Title: J/Y,%20Charm%20and%20intermediate%20mass%20dimuons%20in%20Indium-Indium%20collisions
1J/Y, Charm andintermediate mass dimuonsin
Indium-Indium collisions
, not RHIC!
- Results from recent data (year 2003) from SPS
- Time is limited. I will focus on open
charmintermediate mass dimuons, first. then
move to J/y analysis, if time allowed
- Hiroaki Ohnishi, RIKEN/JAPAN
- For the NA60 collaboration
XXXV International Symposiumon Multiparticle
Dynamics 2005
KROMERÍŽ, CZECH REPUBLIC, August 9-15, 2005
2Search for the QCD phase transition
QCD predicts that strongly interacting matter,
above a critical temperature, undergoes a phase
transition to a state where the quarks and gluons
are no longer confined in hadrons, and chiral
symmetry is restored Such a phase transition
should be seen through dilepton signals
- the suppression of strongly bound heavy
quarkonium states dissolved when certain
critical thresholds are exceeded - the production of thermal dimuons
- changes in the r spectral function (mass
shifts, broadening, disappearance) when chiral
symmetry restoration is approached
3Intermediate mass dimuon measurement from p-A to
Pb-Pb
- NA50 was able to describe the IMR dimuon spectra
in p-A collisions as a sum of Drell-Yan and Open
Charm contributions (but charm production
cross-section higher than the world average)
NA38/NA50 proton-nucleus data
4Intermediate mass dimuon measurement from p-A to
Pb-Pb
- NA50 was able to describe the IMR dimuon spectra
in p-A collisions as a sum of Drell-Yan and Open
Charm contributions (but charm production
cross-section higher than the world average)
- The yield of intermediate mass dimuons measured
in heavy-ion collisions exceeds the sum of
expected sources (Charm and DY)
NA50 Pb-Pbcentral collisions
NA38/NA50 proton-nucleus data
5Explanation of intermediate mass dimuon
- The intermediate mass dimuon yields in heavy-ion
collisions can be reproduced by
- by scaling up the Open Charm contribution by up
to a factor of 3
- by adding thermal radiation from a
quark-gluon-plasma
- To identify the source of enhancement, we need
to separate D meson decays and prompt dimuons
We need to measure secondary vertices with 50
mm precision
6NA60 detector concept
Concept of NA60 place a silicon tracking
telescope in the vertex region to measure the
muons before they suffer multiple scattering in
the absorberand match them to the muon measured
in the spectrometer
Matching in coordinate and in momentum space
?
- Improved dimuon mass resolution
- Origin of muons can be accurately determined
Prompt dimuon
Displaced dimuon
12 tracking planes made with Rad-hard silicon
pixel detector
OR
7Data set
- Two muon spectrometer settings
- 5-week long run in 2003In-In _at_ 158 GeV/nucleon
Events/50 MeV
- Centrality selection using
- beam spectator energy in the ZDC
- or charged multiplicity in the vertex
- spectrometer
Raw ??- invariant mass spectrum
mµµ (GeV/c2)
- 41012 ions on target
- 2108 dimuon triggers collected
8Muon track offset resolution
- Offset resolution is evaluated with prompt dimuon
(J/y) 4050 ?m
9Background subtraction
- Combinatorial background
- Significantly reduced by the track matching
procedure - Nevertheless, still the dominant dimuon source
for m?? lt 2 GeV/c2
Cannot use
- NA60 acceptance quite asymmetric ?
Nback 2vNN--
- Mixed event technique developed ? accurate to
12
- Fake matches background muon matched to a wrong
vertex telescope track - Evaluated with mixed events ? complicated but
rigorous approach
10Background subtraction resulting mass
distribution
Detail will be discussedfollowing
presentationby M. Floris
Data integrated over centrality (Matching ?2 lt
1.5)
This talk focuses on
(if possible)
11Intermediate mass dimuon analysis
12NA60 Signal analysis simulated sources
- Charm and Drell-Yan contributions are calculated
by overlaying Pythia events on real data (using
CTEQ6M PDFs with EKS98 nuclear modifications and
mc1.3 GeV/c2)The fake matches in the MC events
are subtracted as in the real data
- Relative normalizations
- for DY K-factor of 1.8 to reproduce DY
cross-sections of NA3 and NA50 - for charm we use the cross-section needed to
reproduce the NA50 p-A dimuon data (a factor 2
higher than the world average of direct charm
measurements)
- Absolute normalization The expected DY
contribution, as a function of the collision
centrality, is obtained from the number of
observed J/? events and the ? suppression
pattern ? A 10 systematical error is
assigned to this normalization
The fits to mass and weighted offset spectra are
reported in terms ofthe DY and Open Charm
scaling factors needed to describe the data
13IMR mass dimuons analysisa la NA50
- Procedure Fix the Charm and DY contributions to
the expected yields and see if their Sum
describes the measured Data
The expected Charm and DY yields, plus 10,
cannot explain the measured data
An excess is clearly present !
14Question Is it compatible with the NA50
observation?
- Procedure Try to describe the measured mass
spectrum by leaving the Charm normalization as a
free parameter
NA50 would require a factor 3.5 of Charm
enhancement incentral Pb-Pb collisions
Answer Yes, leaving the Charm yield free
describes the In-In data, with 2 times more
charm than needed by the NA50 p-A data
15Question Is this validated by the offsets
information?
- Procedure Fix the prompt contribution to the
expected DY yield and see if the offset
distribution can be described with enhanced Charm
Answer No, Charm is too flat to describe the
remaining spectrum
we need more prompts!
16Question How many more prompts do we need?
- Procedure Leave both contributions freeand see
if we can describe the offset distribution
Answer A good fit requires two times more
prompts than the expected Drell-Yan yield
17Question Is the prompt yield sensitive to the
Charm level?
- Procedure Change the Charm contribution by a
factor of 2and see how that affects the level of
prompts
If we decrease the Charm yield to 0.55,the level
of the Prompts contribution changes from 1.91
0.11 to 2.08 0.07
If we increase the Charm yield by a factor of 2,
the description of the data deteriorates
significantly
Answer No, we always need two times more
prompts than the expected Drell-Yan, within
10 (the Charm contribution is too small to make
a difference)
18Question What is the mass shape of the excess?
- Procedure Fix the DY and Charm contributions to
their expected yields and see how the excess,
relative to DY or Charm, depends on the dimuon
mass
Answer The mass spectrum of the excess dimuons
is steeper than DY and flatter than Open Charm
19Centrality dependence of the Excess Data - DY -
Charm
The yield of excess dimuons increases faster than
linearly with Nparticipants
If the excess dimuons are due to a hard process,
they should have the same centrality dependence
as the expected sources (DY Charm).
Not excluded by the data, at this time.
20Summary
IMR dimuons
- There is an excess of intermediate mass dimuons
in Indium-Indium collisions - The offset distribution requires a factor 2 more
prompts than expected from DY ? The excess
is not due to open charm enhancement - The excess grows faster than linearly with the
number of participants
- Results are very robust with respect to
variations of the matching ?2 cut changing
the Signal / Background ratio by a factor of 2
changes the results by less than 10 The excess
cannot be due to a bias in the background
subtraction
21J/Y suppression
22J/Y production in p-A to Pb-Pb
- The study of J/y production in p-A collisions at
200, 400 and 450 GeV, by NA3, NA38, NA50 and
NA51, gives a J/y absorption cross-section in
normal nuclear matter of 4.18 0.35 mb.
- In p-A, light-ion, the data follow this normal
nuclear absorption which scales with the length
of nuclear matter crossed by the (pre-resonant)
J/y, L.
- peripheral Pb-Pb collisions also follows L
scaling
- In the more central Pb-Pb collisions the L
scaling is broken and an anomalous
suppression sets in
23The J/Y standard analysis
Background
without matching 6500 data set no centrality
selection
- Combinatorial background from ? and K decays
estimated from like-sign pairs(less than 3
under the J/y) - Signal mass shapes from Monte Carlo
- PYTHIA and GRV 94 LO parton densities
- GEANT 3.21 for detector simulation
- reconstructed as the measured data
- Acceptances from Monte Carlo simulation
- for J/y 12.4 (6500 A) 13.8 (4000 A)
- for DY 13.2 (6500 A) 14.1 (4000 A)
- (in mass window 2.94.5 GeV)
J/y
Charm
y
DY
A multi-step fit (max likelihood) is
performed a) M gt 4.2 GeV normalize the DY
b) 2.2 lt M lt 2.5 GeV normalize the charm (with
DY fixed)
c) 2.9 lt M lt 4.2 GeV get the J/y yield (with DY
charm fixed)
24Centrality dependence (standard analysis)
An anomalous suppression is present in the
Indium-Indium data
The small statistics of high mass dimuons limits
the number of centrality bins
25Direct J/Y analysis
- Idea directly compare the measured J/? sample
(only matched dimuons), as a function of
centrality, with the yield expected from the
normal nuclear absorption - The integrated ratio Measured / Expected is
imposed to be the same as in the standard analysis
26Comparison with previous results
S, In and Pb data points do not overlap in
the L variable the physics behind the
anomalous J/? suppression does not depend on
L
The In-In and Pb-Pb J/y suppression
patterns are in fair agreement as a function
of the Npart variable
27Direct J/? sample comparison with theoretical
models
It is important to emphasize that these models
were previously tuned on the p-A, S-U and Pb-Pb
suppression patterns obtained by NA38 and NA50
We consider models for which we have predictions
specifically made for In-In collisions
J/y absorption by produced hadrons (comovers)
Capella and Ferreiro, hep-ph/0505032 J/y
suppression in the QGP and hadronic phases
including thermal regeneration and in-medium
properties of open charm and charmonium states
Grandchamp, Rapp, Brown, Nucl.Phys. A715
(2003) 545 Phys.Rev.Lett. 92 (2004) 212301
hep-ph/0403204 cc suppression by deconfined
partons when geometrical percolation sets in
Digal, Fortunato and Satz, Eur.Phys.J.C32 (2004)
547.
28Suppression by produced hadrons (comovers)
The model takes into account nuclear absorption
and comovers interaction with sco 0.65 mb
(Capella-Ferreiro)
In-In _at_ 158 GeV
J/y / NColl
nuclear absorption
comover nuclear absorption
(E. Ferreiro, private communication)
NA60 In-In 158 GeVpreliminary
Pb-Pb _at_ 158 GeV
The smeared form (dashed line) is obtained taking
into account the resolution on NPart, due to our
experimental resolution
29QGP hadrons regeneration in-medium effects
The model simultaneously takes into account
dissociation and regeneration processes in both
QGP and hadron gas (Grandchamp, Rapp, Brown)
In-In _at_ 158 GeV
fixed thermalization time
fixed thermalization time
centrality dependent thermalization time
BmmsJ/y/sDY
centrality dependent thermalization time
Nuclear Absorption
Suppression Regeneration
QGPhadronic suppression
Regeneration
Number of participants
NA60 In-In 158 GeVpreliminary
The smeared form (dashed line) is obtained taking
into account the resolution on NPart, due to our
experimental resolution
Pb-Pb _at_ 158 GeV
30Suppression due to a percolation phase transition
Model based on percolation (Digal-Fortunato-Satz)
Sharp onset (due to the disappearance of the cc
meson) at Npart 125 for Pb-Pb and 140 for
In-In
The dashed line includes thesmearing due to the
ZDC resolution
Pb-Pb _at_ 158 GeV
31Summary
IMR dimuons
- There is an excess of intermediate mass dimuons
in Indium-Indium collisions - The offset distribution requires a factor 2 more
prompts than expected from DY ? The excess
is not due to open charm enhancement - The excess grows faster than linearly with the
number of participants
J/Y suppression
- The J/y shows an anomalous suppression already
in Indium-Indium - The suppression is centrality dependent and sets
in at 90 Npart
32(No Transcript)
33Background Subtraction method
34Background Subtraction method (offsets)
The mixed background sample (fake matches and
combinatorial) must reproduce the offsets of the
measured events therefore, the offsets of the
single muons (from different events) selected for
mixing must be replicated in the mixed event.
(All masses)
35Comparison with previous results
very preliminary
Bjorken energy density, estimated from VENUS
36Specific questions that remain open
- Is the anomalous suppression also present in
lighter nuclear systems?
- Study collisions between other systems, such as
Indium-Indium
- Which is the variable driving the suppression?
L, Npart, energy density?
- Study the J/? suppression pattern as a function
of different centrality variables, including data
from different collision systems
- What is the normal nuclear absorption cross
section at the energy of the heavy ion data?
- Study J/? production in p-A collisions at 158
GeV
- What is the impact of the cc feed-down on the
observed J/y suppression pattern?
Study the nuclear dependence of cc production in
p-A collisions
- Study the nuclear dependence of cc production
in p-A collisions