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STATISTICAL MODELS in high energy collisions

F. Becattini, BNL, May 10 2004. STATISTICAL MODELS in high energy collisions. OUTLINE Introduction Formulation for full microcanonical ensemble Discussion on “triviality” Numerical methods and comparison micro-can.

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STATISTICAL MODELS in high energy collisions

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  1. F. Becattini, BNL, May 10 2004 STATISTICAL MODELSin high energy collisions OUTLINE Introduction Formulation for full microcanonical ensemble Discussion on “triviality” Numerical methods and comparison micro-can

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

  3. 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

  4. What is the origin of equilibrium ? • Collisions among formed hadrons in a slowly expanding fireball(tscatt << texp)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

  5. A temptative reformulation(F.B., L. Ferroni, “Statistical hadronization and hadronic microcanonical ensemble I” hep-ph 0307061, to appear in Eur. Phys. J. C) Starting from the end: | hV >multihadronic state within the cluster | i >cluster’s initial state

  6. Full microcanonical ensemble The projector can be decomposed as: P 4-momentum J spin l helicity p parity c C-parity Q abelian charges I, I3 isospin The projectorPP,J,l,pcan be written as an integral over the extended Poincare’ groupIO(1,3)↑ Basis for microcanonical calculation

  7. The projectors on 4-momentum, angular momentum and parity factorize ifP=(M,0) Other projectors: Integral projection technique already used in the canonical ensemble. A recursive method for the canonical ensemble recently used by S. Pratt et al. (Phys. Rev.C68 (2003) 024904 and ref. therein)

  8. “Restricted” microcanonical ensemble Neglecting angular momentum, parity and isospin conservation: summing over all J, l, p, I, I3 with equal weights Usual definition of microcanonical ensemble M. Chaichian, R. Hagedorn, Nucl. Phys. B92 (1975) 445

  9. Rate of a multi-hadronic channel{Nj}=(N1,...,NK) 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 V1/3 > lCompt For pions: lCompt = 1.4 fm

  10. Generalized expression: phase space volume as acluster expansion Partitions • The leading term is theW{Nj}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

  11. Phase space and Fermi golden rule VS • Different measures (proper phase spaced3x d3pvs invariant momentum • Spaced3p/2e) leading to different averages • Statistical phase space modelpredictsdefinite ratios between • different channels • Statistical phase space model has built-in quantum statistics effects • (BEC) due to the finite volume

  12. Is statistical population trivial? • J. Hormuzdiar et al., Int. J. Mod. Phys. E (2003) 649, nucl-th 0001044 • D. Rischke, Nucl. Phys. A698 (2001) 153, talk at QM2001 • V. Koch, Nucl. Phys. A715 (2003) 108, nucl-th 0210070, talk given at QM2002 They try to demonstrate that the same results of the statistical model can be obtained starting from different assumptions Correct, but not trivial Relativistic invariant: depends on as well as on

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

  14. Average multiplicities for large M: where b 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) b can indeed fake a temperature

  15. “Triviality” argument advocated in nucl-th 0210070 • |Mif|2depends onN; Nis large; small fluctuations ofN |Mif|2 is unessential at high Nand therefore the statistical model results are trivially recovered |Mif|2may not depend just on N, also on specific particle content in the channel (through mass, isospin etc.) 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! (e.g. ppannihilation at rest) ALL CONSERVATION LAWS MUST BEIMPLEMENTED (W. Blumel et al., Z. Phys. C63 (1994) 637) NEED MICROCANONICAL CALCULATIONS

  16. Size (Mass, Volume) Microcanonical ensemble. All conservation laws including energy-momentum (angular momentum, parity), charges enforced. V > 20 fm3, M > 10 GeV(F. Liu et al., Phys. Rev. C 68 (2003) 024905) F. B., L. Ferroni, talk in ISMD 2003) Canonical ensemble. Energy and momentum conserved on average, charges exactly. Temperature is introduced V > 100 fm3, M > 50 GeV(A. Keranen, F.B., Phys. Rev. C 65 (2002) 044901) Grand-canonical ensemble. Also charges are conserved on average. Chemical potentials are introduced Difficulty of computing

  17. 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.) • Analytical integration impossible • Compute averages numerically via numerical integrations • ofW{Nj} Main difficulty: size 271 light-flavoured species in the hadron-resonance gas give rise to a huge number of channels {Nj} Monte-Carlo methods

  18. Importance sampling Monte-Carlo Random sampling of channels from a known and quick-to-sample distribution P as close as possible to the target distributionW{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)

  19. Speeding up the calculation to affordable computing times Use as P the grand-canonical correspondant of W{Nj} i.e. the multi-poissonian distribution 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

  20. Comparison between mC and C hadron multiplicities Q=0 cluster, M/V=0.4 GeV/fm3 pp-like cluster, M/V=0.4 GeV/fm3 Baryons Mesons

  21. Comparison between mC and C hadron multiplicity distributionsInequivalence between C and mC in the thermodynamic limit Q=0 cluster, M/V=0.4 GeV/fm3 pp-like cluster, M/V=0.4 GeV/fm3

  22. 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

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