Title: Indications of the Onset of Deconfinement at low SPS Energies Recent Results from NA49 ICPAQGP5, Col
1Indications of the Onset of Deconfinementat low
SPS EnergiesRecent Results from
NA49ICPAQGP5, Colcatta, February 2005
V. Friese v.friese_at_gsi.de
for the collaboration
2The NA49 Detector
- Hadron spectrometer
- Large acceptance 4p yields
- PID by dE/dx and TOF
- Centrality by forward calorimeter
Beam energies 20, 30, 40, 80, 158 AGeV Systems
pp, pA, CC, SiSi, PbPb
3Midrapidity mt spectra (central PbPb)
Simultaneous blast wave fit constant ßt p, d
excluded from fit SSH, PRC 48 (1993) 2462
Single fireball model with common temperature and
flow velocity works
Beware Resonance feeddown, velocity profile
4Early freeze out of O ?
Linear velocity profileO agrees better with
charmonia than with other hadrons Indication
for earlier freeze out?
NA49, nucl-ex/0409004
() Gorenstein, Bugaev, Gadzicki, PRL 88 (2002)
132301
5Transverse spectra at lower energies
30 AGeV
20 AGeV
Blast wave fits work at all SPS energies Kinetic
freeze out T 120 130 MeV ßt 0.4 0.5 for
constant ßt
6Kaon Slope Parameters
Kaon spectra almost perfect exponential ? fit
dn/dmt mt e-mt/T
Constant inverse slope at all SPS
energies Constant temperature and pressure? Mixed
phase?
7Average mt
Other particle types No exponential spectrum ?
calculate mean mt
Similar behaviour seen for pions protons less
conclusive
8Longitudinal Distributions (central PbPb)
Gaussianlike rapidity spectra (except p, ?)
9Strange to Nonstrange Ratios Kaons
Sharp structure in K / p, not reproduced by
hadronic models (Full equlibrium) hadron gas
model overpredicts kaons at higher SPS energies
10Strange to Nonstrange Ratios ?
Similar structure seen as in K(sharp peak at 30
AGeV) HGM describes overall structure, but
location of peak different (?) UrQMD not far off
(not shown)
11Total Strangeness
Peak at 30 AGeV,undersaturation at higher SPS
energies
Energy dependence changes at 30 AGeV
12Ruling out hadronic equlibirium ?
- Features of HGM
- No sharp peak
- Overprediction of strangeness yields
at higher SPS energies - Maxima at different positions for K, ?, ?, O
If connected with PT, maxima should be at the
same energy for all strange species
? at 20, 30 AGeV possibly discriminative ? to come
13 one more Parameter
Becattini et al., PRC 69 (2004) 024905
Introducing ?S lt 1 gives better description of
NA49 4p yieldsaround 30 AGeV ?S 1 At higher
energies ?S 0.7what does it mean?
14Indication for deconfinement PT ?
Gazdzicki, Gorenstein, Act. Phys. Polon. B 30
(1999) 2705
Hama et al., Braz. J. Phys. 34 (2004) 322
Phase transition at 30 AGeV
QGP hadronic phases
Features in strangeness / pion and kaon slopes
can be obtained with models assuming a phase
transition
15Relative Strangeness Fluctuations
Dynamical fluctuations in K/p increase towards
low SPS energies Not reproduced in UrQMD p/p in
agreement with hadronic transport (resonance
decays)
16Mean pt Fluctuations
Measured at top SPS as function of system
size Maximum at small Npart ( 100 ) But
similar pattern observed at RHIC Interesting
Measure at lower SPS energies (hint taken)
17System Size Strangeness Enhancement
NA49, 158 AGeV
Tounsi, Redlich, JPG 28 (2002) 2095
Strangeness enhancement ? canonical
suppression Volume effect on strangeness
conservation
But No quantitative agreement with data (rise
too fast) if V Npart
Disagreement between peripheral PbPb and central
SiSi, CC
18Cluster Ansatz bei C. Höhne
Microscopic calculation of overlapping strings
(VENUS, UrQMD) ? correlation volume as fct. of
Npart Calculate ES ? according to statistical
model, taking into account the distribution in
Vcorr
Describes data perfectly ! Application to
fluctuations?
19Summary
- Anomalies at lower SPS energies observed by NA49
- sharp peak in strange particles to pion ratio
- constancy of kaon slopes
- pion production rate increases (not discussed)
- Fluctuation in K/p also increase towards low SPS
energies, other signals less convincing / absent - Best explanation by scenario with onset of
deconfinement - Low SPS is still interesting
- EoI to CERN for SPS running from 2009 on
- Plans of fixed target experiments at RHIC
- FAIR at GSI