strangeness production at ags and sps

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Strangeness production at AGS and SPS Claudia Höhne, GSI Darmstadt

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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 Presentation

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Page 1: Strangeness production at AGS and SPS

Strangeness production at AGS and SPS

Claudia Höhne, GSI Darmstadt

Page 2: Strangeness production at AGS and SPS

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

Page 3: Strangeness production at AGS and SPS

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,)

Page 4: Strangeness production at AGS and SPS

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

Page 5: Strangeness production at AGS and SPS

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, ...

Page 6: Strangeness production at AGS and SPS

6Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006

New data on production from NA49

[M. Mitrovski, SQM06]

Page 7: Strangeness production at AGS and SPS

7Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006

Rapidity spectra of

approximately gaussian shape

[M. Mitrovski, SQM06]

Page 8: Strangeness production at AGS and SPS

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]

Page 9: Strangeness production at AGS and SPS

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 ...

Page 10: Strangeness production at AGS and SPS

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]

Page 11: Strangeness production at AGS and SPS

11Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006

Midrapidity yields vs. energy

CERES

[M. Mitrovski, SQM06]

Page 12: Strangeness production at AGS and SPS

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]

Page 13: Strangeness production at AGS and SPS

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]

Page 14: Strangeness production at AGS and SPS

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

Page 15: Strangeness production at AGS and SPS

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

Page 16: Strangeness production at AGS and SPS

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!

Page 17: Strangeness production at AGS and SPS

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

Page 18: Strangeness production at AGS and SPS

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]

Page 19: Strangeness production at AGS and SPS

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?

Page 20: Strangeness production at AGS and SPS

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]

Page 21: Strangeness production at AGS and SPS

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)

Page 22: Strangeness production at AGS and SPS

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

Page 23: Strangeness production at AGS and SPS

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

Page 24: Strangeness production at AGS and SPS

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]

Page 25: Strangeness production at AGS and SPS

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]

Page 26: Strangeness production at AGS and SPS

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

Page 27: Strangeness production at AGS and SPS

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

Page 28: Strangeness production at AGS and SPS

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

Page 29: Strangeness production at AGS and SPS

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

Page 30: Strangeness production at AGS and SPS

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

Page 31: Strangeness production at AGS and SPS

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)

Page 32: Strangeness production at AGS and SPS

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]

Page 33: Strangeness production at AGS and SPS

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?

Page 34: Strangeness production at AGS and SPS

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!

Page 35: Strangeness production at AGS and SPS

35Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006

Page 36: Strangeness production at AGS and SPS

36Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006

[M. Mitrovski, SQM06]

Page 37: Strangeness production at AGS and SPS

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]

Page 38: Strangeness production at AGS and SPS

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]

Page 39: Strangeness production at AGS and SPS

39Claudia Höhne The Physics of High Baryon Density, ECT* Trento, May 29 – June 2, 2006

Baryon → Meson dominance

CBM