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Alexander Milov for the PHENIX collaboration June 17, 2004

dN ch /d η and dE T /d η at Mid-Rapidity from SIS to LHC. Alexander Milov for the PHENIX collaboration June 17, 2004. Outline. Apparatus, Measurements & Errors: PHENIX detector dN ch /d η and dE T /d η measurement in PHENIX

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Alexander Milov for the PHENIX collaboration June 17, 2004

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  1. dNch/dη and dET/dη at Mid-Rapidity from SIS to LHC Alexander Milov for the PHENIX collaboration June 17, 2004 Sasha Milov Focus on Multiplicity Bari June 17, 2004

  2. Outline. • Apparatus, Measurements & Errors: • PHENIX detector • dNch/dη and dET/dη measurement in PHENIX • Centrality & Trigger efficiency analysis using NBD. • Results: • PHENX results • RHIC and lower energy results • Physics: • √sNN dependencies • Averaged <ET>/<Nch> • Centrality shape • Theoretical Models from Experimental Point of View • Summary Sasha Milov Focus on Multiplicity Bari June 17, 2004

  3. Brazil University of São Paulo, São Paulo China Academia Sinica, Taipei, Taiwan China Institute of Atomic Energy, Beijing Peking University, Beijing France LPC, University de Clermont-Ferrand, Clermont-Ferrand Dapnia, CEA Saclay, Gif-sur-Yvette IPN-Orsay, Universite Paris Sud, CNRS-IN2P3, Orsay LLR, Ecòle Polytechnique, CNRS-IN2P3, Palaiseau SUBATECH, Ecòle des Mines at Nantes, Nantes Germany University of Münster, Münster Hungary Central Research Institute for Physics (KFKI), Budapest Debrecen University, Debrecen Eötvös Loránd University (ELTE), Budapest India Banaras Hindu University, Banaras Bhabha Atomic Research Centre, Bombay Israel Weizmann Institute, Rehovot Japan Center for Nuclear Study, University of Tokyo, Tokyo Hiroshima University, Higashi-Hiroshima KEK, Institute for High Energy Physics, Tsukuba Kyoto University, Kyoto Nagasaki Institute of Applied Science, Nagasaki RIKEN, Institute for Physical and Chemical Research, Wako RIKEN-BNL Research Center, Upton, NY Rikkyo University, Tokyo, Japan Tokyo Institute of Technology, Tokyo University of Tsukuba, Tsukuba Waseda University, Tokyo S. Korea Cyclotron Application Laboratory, KAERI, Seoul Kangnung National University, Kangnung Korea University, Seoul Myong Ji University, Yongin City System Electronics Laboratory, Seoul Nat. University, Seoul Yonsei University, Seoul Russia Institute of High Energy Physics, Protovino Joint Institute for Nuclear Research, Dubna Kurchatov Institute, Moscow PNPI, St. Petersburg Nuclear Physics Institute, St. Petersburg St. Petersburg State Technical University, St. Petersburg Sweden Lund University, Lund 12 Countries; 58 Institutions; 480 Participants* USA Abilene Christian University, Abilene, TX Brookhaven National Laboratory, Upton, NY University of California - Riverside, Riverside, CA University of Colorado, Boulder, CO Columbia University, Nevis Laboratories, Irvington, NY Florida State University, Tallahassee, FL Florida Technical University, Melbourne, FL Georgia State University, Atlanta, GA University of Illinois Urbana Champaign, Urbana-Champaign, IL Iowa State University and Ames Laboratory, Ames, IA Los Alamos National Laboratory, Los Alamos, NM Lawrence Livermore National Laboratory, Livermore, CA University of New Mexico, Albuquerque, NM New Mexico State University, Las Cruces, NM Dept. of Chemistry, Stony Brook Univ., Stony Brook, NY Dept. Phys. and Astronomy, Stony Brook Univ., Stony Brook, NY Oak Ridge National Laboratory, Oak Ridge, TN University of Tennessee, Knoxville, TN Vanderbilt University, Nashville, TN *as of January 2004 Sasha Milov Focus on Multiplicity Bari June 17, 2004

  4. PHENIX Detector. • Pad Chamber Detectors: • MWPC with binary pad readout • 2.5m and 5.0m from the IP • |η|< 0.35 Δφ = 900 • σφ= 1.4mrad (1.7mm PC1) • ση= 0.7×10-3 (3.6mm PC1) • Double Hit Resolution ~4cm • Electromagnetic Calorimeter: • Lead+Scintillator 18 X0 • 5.1m from the IP • |η|< 0.38 Δφ = 900 • σE= 8.1%/√E[GeV] ×2.1% • Beam-Beam Counters: • 64 Cherenkov Counters • 3.1<|η|< 3.9 Δφ = 3600 • σvertex= ~5mm (central) • σt= ~100 ps Sasha Milov Focus on Multiplicity Bari June 17, 2004

  5. Multiplicity analysis. • Counting tracks on statistical basis: • Combine all hits in PC1 to hits in PC3 • Project lines onto the plane through the beam pipe • Count tracks inside the acceptance • Subtract combinatorial background by event mixing. • Corrections: • Tracks outside acceptance and background subtraction 4.3%±1% • Inactive regions 15%±2.3% • Double hit resolution Hit losses 2×7% Background subtraction 3.6% of bkg Uncertainty (in central) ±3.6% • Particle in-flow and out-flow Low energy 10%±5.5% Higher energy 1% ±2% No Field Sasha Milov Focus on Multiplicity Bari June 17, 2004

  6. Transverse Energy analysis. • ET definition: • ET = E×sin(θ) • ET ≈ mT at Mid-Rapidity in C.M.S. • E is full E for leptons and mesons • E is E±m for (anti) baryons • EMCal energy scale: • Measures full energy of e± and γ (π0) • Slow hadrons are fully absorbed. • Relativistic hadrons leave M.I.P. peak • EMCal measures >75% of energy • Systematic errors: • Energy response 3.9%-4.7% • Noise in central: <0.5% in peripheral: 3.5%-6.% • In-flow and out-flow 3.0% AGS test RHIC data Sasha Milov Focus on Multiplicity Bari June 17, 2004

  7. Centrality and trigger analysis. Assumed Nch ~ Np Shape of η-profile Knowledge of Nch = f(Np) Np using Glauber Nch using Generator Nhits using Detector MC Np, Nc εtrigger Match to the data Sasha Milov Focus on Multiplicity Bari June 17, 2004

  8. Centrality and trigger using NBD. Shape of η-profile Knowledge of Nch = f(Np) Uncorrelated Nch production Np using Glauber Nch using Generator Nhits using Detector MC Use N.B. statistics Np, Nc εtrigger Match to the data Assumed Nch ~ Np Negative Binominal Distribution: is the statistics describing distribution of number of trials (n) which are necessary to get a number of successes, if the probability of success (μ) is known: P(n,,k) = (n + k) / ((k) n!)  (/k)n / (1 + /k)n+k where k is a N.B.D. parameter related to the width of the distribution  in a following way: (/)2 = 1/k + 1/ Sasha Milov Focus on Multiplicity Bari June 17, 2004

  9. d-Au example. Assumed Nch ~ Np & uncorrelated Nch production Np, Nc εtrigger Match to the data Use N.B. statistics Np using Glauber Sasha Milov Focus on Multiplicity Bari June 17, 2004

  10. Other examples: Sasha Milov Focus on Multiplicity Bari June 17, 2004

  11. Results: The distributions. • Only part of the acceptance shown • “Classical” Shape: Peak, Valley, Edge. • Centrality classes shown. • Edge might be modified due to acceptance limitation Sasha Milov Focus on Multiplicity Bari June 17, 2004

  12. Results: Centrality curves. • Consistent behavior for ET and Nch • Both increase with energy • Both show steady rise from peripheral to central Sasha Milov Focus on Multiplicity Bari June 17, 2004

  13. Results: Systematic errors. • Three types of errors • All plotted as 1 standard deviation • Statistical error: • Point-by-point error (<1%). In all points is smaller than the marker size. • Systematic errors: • Band (correlated) allow to tilt points within the limit of the band. In peripheral (~20%) due to trigger uncertainty. In central (~4%) are due to DHR of the detectors • Scaling (correlated) allow to shift curves up and down. • Total systematic error is a quadratic sum of two. It is shown with the bars. Sasha Milov Focus on Multiplicity Bari June 17, 2004

  14. Results: Ratios at different energies. • R200/19.6 is larger for ET than for Nch • Both are flat within systematic errors • Both show steady rise from peripheral to central Sasha Milov Focus on Multiplicity Bari June 17, 2004

  15. Results: Ratios <ET>/<Nch>. • Ratio <ET>/<Nch> increases by ~20% from 19.6 GeV to 200 GeV and stays the same between 200 GeV and 130 GeV • Consistent with the average particle momentum increase between those two energies. • Ratio <ET>/<Nch> is independent of centrality • Still a puzzle. • Same freeze-out conditions? • Since trigger and centrality related uncertainties cancel out, the flatness of the curves is quite precise statement. Sasha Milov Focus on Multiplicity Bari June 17, 2004

  16. Comparison to other RHIC results. • Spectacular agreement between all 4 RHIC experiments: • All measurements are absolutely independent (including human factor) besides similar approach of using Glauber model. • BRAHMS: Si detectors + tracking • PHENIX: PC at 2.5m and 5m • PHOBOS: Si detectors • STAR: Tracking in magnetic field. • Would allow to calculate averaged values and reduce systematic errors Sasha Milov Focus on Multiplicity Bari June 17, 2004

  17. Recalculation between systems. • In C.M.S.: • At Mid-Rapidity: ET~mT • dET/dy ≈ 1.25 dET/dη • In Lab: • dmT/dy ≈ 1.25 dET/dy • dET/dy ≈ dET/dη • In C.M.S.: • dNch/dy ≈ 1.25 dNch/dη • In Lab: • dNch/dy ≈ 1.04 dNch/dη • Recalculation parameters are “rather” independent on energy • A systematic error of 5% is assigned to any recalculated value Sasha Milov Focus on Multiplicity Bari June 17, 2004

  18. Comparison to other SPS results. • Good agreement between PHENIX measurements at 19.6 GeV and SPS measurements at 17.2 GeV in both measured values. • SPS spread of the data is larger than RHIC, but the same averaging should be possible to reduce the systematic errors. Sasha Milov Focus on Multiplicity Bari June 17, 2004

  19. Comparison of SPS results. • At intermediate SPS energy the energy spread between points is relatively large. • Using weighted average and error scaling by S-factor (see PDG) • S=1 if χ2/n.d.f. < 1 • S=√χ2/n.d.f. if χ2/n.d.f. > 1 • At lower SPS energy the data spread is even larger, a higher quality data is highly desirable. • At AGS energy the Centrality curve is deduced from a combined data. Sasha Milov Focus on Multiplicity Bari June 17, 2004

  20. Comparison to other results. • Averaged SPS data at 17,3 GeV is in very good agreement to averaged RHIC data at 19.6 GeV (expected difference ~4%) • There is a continuous set of measurements from AGS to RHIC data. Sasha Milov Focus on Multiplicity Bari June 17, 2004

  21. √sNN dependence. • PHENX suggested ln(sNN) at QM01 and it works well with better and larger data-set. • Both in ET and in Nch show log-scaling. • Works even better on Nch for Np = 350. Band on the right is 2σ error! • Extrapolation to LHC dNch/dη = (6.1±0.13)×(0.5Np). • Extrapolation to lowest energy gives: • for ET: √s0NN = 2.35 ± 0.2 GeV • for Nch: √s0NN = 1.48 ± 0.02 GeV Sasha Milov Focus on Multiplicity Bari June 17, 2004

  22. Low √sNN story Nch ET FOPI ln(√sNN) 2a.m.u. • Higher energy: <ET>/<Nch> ~ constant √soNN Nch • Lower energy: √soNN <ET>/<Nch>  <mT> • That’s what we see • What √soNN mean? Caution: they are in GeV! • Energy conservation law. • Now comes FOPI at <0.1 GeV kinetic energy! -0.5 GeV +0.5 GeV Sasha Milov Focus on Multiplicity Bari June 17, 2004

  23. What happens to <mT>? • At low √sNN: • ET is “produced” energy only. • Nch can benefit from pre-existing particles (baryons). • At higher √sNN: • Critical temperature Tc=0.17GeV. • Assuming: <Ekin>=3/2Tc ≈ 0.26 GeV<m0> ≈ 0.25 GeV <mT> = <Ekin> + <m0> ≈ 0.51 GeV <ET>/<Nch> ≈ 1.6 <mT> ≈ 0.82 GeV • Prediction for LHC: 0.93±0.04 GeV • How does flow work? Sasha Milov Focus on Multiplicity Bari June 17, 2004

  24. Centrality shapes. • Hard/Soft approach: • Might be deceiving: e.g. strangeness turn on. • Negatively correlated errors are huge. • Npα parameterizations: • assumes a power law • what does α mean? • Still large errors • PHOBOS as of June 2,2004 nucl-ex/0405027: • Bottom line: inconclusive! Sasha Milov Focus on Multiplicity Bari June 17, 2004

  25. Centrality shapes: basic approach • three centrality bins divided by ln(√sNN)-parameterization. • Central bin Np = 350 is just consistent with 1 as expected • Mid-central bin Np=100 with large systematic errors is just an offset • Most peripheral: Np = 2 (pp) for a moment needs more data at low energy. Turns out to be quite difficult to get it right. Sasha Milov Focus on Multiplicity Bari June 17, 2004

  26. Bjorken energy. • Done at all three energies • STAR advocates another approach taking for overlap area S ~Np3/2. • Difference to standard approach: area of the nuclei vs. area of the nucleons • Makes some difference at low Np • Recent STAR finding: (nucl-ex/03011017) dET/dy / (0.5 Np) decreases with Np ?! Sasha Milov Focus on Multiplicity Bari June 17, 2004

  27. Models: experimentalist’s view • Model vs. Generator: • Do you know why we are such in love with HIJING? • IMHO: Model is a precursor to the Generator. • Major difference besides completeness and ease of use: Generator does partial probabilities! • What happened to systematic errors? • How well defined a model is within itself? • Only Mini-Jet gives a band. • How should experimentalist compare models to data? • Thanks to all authors who sent us their data! Sasha Milov Focus on Multiplicity Bari June 17, 2004

  28. Models I LUCIFER Hadronic cascade model, input fixed from lower energy. D.E.Kahana & S.H.Kahana, nucl-th/0208063. Minijet Multiphase transport model, includes both initial partonic and final hadronic interactions. S. Lee and X.N. Wang, Phys Lett B527, 85 (2002) EKRT K.J. Eskola, et al., Nucl. Phys. B570, 379 (2000), Phys Lett B497, 39 (2001). SSHM Saturation for Semi-Hard Minijetis. pQCD-based for semi-hard partonic interaction WNM for soft particle production. A.Accardi, Phys Rev C64, 064905 (2001). KLN D. Kharzeev and M. Nardi, Phys Lett B507, 121(2001), D. Kharzeev and E. Levin, Phys Lett B523, 79 (2001). Sasha Milov Focus on Multiplicity Bari June 17, 2004

  29. Models II DSM: Dual String Model, Dual Parton Model + strings. R. Ugoccioni, Phys Lett B49, 253 (2000). A. Capella et al, Phys Lett C236, 225 (1994). HIJING: pQCD for initial minijet production and the Lund string model for jet fragmentation and hadronization, +jet quenching +nuclear shadowing. X.N. Wang et al. PRC 68, 054902 (2003). LEXUS: Linear EXtrapolation of UltraRrelativsitic nucleon-nucleon scattering data to nucleus- nucleus collisions. S. Jeon and J. Kapusta, Phys Rew C63, 011901 (2001) AMPT: multiphase transport model +initial partonic and final hadronic interactions. Z. Lin et al. Phys Rew. C64, 011902 (2001). SFM: String Fusion Model string model, includes hard collisions, collectivity in the initial state (string fusion), and final state. N. Armesto Perez et al., Phys Lett B527, 92 (2002) Sasha Milov Focus on Multiplicity Bari June 17, 2004

  30. Models III Sasha Milov Focus on Multiplicity Bari June 17, 2004

  31. What else do we need. • We expect collaboration to fill the missing gaps in the paper and give it more physical impact: • what do parameters of the ln(√sNN)-scaling mean? • help with quality pp data at low energy • polish the model section 62 GeV data. • PPG19 draft to be released to collaboration today without 62 GeV • Michael Mendenhall from VU is working on the data. • We might have results + an analysis note in scope of weeks. • Impact on the paper: • for physics: minimal • for completeness: desirable • for future references: good • text/structure change to incorporate: minimal (~1 day) • If we have the data my suggestion is to bring it to convenor’s meeting to decide when it happens, if not too late. Sasha Milov Focus on Multiplicity Bari June 17, 2004

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