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Review of Tsallis distribution applied to RHIC data? NO! Theory about why is it applicable: yes! T.S.Bíró, G.Purcsel and K.Ürmössy MTA KFKI RMKI Budapest.

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Presentation on theme: "Review of Tsallis distribution applied to RHIC data? NO! Theory about why is it applicable: yes! T.S.Bíró, G.Purcsel and K.Ürmössy MTA KFKI RMKI Budapest."— Presentation transcript:

1 Review of Tsallis distribution applied to RHIC data? NO! Theory about why is it applicable: yes! T.S.Bíró, G.Purcsel and K.Ürmössy MTA KFKI RMKI Budapest Talk given at Zimányi Winter School, 2008. nov. 25-29. Budapest, Hungary

2 Transverse momentum spectra

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7 What all it can… dN/dy rapidity distribution: reduced phase space (q < 1) Multiplicity distribution: negative binomial Temperature – average energy fluctuation Superstatistics Coalescence scaling for (q-1) Theory: thermodynamics with power-law tailed energy distributions

8 Power-law tailed distributions and abstract composition rules Extensivity and non-extensivity Composition rules in the large-N limit Entropy formulas and distributions Relativistic kinetic energy composition T.S.Bíró, MTA KFKI RMKI Budapest Talk given at Zimanyi Winter School, 2008. nov. 25-29. Budapest, Hungary

9 Extensivity and non-extensivity T.S.Biro, arxiv:0809.4675 Europhysics Letters 2008 T.S.Biro, G.Purcsel, Phys.Lett.A 372, 1174, 2008 T.S.Biro, K.Urmossy, G.G.Barnafoldi, J.Phys.G 35:044012, 2008

10 Extensive is not always additive

11 Nonextensive is less tahn nonadditive

12 Nonextensive as composite sums Pl. x_i=i, L(x)=exp(ax)

13 What is a problem? no problem: additive hence extensive problem: non-additive  belief: it becomes extensive in the large-N limit What to do if non-additive and non-extensive?

14 Example

15 Normalizations

16 Entropy: contribution of a pair

17 Entropy: N ptl-s N (N-1) / 2 pairs

18 Energy: N ptl-s N (N-1) / 2 pairs

19 Characteristic g(r) and … g(r) - g(r) ln g(r) g(r) v(r) weakly interacting pairs: Vinfo finite confined pairs: Vinfo may diverge

20 Large distance behavior

21 Composition, large-N limit

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23 n = t N

24 Composition by formal logarithm

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26 Asymptotic rules are associative

27 Associative rules are asymptotic

28 Associative rules are attractors among more general rules

29 Entropy formulas, distributions

30 Formal logarithm

31 Deformed logarithm Deformed exponential

32 Non-extensive entropy and energy

33 Entropy maximum at fixed energy

34 Canonical distribution and detailed balance solution in generalized Boltzmann equation:

35 Example: Gibbs-Boltzmann

36 Example: Tsallis

37 Example: Kaniadakis

38 Example: Einstein

39 Example: Non associative

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41 Generalized Boltzmann equation

42 H theorem

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44 Relativistic energy composition

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46 Angle averaged Q dependent composition rule for the relativistic kinetic energies

47 Formal logarithm and asymptotic rule for the relativistic kinetic energies

48 Asymptotic rule for m=0

49 Summary Non-extensive thermodynamics requires non-additive composition rules Large N limit: rules are associative and symmetric, formal logarithm L Entropy formulas, equilibrium distributions, H-theorem based on L Relativistic kinematics  Tsallis-Pareto

50 Appendix: how to throw new momenta?

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52 Appendix: how to throw new momenta for BG?

53 Appendix: how to throw new momenta for Tsallis?


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