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Can we discover the critical point at RHIC? Experimental Overview Gunther Roland BNL March 9 2006 Thanks to Burak Alver, Ed Wenger, Siarhei Vaurynovich,

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Presentation on theme: "Can we discover the critical point at RHIC? Experimental Overview Gunther Roland BNL March 9 2006 Thanks to Burak Alver, Ed Wenger, Siarhei Vaurynovich,"— Presentation transcript:

1 Can we discover the critical point at RHIC? Experimental Overview Gunther Roland BNL March 9 2006 Thanks to Burak Alver, Ed Wenger, Siarhei Vaurynovich, Wei LI

2 Gunther Roland BNL Workshop March 2006 Matter Density μ B (GeV) Temperature (MeV) Quark-Gluon Plasma Hadron Gas Phase Boundary 0 200 0 Atomic Nuclei 1 Critical Point Exploring the QCD Phasediagram Critical Point

3 Gunther Roland BNL Workshop March 2006 Exploring the QCD Phasediagram Matter Density μ B (GeV) Temperature (MeV) Quark-Gluon Plasma Hadron Gas Phase Boundary 0 200 0 Atomic Nuclei 1 Critical Point Susceptibilities diverge near critical point Locate the critical point using correlation/fluctuation measurements √s ) 2 > Enhanced Fluctuations near Critical Point Rajagopal, Shuryak, Stephanov Critical Point

4 Gunther Roland BNL Workshop March 2006 Matter Density μ B (GeV) Temperature (MeV) Quark-Gluon Plasma Hadron Gas Phase Boundary 0 200 0 Atomic Nuclei 1 Critical Point Exploring the QCD Phasediagram Plot from M. Stephanov, Correlations ‘05 Challenge: Guidance on exact location and strength of correlation signals is limited

5 Gunther Roland BNL Workshop March 2006 Experimental Search for the Critical Point Theoretical guidance is limited Experimental strategy:  Search in different observables, correlate observables  Maximize experimental sensitivity  Fine grained exploration of μ B, T space Side effect:  Sensitivity to critical phenomena at 1st order transition, Onset of Deconfinement, EOS softest point, changes in bulk dynamics etc ➡ NA49

6 Gunther Roland BNL Workshop March 2006 Experimental Search for the Critical Point This idea/strategy is not new This talk (this workshop)  What is known from excitation functions?  What could be done better at RHIC (and how good)? RHIC SPS AGS First of many experimental talks

7 Gunther Roland BNL Workshop March 2006 Fixed target vs collider experiments If rates O(1Hz) or greater: √s scan of hadronic observables feasible 1/γ 2 1/γ 3 NA49 K/π fluctuations CERES low mass e+e- CERES fluctuations min-bias 0-5% central (optimistic) c.f. Todd Satogata c.f. Peter Steinberg (PHENIX) Harald Appelshaeuser (CERES) (known)

8 Gunther Roland BNL Workshop March 2006 Suitable hadronic observables Here: Simple observables  Multiplicities and multiplicity correlations  Spectra and momentum correlations  Net charge correlations  Elliptic flow  Particle ratios and ratio fluctuations

9 Gunther Roland BNL Workshop March 2006 Excitation Function: Mid-rapidity Multiplicities RHIC SPS AGS Compilation by PHOBOS Nucl. Phys. A 757, 28 Cu+Cu PHOBOS QM’05 ? ? RHIC SPSAGS - Logarithmic growth of mid-rapidity particle density - Structure at SPS energy range and/or around √s ≈ 60 GeV? - Precision of ≈ 5-10% - better if doing relative scan in single experiment (≈ 3%)?

10 Gunther Roland BNL Workshop March 2006 Excitation Function: Total Multiplicities RHIC SPS AGS Compilation by PHOBOS nucl-ex/0301017 submitted to PRC e+e- - A+A N ch /participant pair approaches N ch in e+e- - A+A by itself can be fit with log 2 (s) - Structure at SPS energy IF compared to e+e- or p+p RHIC SPS AGS e+e- log 2 (s) Wit Busza, Zakopane ‘04 c.f. Gazdzicki, Steinberg log 2 (s) Wit Busza, Zakopane ‘04

11 Gunther Roland BNL Workshop March 2006 Fraction of produced hadrons in N ch Change from baryon- to meson dominated system over the energy range of interest! RHIC SPS AGS Excitation Function: Total Multiplicities c.f. Gazdzicki, Steinberg

12 Gunther Roland BNL Workshop March 2006 Excitation Function: Momentum Spectra Compilation by NA49 Plot from Claudia Hoehne, QM’05 filled symbol: particle open symbol: antiparticle - Structure in energy dependence of - Reminiscent of Van Hove’s T vs ε prediction (1982) - Surprisingly difficult measurement ● Decay corrections, PID acceptance “The Kink”

13 Gunther Roland BNL Workshop March 2006 RHIC STAR SPS CERES AGS? Compilation by STAR STAR PRC 72 044902 (2005) Central A+A Excitation Function: Momentum Fluctuations “The Kink” Monotonic energy dependence over measured range No results near “kink” region

14 Gunther Roland BNL Workshop March 2006 STAR STAR preliminary CERES STAR Interpretation connected to choice of variables Connection to 2-particle correlations Scaling: Connection between, N, fluctuations? Σ pT ≈ Excitation Function: Momentum Fluctuations

15 Gunther Roland BNL Workshop March 2006 QGP Little (no) √s dependence of charge fluctuations Excitation Function: Charge Fluctuations Plot from Claude Pruneau RHIC Users meeting workshop ‘04 NA49, PRC 70 064903 (2004) PHENIX: PRL 89 082301 (2002)

16 Gunther Roland BNL Workshop March 2006 N.B. Multiplicity Fluctuations Particles produced independently: σ 2 C = 1 Particles produced in clusters of size K: 0-20% central PHOBOS 200 GeV Au+Au preliminary effective cluster size ≈ 2-2.5 for 200 GeV Au+Au Analysis of forward/backward multiplicity correlations Particles are produced in clusters of 2-3 PHOBOS, Peter Steinberg, QM’05

17 Gunther Roland BNL Workshop March 2006 N.B. Multiplicity Fluctuations 0-20% central PHOBOS 200 GeV Au+Au preliminary effective cluster size ≈ 2-2.5 for 200 GeV Au+Au “Cluster” in Δη,Δφ space via 2-particle correlations (pythia p+p @200 GeV, η<3) Lesson: Hadronization cannot be ignored in discussion of early stage fluctuations PHOBOS, Peter Steinberg, QM’05

18 Gunther Roland BNL Workshop March 2006 Low Density Limit: STAR, PRC 66 034904 (2002) Voloshin, Poskanzer, PLB 474 27 (2000) Heiselberg, Levy, PRC 59 2716, (1999) Excitation Function: Elliptic flow Cu+Cu: PHOBOS QM 2005 Cu+Cu Au+Au “Participant Eccentricity” provides universal scaling Approach to equilibrium or sampling different regions of EOS? “Hydro- Limit” Collapse of proton flow at 40AGeV? provides universal scaling c.f. Shuryak, Stoecker NA49 PRC C68 034903 (2003)

19 Gunther Roland BNL Workshop March 2006 Now to the main event.....

20 Gunther Roland BNL Workshop March 2006 Excitation Function: Particle Ratios Non-monotonic behavior at AGS/SPS boundary NA49 Phys.Rev.C66:054902,2002 Plot from Claudia Hoehne, QM’05 “The Horn” e + e - (Canonical Ensemble) “The Horn” A+A e + e - (Canonical Ensemble) Becattini et al.

21 Gunther Roland BNL Workshop March 2006 Lesson: Keeping acceptance/experimental technique constant is essential for precision studies “The Horn” RHIC STAR Preliminary SPS NA49 Preliminary AGS? NA49, Christof Roland, QM’04STAR, Supriya Das, VI Workshop ‘05 Excitation Function: K/π Fluctuations

22 Gunther Roland BNL Workshop March 2006 RHIC SPS AGS? Normalized by dN/dy Scaling by dN/dy or (dN/dy) 1/2 does not work over full energy range Excitation Function: K/π Fluctuations

23 Gunther Roland BNL Workshop March 2006 Why use a collider? Can RHIC low-√s scan improve on SPS measurements? Use particle ratio fluctuations as case study K/π Fluctuationsp/π Fluctuations NA49, Christof Roland, QM’04

24 Gunther Roland BNL Workshop March 2006 Event-by-event fit of K/π (NA49) One Event: Event Ensemble: log(p tot [GeV]) Probability density function: log(p tot [GeV]) Fit dE/dx spectra in 4D binning Extract ratios with maximum likelihood fit Vary relative normalization of the particle species (K/π,p/π) in the PDF Slide from Christof Roland, Correlations ‘05, MIT

25 Gunther Roland BNL Workshop March 2006 Extracting dynamical fluctuations (NA49) Compare data to mixed events: σ2 data - σ2 mix = σ2 dynamic Process the relative widths of the distributions:σ = RMS/Mean * 100 [%] + Dynamical Fluctuations σ = 2.8% E-by-E K/π ratio Events + Finite Number Statistics Experimental Resolution σ = 15.9%σ = 16.7% E-by-E K/π ratio Events Statistical fluctuations = “mixed” Events σ = 23.1% E-by-E K/π ratio Events = “Data” Events E-by-E K/π ratio σ = 23.27% Events Slide from Christof Roland, Correlations ‘05, MIT

26 Gunther Roland BNL Workshop March 2006 Challenge: Changing acceptance (NA49) 20 GeV: 40 GeV:160 GeV: Slide from Christof Roland, Correlations ‘05, MIT

27 Gunther Roland BNL Workshop March 2006 Mid-rapidity spatial track density “You prefer your collider” Les Horribles Cernettes Fixed target Collider Fixed target Track density only rise logarithmically at collider from this:Occupancy Double hits Space Charge Baseline shifts etc

28 Gunther Roland BNL Workshop March 2006 What can be achieved at RHIC? “Ideal Detector” * >80% tracking + PID efficiency from 0.1 < pT < 2.0 GeV/c, over 2+ units of rapidity * Large acceptance trigger/centrality counters * High resolution vertexing Assume 100k central sample at each √s * 2π ToF PID coverage near y=0 possible * Acceptance in (pT,y) independent of √s * Track density grows logarithmically with√s * Consistent centrality determination from N ch But: give up very low p T, luminosity vs fixed target PID + trigger Tracking Vertexing TriggerTracking Vertexing Trigger PID + trigger

29 Gunther Roland BNL Workshop March 2006 K/π fluctuations at low-√s RHIC NA49 SPS Low √s RHIC 100k central events Relative error on K/π fluctuations Estimate that RHIC low-√s scan could allow reduction of statistical errors to ~ 1/4 of NA49 Significant reduction of systematics of √s dependence RHIC SPS

30 Gunther Roland BNL Workshop March 2006 What about low p T ? Median Kaon p T ~ 0.5 GeV (constant over SPS range) Critical fluctuations: Long Wavelength ➡ look at low p T A low p T measurement (0.1 - 0.5 GeV/c) would capture ~ 45% (75%) of all kaons (pions) Fraction of particles below pT based on NA49

31 Gunther Roland BNL Workshop March 2006 Low p T K/π Fluctuations at √s RHIC Simulation Statistical errors only Assumptions: * Ideal RHIC detector (see above) * 100k central Au+Au at each √s * K/π Fluctuations from NA49 are correct * 0.1 < p T < 0.5 GeV/c Fluctuations only at low p T Fluctuations at all p T Conclusion: RHIC low-√s scan should allow precision measurement of (low p T ) K/π fluctuations

32 Gunther Roland BNL Workshop March 2006 Summary Strong theoretical motivation for A+A at √s from 5-50 GeV Rich existing data set in this range Non-trivial structure/change in yields, ratios, fluctuations/correlations Limited statistical/systematic significance Low-√s scan at RHIC could confirm and improve experimental results

33 Gunther Roland BNL Workshop March 2006 Summary cntd To improve on SPS, low-√s run needs to be done right Sufficient run time (e.g. 1 RHIC run) Large acceptance ToF PID High resolution vertexing Careful event selection/triggering Sufficient number of energies (≥ 5)

34 Gunther Roland BNL Workshop March 2006

35 Correlations and Fluctuations, revisited centrality → Central A+A Text p+p Net-charge correlations (c.f. Balance Function) Net-charge Fluctuations Global scaling, even though underlying correlations change

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