NEUTRAL MESON PRODUCTION IN PP AND PB-PB COLLISIONS AT LHC Dmitry Blau, for the ALICE collaboration NRC “Kurchatov Institute” LHC on the March 21.11.2012.

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NEUTRAL MESON PRODUCTION IN PP AND PB-PB COLLISIONS AT LHC Dmitry Blau, for the ALICE collaboration NRC “Kurchatov Institute” LHC on the March

Physics motivation: why neutral mesons? 2  Inclusive identified hadron production is a probe for NLO pQCD   0,  and  can be detected and identified via photonic decay channels in a wide p T range.  At LHC, the PDF and FF can be probed at lower x and z than it was at previous colliders, and thus provide further constraints on these functions, which are crucial for pQCD predictions for LHC energies.  Meson production at LHC energies is dominated by gluon fragmentation at p T < 100 GeV/c: Constraints on gluon FF   meson spectrum imposes constraints on strange quark FF.  Precise measurement of neutral meson spectra is important for studying the decay photon (electron) background for a direct photon (charm and beauty) measurement  Neutral meson spectra in AA collisions, and R AA provide constraints on the energy loss models.

Detectors used in analysis 3 PHOS Central tracker Three detectors provide complementary methods with different resolution and independent systematic uncertainties. EMCAL

 0 detection in ALICE calorimeters 4 Active element: crystal of lead tungstate (PbWO 4 ) 2.2  2.2  18 cm 3 Geometry: 3 modules 64  56 crystals each; distance from IP to active surface: 460 cm Aperture: |  |<0.13, 260  <  <320  Energy range: 0<E<100 GeV Material budget from IP to PHOS: 0.2X 0  0 reconstruction via invariant mass method is possible up to p T  50 GeV/c Active element: tower of 77 layers 1.4mm lead mm scintillator 6  6  25 cm 3 Geometry: 10 modules 24  48 towers each; distance from IP to active surface: 450 cm Aperture: |  |<0.7, 80  <  <180  Energy range: 0<E<250 GeV Material budget from IP to EMCAL: 0.8X 0  0 reconstruction via invariant mass method is possible up to p T  25 GeV/c PHOSEMCAL

 0 detection via converted photons 5 Photons convert in the medium of ALICE detectors Reconstructed converted photons  tomography of ALICE ALICE material budget is well described in GEANT  0 is reconstructed via invariant mass spectra of photon pairs.

Comparison of spectra measured in PHOS and with conversion method 6 Neutral pion spectra measured in PHOS and Photon Conversion Method (PCM) agree within errors ALICE data: CERN-PH-EP , Phys.Lett. B717 (2012)

pQCD NLO calculations [*] reproduce data at  s=0.9 TeV, but overestimate  0 spectrum at  s=2.76 and 7 TeV. [*] P. Aurenche et al., Eur. Phys. J. C13, (2000).  0 spectrum in pp at 0.9, 2.76, 7 TeV 7 ALICE data: CERN-PH-EP , Phys.Lett. B717 (2012)

 spectrum in pp at 0.9, 2.76, 7 TeV 8 pQCD NLO calculations can reproduce data at  s=0.9 TeV, but overestimate  spectrum at  s=2.76 and 7 TeV. ALICE data: CERN-PH-EP , Phys.Lett. B717 (2012)

 /  0 ratio in pp at 0.9, 2.76, 7 TeV 9 Compilation of  /  0 in pp at  s= GeV ALICE measurement of the  /  0 ratio is consistent with world results in pp collisions at all energies. The measured  /  0 ratio is reproduced by pQCD. Comparison with NLO pQCD ALICE data: CERN-PH-EP , Phys.Lett. B717 (2012)

 reconstruction in pp at 7 TeV 10  0 0 Using  ± reconstructed in Central Tracking System and  0 – in PHOS Data collected in 2010: ~400 Mevents, ~ 6 nb -1 PHOS trigger data Minimum Bias trigger

 spectrum in pp at 7 TeV 11 Spectrum of  has a slope consistent with that of  0 above 4 GeV/c

Comparison of  /  0 ratio 12 ALICE measurement of the  /  0 ratio is consistent with world results in pp collisions at all energies. Comparison to theory prediction would be interesting (NLO Fragmentation Function for  is missing…)

Pb-Pb collisions 13

 0 in Pb-Pb 14 High combinatorial background in invariant mass spectra. Background is evaluated using mixed event technique. [PHOS] Efficiency is calculated via embedding. PHOS EMCAL PCM

 0 spectrum in Pb-Pb at 2.76 TeV 15

 0 R AA in Pb-Pb at 2.76 TeV 16 Suppression follows the energy dependence seen at RHIC energies Suppression agrees with charged pion R AA within errors [S.Bathe et al., PHENIX collaboration. J. Phys. G: Nucl. Part. Phys. 38 (2011) ]

Comparison to theory predictions 17 WHDG model reproduces both strength and centrality dependence Chen (HT) fails to reproduce centrality dependence Vitev’s model agrees with data in central collisions. W. A. Horowitz. Int.J.Mod.Phys. E16 (2007) 2193–2199, arXiv:nucl-th/ [NUCL-TH]. X.-F. Chen, T. Hirano, E. Wang, X.-N. Wang, and H. Zhang. Phys.Rev. C84 (2011) , ArXiv: [nucl-th]. R. Sharma, I. Vitev, and B.-W. Zhang. Phys.Rev. C80 (2009) , arXiv: [hep-ph].

Summary 18   0,  and  spectra are measured over a wide p T range  Measurements performed by several complementary subsystems  NLO pQCD describes  0,  production in pp at  s=0.9 TeV  NLO pQCD overestimates  0,  production in pp at  s=2.76 and 7 TeV  NLO pQCD describes  /  0 ratio at all energies  Suppression of  0 in Pb-Pb at  s NN =2.76 TeV is stronger than one observed at RHIC

Backup slides 19

Data samples and trigger 20  Triggers: minimum bias in pp and Pb-Pb.  Trigger detectors: SPD | VZERO-A | VZERO-C Collision system  LdT Run # pp at  s=0.9 TeV 0.14 nb -1 May 2010 pp at  s=2.76 TeV 0.7 nb -1 Apr 2011 pp at  s=7 TeV 5.5 nb -1 Jun-Aug 2010 Pb-Pb at  s NN =2.76 TeV2  b -1 Nov 2010 VZERO-CVZERO-A

Pb-Pb collisions: event characterization 21  Centrality can be determined in ALICE by various estimator. [A.Toia et al., ALICE collaboration. J. Phys. G: Nucl. Part. Phys. 38 (2011) ] The best centrality accuracy is provided by VZERO: from 0.5% in most central to 1.5% in most peripheral events [K.Aamodt et al., ALICE collaboration. PRL, 106, (2011)] See M.Floris talk at HP2012

Efficiency and Monte Carlo tuning 22 Detailed description of the ALICE environment is important for precise efficiency calculation Residual de-calibration and alignment is also taken into account in simulations Peak position and width of  0 and  mesons on invariant mass spectra were used to tune Monte Carlo simulations. ALICE data: CERN-PH-EP , arXiv