Transport of Fluctuations Masakiyo Kitazawa Osaka U INT

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Transport of Fluctuations Masakiyo Kitazawa (Osaka U. ) INT Workshop 16 -3 Exploring the

Transport of Fluctuations Masakiyo Kitazawa (Osaka U. ) INT Workshop 16 -3 Exploring the QCD Phase Diagram through Energy Scan INT, Seattle, 6/Oct. /2016

J-PARC Heavy-Ion Program (J-PARC-HI)

J-PARC Heavy-Ion Program (J-PARC-HI)

J-PARC-HI Program New HI Injector J-PARC Heavy Ion Toroidal Spectrometer high intensity RCS &

J-PARC-HI Program New HI Injector J-PARC Heavy Ion Toroidal Spectrometer high intensity RCS & Main Ring J-PARC-HI stable well established p fixed target HI experiment p Elab<20 Ge. V/A (√s. NN<6. 2 Ge. V) p High luminosity beam

J-PARC-HI Program White Paper Recent Activities June 2016 July 2016 Aug. 2016 Sep. 2016

J-PARC-HI Program White Paper Recent Activities June 2016 July 2016 Aug. 2016 Sep. 2016 White Paper uploaded Submission of LOI International Workshop Symposium @ JPS meeting Future Plan 2020 2021 -2022 2021 -2023 -2024 2025 Visit J-PARC-HI Web Page Funding request to MEXT http: //asrc. jaea. go. jp/soshiki/gr/hadron/jparc-h Earliest approval of funding Construction of HI Injector Construction of HI injection system in RCS Construction of HI spectrometer First collision

Fluctuations

Fluctuations

Contents 1. Transport of fluctuations MK, Asakawa, Ono, PLB (2014); MK, NPA (2015) 2.

Contents 1. Transport of fluctuations MK, Asakawa, Ono, PLB (2014); MK, NPA (2015) 2. Thermal blurring by rapidity conversion Ohnishi, MK, Asakawa, PRC (2016) 3. Transport near QCD critical point Sakaida, Asakawa, Fujii, MK, in prep. Review: Asakawa, MK, PPNP (2016)

Before Main Topics… Fluctuations = Regular + Singular

Before Main Topics… Fluctuations = Regular + Singular

Before Main Topics… Fluctuations = Regular Poisson Noise + Singular NON-Poisson Signal

Before Main Topics… Fluctuations = Regular Poisson Noise + Singular NON-Poisson Signal

Before Main Topics… Fluctuations = Regular Poisson Noise + Singular NON-Poisson Signal

Before Main Topics… Fluctuations = Regular Poisson Noise + Singular NON-Poisson Signal

Before Main Topics… Fluctuations = Regular Poisson Noise + Singular NON-Poisson Signal

Before Main Topics… Fluctuations = Regular Poisson Noise + Singular NON-Poisson Signal

Before Main Topics… Fluctuations = Regular Poisson Noise + Singular NON-Poisson Signal

Before Main Topics… Fluctuations = Regular Poisson Noise + Singular NON-Poisson Signal

Before Main Topics… Fluctuations = Regular Poisson Noise + Off-equilibrium effects make the separation

Before Main Topics… Fluctuations = Regular Poisson Noise + Off-equilibrium effects make the separation of two contributions impossible. (diffusion, experimental cuts, efficiency, … )

Fragile Higher Orders

Fragile Higher Orders

Fragile Higher Orders Ex. : Relation b/w baryon & proton # cumulants (with an

Fragile Higher Orders Ex. : Relation b/w baryon & proton # cumulants (with an approximation) MK, Asakawa, 2012 genuine info. Poisson noise Higher orders are more seriously affected by efficiency loss.

Transport of Fluctuations

Transport of Fluctuations

Diffusion After Chemical F. O. Asakawa, Heinz, Muller (2000) Jeon, Koch (2000) Shuryak, Stephanov

Diffusion After Chemical F. O. Asakawa, Heinz, Muller (2000) Jeon, Koch (2000) Shuryak, Stephanov (2001) Detector Distributions in DY and Dy are different due to “thermal blurring”. Fluctuations in DY continue to change until kinetic f. o.

How to Describe Transport of Fluctuations? A candidate Stochastic diffusion equation Fluctuation in equil.

How to Describe Transport of Fluctuations? A candidate Stochastic diffusion equation Fluctuation in equil. is Gaussian. Noise: Gaussian Undesirable to describe relaxation of cumulants toward Poisson value.

Non-Interacting Brownian Particle System Initial condition (uniform) cumulants: random walk diffusion master equation: MK+,

Non-Interacting Brownian Particle System Initial condition (uniform) cumulants: random walk diffusion master equation: MK+, PLB(2014) probabilistic argument: Ohnishi+, PRC(2016)

Non-Interacting Brownian Particle System Initial condition (uniform) cumulants: diffusion distance random walk Study DY

Non-Interacting Brownian Particle System Initial condition (uniform) cumulants: diffusion distance random walk Study DY dependence Poisson distribution diffusion master equation: MK+, PLB(2014) probabilistic argument: Ohnishi+, PRC(2016)

Rapidity Window Dependence ALICE, PRL (2013) X. Luo, CPOD 2014 Cumulants are dependent on

Rapidity Window Dependence ALICE, PRL (2013) X. Luo, CPOD 2014 Cumulants are dependent on rapidity window.

10~20 fm mesons baryons time kinetic f. o. chem. f. o. hadronize Baryons in

10~20 fm mesons baryons time kinetic f. o. chem. f. o. hadronize Baryons in Hadronic Phase e k i l e v a h e b s n Baryo r e t a w n i s n e l l o p n a i n w o r B

Rapidity Window Dependence No initial net fluctuation: 2 nd 4 th parameter sensitive to

Rapidity Window Dependence No initial net fluctuation: 2 nd 4 th parameter sensitive to hadronization

Rapidity Window Dependence MK+, PLB(2014) p Cumulants at finite Dy is different from initial

Rapidity Window Dependence MK+, PLB(2014) p Cumulants at finite Dy is different from initial value. p 4 th cumulant can have a sign change. p 4 th cumulant can have non-monotonic behavior. p Poisson / non-Poisson : Not separable!

Dh Dependence: 4 th order MK, NPA(2015) Initial Condition Characteristic Dh dependences!

Dh Dependence: 4 th order MK, NPA(2015) Initial Condition Characteristic Dh dependences!

Dh Dependence: 4 th order MK, NPA(2015) Initial Condition at ALICE baryon #

Dh Dependence: 4 th order MK, NPA(2015) Initial Condition at ALICE baryon #

4 th order : w/ Critical Fluctuation Initial Condition at ALICE baryon #

4 th order : w/ Critical Fluctuation Initial Condition at ALICE baryon #

Dh Dependence @ STAR MK+ (2014) MK (2015) X. Luo, CPOD 2014 p Approach

Dh Dependence @ STAR MK+ (2014) MK (2015) X. Luo, CPOD 2014 p Approach initial value as Dy large Ling, Stephanov (2016) p No power law ~(Dy)4 behavior at small Dy finite volume effect: Sakaida+, PRC 064911(2014)

Non-Interacting Brownian Particle System Initial condition (uniform) cumulants: trace back time evolution Compare with

Non-Interacting Brownian Particle System Initial condition (uniform) cumulants: trace back time evolution Compare with lattice diffusion distance diffusion coefficient

Dh Dependence: 3 rd order Initial Condition at ALICE baryon #

Dh Dependence: 3 rd order Initial Condition at ALICE baryon #

Themal Blurring Ohnishi, MK, Asakawa, PRC, in press

Themal Blurring Ohnishi, MK, Asakawa, PRC, in press

Fluctuations: Theory vs Experiment Theoretical analyses Experiments based on statistical mechanics lattice, critical point,

Fluctuations: Theory vs Experiment Theoretical analyses Experiments based on statistical mechanics lattice, critical point, effective models, … Fluctuation in a spatial volume Fluctuations in a momentum space discrepancy in phase spaces Asakawa, Heinz, Muller, 2000; Jeon, Koch, 2000; Shuryak, Stephanov, 2001

Connecting Phase Spaces Asakawa, Heinz, Muller, 2000 Jeon, Koch, 2000 Under Bjorken picture, coordinate-space

Connecting Phase Spaces Asakawa, Heinz, Muller, 2000 Jeon, Koch, 2000 Under Bjorken picture, coordinate-space rapidity Y momentum-space rapidity y of medium momentum-space rapidity y of individual particles

Thermal distribution in y space nucleon pion Blast wave squeezes the distribution in rapidity

Thermal distribution in y space nucleon pion Blast wave squeezes the distribution in rapidity space • pions • nucleons • blast wave • flat freezeout surface

 • pions • nucleons kurtosis half-width (Dy) Thermal distribution in y space Rapidity

• pions • nucleons kurtosis half-width (Dy) Thermal distribution in y space Rapidity distribution can be well approximated by Gaussian. • blast wave • flat freezeout surface

Dh Dependence Initial condition (before blurring) Cumulants after blurring no e-v-e fluctuations Cumulants after

Dh Dependence Initial condition (before blurring) Cumulants after blurring no e-v-e fluctuations Cumulants after blurring can take nonzero values With Dy=1, the effect is not well suppressed • pions • nucleons

Diffusion + Thermal Blurring Thermal blurring can be regarded as a part of diffusion

Diffusion + Thermal Blurring Thermal blurring can be regarded as a part of diffusion Chemical f. o. (coordinate space) diffusion Kinetic f. o. (coordinate space) blurring Kinetic f. o. (momentum space) Total diffusion:

Centrality Dependence ALICE, 2013 More central lower T larger b Weaker blurring Is the

Centrality Dependence ALICE, 2013 More central lower T larger b Weaker blurring Is the centrality dependence understood solely by thermal blurring at kinetic f. o. ?

Centrality Dependence @ ALICE Assumptions: • Centrality independent cumulant at kinetic f. o. •

Centrality Dependence @ ALICE Assumptions: • Centrality independent cumulant at kinetic f. o. • Thermal blurring at kinetic f. o. p Centrality dep. of fluctuation can be described by a simple thermal blurring picture.

Time Evolution of Fluctuation near QCD Critical Point Sakaida, Asakawa, Fujii, MK, in preparation

Time Evolution of Fluctuation near QCD Critical Point Sakaida, Asakawa, Fujii, MK, in preparation

Dynamical Evolution of Critical Fluctuations p Evolution of correlation length Berdnikov, Rajagopal (2000) Asakawa,

Dynamical Evolution of Critical Fluctuations p Evolution of correlation length Berdnikov, Rajagopal (2000) Asakawa, Nonaka (2002) p Higher orders (spatially uniform “s” mode) Mukherjee, Venugopalan, Yin (2015) p Correlation functions Kapusta, Torres-Rincon (2012)

Critical Mode = Diffusive Mode m t f So e d o Fujii (2004)

Critical Mode = Diffusive Mode m t f So e d o Fujii (2004) Fujii, Ohtani (2005) Son, Stephanov (2005) Soft mode of QCD CP s: fast damping Evolution of baryon number density : parameters characterizing criticality

Parametrization of D & c 2 p model-H (3 d-Ising) p p mapping to

Parametrization of D & c 2 p model-H (3 d-Ising) p p mapping to (T, m) / time evolution 1 D Bjorken expansion p p QCD CP at T=160 Me. V p kinetic f. o. at T=100 Me. V Berdnikov, Rajagopal (2000) Stephanov (2011) Mukherjee, Venugopalan, Yin (2015)

Time Evolution 1: No CP

Time Evolution 1: No CP

2: Critical Point p Non-monotonic Dy dependence manifests itself. Robust experimental evidence of the

2: Critical Point p Non-monotonic Dy dependence manifests itself. Robust experimental evidence of the existence of a peak in c(T)

3: Critical Point (Narrower Critical Region) non-monotonic behavior Peak in

3: Critical Point (Narrower Critical Region) non-monotonic behavior Peak in

Net-Electric Charge From N. Sahoo, Ph. D thesis p No non-monotonic dependence in net-electric

Net-Electric Charge From N. Sahoo, Ph. D thesis p No non-monotonic dependence in net-electric charge fluc. p How about net-proton number fluctuation? ?

Summary Fragile Higher Orders • Interpret experimental results carefully. Plenty of information in Dh

Summary Fragile Higher Orders • Interpret experimental results carefully. Plenty of information in Dh dependences • Cumulants at chemical freezeout • Diffusion coefficients / thermal blurring • Signal of QCD-CP as a non-monotonic behavior in 2 nd order Future • Dy dependence of • Evolution of higher orders near CP with diffusive nature

Higher Order Cumulants? ? p Relaxation of cumulants is slower for higher order. •

Higher Order Cumulants? ? p Relaxation of cumulants is slower for higher order. • Longer survival? • Slower enhancement? p Non-monotonic Dy dependence can appear only by diffusion It’s not the experimental evidence of peak in (higher order) susceptibility. p Non-linear equation has to be solved.