Title: Frdric FLEURET
1Recent RHIC results on photon, dilepton and heavy
quarks
- Frédéric FLEURET
- LLR - École polytechnique, France
- X Whorkshop on High Energy Physics
Phenomenology - PHENIX collaboration
2Deconfined matter Quark Gluon Plasma
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
3History of experimental facilites
BNL - AGS 4 GeV
CERN - SPS 20 GeV
Fixed target Experiments
BNL - RHIC 200 GeV
CERN - LHC 5.5 TeV
Collider Experiments
4Experimental 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)
5Experimental 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
6Centrality 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
7The smoking gun _at_ RHIC
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
8Electromagnetic 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)
9Electromagnetic 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
10Photons
- pQCD photons
- Thermal photons
11Sources 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)
12Sources 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
13pQCD 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
14pQCD 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
15pQCD 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
16pQCD 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
17Thermal 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
18Dileptons
- Vector mesons in medium
- (Low Mass Region)
- Thermal dileptons
- (Intermediate Mass Region)
19Vector 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)
20Thermal 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
21LMR 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
22LMR 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
23Low 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
24Intermediate 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
25Closer 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
26Heavy 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)
27Heavy 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
28Heavy 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
29Elliptic 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
reaction plane
v2gt0 ? flow in the reaction plane v2lt0 ? flow out
of the reaction plane
30Charm 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)
31Quarkonia
- J/Y cross section
- J/Y CNM effects
- (Cold Nuclear Matter)
- J/Y HDM effects
- (Hot and Dense Matter)
- Other quarkonia
32Quarkonia
Matsui and Satz first proposed the study of
quarkonia as a signature of Quark Gluon Plasma
(QGP) Phys. Lett. B 178 (1986) 416
- Â 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 formationÂ
33Quarkonia
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
34J/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.
35J/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)
36Cold 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.
37CNM 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
38AuAu 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
39AA 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.
40Interpretations
- 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)
41Interpretations
- 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)
42Futur quarkonia measurements
- Measuring other quarkonia would help to
understand J/Y cc, Y, U
PHENIX Run 5 200GeV pp
43Conclusions
- 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
44Backup slides
45Sources 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
46pQCD 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.
47Thermal 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
48Low Mass Region NA60
- Phys. Rev. Lett 96, 162302 (2006)
49Low Mass Region CERES
Nucl. Phys. A774, 43 (2006)
50Heavy 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)
51Heavy 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 ?
52Understanding the dissociation
53Measuring J/Y
54Experimental 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,..
55STAR upgrades
56PHENIX ugrades
57quarkonia
July 1997
- Â 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 formationÂ
Mid-central
central
peripheral
Anomalous suppression observed in PbPb (NA50)
and InIn (NA60) at CERN/SPS
58A 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
Peripheral Collision
Central Collision
Semi-Central Collision
b
b
b
large impact parameter small Npart small Ncoll
small impact parameter large Npart large Ncoll