strangeness production at ags and sps
DESCRIPTION
Strangeness production at AGS and SPS. Claudia Höhne, GSI Darmstadt. Outline – December 2005. FAIR. "Strangeness is a vast subject." F.Antinori, proceedings QM04. motivation data (SIS), AGS, SPS, (RHIC) particle yields, spectra, flow, fluctuations, (high-p t , correlations) - PowerPoint PPT PresentationTRANSCRIPT
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Strangeness production at AGS and SPS
Claudia Höhne, GSI Darmstadt
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2Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
FAIR
Outline – December 2005
• motivation
• data
• (SIS), AGS, SPS, (RHIC)
• particle yields, spectra, flow, fluctuations, (high-pt, correlations)
• strangeness production at top SPS energy (158 AGeV)
• system-size dependence
• energy dependence of strangeness production
• summary
"Strangeness is a vast subject." F.Antinori, proceedings QM04
largest amount of data
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3Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Outline
• summary december
• new data (see SQM06): yields (+ rapidity and pt-distributions)
elliptic flow
fluctuations
• yields
→ hadron gas model fits: s-undersaturation at 158 AGeV (no s)?
→ ... s-oversaturation at lower SPS energies (s)?
→ inhomogeneous freeze-out?
→ equilibration?
• energy dependence of size-dependence of relative s-production
• elliptic flow
• particle ratio fluctuations (K,)
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4Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Summary – December 2005
• (selected) overview on strangeness production from AGS, SPS experiments
• "most" of the particles are strange:
understanding strangeness production → learn about "bulk" hadron production
• particle yields/ ratios well described by (~) chemically equilibrated hadron gas
for smaller systems take smaller hadronization volume into account (properly !)
→ strangeness enhancement due to release of canonical s-suppression
interesting: change of "shape" of s-increase with centrality for lower energies!
• distinct features observed in energy dependence of (strange) particle production
maximum in relative s-production at ~30 AGeV
step-like structure in <mt>-values in SPS energy range
• strong common transverse flow: earlier kinetic decoupling in peripheral Pb+Pb?
earlier decoupling of in central Pb+Pb?
"-puzzle" solved: no difference between hadronic and leptonic decay channel
elliptic flow of K/ fluctuations
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5Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Particle yields
C. Blume, NA49, SQM04
4 multiplicities only
• central Au+Au, Pb+Pb
→ extract hadrochemical freezeout parameters (T, B)
understanding strangeness production ↔
understanding (bulk) hadron production: mechanism, environment, ...
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6Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
New data on production from NA49
[M. Mitrovski, SQM06]
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7Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Rapidity spectra of
approximately gaussian shape
[M. Mitrovski, SQM06]
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8Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Mass dependence of rapidity width
• ~ linear dependence on particle mass for mesons and antibaryons
• similar slope at all SPS energies
• explainable by hydro-inspired models?
[M. Mitrovski, SQM06]
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9Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Mean transverse momenta vs. energy
filled symbol: particleopen symbol: antiparticle
C.
Blu
me,
NA
49,
SQ
M04
• energy dependence of mt changes at lower SPS energies
• not described by HSD, UrQMD but by Hydro models with phase transition
• seen for pions, kaons, protons and their antiparticles ...
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10Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Mean transverse momenta vs. energy (II)
... and (more or less) seen for other strange particles as well!
• AGS measurements missing for complete picture!
[M. Mitrovski, SQM06]
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11Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Midrapidity yields vs. energy
CERES
[M. Mitrovski, SQM06]
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12Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
K0S at 158 AGeV from CERES
• 2 independent K0S analysis for 7% central Pb+Au collisions from CERES
• reconstruction without PID and 2nd vertex reconstruction
• reconstruction without PID but with 2nd vertex reconstruction
• ~ agreement with NA57 for same y-bins but disagreement in fit
• rather good agreement to NA49 (K+ + K-) data (5% difference only)!
[J. Milosevic, SQM06]
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13Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
K0S at 158 AGeV from CERES (II)
• good agreement of the 2 CERES analysis
• same temperatur as for NA49 (T = 230 MeV)
[J. Milosevic, SQM06]
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14Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Ratios – midrapidity yields
[M. Mitrovski, SQM06]
• pronounced maximum also for -/ ratio!
HSDUrQMD 2.0
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15Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Ratios – 4 yields
[M. Mitrovski, SQM06]
• pronounced maximum also for -/ ratio!
• disagreement with HSD/ UrQMD in particular at lower SPS energies
• disagreement to HGM in particular at higher SPS energies!
"s-undersaturation"
HSDUrQMD 2.0HGM
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16Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Particle ratios at midrapidity (HGM)
[A. Andronic et al, nucl-th/0511071]
lower than thermal yields confirmed by new CERES result!
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17Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Energy dependence of T,B (HGM)
[A. Andronic et al, nucl-th/0511071]
problems with fit quality at higher SPS energies
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18Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Energy dependence of T, B (HGM) (II)
CBM
CBM[A. Andronic et al, nucl-th/0511071]
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19Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Strangeness undersaturation parameter s
[Becattini et al, PRC 73, 044905 (2006)]
• lesson to learn from s-undersaturation at lower energies?
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20Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Inhomogenous scenario?• Is there something to learn from these deviations? (equilibrium??)
• interesting ansatz: Dumitru el al, nucl-th/0511084
• allow for an inhomogenous fireball at chemical decoupling (T,T,B,B)
→ significant improvement in fit quality for 30 – 158 AGeV beam energy
• relation to 1st order phase transition?
[Dumitru et al, Nucl-th/0511084]
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21Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
QCD phase diagram
[A. Andronic et al, nucl-th/0511071]
• statistical model only way to put points on the QCD phase diagram
• different approaches agree rather well on (T,B)
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22Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Canonical s-suppression
CBM[A. Andronic et al, nucl-th/0511071]
• (very low) energies: well defined case for s-undersaturaion
• for central Au+Au grand canonical ensemble applicable for CBM energies
→ saturation of relative s-production expected with centrality/ size
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23Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
B = const
Energy dep. of centrality dep. of rel. s-prod.
[H. Oeschler, priv. com.]
• earlier saturation for higher energies, saturation also for KAOS?
• shape explainable by release of can. s-suppression alone?
PHENIX s = 200 GeVNA49 Ebeam = 40 AGeVE802 Ebeam = 11.1 AGeVKAOS Ebeam = 1.5 AGeV
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24Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Size-dependence of relative s-production
V=V0 Npart/2
V from percolation
[CH, hep-ph/0507276]
• non-linear dependence of volume on Npart
• V=V0(Npart/2) (=1, 2/3, 1/3)
• V from percolation
• include additional s-undersaturation factor s
[H. Caines, SQM06][Becattini, PRC73,044905,2006]
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25Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Size dependence of rel. s-production (II)
• model including s: (T,B) vary with size → smaller systems freeze-out closer to phase boundary?
• ... or (T,B) constant?
[Becattini, PRC73,044905,2006]
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26Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Elliptic flow of strange particles
• strangeness (s=1) flows at top-SPS energies!
• v2 at RHIC (rescaled to same centrality) larger due to higher beam energy
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27Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Elliptic flow of strange particles (II)
• mass ordering for pt < 1.5 GeV, opposite above
• meson – baryon difference as for RHIC? NCQ scaling works only appr. for pt/nq > 0.5 GeV
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28Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
K/ fluctuations
• role of resonance decays?
• acceptance effects?
• alternative measurement?
[S. Das, SQM06]
22mixeddatadyn
K*
very good agreement between top SPS – low RHIC
dyn,K
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29Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Role of resonances for K/ fluc. (UrQMD) ?
4pi
2pi
CBM
Simulations by D. Kresan (GSI), M. Bleicher (Frankfurt): Au+Au 25 AGeV
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30Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
K*/K versus energy (pp)
• K*/K ratio rater constant with energy in pp
• A+A: suppression towards central collisions – energy dependent?
[CH, PhD thesis]
[STAR, PRC 71, 064902 (2005)]
][GeVs10 102
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31Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
K*/K versus centrality (STAR)
s = 200 GeV, norm. to pp
• energy dependence? ("length" of rescattering phase)
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32Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
How to measure best?
The use of dyn is problematic because it involves event-by-event fluctuations of a ratio
A better measure is dyn,K
Insensitive to efficiency Properly deals with small multiplicities Centrality studies
We will use dyn,K for our systematic studies of K/ fluctuations
dyn,K NK NK 1 NK
2 N N 1 N
2 2NKN
NK N
First proposed by First proposed by Pruneau, Gavin and VoloshinPruneau, Gavin and Voloshin PRC 66 (2002) PRC 66 (2002)Used in Used in STAR Net Charge fluctuation paperSTAR Net Charge fluctuation paper – PRC 68 (2003) – PRC 68 (2003)
[S. Das, SQM06]
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33Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Centrality dependence of K/ fluc.
[S. Das, SQM06]
• continous rise towards the most peripheral Au+Au collisions
(similar to <pt> - fluctuations from STAR)
• influence of centrality determination or acceptance?
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34Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Summary
• new data on and K0S production at SPS!
• "step" in mean transverse masses vs. energy also for
... however, AGS data missing!
• s-undersaturation at higher SPS energies? (no s)
• can we learn something from deviations of the data from hadron gas model fits: anything beyond thermal?
• smaller systems: freeze-out closer to phase boundary?
• strangeness (s=1) flows at top SPS!
• K/ fluctuations: more understanding needed ...
better data on K* production in A+A at lower energies!
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35Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
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36Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
[M. Mitrovski, SQM06]
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37Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Particle yields at midrapidity
CBM[A. Andronic et al, nucl-th/0511071]
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38Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Parametrization of energy-dep.
CBM[A. Andronic et al, nucl-th/0511071]
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39Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006
Baryon → Meson dominance
CBM