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Outline Background Global Observables in Heavy Ion Collisions

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Presentation on theme: "Outline Background Global Observables in Heavy Ion Collisions"— Presentation transcript:

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2 Outline Background Global Observables in Heavy Ion Collisions
Quark-Gluon Plasma and Heavy Ions Global Observables in Heavy Ion Collisions What are they? What do we learn from them? The STAR Experiment Analysis of Charged Particles in STAR Results Charged hadrons: h- Identified particles Conclusions January 7, 2002

3 Phase Diagram e ~ 1-3 GeV/fm3 F. Wilczek hep-ph/ Heavy Ions: How does nuclear matter look at high temperature? January 7, 2002

4 QGP in the Laboratory Space-time evolution of HI collision
January 7, 2002

5 Global observables First tool to probe the collision environment
Multiplicity distribution Inclusive single particle spectra at low p^ Represent system at Kinetic Freeze-out Thermalization, Expansion Boost invariance? Initial conditions & Evolution of the system Essential reference for systematic studies of probes of deconfinement January 7, 2002

6 Glauber Model: TAA, Npart, Ncoll
Collision Geometry Use Woods-Saxon density profile: from e-A Overlap Integral: s: Binary Collisions: Participants: January 7, 2002

7 Charged particle production
How many particles? Multiplicity distribution Geometry of the collision Correlated with impact parameter January 7, 2002

8 Momentum distributions
Difference between SPS and RHIC At high energy larger contribution from jets, mini-jets h- p^ distribution closer to power law than exponential y distribution  plateau at mid-rapidity spectra peaked at low energy (“stopping”), boost invariance at RHIC? Factorize? January 7, 2002

9 Predictions (s = 200 GeV) Different models  different predictions
pQCD parton models : Hijing dNch/dh = EKS dNch/dh = Parton hard scattering : Nexus dNch/dy ~ 1100 Microscopic Transport : UrQMD dNch/dy ~ 900 Different models  different predictions Within any model, data needed as initial conditions January 7, 2002

10 The STAR Detector at RHIC
January 7, 2002

11 Time evolution of STAR 1st year detectors (2000) 2nd year detectors 3rd year detectors Magnet Time Projection Chamber Coils Barrel EM Calorimeter Endcap Calorimeter Silicon Strip Detector Photon Multiplicity Detector Silicon Vertex Tracker Forward Time Projection Chambers Vertex Position Detectors + TOF patch TPC Endcap & MWPC Zero Degree Calorimeter Central Trigger Barrel RICH January 7, 2002

12 Au+Au in STAR TPC High Multiplicity Event  End view of detector
Side View  January 7, 2002

13 Physics Run 2000 zvertex Multiplicity distribution
Event selection, triggers, vertex finding efficiency Inclusive single particle spectra Track finding Corrections: acceptance, efficiency, etc. as a function of momentum space cell h-pt, h- y-pt, p- zvertex multiplicity particle species This analysis: Tracking: TPC Trigger ZDC + CTB PID: de/dx in TPC TPC: || < 1.8 0 < f < 2p P > 75 MeV/c Bfield: 0.25 T (1/2 nominal) Trigger: ZDC at  18 m CTB || < 1 January 7, 2002

14 Event Selection and Triggers
Zero Deg. Cal. Main Minimum Bias Trigger 99% Efficient even at high multiplicity Trigger ZDC Coincidence (East and West) OR High CTB Signal Au Au ZDC East ZDC West Central Trigger Barrel (CTB) 5% Central January 7, 2002

15 Primary h- Multiplicity
6% sys. error shown on 3 points only January 7, 2002

16 h- & h+ dN/dh, Central Events
Jacobian dN/dh, |h|<0.1 h- : 280 1 20 h+ : 287 1 20 Approaching boost invariance at RHIC January 7, 2002

17 h- p Distribution, Central
Power Law Fit (p^ = GeV/c) A (1+p  /p0) - n p0 =3.0 ± 0.3 GeV/c n= 14.8 ± 1.2 STAR <p>=0.508 ± GeV/c NA49 <p>=0.414 ± GeV/c UA1 <p>=0.392 ±0.003 GeV/c January 7, 2002

18 p Spectra in pp Collisions
Data available for s = , but not at 130 GeV Power law: E d3/d3p = A (1+p^/p0) –n interpolate A, p0, n to 130 GeV Extrapolation used in STAR January 7, 2002

19 Comparison topp Low pt  Wounded Nucleon applies
Compare to UA1 Problem UA1 s = 200 R(130/200) From power law scaling R = 0.92 at 0.2 GeV/c R = 0.70 at 2 GeV/c “Hard” Scaling Nuclear Overlap Integral TAA = 26 mb-1 for 5% most central NAA/Npp= Nbin coll=1050 “Soft” Scaling NAA / Npp=( 344/ 2 ) Low pt  Wounded Nucleon applies Rising pt  Approaching hard scaling limit? January 7, 2002

20 High p Analysis Preliminary High-pt analysis shows turnover Quenching? January 7, 2002

21 h- Centrality Classes Central collisions: cut on ZDC only (CTB veto on low multiplicity) Peripheral collisions: Cut in ZDC+CTB space STAR January 7, 2002

22 h- , Centrality dependence
Power Law behavior is observed in all centrality classes, although curvature varies. STAR Shape of dN/dh at mid-rapidity does not change with centrality. Power Law A (1+p  /p0) - n January 7, 2002

23 h- <p>, Centrality Dependence
15% Increase in <p> from 80% sample to 5% central Increase with respect to pp Collective effects Systematic uncertainty shown for STAR data January 7, 2002

24 - m Spectra (centrality, y)
Fits to Bose-Einstein Including low-pt No additional low-pt enhancement January 7, 2002

25 K- and p, m Distribution
K- Slope: moderate centrality dependence Stronger for p January 7, 2002

26 m Inverse Slopes Slope: stronger centrality dependence
with increasing particle mass Radial flow? January 7, 2002

27 - rapidity distribution
Yield fairly flat decreasing slightly with increasing y |y| < 0.1 dN/dy = 286 ± 10 y= ± 0.8 dN/dy = 271 ± 13 January 7, 2002

28 Teff vs y Teff shows more pronounced y dependence
Boost invariance does not yet hold at RHIC Flow? Additional baryons with increasing y? January 7, 2002

29 Conclusions Collisions dominated by geometry
Negative hadron distributions (Central collisions) Increased particle production relative to SPS and UA1 <p> = GeV/c (NA49 = 0.414, UA1 = 0.392) low p: ‘Wounded nucleon’ scaling; rising p: ‘binary collisions’ scaling ? Negative hadrons, centrality dependence <p> shows weak dependence  dependence ~flat, small dependence on centrality Identified  slope parameter T, weak centrality dependence Increase is most dramatic in anti-protons (Radial flow) visible y dependence: boost invariance not yet reached Collision picture including other observables is beginning to emerge January 7, 2002

30 Identified Spectra: dE/dx
Use calibrated curves: Z variable zp = ln(Imeas/Ip) p K- - e- January 7, 2002

31 - p^ distribution, centrality
Fits to Bose-Einstein Including low-pt No additional low-pt enhancement 0.05 < p^ < 0.75 Measure >80% of total yield Teff almost constant with centrality January 7, 2002

32 - Teff, centrality dependence
Slight increase in Teff with centrality Mainly in peripheral From 3d bin, consistent with no centrality dependence Even with radial flow, p are only slightly affected, small m January 7, 2002

33 - p^ distribution, rapidity
5% Most Central Mid-rapidity region range |y|<0.8  Fits to Bose-Einstein No low-p^ enhancement Each y bin scaled by factors of 2 January 7, 2002

34 PID & dE/dx Resolution p - e- K- dN/dZp Resolution ~9%
0.4 < p <0.45 GeV/c |y| < 0.1 Resolution ~9% Approaching design value of 8 % January 7, 2002


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