49
Low Mass Region CERES
Nucl. Phys. A774, 43 (2006)
50
Heavy flavor production
  • Onia production
  • Leading order at low x gluon
    fusion
  • Sensitive to

J/y or ?
  • Initial state
  • Parton distribution functions
  • pT broadening
  • Parton energy loss in the initial state ?
  • Polarization ?
  • Final state
  • Parton energy loss in the hot dense medium ?
  • Thermal enhancement ?
  • Flow ?

feed-down (e.g. B or ?c-gt J/y)
51
Heavy flavor production
  • Open charm (or beauty) production
  • Leading order at low x gluon
    fusion
  • Sensitive to
  • Initial state
  • Parton distribution functions
  • pT broadening
  • Parton energy loss in the initial state ?
  • Polarization ?
  • Final state
  • Parton energy loss in the hot dense medium ?
  • Thermal enhancement ?
  • Flow ?

52
Understanding the dissociation
53
Measuring J/Y
54
Experimental facility PHENIX STAR
  • PHENIX
  • Central arm
  • ylt0.35, dfp
  • Tracking DC, PC and TEC
  • Calorimetry PbGl and PbSc (EMCal)
  • Particle ID RICH and TOF
  • Muon arms
  • 1.2 lt y lt 2.2
  • Df 2p
  • Tracking MuTr
  • Particle ID MuID
  • Global detectors
  • BBC centrality, vertex,..

55
STAR upgrades
56
PHENIX ugrades
57
quarkonia
July 1997
  •  if high energy heavy ion collisions lead to the
    formation of a hot quark-gluon plasma, then color
    screening prevents cc binding in the deconfined
    interior of the interaction region / it is
    concluded that J/Y suppression in nuclear
    collisions should provide an unambigous signature
    of quark-gluon plasma formation 

Mid-central
central
peripheral
Anomalous suppression observed in PbPb (NA50)
and InIn (NA60) at CERN/SPS
58
A key HI variable centrality of the collision
  • Npart number of interacting nucleons
  • Ncoll number of binary nucleon-nucleon
    collisions
  • small impact parameter b ? large Npart, large
    Ncoll
  • large impact parameter ?b ? small Npart, small
    Ncoll
  • Determining Npart, Ncoll

Peripheral Collision
Central Collision
Semi-Central Collision
b
b
b
large impact parameter small Npart small Ncoll
small impact parameter large Npart large Ncoll
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