Title: NICA
1NICA Round Table IVJINR, Dubna, September
9-12, 2009
Dileptons in Heavy Ion Collisions
2Outline
- Introduction
- Low energies DLS and HADES
- SPS results
- CERES - Low-mass region
- NA60 - Low and intermediate mass region
- RHIC first results from PHENIX
- Elementary collisions search for cold nuclear
matter effects - Summary and outlook
3Introduction
- Electromagnetic probes (real or virtual photons)
are sensitive probes of the two fundamental
properties of the QGP - Deconfinement
- Chiral symmetry restoration
- Lepton pairs are unique probes of CSR
- The therrmal radiation emitted in the form of
dileptons (virtual photons) provides a direct
fingerprint of the matter created first the QGP
(qqbar ? ee-) and subsequently a dense HG
(??- ? ee-) - What have we learned in about 20 years of
dilepton measurements? What is the NICA
potential?
4Low-mass dilepton experiments
- Nuclear Collisions
- CERES
- DLS
- HADES
- HELIOS
- NA38/50
- NA60
- PHENIX
- Elementary Reactions
- CLAS
- CBELSA/TAPS
- KEK E235
- TAGX
5Dileptons in AA at a Glance
Time Scale
6- Low-energies
- DLS and HADES
-
-
7DLS puzzle
DLS data Porter et al., PRL 79, 1229 (1997)
Calculations Bratkovskaya et al., NP A634, 168
(1998)
- Enhancement not described by in-medium ?
spectral function - All other attempts to reproduce the DLS results
failed - Main motivation for the HADES experiment
Strong enhancement over hadronic cocktail with
free ? spectral function
8HADES confirms the DLS results
CC 1 AGeV
Mass distribution
pT distribution
Good agreement between DLS and HADES in
di-electron mass and pT distributions
9Putting the puzzle together (I)
CC _at_ 1 AGeV pp pd _at_ 1.25 GeV
- Spectra normalized to ?0 measured in CC and NN
- CC _at_ 1 AGeV
- ltM?gt/Apart 0.06 0.07
- NN _at_ 1.25 GeV (using pp and pd measurements)
- ltM?NNgt/Apart 1/4(pp2pnnn)/2
- 1/2(pppn) 0.076?0.015
Dielectron spectrum from CC consistent with
superposition of NN collisions! No compelling
evidence for in-medium effects in CC
10Putting the puzzle together (II)
Recent transport calculations enhanced NN
bremsstrahlung , in line with recent OBE
calculations) HSD Bratkovskaya et al. NPA
807214 (2008)
The DLS puzzle seems to be reduced to an
understanding of the elementary contributions to
NN reactions.
11 12CERES Pioneering Results (I)
Strong enhancement of low-mass ee- pairs (wrt
to expected yield from known sources)
Last CERES result (2000 Pb run PLB 666(2008) 425)
Enhancement factor (0.2 ltm lt 1.1 GeV/c2 ) 2.45
0.21 (stat) 0.35 (syst) 0.58 (decays)
13CERES Pioneering Results (II)
First CERES result PRL 75, (1995) 1272
Last CERES result PLB 666 (2008) 425
Strong enhancement of low-mass ee- pairs in all
A-A systems studied
Eur. Phys J. C41 (2005) 475
PRL 91 (2003) 042301
14pT and Multiplicity Dependencies
Enhancement is at low pT
Increases faster than linearly with multiplicity
15Dropping Mass or Broadening (I) ?
Interpretations invoke ??- ???
? ? ee- thermal radiation from HG
CERES Pb-Au 158 A GeV 2000 data
vacuum ? not enough to reproduce data
- in-medium modifications of ?
- broadening ? spectral shape
- (Rapp and Wambach)
- dropping ? meson mass
- (Brown et al)
-
Data favor the broadening scenario.
16NA60 Low-mass dimuons in In-In at 158 AGeV
Real data !
Superb data!
- Mass resolution23 MeV at the ? position
- ?, ? and even ? peaks clearly visible in
dimuon channel
17Dimuon Excess
Dimuon excess isolated by subtracting the hadron
cocktail (without the ?)
- Excess centered at the nominal ? pole
- Excess rises and broadens with centrality
- More pronounced at low pT
confirms consistent with, CERES results
18NA60 low mass comparison with models
PRL 96 (2006) 162302
- Subtract the cocktail from the data (without the
?)
- Excess shape consistent with broadening of the ?
- (Rapp-Wambach)
- Mass shift of the ? (Brown-Rho)
- is ruled out
- Is this telling us something
- about CSR?
- All calculations normalized to data at m?? lt 0.9
GeV performed by Rapp et al., for ltdNch/d?gt 140
19NA60 low mass comparison with models
- Subtract the cocktail from the data (without the
?)
NP A806, 339 (2008)
- Excess shape consistent with broadening of the ?
- (Rapp-Wambach)
- Mass shift of the ? (Brown-Rho)
- is ruled out
- Is this telling us something
- about CSR?
20 21Dileptons in PHENIX pp collisions
- Mass spectrum measured from m0 up to m8
GeV/c2 - Very well understood in terms of
- hadron cocktail at low masses
- heavy flavor DY at high masses
22Dileptons in PHENIX AuAu collisions
- Strong enhancement of ee- pairs at low masses
- m 0.2 0.7 GeV/c2.
- Very different from SPS
- Enhancement down to very low masses
- Enhancement concentrated at central collisions
- No enhancement in the IMR
23Comparison to theoretical model (AuAu)
PHENIX
All models and groups that successfully described
the SPS data fail in describing the PHENIX results
24Dileptons in PHENIX AuAu collisions
Min bias AuAu vsNN 200 GeV arXiv 0706.3034
nucl-ex
Integral180,000 above p015,000
All pairs Combinatorial BG Signal
- BG determined by event mixing technique,
normalized to like sign yield
- Green band systematic error w/o error on CB
PHENIX has mastered the event mixing technique to
unprecedented precision (0.25). But with a S/B
1/200 the statistical significance is
largely reduced and the systematic errors
are large
25HBD
Single vs double e separation
Installed and fully operational in Run-9
26- LVM in Elementary Collisions
-
-
27 KEK E235 pC, Cu _at_ E12 GeV Cold nuclear matter
Excellent mass resolution ?m 8.9-0.2 MeV/c2 _at_
m?1017 MeV/c2
28 Raw spectra
29 Raw spectra fitted with known sources.
- Hadronic sources ?, ?, ? -gt ee-, ? -gt? ee- , ?
-gt ? ee- - Width Breit-Wigner shape convoluted
with experimental resolution. - Position PDG values
- Relative abundances determined by fit
- Combinatorial background event mixing method
Cannot fit the ? with m and ? from PDG ? yield
consistent with zero
30Dropping ? and ? masses
KEK E325 PRL 96, 092301 (2006)
Model ? and ? produced at nuclear surface,
decay with modified mass if decay point is
inside nucleus mV(?) / mV(0) 1 k(?/?0)
common k parameter for C and Cu target and for ?
and ?. k 9.2
? and ? masses drop by 9.2 at normal nuclear
matter density
31CBELSA / TAPS
32CLAS
No effect seen in ? ee- photo-produced
on H2, C, Fe and Ti targets Mass spectra look
very similar to those measured by KEK . However,
CLAS results can be very well reproduced by a
transport model using the vacuum mass values of
?, ? and ?.
k 2 ? 2
33Summary and outlook
- DLS puzzle solved in CC. Dilepton spectrum
understood as mere superposition of NN
collisions. Is that so also for heavier system?
Onset of low-mass pair enhancement? - Consistent picture from the SPS
- Low-mass pair enhancement thermal radiation from
the HG - Approach to CSR proceeds through broadening
(melting) of the resonances - Enhancement persists down to 40 AGeV
- RHIC results very intriguing
- Strong enhancement of low-mass pairs down to very
low masses - No enhancement in the IMR
- Challenge for theoretical models
- Looking forward to more precise results with the
HBD - Elementary collisions no coherent picture and no
compelling evidence of in-medium modification
effects of LVM in cold nuclear matter - NICAs energy range very well suited to fill an
important niche - unveil the onset of the low-mass pair
enhancement. - Systematic studies of pA colliisions
- Study pair enhancement under highest baryon
density conditions