Statistical Model Predictions for p+p and Pb+Pb Collisions at LHC Ingrid Kraus Nikhef and TU Darmstadt.

Slides:



Advertisements
Similar presentations
Physics Results of the NA49 exp. on Nucleus – Nucleus Collisions at SPS Energies P. Christakoglou, A. Petridis, M. Vassiliou Athens University HEP2006,
Advertisements

K*(892) Resonance Production in Au+Au and Cu+Cu Collisions at  s NN = 200 GeV & 62.4 GeV Motivation Analysis and Results Summary 1 Sadhana Dash Institute.
R. L. Thews Hard Probes 2004 Lisbon QUARKONIUM FORMATION IN STATISTICAL AND KINETIC MODELS R. L. THEWS UNIVERSITY OF ARIZONA HARD PROBES 2004 LISBON November.
Strangeness production in STAR Jun Takahashi for the STAR collaboration.
DNP03, Tucson, Oct 29, Kai Schweda Lawrence Berkeley National Laboratory for the STAR collaboration Hadron Yields, Hadrochemistry, and Hadronization.
STAR Patricia Fachini 1 Brookhaven National Laboratory Motivation Data Analysis Results Conclusions Resonance Production in Au+Au and p+p Collisions at.
1 Baryonic Resonance Why resonances and why  * ? How do we search for them ? What did we learn so far? What else can we do in the.
5-12 April 2008 Winter Workshop on Nuclear Dynamics STAR Particle production at RHIC Aneta Iordanova for the STAR collaboration.
Resonance Dynamics in Heavy Ion Collisions 22nd Winter Workshop on Nuclear Dynamics , La Jolla, California Sascha Vogel, Marcus Bleicher UrQMD.
Statistical Models A.) Chemical equilibration (Braun-Munzinger, Stachel, Redlich, Tounsi) B.) Thermal equilibration (Schnedermann, Heinz) C.) Hydrodynamics.
1 A simple model to study the centrality dependence of observables from SPS to RHIC energies inspired by the first CuCu results to extract the physics.
Helen Caines Yale University SQM – L.A.– March 2006 Using strange hadron yields as probes of dense matter. Outline Can we use thermal models to describe.
Recent Developments in THERMUS “The Wonders of Z ” Spencer Wheaton Dept of Physics University of Cape Town.
1 Statistical Models and STAR’s Strange Data Sevil Salur Yale University for the STAR Collaboration.
Hadronic Resonances in Heavy-Ion Collisions at ALICE A.G. Knospe for the ALICE Collaboration The University of Texas at Austin 25 July 2013.
Masashi Kaneta, LBNL Masashi Kaneta for the STAR collaboration Lawrence Berkeley National Lab. First results from STAR experiment at RHIC - Soft hadron.
Measurements of the Charge Balance Function at RHIC from √s NN = 7.7 to 200 GeV Gary D. Westfall, for the STAR Collaboration (Michigan State University)
M. Beitel, K. Gallmeister, CG, arXiv: in collaboration with: M. Beitel, K. Gallmeister and J. Noronha-Hostler - history of Hagedorn States - nuclear.
Thermal Production of particles at RHIC (Test of Chemical Freeze-out at RHIC) Jun Takahashi for the STAR collaboration SQM2008, Beijing, China.
Spectra Physics at RHIC : Highlights from 200 GeV data Manuel Calderón de la Barca Sánchez ISMD ‘02, Alushta, Ukraine Sep 9, 2002.
T BB Hadronic matter Quark-Gluon Plasma Chiral symmetry broken Chiral symmetry restored LHC Modelling Statistical Operator: implementic conservation.
In-Kwon YOO Pusan National University Busan, Republic of KOREA SPS Results Review.
Matter System Size and Energy Dependence of Strangeness Production Sevil Salur Yale University for the STAR Collaboration.
Statistical Model Predictions for p+p and Pb+Pb Collisions at LHC Ingrid Kraus Nikhef and TU Darmstadt.
Do small systems equilibrate chemically? Ingrid Kraus TU Darmstadt.
Lecture 10 : Statistical thermal model Hadron multiplicities and their correlations and fluctuations (event-by-event) are observables which can provide.
Introduction The statistical model approach is established by analysis of particle ratios of the high energy heavy ion collisions in GSI-SIS to CERN-SPS.
1 Jeffery T. Mitchell – Quark Matter /17/12 The RHIC Beam Energy Scan Program: Results from the PHENIX Experiment Jeffery T. Mitchell Brookhaven.
Energy Scan of Hadron (  0 ) Suppression and Flow in Au+Au Collisions at PHENIX Norbert Novitzky for PHENIX collaboration University of Jyväskylä, Finland.
Helen Caines Yale University Soft Physics at the LHC - Catania - Sept Questions for the LHC resulting from RHIC Strangeness Outline Chemistry Yields.
Strangeness opportunities at the LHC RIKEN BNL Research Center Workshop - BNL - 15/02/06 1.Strangeness at LHC energies Extrapolations / Motivations 2.Strange.
Strangeness production in HIC Evgeni E. Kolomeitsev Matej Bel University Banska Bystrica hidden open.
Helen Caines Yale University 1 st Meeting of the Group on Hadronic Physics, Fermi Lab. – Oct Bulk matter properties in RHIC collisions.
Masashi Kaneta, First joint Meeting of the Nuclear Physics Divisions of APS and JPS 1 / Masashi Kaneta LBNL
ALICE Overview Ju Hwan Kang (Yonsei) Heavy Ion Meeting June 10, 2011 Korea University, Seoul, Korea.
First measurements in Pb—Pb collisions at  s NN =2.76 TeV with ALICE at the LHC M. Nicassio (University and INFN Bari) for the ALICE Collaboration Rencontres.
Robert Pak (BNL) 2012 RHIC & AGS Annual Users' Meeting 0 Energy Ro Robert Pak for PHENIX Collaboration.
1 Energy and system size dependence of strangeness production, from SPS to RHIC Jun Takahashi & Marcelo Munhoz for the STAR collaboration.
A Blast-wave Model with Two Freeze-outs Kang Seog Lee (Chonnam Nat’l Univ.)  Chemical and thermal analysis, done in a single model HIM
9 th June 2008 Seminar at UC Riverside Probing the QCD Phase Diagram Aneta Iordanova.
System-size dependence of strangeness production, canonical strangeness suppression, and percolation Claudia Höhne, GSI Darmstadt.
Selected topics in Heavy Ion Physics Primorsko 2014 Peter Hristov.
Two freeze-out model for the hadrons produced in the Relativistic Heavy-Ion Collisions. New Frontiers in QCD 28 Oct, 2011, Yonsei Univ., Seoul, Korea Suk.
School of Collective Dynamics in High-Energy CollisionsLevente Molnar, Purdue University 1 Effect of resonance decays on the extracted kinetic freeze-out.
R. Lednicky: Joint Institute for Nuclear Research, Dubna, Russia I.P. Lokhtin, A.M. Snigirev, L.V. Malinina: Moscow State University, Institute of Nuclear.
Bulk properties of the system formed in Au+Au collisions at √s NN = 14.5 GeV using the STAR detector at RHIC Vipul Bairathi (for the STAR Collaboration)
Itzhak Tserruya Initial Conditions at RHIC: an Experimental Perspective RHIC-INT Workshop LBNL, May31 – June 2, 2001 Itzhak Tserruya Weizmann.
Hadronic resonance production in Pb+Pb collisions from the ALICE experiment Anders Knospe on behalf of the ALICE Collaboration The University of Texas.
Helmut Oeschler Darmstadt University of Technology Transition from Baryonic to Mesonic Freeze Out SQM2006, March 28 th, 2006.
QM08, Jaipur, 9 th February, 2008 Raghunath Sahoo Saturation of E T /N ch and Freeze-out Criteria in Heavy Ion Collisions Raghunath Sahoo Institute of.
Christina MarkertHirschegg, Jan 16-22, Resonance Production in Heavy Ion Collisions Christina Markert, Kent State University Resonances in Medium.
24 June 2007 Strangeness in Quark Matter 2007 STAR 2S0Q0M72S0Q0M7 Strangeness and bulk freeze- out properties at RHIC Aneta Iordanova.
Japanese Physics Society meeting, Hokkaido Univ. 23/Sep/2007, JPS meeting, Sapporo, JapanShinIchi Esumi, Inst. of Physics, Univ. of Tsukuba1 Collective.
Helen Caines Yale University Strasbourg - May 2006 Strangeness and entropy.
PHENIX Results from the RHIC Beam Energy Scan Brett Fadem for the PHENIX Collaboration Winter Workshop on Nuclear Dynamics 2016.
Hadron Spectra and Yields Experimental Overview Julia Velkovska INT/RHIC Winter Workshop, Dec 13-15, 2002.
Soft physics in PbPb at the LHC Hadron Collider Physics 2011 P. Kuijer ALICECMSATLAS Necessarily incomplete.
1 A simple model to study the centrality dependence of observables from SPS to RHIC energies inspired by the first CuCu results later checked against EPOS.
Strange hadrons and resonances at LHC energies with the ALICE detector INPC 2013 Firenze, Italy 2 -7 June 2013 A. Badalà (INFN Sezione di Catania) for.
1 Strange Resonance Production in p+p and Au+Au Collisions at RHIC energies. Christina Markert, Yale University for the STAR Collaboration QM2004,
ENERGY AND SYSTEM SIZE DEPENDENCE OF CHEMICAL FREEZE-OUT
P. Castorina Dipartimento di Fisica ed Astronomia
A few observations on strangeness production at SPS and RHIC
Statistical Model Predictions for p+p and Pb+Pb Collisions at LHC
Summary Model Data from RHIC experiments Introduction
Panos Christakoglou1 for the ALICE Collaboration 1Nikhef
Strangeness with CBM Volker Friese
Identified Charged Hadron Production
Dipartimento Interateneo di Fisica, Bari (Italy)
Claudia Höhne, GSI Darmstadt
Presentation transcript:

Statistical Model Predictions for p+p and Pb+Pb Collisions at LHC Ingrid Kraus Nikhef and TU Darmstadt

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Outline Predictions for Pb+Pb collisions at LHC –Extrapolation of thermal parameters, predictions –Experimental observables for T and μ B determination From Pb+Pb to p+p: system size and energy dependence –Model ansatz with correlated, equilibrated clusters –Analysed data and results Predictions for p+p collisions at LHC –Driven by initial or final state? Summary in Collaboration with H. Oeschler, K. Redlich, J. Cleymans, S. Wheaton

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Hadron ratios in the grand canonical ensemble Grand canonical ensemble –large systems, large number of produced hadrons –two parameters describe particle ratios in the hadronic final state A. Andronic, P. Braun-Munzinger, J. Stachel, Nucl. Phys. A772 (2006) 167 T, V,  T, V b, N b

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, On the freeze-out curve: T LHC ≈ T RHIC ≈ 170 MeV T ≤ T C ≈ 170 MeV μ B from parametrised freeze-out curve: μ B (√(s NN ) = 5.5TeV) = 1 MeV Phys. Rev. C 73 (2006) Grand canonical ensemble for Pb+Pb predictions Thermal Parameters in Pb+Pb Phys. Rev. C 73(2006)

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Predictions for Pb+Pb Reliable for stable particles Benchmark for resonances Errors: T = 170 +/- 5 MeV μ B = MeV Phys. Rev. C 74 (2006) All calculations with THER MUS hep-ph/

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, T and μ B dependence I: mixed ratios Controlled by masses Weakly dep. on μ B and T –μ B term cancels –larger contributions from resonances at higher T

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, T and μ B dependence I: mixed ratios Controlled by masses Weakly dep. on μ B and T –μ B term cancels –larger contributions from resonances at higher T

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, T and μ B dependence I: mixed ratios Controlled by masses Weakly dep. on μ B and T –μ B term cancels –larger contributions from resonances at higher T K/  –not usable for T and  B determination –good test of predictions

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, T and μ B dependence II: h/h ratios Sensitive on μ B – μ S opposite trend of μ B –determine μ B from p/p weakly dep. on T _ _ ☺

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, T dependence: ratios with large mass differences ☺ Ratios with larger mass differences are more sensitive T from  and/or  K

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Canonical suppression Canonical ensemble –small systems / peripheral collisions, low energies –suppressed phase-space for particles related to conserved charges –Stronger suppression for multi-strange hadrons –Suppression depends on strangeness content, not difference

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Canonical suppression Canonical ensemble –small systems / peripheral collisions, low energies –suppressed phase-space for particles related to conserved charges –Stronger suppression for multi-strange hadrons –Suppression depends on strangeness content, not difference –Suppressed strangeness production beyond canonical suppression SPS √(s NN ) = 17 AGeV

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Modification of the model Statistical Model approach: T and μ B –Volume for yields → radius R used here Deviations: strangeness undersaturation factor  S –Fit parameter Alternative: small clusters (R C ) in fireball (R): R C ≤ R –Chemical equilibrium in subvolumes: canonical suppression –R C free parameter Study –p+p, C+C, Si+Si, Pb+Pb / Au+Au collisions –at SPS and RHIC energies R RCRC

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, System size and energy dependence of the cluster size Small clusters in all systems Small system size dependence p+p –energy dependence? Pb+Pb / Au+Au –data consistent with saturated strangeness production p+p C+C Si+Si Pb/Au

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, System size and energy dependence of the cluster size A+A: clusters smaller than fireball R C not well defined for R C ≥ 2 fm because suppression vanishes R C = R Pb+Pb Au+Au

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, System size and energy dependence of the cluster size Particle ratios saturate at R C ≈ fm –no precise determination for weak strangeness suppression Pb+Pb Au+Au R C = R

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Extrapolation to LHC: T -  B – systematics Chemical decoupling conditions extracted from SIS up to RHIC feature common behavior Extrapolation to LHC energy with parametrisation e.g. Nucl. Phys. A 697 (2002) 902 Phys. Rev. C 73(2006)

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, System size and energy dependence of T and  B p+p C+C Si+Si Pb/Au T, μ B weakly dependent on system size

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Extrapolation to LHC: cluster size what defines R C in p+p? initial size of p+p system relevant –R C const final state of large number of produced hadrons relevant –R C increases with multiplicity

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Prediction for p+p significant increase of ratios at R C ≈ 1.5 fm K /  and  behave differently –multistrange hadrons suffer stronger suppression R C will be determined with ALICE data

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Extraction of R C Particle ratios w/o strangeness are insensitive to R C Sensitivity increases with strangeness difference R C from  ☺

Ingrid Kraus, NikhefLast call for predictions workshop, CERN, May 30, Summary Pb+Pb –predictions for particle ratios with extrapolated parameters T, μ B –T, μ B determination with p / p and  / K or  /  ratios _ p+p –predictions difficult due to unknown degree of canonical suppression –Cluster radius R C from data