J production in Cu Cu and Au Au collisions at vsNN 200 GeV measured by PHENIX at RHIC - PowerPoint PPT Presentation

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J production in Cu Cu and Au Au collisions at vsNN 200 GeV measured by PHENIX at RHIC

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Title: J production in Cu Cu and Au Au collisions at vsNN 200 GeV measured by PHENIX at RHIC


1
J/? production in CuCu and AuAu collisions at
vsNN 200 GeV measured by PHENIX at RHIC
  • Andry Rakotozafindrabe
  • LLR École Polytechnique

42nd Rencontres de Moriond QCD session Italy
(March 2007)
2
Physics motivation the starting point
  • What are the properties of the hot and dense
    matter produced in relativistic heavy ion
    collisions ?
  • c and b are produced in the initial parton
    collisions, so they can be used to probe the
    created medium
  • open charm (or beauty) energy loss ? energy
    density
  • Topic already covered this morning by Alan Dion
  • , (quarkonia) suppressed by color
    screening ? deconfinement
  • At lower energy, NA50 (CERN) experiment measured
    an anomalous J/? suppression in PbPb collisions,
    in excess of the normal suppression expected from
    the nuclear absorption.
  • NA50 Collaboration, Eur. Phys. J. C39 (2005) 335
  • At lower energy, NA60 (CERN) recent results in
    InIn
  • At RHIC energy ?
  • 10x vsNN
  • 2-3x gluon density

3
Screening the J/? in a QGP
  • Production
  • 60 direct production J/?
  • 30 via ?c? J/? x
  • 10 via ?? J/? x
  • Temperature of dissociation Td
  • for ?c and ? Td 1.1 Tc
  • for J/? Td 1.5 to 2 Tc
  • Sequential dissociation as the temperature (or
    energy density) increases

?c
?
J/?
  • Energy density (t0 1fm) vs the max. vs for SPS,
    RHIC and LHC

4
Physics motivation a few complications
  • Final state
  • Normal nuclear absorption
  • Absorption by (hadronic ?) comovers ?
  • Color screening ?
  • In-medium formation (recombination) ?
  • Flow ?
  • Sensitive to
  • Initial state
  • Modification of the parton distribution functions
    (shadowing, CGC)
  • pT broadening (Cronin effect)
  • Parton energy loss in the initial state ?

5
J/? in PHENIX capsule history
6
PHENIX detector
  • J/? ? ee
  • y lt 0.35
  • Pe gt 0.2 GeV/c
  • ?? ?
  • Tracking, momentum measurement with drift
    chambers, pixel pad chambers
  • e ID with EmCAL RICH
  • J/??µµ
  • 1.2lt y lt 2.2
  • Pµ gt 2 GeV/c
  • ?? 2?
  • Tracking, momentum measurement with cathode
    strip chambers
  • µ ID with penetration depth / momentum match

Centrality measurement, vertex position
Beam-beam counters (charged particle production)
Zero-degree calorimeters (spectator neutrons)
7
Production baseline (Run5) pp?J/? _at_ vs 200
GeV
hep-ex/0611020
Cross section vs rapidity better constraints on
available J/? production mechanisms
  • Total cross section in pp
  • Bll.?pp(J/? ) 178 3(stat)
  • 53(sys) 18(norm) nb
  • in agreement with COM

Cross section vs pT Forward rapidity ltpT2gt 3.59
0.06 0.16 Central rapidity
pp?J/? measurement used as a reference for
AB?J/?
8
Heavy ion results _at_ vs 200 GeV
  • AuAu final results nucl-ex/0611020
  • CuCu preliminary results (QM05)
  • but forthcoming final results (article in
    preparation) with
  • increased statistics in the dielectron channel (a
    factor 2)
  • significant improvement of systematic errors
  • better precision measurement than the present
    AuAu results for Npartlt100

9
RHIC beyond cold nuclear matter effects
  • Available dAu data
  • ?qCNM
  • Weak shadowing and weak nuclear absorption (sabs
    1mb favored) derived from model Vogt PRC71,
    054902 (2005)
  • AuAu data even compared to the  worst  sabs
    2mb case shown here
  • suppression beyond cold effects for
  • Npartgt100 at y1.7
  • Npartgt200 at y0
  • Need to improve the knowledge of CNM effects at
    RHIC

nucl-ex/0611020
RHIC CNM effects s abs 0, 1, 2 mb _at_ y0, y2
Cold nuclear matter predictions from Vogt,
nucl-th/0507027 (shadowing sabs)
10
RHIC different amount of suppression at
different rapidities
nucl-ex/0611020
  • RAA vs Npart
  • Stronger suppression at forward rapidity than at
    central rapidity
  • Ratio forward/central 0.6 for Npartgt100
  • CGC (initial state effect) ?
  • models predicts less heavy quark production at
    forward rapidity than at mid rapidity
  • K. L. Tuchin J.Phys. G30 (2004) S1167

11
RHIC vs SPS
  • SPS _at_ 0ltylt1
  • vs 17 GeV
  • CNM normal nuclear absorption sabs 4.18
    0.35 mb
  • Maximum e 3 GeV/fm3 (t0 1)
  • Compare to RHIC _at_ ylt0.35
  • x10 vs
  • CNM shadowing nuclear absorption sabs from 0
    to 2mb (Vogt, nucl-th/0507027)
  • Maximum e 5 GeV/fm3 (t0 1), higher than at
    SPS
  • Same pattern of J/? suppression for the same
    rapidity!
  • Suppression beyond CNM larger at RHIC

Bar uncorrelated error Bracket correlated
error Global error 12 is not shown
12
RHIC vs SPS (II) extrapolating suppression
models
  • Suppression models in agreement with NA50 data
    extrapolated at RHIC energies
  • Opposite suppression behaviour vs rapidity
  • Unmatched suppression pattern at central rapidity
  • Recombination at work at RHIC ?

Dissociation by thermal gluons (R. Rapp et al.,
nucl-th/0608033 Nu Xu et al., Phys.Rev.Lett. 97
(2006) 232301)
Dissociation by comovers (Capella et al.,
hep-ph/0610313)
13
Recombination at RHIC ?
  • Suppressionrecombination predictions compared to
    data
  • RAA vs Npart

Better matching with the data but regeneration
goes as the (single) charm density which is
poorly known at RHIC What about the other
variables ?
14
Recombination at RHIC ?
  • Suppressionrecombination predictions compared to
    data
  • RAA vs Npart
  • Yield vs rapidity

RMS 1.320.06
RMS 1.300.05
Recombination predicts a narrower rapidity
distribution with an increasing
Npart Data shows a slight decrease of the
RMS with increasing centrality
Thews Mangano, PRC73 (2006) 014904c
RMS 1.430.04
RMS 1.400.04
nucl-ex/0611020
15
Recombination at RHIC ?
  • Suppressionrecombination predictions compared to
    data
  • RAA vs Npart
  • Yield vs rapidity
  • ltpT2gt vs Ncoll

No recombination
Recombination predicts a narrower pT
distribution with an increasing centrality, thus
leading to a lower ltpT²gt Data shows a rather
flat dependence of ltpT²gt with centrality
With recombination
Thews, Eur.Phys.J. C43 (2005) 97, Phys.Rev. C73
(2006) 014904 (and private communication).
16
Ending where it began revisiting the sequential
dissociation (I)
  • Karsch, Kharzeev Satz, PLB 637 (2006) 75
  • Sequential melting ? overall J/? survival
    probability (measured/expected)
  • S 0.6 S direct J/ ? 0.4 S J/???, ?c
  • Recent lattice QCD results direct J/? melting
    at 10-30 GeV/fm3
  • ? S 0.6 at RHIC
  • RAA/CNM vs.
  • Bjorken energy density

Sequential dissociation of ? and ?c only does
not seem to be consistent with the data
17
Refinement 3D hydro sequential dissociation
(II)
  • Gunji et al., hep-ph/0703061
  • Charmonia
  • initial spatial distribution from collisions in
    the Glauber model
  • free streaming in a full (3D1) hydro
  • J/? survival probability ( RAA/CNM with CNM
    shadowing nuclear absorption sabs 1mb )
  • S (1 fFD) S direct J/ ? fFD S J/???, ?c
  • 3 free parameters feed-down fFD , melting
    temperatures TJ/? and T?,?c
  • (3D1) hydro same setup as the one used to
    reproduce charged dN/d? measured at RHIC
  • Assuming thermalization for t0.6fm, initial
    energy density distribution in the transverse
    plane, EOS of the medium (TltTc and TgtTc),

18
Refinement 3D hydro sequential dissociation
(II)
  • Gunji et al., hep-ph/0703061
  • Charmonia
  • J/? survival probability ( RAA/CNM with CNM
    shadowing nuclear absorption sabs 1mb )
  • S (1 fFD) S direct J/ ? fFD S J/???, ?c
  • 3 free parameters Feed-down fFD , melting
    temperatures TJ/? and T?,?c
  • (3D1) hydro
  • ? best fit with
  • TJ/? 2.12 Tc
  • T?,?c 1.34 Tc
  • fFD 0.25
  • 0.10 due to uncertainty
  • on sabs (1 1mb)

Better matching with the data
19
Summary (I)
  • PHENIX final results on J/??dileptons at forward
    and mid-rapidity in pp, AuAu, and preliminary
    results in CuCu
  • Improved baseline
  • Run 5 pp with x10 more statistics than Run 3
  • Suppression pattern
  • Beyond cold nuclear effects for Npart gt 200
  • More suppression at forward than at central
    rapidity
  • Ratio forward/central 0.6 for Npartgt100
  • May be accounted for by CGC models
  • Suppression models (comover) predicts the
    opposite behaviour
  • Similar to SPS suppression in the same rapidity
    region? despite a higher energy density reached
  • Understandable as recombinations that
    partially compensate the J/? suppression ?
  • Still open question (test vs ltpT²gt dependance and
    rapidity distribution)

20
Summary (II)
  • Alternate explanations ?
  • Sequential dissociation with feed-down assumed to
    be 40 and direct J/? not melting at present
    energy densities is not consistent with data
  • (3D1) hydro sequential dissociation in
    agreement with mid-rapidity data if direct J/? is
    melting (at T 2.12 Tc) and if feed-down is
    assumed to be (25 10)
  • Feed-down not measured at RHIC energies
  • At lower energies, large deviations between
    experiments
  • Need to improve knowledge on cold nuclear effects
    at RHIC
  • Stay tuned forthcoming final results for CuCu
    !
  • Improved precision for the measurements in the
    range Npart lt 100

21
Back-up
22
Hint of things to come
  • Final results for CuCu
  • What about the forward vs central suppression at
    lower Npart ?
  • Improved reference pp
  • x3 higher statistics from run 6
  • Future measurements in ? ?
  • Future measurements in ?c
  • Planning AuAu (1 nb-1 vs 0.24 nb-1 in run 4 )
    with high luminosity during Run 7
  • Later runs dAu with higher luminosity (28 nb-1
    vs 2.7 nb-1 in run 3) ?

Work under progress
23
Upsilon measurement
PHENIX QM05
Dimuon mass spectrum for the two muon arms added
together.
y1.7 10 counts
PHENIX 1st Upsilons at RHIC from 3pb-1
collected during the 2005 pp run.
y0 50 cnts
STAR QM06
STAR Preliminary pp 200 GeV
ee- Minv Background
Subtracted
24
STAR results and near future
M. Cosentino, QWG06
STAR Preliminary
STAR J/? Run5 pp
STAR J/? Run4 AuAu
  • Dataset AuAu_at_200 GeV
  • No trigger due to high background
  • Just a faint signal
  • For efficient J/y trigger, full barrel ToF is
    needed (just patch in Run5)
  • pp_at_200GeV (Run5)
  • trigger commissioning (1.7M events)
  • Run 6 expect 500-1000 (work in progress)

Upsilon
25
J/? production
  • Production
  • 60 direct production J/?
  • 30 via ?c? J/? x
  • 10 via ?? J/? x
  • Large deviations between experiments ?c
    feed-down fraction vs vs
  • Not measured at RHIC energies

26
Invariant yield vs tranverse momentum
27
ltpT2gt vs Npart
  • A closer look at ltpT2gt vs Npart

28
Cold nuclear effects dAu?J/?
gluons in Pb / gluons in p
x
Nucl. Phys. A696 (2001) 729-746
  • Available dAu data ? CNM
  • Weak shadowing (modification of gluon
    distribution) and weak nuclear absorption (sabs
    1mb favored) derived from model Vogt PRC71,
    054902 (2005)
  • Data driven parametrizations of CNM
  • Karsch, Kharzeev Satz, PLB 637 (2006) 75
  • Granier de Cassagnac, hep-ph/0701222

y 0 intermediate xAu 0.020
29
RHIC beyond cold nuclear effects (II) ?
  • Comparison to a data driven parametrization of
    CNM (Granier de Cassagnac, hep-ph/0701222) in the
    same centrality classes
  • CNM RAA(y, b) ScollisionsRdA(-y,b1i).RdA(y,b
    2i)/Ncoll
  • Essentially the same conclusions as the previous
    slide
  • But statsyst error that comes from dAu data are
    visible
  • Need a higher luminosity dAu sample

30
J/? production in dAu vs centrality
High x2 0.09
  • Small centrality dependence
  • Model with absorption shadowing ( black lines
    )
  • shadowing EKS98
  • sabs 0 to 3 mb
  • sabs 1 mb good agreement
  • sabs 3 mb is an upper limit
  • weak shadowing and weak nuclear absorption

Low x2 0.003
Colored lines FGS shadowing for 3 mb
31
SPS vs RHIC (III) RAA/CNM vs Npart
NA50 at SPS (0ltylt1) PHENIX at RHIC
(ylt0.35) PHENIX at RHIC (1.2ltylt2.2)
  • SPS _at_ 0ltylt1
  • CNM normal nuclear absorption sabs 4.18
    0.35 mb
  • Compare to RHIC _at_ ylt0.35
  • CNM shadowing nuclear absorption sabs1 mb
    (Vogt, nucl-th/0507027)
  • Additionnal syst. error from uncertainity on CNM
  • Need to improve knowledge on cold nuclear effects
    at RHIC
  • Suppression beyond CNM larger at RHIC

Bar uncorrelated error Bracket correlated
error Global errors (12 and 7) are not shown
here. Box uncertainty from CNM effect
32
Recombination at RHIC ?
RAA vs y
100 Recombination(shape only)
R. Vogt nucl-th/0507027 (EKS)
R. L. Thews, M. L. Mangano Phys.Rev. C73 (2006)
014904
33
Charm flow
S. Sakai QM06
M. Djordjevic et al., Phys.Lett.B632 (2006) 81
c and b quark pT distributions at mid-rapidity
before fragmentation b contribution is dominant
at high pT
  • Significant flow observed for heavy flavor
    electrons
  • Main source is D meson
  • (1) Consistent with c-quark thermalization
  • (2) large cross section is needed in AMPT 10 mb
  • (3) Resonance state of D B in sQGP
  • Charm quark strongly coupled to the matter

Phys.Lett. B595 202-208
PRC72,024906
PRC73,034913
34
Computing the J/? yield
Invariant yield
i i-th bin (centrality for e.g.)
  • number of s reconstructed
  • probability for a thrown and embeded
  • into real data to be found
  • (considering reconstruction and trigger
    efficiency)
  • total number of events
  • BBC trigger efficiency for events with a
  • BBC trigger efficiency for minimum bias events

35
Collision geometry and centrality (eg CuCu)
  • For a given b, Glauber model (Woods-Saxon
    function) predicts
  • Npart (No. participants)
  • Ncoll (No. binary collisions)

Monte-Carlo Glauber model Probability for a
given Npart Each participant contributes to a
Negative Binomial distribution of hits Fit BBC
charge distribution
36
Energy density
  • Longitudinally expanding plasma
  • dET/d? measurement at mid-rapidity by PHENIX
    EMCal
  • Which t0 ?
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