STATISTICAL MODELS in high energy collisions OUTLINE oIntroduction oFormulation for full microcanonical ensemble oDiscussion on “triviality” oNumerical.

Slides:



Advertisements
Similar presentations
Ch2. Elements of Ensemble Theory
Advertisements

Review Of Statistical Mechanics
Molecular Dynamics at Constant Temperature and Pressure Section 6.7 in M.M.
, CZE ISMD2005 Zhiming LI 11/08/ and collisions at GeV Entropy analysis in and collisions at GeV Zhiming LI (For the NA22 Collaboration)
Prethermalization. Heavy ion collision Heavy ion collision.
Hard Photon Production in a Chemically Equilibrating QGP at Finite Baryon Density Zejun He Zejun He Shanghai Institute of Applied Physics Research Chinese.
What is the meaning of the statistical model ? F.B. hep-ph OUTLINE oIntroduction oDiscussion: phase space dominance, triviality and Lagrange multipliers.
Effects of Bulk Viscosity on p T -Spectra and Elliptic Flow Parameter Akihiko Monnai Department of Physics, The University of Tokyo, Japan Collaborator:
1 Lecture 6 Ideal gas in microcanonical ensemble. Entropy. Sackur-Tetrode formula. De Broglie wavelength. Chemical potential. Ideal gas in canonical ensemble.
1 Lecture 5 The grand canonical ensemble. Density and energy fluctuations in the grand canonical ensemble: correspondence with other ensembles. Fermi-Dirac.
The Electromagnetic Structure of Hadrons Elastic scattering of spinless electrons by (pointlike) nuclei (Rutherford scattering) A A ZZ  1/q 2.
Phase transition of hadronic matter in a non-equilibrium approach Graduate Days, Frankfurt, , Hannah Petersen, Universität Frankfurt.
First Results From a Hydro + Boltzmann Hybrid Approach DPG-Tagung, Darmstadt, , Hannah Petersen, Universität Frankfurt.
Chemical Equilibration at the Hagedorn Temperature Jaki Noronha-Hostler Collaborators: C. Greiner and I. Shovkovy.
R Measurement at charm resonant region Haiming HU BES Collaboration Charm 2007 Cornell University Ithaca, NY. US.
STAR Patricia Fachini 1 Brookhaven National Laboratory Motivation Data Analysis Results Conclusions Resonance Production in Au+Au and p+p Collisions at.
Symmetries By Dong Xue Physics & Astronomy University of South Carolina.
DPF Victor Pavlunin on behalf of the CLEO Collaboration DPF-2006 Results from four CLEO Y (5S) analyses:  Exclusive B s and B Reconstruction at.
STAR Looking Through the “Veil of Hadronization”: Pion Entropy & PSD at RHIC John G. Cramer Department of Physics University of Washington, Seattle, WA,
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.
Effects of Bulk Viscosity at Freezeout Akihiko Monnai Department of Physics, The University of Tokyo Collaborator: Tetsufumi Hirano Nagoya Mini-Workshop.
Lecture 5: Electron Scattering, continued... 18/9/2003 1
REGGAE – Generator for Uniform Filling of LIPS Ivan Melo, Boris Tomášik, Michal Mereš, Vlado Balek, Vlado Černý Zimanyi Winter School
Introduction to (Statistical) Thermodynamics
Ultracold Fermi gases University of Trento BEC Meeting, Trento, 2-3 May 2006 INFM-CNR Sandro Stringari.
Identified Particle Ratios at large p T in Au+Au collisions at  s NN = 200 GeV Matthew A. C. Lamont for the STAR Collaboration - Talk Outline - Physics.
Irakli Chakaberia Final Examination April 28, 2014.
Uniform Filling of Multiparticle Phase Space Ivan Melo, Boris Tomášik, Michal Mereš, Vlado Balek, Vlado Černý Seminár Bratislava
1 CE 530 Molecular Simulation Lecture 6 David A. Kofke Department of Chemical Engineering SUNY Buffalo
STRING PERCOLATION AND THE GLASMA C.Pajares Dept Particle Physics and IGFAE University Santiago de Compostela CERN The first heavy ion collisions at the.
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.
Chemical Reactions in Ideal Gases. Non-reacting ideal gas mixture Consider a binary mixture of molecules of types A and B. The canonical partition function.
Lecture III Trapped gases in the classical regime Bilbao 2004.
Chiral phase transition and chemical freeze out Chiral phase transition and chemical freeze out.
BEC from "inside" O.Utyuzh The Andrzej Sołtan Institute for Nuclear Studies (SINS), Warsaw, Poland * In collaboration with G.Wilk and Z.Wlodarczyk.
Summary Boltzman statistics: Fermi-Dirac statistics:
Shear Viscosity and Viscous Entropy Production in Hot QGP at Finite Density 报告人: 刘 绘 华中师范大学 粒子所.
Ch 22 pp Lecture 2 – The Boltzmann distribution.
Víctor M. Castillo-Vallejo 1,2, Virendra Gupta 1, Julián Félix 2 1 Cinvestav-IPN, Unidad Mérida 2 Instituto de Física, Universidad de Guanajuato 2 Instituto.
Probing QCD Phase Diagram with Fluctuations of conserved charges Krzysztof Redlich University of Wroclaw & EMMI/GSI QCD phase boundary and its O(4) „scaling”
Heavy Flavor Productions & Hot/Dense Quark Matter 1 Lattice calculations on Heavy flavor ~ Open and Hidden charm states above Tc ~ Takashi Umeda (BNL)
ChE 452 Lecture 17 Review Of Statistical Mechanics 1.
June 25, 2004 Jianwei Qiu, ISU 1 Introduction to Heavy Quark Production Jianwei Qiu Iowa State University CTEQ Summer School on QCD Analysis and Phenomenology.
Measurements of Top Quark Properties at Run II of the Tevatron Erich W.Varnes University of Arizona for the CDF and DØ Collaborations International Workshop.
Lecture 2: The First Second Baryogenisis: origin of neutrons and protons Hot Big Bang Expanding and cooling “Pair Soup” free particle + anti-particle pairs.
Coulomb final state interactions and modelling B-E correlations O.Utyuzh The Andrzej Sołtan Institute for Nuclear Studies (SINS), Warsaw, Poland.
1 Lecture-03 The Thermal History of the universe Ping He ITP.CAS.CN
Other Partition Functions
Results from an Integrated Boltzmann+Hydrodynamics Approach WPCF 2008, Krakau, Jan Steinheimer-Froschauer, Universität Frankfurt.
R. Lednicky: Joint Institute for Nuclear Research, Dubna, Russia I.P. Lokhtin, A.M. Snigirev, L.V. Malinina: Moscow State University, Institute of Nuclear.
Statistical Mechanics and Multi-Scale Simulation Methods ChBE
ELECTROMAGNETIC PARTICLE: MASS, SPIN, CHARGE, AND MAGNETIC MOMENT Alexander A. Chernitskii.
Hua Zheng a and Aldo Bonasera a,b a)Cyclotron Institute, Texas A&M University b)LNS-INFN, Catania-Italy Density and Temperature of Fermions.
Statistical Fluctuations in Different Ensembles Begun Victor Bogolyubov Institute for Theoretical Physics Ukraine.
10/29/2007Julia VelkovskaPHY 340a Lecture 4: Last time we talked about deep- inelastic scattering and the evidence of quarks Next time we will talk about.
ICPAQGP 2010 Goa, Dec. 6-10, Percolation & Deconfinement Brijesh K Srivastava Department of Physics Purdue University USA.
Equation of State and Unruh temperature
Handout 3 : Interaction by Particle Exchange and QED
The units of g(): (energy)-1
Lecture 3 Weak Interactions (continued) muon decay Pion decay
Effects of Bulk Viscosity at Freezeout
Effects of Bulk Viscosity on pT Spectra and Elliptic Flow Coefficients
Fermi statistics and Bose Statistics
A possible approach to the CEP location
Volume effects on strangeness production
Quantum One.
Presentation transcript:

STATISTICAL MODELS in high energy collisions OUTLINE oIntroduction oFormulation for full microcanonical ensemble oDiscussion on “triviality” oNumerical methods and comparison micro-can F. Becattini, BNL, May

Hadronization : formation of extended massive regions (clusters or fireballs) emitting hadrons according to a pure statistical law

The statistical law Every multihadronic state within the cluster compatible with conservation laws is equally likely Statistical equilibrium  Set of multi-hadronic states having the energy-momentum, angular momentum, parity and charges of the cluster = the microcanonical ensemble  Hadrons and resonances treated as free states (Hagedorn, on the basis of BDM paper) – ideal hadron-resonance gas  Cluster has a spacial extension (like in the MIT bag model and unlike in HERWIG MC) Statistical model can be considered a model for the decays of MIT bags

What is the origin of equilibrium ?  Collisions among formed hadrons in a slowly expanding fireball (  scatt <<  exp ) until decoupling like in the Hot Big Bang theory (thermalization)  Quantum evolution leads to a uniform superposition over the multihadronic states within the cluster and, as a consequence, equiprobability of observation when measurement is made

A temptative reformulation (F.B., L. Ferroni, “Statistical hadronization and hadronic microcanonical ensemble I” hep-ph , to appear in Eur. Phys. J. C) | i > cluster’s initial state | h V > multihadronic state within the cluster Starting from the end:

Full microcanonical ensemble P 4-momentum J spin helicity helicity  parity  C-parity Qabelian charges I, I 3 isospin The projector can be decomposed as: The projector P P,J,  can be written as an integral over the extended Poincare’ group IO(1,3) ↑ The projector P P,J,  can be written as an integral over the extended Poincare’ group IO(1,3) ↑ Basis for microcanonical calculation

The projectors on 4-momentum, angular momentum and parity factorize if P=(M,0) Other projectors: Integral projection technique already used in the canonical ensemble. Integral projection technique already used in the canonical ensemble. A recursive method for the canonical ensemble recently used by S. Pratt et al. A recursive method for the canonical ensemble recently used by S. Pratt et al. (Phys. Rev.C68 (2003) and ref. therein) (Phys. Rev.C68 (2003) and ref. therein)

“Restricted” microcanonical ensemble Neglecting angular momentum, parity and isospin conservation: summing over all J, , I, I 3 with equal weights Usual definition of microcanonical ensemble M. Chaichian, R. Hagedorn, Nucl. Phys. B92 (1975) 445

Rate of a multi-hadronic channel {N j }=(N 1,...,N K ) It can be shown that, for non-identical particles: Usually found in literature (e.g. K. Werner, J. Aichelin Phys. Rev. C 52 (1995) 1584) In relativistic quantum field theory, confined states are NOT eigenstates of properly defined particle number operator. The above expression holds provided that V 1/3 > Compt For pions: Compt = 1.4 fm

Generalized expression: phase space volume as a cluster expansion Partitions  The leading term is the  {N j } for the classical Boltzmann statistics  Subleading terms enhance phase space volume for identical bosons and suppress it for identical fermions. They disappear in the limit V   Generalization of the expression in M. Chaichian, R. Hagedorn, Nucl. Phys. B92 (1975) 445 which holds only for large V

Phase space and Fermi golden rule  Different measures (proper phase space d 3 x d 3 p vs invariant momentum Space d 3 p/2  ) leading to different averages  Statistical phase space model predicts definite ratios between different channels  Statistical phase space model has built-in quantum statistics effects (BEC) due to the finite volume VS

They try to demonstrate that the same results of the statistical model can be obtained starting from different assumptions Is statistical population trivial?  J. Hormuzdiar et al., Int. J. Mod. Phys. E (2003) 649, nucl-th  D. Rischke, Nucl. Phys. A698 (2001) 153, talk at QM2001  V. Koch, Nucl. Phys. A715 (2003) 108, nucl-th , talk given at QM2002 Relativistic invariant: depends on as well as on Correct, but not trivial

The peculiar prediction of the statistical model which can be easily spoiled by most |M if | 2 if channel constants depend on particle content Example Quite restrictive: only a single scale  and factorization

Average multiplicities for large M: where  is such that The actual production pattern may be similar to the prediction of the statistical model, though this is not trivial (e.g. if f is a steep function of the mass)  can indeed fake a temperature

“Triviality” argument advocated in nucl-th  |M if | 2 depends on N; N is large; small fluctuations of N  |M if | 2 is unessential at high N and therefore the statistical model results are trivially recovered |M if | 2 is unessential at high N and therefore the statistical model results are trivially recovered 1.|M if | 2 may not depend just on N, also on specific particle content in the channel (through mass, isospin etc.) 2.In analyses of e.g. pp collisions overall multiplicities are not large enough to make fluctuations negligible Verify statistical model with exclusive channels BR’s! Verify statistical model with exclusive channels BR’s! (e.g.  pp annihilation at rest) ALL CONSERVATION LAWS MUST BE IMPLEMENTED (W. Blumel et al., Z. Phys. C63 (1994) 637) NEED MICROCANONICAL CALCULATIONS

Size (Mass, Volume) Microcanonical ensemble. All conservation laws including energy-momentum (angular momentum, parity), charges enforced. V > 20 fm 3, M > 10 GeV (F. Liu et al., Phys. Rev. C 68 (2003) ) F. B., L. Ferroni, talk in ISMD 2003) Canonical ensemble. Energy and momentum conserved on average, charges exactly. Temperature is introduced V > 100 fm 3, M > 50 GeV (A. Keranen, F.B., Phys. Rev. C 65 (2002) ) Grand-canonical ensemble. Also charges are conserved on average. Chemical potentials are introduced Difficulty of computing

Microcanonical ensemble calculation (angular momentum, parities, isospin neglected) (F.B., L. Ferroni, talk given in ISMD 2003 and “Statistical hadronization and hadronic microcanonical ensemble II”, in prep.) Main difficulty: size 271 light-flavoured species in the hadron-resonance gas give rise to a huge number of channels {N j }  Analytical integration impossible  Compute averages numerically via numerical integrations of  {Nj} of  {Nj} Monte-Carlo methods

 Importance sampling Monte-Carlo Random sampling of channels from a known and quick-to- sample distribution  as close as possible to the target distribution   Nj} Random sampling of channels from a known and quick-to- sample distribution  as close as possible to the target distribution   Nj} Calculate average as (for M samples):  Metropolis algorithm (suitable for event generation) Random walk in the channel space governed by gain-loss equations. At equilibrium, points of the walk are samples of the distribution (K. Werner, J. Aichelin, Phys. Rev. C 52 (1995) 1584) Random walk in the channel space governed by gain-loss equations. At equilibrium, points of the walk are samples of the distribution (K. Werner, J. Aichelin, Phys. Rev. C 52 (1995) 1584)

Speeding up the calculation to affordable computing times Use as  the grand-canonical correspondant of   Nj} Use as  the grand-canonical correspondant of   Nj} i.e. the multi-poissonian distribution This greatly enhances the performance of the This greatly enhances the performance of the computation in terms of efficiency in the importance sampling method and reducing the relaxation time in the Metropolis algorithm This method can be made even more effective for LARGE systems and opens the way to make fast event generators for the statistical model

Comparison between  C and C hadron multiplicities Q=0 cluster, M/V=0.4 GeV/fm 3 Mesons Baryons pp-like cluster, M/V=0.4 GeV/fm 3

Comparison between  C and C hadron multiplicity distributions Inequivalence between C and  C in the thermodynamic limit Q=0 cluster, M/V=0.4 GeV/fm 3 pp-like cluster, M/V=0.4 GeV/fm 3

Conclusions  A formulation of the statistical model suitable for small systems  More stringent tests: exclusive channels ? Involves full microcanonical calculations  Microcanonical ensemble calculations techniques. Fast and reliable.  Future: release of an event generator based on Metropolis algorithm