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Diffusion of Non- Gaussianity in Heavy Ion Collisions

Diffusion of Non- Gaussianity in Heavy Ion Collisions. Masakiyo Kitazawa （ Osaka U. ）. MK, Asakawa , Ono, arXiv:1307.2978. SQM , Birmingham, 2 3, July 2013. Beam-Energy Scan. STAR 2012. high. beam energy. T. low. Hadrons. Color SC. m. 0. Fluctuations .

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Diffusion of Non- Gaussianity in Heavy Ion Collisions

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  1. Diffusion of Non-Gaussianityin Heavy Ion Collisions Masakiyo Kitazawa （Osaka U.） MK, Asakawa, Ono, arXiv:1307.2978 SQM, Birmingham, 23, July 2013

  2. Beam-Energy Scan STAR 2012 high beam energy T low Hadrons Color SC m 0

  3. Fluctuations • Fluctuations reflect properties of matter. • Enhancement near the critical point • Stephanov,Rajagopal,Shuryak(’98); Hatta,Stephanov(’02); Stephanov(’09);… • Ratios between cumulants of conserved charges • Asakawa,Heintz,Muller(’00); Jeon, Koch(’00); Ejiri,Karsch,Redlich(’06) • Signs of higher order cumulants • Asakawa,Ejiri,MK(’09); Friman,et al.(’11); Stephanov(’11)

  4. Conserved Charges : Theoretical Advantage • Definite definition for operators • as a Noether current • calculable on any theory ex: on the lattice

  5. Conserved Charges : Theoretical Advantage • Definite definition for operators • as a Noether current • calculable on any theory ex: on the lattice • Simple thermodynamic relations • Intuitive interpretation for the behaviors of cumulants ex: Asakawa, Ejiri, MK, 2009

  6. Conserved Charge Fluctuations RBC-Bielefeld ’09 Cumulants of NB and NQ are suppressedat high T. Asakawa, Heintz, Muller, 2000; Jeon, Koch, 2000; Ejiri, Karsch, Redlich, 2006; Asakawa, Ejiri, MK, 2009; Friman, et al., 2011; Stephanov, 2011

  7. Proton # Cumulants @ STAR-BES STAR,QM2012 CAUTION! Something interesting?? proton number baryon number MK, Asakawa, 2011;2012

  8. Charge Fluctuation @ LHC ALICE, PRL110,152301(2013) D-measure • D ~ 3-4 Hadronic • D ~ 1 Quark significant suppression from hadronic value at LHC energy! is not equilibrated at freeze-out at LHC energy!

  9. Dh Dependence @ ALICE ALICE PRL 2013 t Dh z rapidity window

  10. Time Evolution of CC t Dy NQ z Dy • Variation of a conserved charge in Dy is achieved only through diffusion. • The larger Dy, the slower diffusion

  11. Dh Dependence @ ALICE ALICE PRL 2013 t Dh z Dh dependences of fluctuation observables encode history of the hot medium! Higher-order cumulants as thermometer?

  12. <dNB2> and <dNp2 > @ LHC ? should have different Dh dependence. Baryon # cumulants are experimentally observable! MK, Asakawa, 2011;2012

  13. <dNB2> and <dNp2 > @ LHC ? should have different Dh dependence. Baryon # cumulants are experimentally observable! MK, Asakawa, 2011;2012

  14. <dNB2> and <dNp2 > @ LHC ? should have different Dh dependence. Baryon # cumulants are experimentally observable! MK, Asakawa, 2011;2012

  15. <dNQ4> @ LHC ? How does behave as a function of Dh? enhancement suppression or

  16. Three “NON”s Physics of non-Gaussianity in heavy-ion is a particularproblem! Non-Gaussianitiy is irrelevant in large systems • Non-Gaussian • Non-critical • Non-equilibrium critical enhancement is not observed in HIC so far Fluctuations are not equilibrated in HIC

  17. Three “NON”s Physics of non-Gaussianity in heavy-ion is a particularproblem! Non-Gaussianitiy is irrelevant in large systems • Non-Gaussian • Non-critical • Non-equilibrium critical enhancement is not observed in HIC so far Fluctuations are not equilibrated in HIC It is impossible to directly extend the theory ofhydro fluctuationsto treat higher orders.

  18. Diffusion Master Equation Divide spatial coordinate into discrete cells probability

  19. Diffusion Master Equation Divide spatial coordinate into discrete cells probability Master Equation for P(n) x-hat: lattice-QCD notation Solve the DME exactly, and take a0 limit No approx., ex. van Kampen’s system size expansion

  20. Solution of DME 1st initial Deterministic part  diffusion equation at long wave length (1/a<<k) Appropriate continuum limit with ga2=D

  21. Solution of DME 1st initial Deterministic part  diffusion equation at long wave length (1/a<<k) Appropriate continuum limit with ga2=D 2nd Consistent with stochastic diffusion eq. (for smooth initial condition) Shuryak, Stephanov, 2001

  22. Net Charge Number Prepare 2 species of (non-interacting) particles Let us investigate at freezeout time t

  23. Time Evolution in Hadronic Phase Hadronization(initial condition) • Boost invariance / infinitely long system • Local equilibration / local correlation suppression owing to local charge conservation strongly dependent on hadronization mechanism

  24. Time Evolution in Hadronic Phase Hadronization(initial condition) • Boost invariance / infinitely long system • Local equilibration / local correlation Time evolution via DME suppression owing to local charge conservation strongly dependent on hadronization mechanism Freezeout

  25. Dh Dependence at Freezeout Initial fluctuations: 2nd 4th parameter sensitive to hadronization

  26. Dh Dependence at Freezeout Initial fluctuations: 2nd 4th parameter sensitive to hadronization

  27. <dNQ4> @ LHC • boost invariant system • small fluctuations of CC at hadronization • short correlation in hadronic stage Assumptions 1 4th-order cumulant will besuppressed at LHC energy! Dh dependences encode various information on the dynamics of HIC! 0.5

  28. Summary Plenty of physics in Dhdependences of various cumulants • Diagnosing dynamics of HIC • history of hot medium • mechanism of hadronization • diffusion constant Physical meanings of fluctuation obs. in experiments.

  29. Summary Plenty of physics in Dhdependences of various cumulants • Diagnosing dynamics of HIC • history of hot medium • mechanism of hadronization • diffusion constant Physical meanings of fluctuation obs. in experiments. Search of QCD Phase Structure

  30. Open Questions & Future Work • Why the primordial fluctuations are observed only at LHC, and not RHIC ? • Extract more information on each stage of fireballs using fluctuations • Model refinement • Including the effects of • nonzero correlation length / relaxation time • global charge conservation • Non Poissonian system  interaction of particles

  31. Dh Dependence at STAR STAR, QM2012 decreases as Dh becomes larger at RHIC energy.

  32. Chemical Reaction 1 x: # of X a: # of A (fixed) Master eq.: Cumulants with fixed initial condition equilibrium initial

  33. Chemical Reaction 2 2nd 3rd 4th Higher-order cumulants grow slower.

  34. Time Evolution in HIC Quark-Gluon Plasma Hadronization Freezeout

  35. Hydrodynamic Fluctuations Landau, Lifshitz, Statistical Mechaniqs II Kapusta, Muller, Stephanov, 2012 Diffusion equation Stochastic diffusion equation Stochastic Force determined by fluctuation-dissipation relation

  36. Dh Dependence Shuryak, Stephanov, 2001 • Initial condition: • Translational invariance equilibrium initial equilibrium initial

  37. Non-Gaussianity in Fluctuating Hydro? It is impossible to directly extend the theory ofhydro fluctuations to treat higher orders. • No a priori extension of FD relations to higher orders Markov process＋continuous variable • Theorem Gaussian random force cf) Gardiner, “Stochastic Methods”

  38. Event-by-Event Analysis @ HIC Fluctuationscan be measured by e-by-e analysis in HIC. STAR, PRL105(2010) Detector

  39. Non-Gaussianity fluctuations (correlations) Non-Gaussianity PLANCK : statistics insufficient to see non-Gaussianity…(2013)

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