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Jeffery T. Mitchell (BNL) – Jeffery T. Mitchell (BNL) – QM2004 QM2004 1 Outline: - Charge Fluctuations - Balance Functions - Event-by-event <p T > Fluctuations - Looking Ahead - Conclusions, Credits, Apologies Fluctuations and Fluctuations and Correlations in Correlations in Relativistic Heavy Ion Relativistic Heavy Ion Collisions Collisions Jeffery T. Mitchell Jeffery T. Mitchell (Brookhaven National Laboratory) (Brookhaven National Laboratory)

Fluctuations and Correlations in Relativistic Heavy Ion Collisions

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Jeffery T. Mitchell (Brookhaven National Laboratory). Fluctuations and Correlations in Relativistic Heavy Ion Collisions. Outline: Charge Fluctuations Balance Functions Event-by-event Fluctuations Looking Ahead Conclusions, Credits, Apologies. Charge Fluctuations. - PowerPoint PPT Presentation

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Page 1: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 11

Outline:

- Charge Fluctuations

- Balance Functions

- Event-by-event <pT> Fluctuations

- Looking Ahead

- Conclusions, Credits, Apologies

Fluctuations and Correlations Fluctuations and Correlations in Relativistic Heavy Ion in Relativistic Heavy Ion

Collisions Collisions Jeffery T. MitchellJeffery T. Mitchell

(Brookhaven National Laboratory)(Brookhaven National Laboratory)

Page 2: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 22

Charge FluctuationsCharge Fluctuations

Hadron Gas Scenario Quark-Gluon Plasma Scenario

Fractional electric charges of the quarks ==> Charges more evenly spread in a plasma ==> Reduced net charge

fluctuations in a small region of phase-space

Hypothesis: Fluctuations in net charge and net baryon number may be significantly reduced if a QGP is formed in the collisionsAsakawa, Heinz, Müller PRL 85(2000)2072; Jeon & Koch PRL 85(2000)2076

Page 3: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 33

Summary of Charge Fluctuation Summary of Charge Fluctuation MeasuresMeasures

CHNQQv 2)(

N

NR

CHch N

QRND

2

2 4

2

2

zN

Z

CHq

2

N

N

N

N

NNstat11

,

dyn

NNQv ,4

1)(

dynNND ,4

222: XXXVariance NNNCH

NNQ

dyn

CH

qN

NN,2

2/32/3

2

2 4CHN

NNz

CHCH

NN

QQZ

2

1

CH

CHCH

NN

QQ

N

)(4 QD

)(Qv

Quoted in this presentation

Page 4: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 44

Charge Fluctuation Magnitude Charge Fluctuation Magnitude ExpectationsExpectations

v(Q)v(Q) DD+-,dyn+-,dyn

(STAR)(STAR)

+-,dyn+-,dyn

(PHENIX)(PHENIX)

qq

(NA49)(NA49)

Independent Independent Particle Particle EmissionEmission

1.01.0 4.04.0 0.00.0 0.00.0 0.00.0

Resonance Resonance GasGas 0.750.75 3.03.0 -0.0013-0.0013 -0.006-0.006 -0.125-0.125

Quark-Gluon Quark-Gluon PlasmaPlasma 0.250.25 1.01.0 -0.0038-0.0038 -0.019-0.019 -0.375-0.375

Quark Quark CoalescenceCoalescence 0.830.83 3.333.33 -0.0008-0.0008 -0.004-0.004 -0.084-0.084

Page 5: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 55

Charge Fluctuations vs. Rapidity Charge Fluctuations vs. Rapidity Acceptance (Excitation Function): Acceptance (Excitation Function):

NA49NA49

11

totCH

CHccq N

yN

Correction for fluctuations due to

charge conservation.

Quark Coalescence

Resonance GasQuark-Gluon Plasma

Charge Conservation

See poster by P. Chrisakogiou

Also see talk by H. Sako for new CERES results.

Page 6: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 66

= /2,0.3 pT 2.0 GeV/c

Charge Fluctuations vs. Rapidity AcceptanceCharge Fluctuations vs. Rapidity Acceptance

Charge ConservationQuark Coalescence

Resonance Gas

Quark-Gluon Plasma

Phys. Rev. Lett. 89 (2002) 082301, 130 GeV.

Page 7: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 77

Charge Fluctuations vs. Rapidity AcceptanceCharge Fluctuations vs. Rapidity Acceptance

Charge ConservationQuark Coalescence

Resonance Gas

Quark-Gluon Plasma

Phys. Rev. C68 (2003) 044905, 130 GeV.

Page 8: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 88

Balance FunctionsBalance Functions

222thermaly

Bass, Danielewicz, & Pratt, Phys. Rev. Lett. 85, 2689 (2000)

+ - (y) = Histogram of | y(+) - y(--) |, for all possible pairs within an event. This histogram is summed over all events.

B(y) 12

N (y) N (y)

N

N (y) N (y)

N

• Designed to determine whether hadronization from a QGP occurs early (<1 fm/c) or late.

• Based upon the fact that charge is conserved locally, and produced pairs are initially correlated in coordinate space.

• Bottom line: The balance function is narrower in the delayed hadronization scenario.

Early hadronization scenario: Pairs separate in rapidity due to expansion and

rescattering.

Delayed hadronization scenario: Pairs are more strongly correlated in rapidity.

Page 9: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 99

STAR 130 GeV Balance Function STAR 130 GeV Balance Function ResultsResultsPhys. Rev. Lett. 90 (2003) 172301.

All Charged Hadron Pairs

All Charged Hadron Pairs

Identified Pion Pairs

Identified Pion Pairs

Page 10: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1010

STAR 200 GeV Balance Function STAR 200 GeV Balance Function WidthsWidths

The balance function gets narrower in central collisions Delayed

hadronization scenario?

Increasing Centrality

See talk tomorrow by G. Westfall

Page 11: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1111

NA49 17 GeV Balance Function NA49 17 GeV Balance Function WidthsWidths

A similar behavior AND

narrowing magnitude is

observed compared to

the STAR data!The balance function gets

narrower in central collisions.

See talk by M. GazdzickiPreliminary

Increasing Centrality

Page 12: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1212

Other explanations for the broadening of Other explanations for the broadening of the balance functionthe balance function

Resonance contributions

P. Bozek, W. Broniowski, and W. Florkowski, nucl-th/0310062

Computing balance functions in a thermal model with neutral resonance decay.

The calculations including resonances are consistent with the STAR results.

0-10% centralit

y

10-40% centralit

y

40-70% centralit

y

70-96% centralit

y

Quark Coalescence Model Predictions

A. Bialas, hep-ph/0308245.

Predicts a width consistent with the STAR result for central collisions with a transverse flow velocity

below 0.5c.

Page 13: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1313

<p<pTT> Fluctuations: Probing for > Fluctuations: Probing for Signs of a Phase TransitionSigns of a Phase Transition

Analogy: Critical Opalescence

Movie by the University of Minnesota Physics Department

Movie of a sealed container containing freon on a hot plate at

the critical point.The image is projected onto a wall.

M. Stephanov et al., Phys. Rev. Lett. 81

(1998) 4816: Suggest that near a tri-critical end-point in the QCD

phase diagram, event-by-event fluctuations in

average pT could increase significantly.

B. Berdnikov and K. Rajagopal, Phys. Rev. D61 (2000) 105017:

Estimate that the effect could be a 10-20%

increase in average pT

fluctuations.

Page 14: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1414

Behold The Signal!Behold The Signal!

Page 15: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1515

Summary of Event-by-event <pSummary of Event-by-event <pTT> > Fluctuation MeasuresFluctuation Measures

2.,

2.,, inclpinclppnp TTTT

.,inclp

pp

T

T

TF

22., TTinclp pp

T

pTpT

pT,n

FpT

T

dynp

dynpp pT

TT

||sgn

2,2

,

pT,dyn

N

pTpdynp

T

T

22

,

2

222TTT ppp

Goal of the observables:

State a comparison to the expectation of statistically

independent particle emission.

N

F

pTT

T

p

T

pp

2Quoted in this presentation

Page 16: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1616

How To Measure A FluctuationHow To Measure A Fluctuation

Red: Random Expectation

( distribution)

Blue: STAR acceptance

fluctuation of:

pT=52.6 MeV,

FpT=14%,

2pT,dyn=52.3 (MeV/c2),

pT=9.8%

MpT = Event-by-Event Average pT

Gamma distribution calculation for statistically independent particle emission with input parameters taken from the inclusive spectra. See M. Tannenbaum, Phys. Lett.

B498 (2001) 29.

Page 17: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1717

A Positive Signal is Observed!A Positive Signal is Observed!Known contributions to the <pKnown contributions to the <pTT> >

fluctuation signal should be fluctuation signal should be subtracted.subtracted.

Contributions from Known ProcessesContributions from Known Processes HBT – too small (NA49, STAR, CERES)HBT – too small (NA49, STAR, CERES) Resonances – too small (NA49, STAR)Resonances – too small (NA49, STAR) Elliptic Flow – too small/negligible (PHENIX, Elliptic Flow – too small/negligible (PHENIX,

CERES, NA49)CERES, NA49) Hard Processes…Hard Processes… Or onset of thermalization…Or onset of thermalization…

A Schematic Illustration of Elliptic Flow

Page 18: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1818

A Possible Explanation of the Signal: A A Possible Explanation of the Signal: A System in Near-local Thermal System in Near-local Thermal

EquilibriumEquilibriumSean Gavin, nucl-th/0308067, see his talk tomorrow for more details.

Page 19: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 1919

The onset of thermalization?The onset of thermalization?

tptt ppd

dN21

See talks tomorrow by S. Gavin (model)

and G. Westfall (data)

Page 20: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2020

A Large Fluctuation Contribution at A Large Fluctuation Contribution at high phigh pTT

An increase in observed fluctuations grows primarily in a

pT region where number fluctuations vary little.

0.2 < pT < pTmax

Preliminary

Increases from pTmax=1.0 to 2.0

GeV/c

PHENIX Fluctuations: 243%

CERES Fluctuations: 34%

<N>: < 15%

20-25% centrality

20-30% centrality

This trend is

observed at all

centralities.

See talk by H. Sako

0.1 < pT < pTmax

See talk by M. Tannenbaum

Page 21: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2121

Fluctuations: A Jet Fluctuations: A Jet Contribution?Contribution?

Jets inherently add particles that are correlated in pT to the event, so

a contribution due to hard processes is expected, but how

much? What about jet suppression?

A Schematic Illustration of Jet

Suppression

Page 22: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2222

Jet Simulation Results: PHENIX at 200 GeVJet Simulation Results: PHENIX at 200 GeV

20-25% centrality

PHENIX Data: nucl-ex/0310005

Results from a 2-component hybrid simulation.

Component 1: Reproduce soft processes by sampling the inclusive pT and N data distributions.

Component 2: Embed PYTHIA hard scattering events at a given rate per particle produced in Part 1. Keep

the rate fixed, or scale it by RAA.

This decrease is due to the

signal competing with the MpT width increase for

low N.

This decrease is due to jet suppression?

See poster by J. T. Mitchell

Page 23: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2323

Jet Simulation Results: STAR at 130 Jet Simulation Results: STAR at 130 GeVGeV

STAR data: nucl-ex/0308033

Error bars are the quoted total systematic error.

The simulation predicts ~15-20% increase when going

from 130 to 200 GeV

Page 24: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2424

Jet Simulation Results: NA49 at 17 GeVJet Simulation Results: NA49 at 17 GeVNA49 Preliminary Data: See poster by

K. Grebieszkow & M. Rybczynski

Page 25: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2525

Estimate of the Magnitude of Residual Estimate of the Magnitude of Residual Event-by-Event Temperature Event-by-Event Temperature

FluctuationsFluctuations

MeasuremenMeasurementt

sqrt(ssqrt(sNNNN)) TT/<T>,/<T>,

Most Most centralcentral

TT/<T>,/<T>,

At the At the peakpeak

PHENIXPHENIX 200200 1.8%1.8% 3.7%3.7%

STARSTAR 130130 1.7%1.7% 3.8%3.8%

CERESCERES 1717 1.3%1.3% 2.2%2.2%

NA49NA49 1717 0.6%0.6% 1.7%1.7%

)Np(

F

T

σTpT

1

2

R. Korus and S. Mrowczynski,

Phys. Rev. C64 (2001) 054908.

p inclusive pT, (p,b), p~1

Page 26: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2626

Add a dimension: 2-point transverse Add a dimension: 2-point transverse momentum correlationsmomentum correlations

STAR

Preliminary

HBT and Coulomb interaction

Higher pt pairs fromhard scattering ?

Like sign

In PHENIX, x(1.5 GeV/c) ~ 0.93

0

0

)(

TT

p

TT

T

dpdpdN

dpdpdN

px

T

NA49 17 GeV Pb+Pb

Thermal Fluctuation Model Simulations

STAR Preliminary 130

GeV Au+AuData (T) = 5 MeV

(T) = 10 MeV (T) = 20 MeV

L. Ray, DNP 2003, see his poster

hep-ex/0311009

Page 27: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2727

Coming Soon: A Multi-dimensional Coming Soon: A Multi-dimensional AnalysisAnalysis

STAR Preliminary

(centrality, pT,1, pT,2, pseudorapidity, azimuth)

Same side

Opposite side

See poster by D. Prindle

Elliptic flow has been removed.

T. Trainor, DNP 2003

Page 28: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2828

SynopsisSynopsis Charge fluctuations:Charge fluctuations:

SPS results and RHIC-PHENIX results are close to the random SPS results and RHIC-PHENIX results are close to the random expectation after correcting for charge conservation.expectation after correcting for charge conservation.

RHIC-STAR results are consistent with a quark coalescence model RHIC-STAR results are consistent with a quark coalescence model prediction in central collisions.prediction in central collisions.

Balance Functions:Balance Functions: Both SPS (NA49) and RHIC (STAR) results show a narrowing of the Both SPS (NA49) and RHIC (STAR) results show a narrowing of the

balance function in central collisions.balance function in central collisions. The narrowing is indicative of delayed hadronization.The narrowing is indicative of delayed hadronization. The narrowing may also be explained within the quark The narrowing may also be explained within the quark

coalescence picture, or by resonance decay contributions.coalescence picture, or by resonance decay contributions. <p<pTT> Fluctuations:> Fluctuations:

A positive fluctuation signal that decreases for more central A positive fluctuation signal that decreases for more central collisions is seen at the SPS and at RHIC.collisions is seen at the SPS and at RHIC.

The signal can be explained within a model that simulates jet The signal can be explained within a model that simulates jet production, however, a jet suppression scenario must be production, however, a jet suppression scenario must be introduced to describe the most central collisions at RHIC.introduced to describe the most central collisions at RHIC.

The signal can also be explained within a thermalization onset The signal can also be explained within a thermalization onset scenario.scenario.

Stay tuned for more exciting results soon!Stay tuned for more exciting results soon!

Page 29: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 2929

AcknowledgementsAcknowledgementsMany thanks to H. Appelshauser (CERES), M. Gazdzicki (NA49), Many thanks to H. Appelshauser (CERES), M. Gazdzicki (NA49),

S. Gavin, D. Prindle (STAR), L. Ray (STAR), C. Roland S. Gavin, D. Prindle (STAR), L. Ray (STAR), C. Roland (NA49), H. Sako (CERES), T. Trainor (STAR), G. Westfall (NA49), H. Sako (CERES), T. Trainor (STAR), G. Westfall (STAR), for providing input into this presentation.(STAR), for providing input into this presentation.

But wait! There’s more!But wait! There’s more!

• Multiplicity Fluctuations

• Spatial Fluctuations, or “Event Texture”

• Charge/Neutral (Isospin) Fluctuations

• Particle Ratio Fluctuations

The following topics could not be covered in this presentation.

Page 30: Fluctuations and Correlations in Relativistic Heavy Ion Collisions

Jeffery T. Mitchell (BNL) – QM2004Jeffery T. Mitchell (BNL) – QM2004 3030

Fluctuations According to Fluctuations According to HIJINGHIJING

HIJING cannot reproduce the centrality dependence of the fluctuations.

One problem is that <N> changes depending on the HIJING settings – not matched to the observed dataset.

Example for 0-5% centrality: <N> = 93.0 for jet suppression, 76.6 without suppression, and 51.2 without jets.

20-25% centrality

Auxiliary Slide