Title: Event by Event Fluctuations
1Event by Event Fluctuations
CERN Heavy Ion Forum May 24 2006
2What can we learn from fluctuations?
3What can we learn from fluctuations?
Nature of the phase transition?
(How) Does matter thermalize?
How is entropy produced?
Properties of the medium?
How are hadrons made?
ca 1990
4Nature of the Phase Transition
Search for critical phenomena induced near phase
transition
5Nature of the Phase Transition
ca 1998
6Nature of the Phase Transition
Temperature (MeV)
Quark-Gluon Plasma
200
Phase Boundary
Hadron Gas
Atomic Nuclei
0
Plot from M. Stephanov, Correlations 05
0
1
Matter Density µB (GeV)
7Nature of the Phase Transition
- Theoretical guidance is limited
- Experimental strategy
- Search in different observables, correlate
observables - Fine grained exploration of µB, T space
time
8Nature of the Phase Transition
- Theoretical guidance is limited
- Experimental strategy
- Search in different observables, correlate
observables - Fine grained exploration of µB, T space
Experiments only see final state particles
9Nature of the Phase Transition
- Theoretical guidance is limited
- Experimental strategy
- Search in different observables, correlate
observables - Fine grained exploration of µB, T space
lt(X - ltXgt)2gt
Enhanced Fluctuations near Critical Point
vs
Rajagopal, Shuryak, Stephanov
10Energy Regimes and Accelerators
RHIC
SPS
Fit by Becattini et al.
AGS
central AA
SPS
AGS
RHIC
Change from baryon- to meson dominated system
11First result on ltpTgt fluctuations (1999)
- pT - simple observable (supposedly...)
- High statistical precision
- spT/ltpTgtinclt 0.1
- Sensitive to many interesting scenarios
- Critical Point
- DCC production
- Droplet formation
- Any non-statistical, momentum-localized process
12First result on ltpTgt fluctuations (1999)
- pT - simple observable (supposedly...)
- High statistical precision
- spT/ltpTgtinclt 0.1
- Sensitive to many interesting scenarios
- Critical Point
- DCC production
- Droplet formation
- Any non-statistical, momentum-localized process
s2pT,dyn s2M(pT) - s2M(pT),mixed
Dynamical Fluctuations
13Excitation Function Momentum Spectra
Compilation by NA49 Plot from Claudia Hoehne,
QM05
filled symbol particle open symbol antiparticle
The Step
- Structure in energy dependence of ltmTgt -
Reminiscent of Van Hoves T vs e prediction
(1982) - Surprisingly difficult measurement ?
Decay corrections, PID acceptance
14Excitation Function Momentum Fluctuations
Compilation by STAR STAR PRC 72 044902 (2005)
SPS CERES
The Step
RHIC STAR
AGS?
Central AA
Monotonic energy dependence over measured
range No results near step region
15Nature of the Phase Transition
ltpTgt Fluctuations
STAR
SpT
16- Is strangeness enhanced in every event?
- Can we see signs of super-cooling below Tcrit?
K/p
T
17Event-by-event fit of K/p (NA49)
One Event
Event Ensemble
ltdE/dxgt
ltdE/dxgt
log(ptot GeV)
log(ptot GeV)
Slide from Christof Roland, Correlations 05, MIT
18PbPb, 17.2 GeV NA49, PRL 86 (2001) 1965
- Dynamical fluctuations are small ( lt 5)
- Compatible with resonance gas (Jeon, Koch
nucl-th/9906074) - Strangeness enhancement in every event
- Chemical freeze-out at same T in every event
PhD thesis Christof Roland, 2000
19Particle Ratios
Nature of the Phase Transition
The Horn
NA49 Phys.Rev.C66054902,2002 Plot from Claudia
Hoehne, QM05
Average K/p ratio
Non-monotonic behavior at AGS/SPS boundary
20Nature of the Phase Transition
NA49, Christof Roland, QM04
STAR, Supriya Das, VI Workshop 05
The Horn
AGS?
RHIC STAR Preliminary
SPS NA49 Preliminary
Strong increase at low energy Comparison between
experiments difficult
21Nature of the Phase Transition
NA49, Christof Roland, QM04
K/p Fluctuations
p/p Fluctuations
Proton/p fluctuations negative ? Correlated
production of protons and pions
22What can we learn from fluctuations?
Nature of the phase transition?
(How) Does matter thermalize?
How is entropy produced?
Properties of the medium?
How are hadrons made?
Monotonic vs evolution of global
fluctuations Magnitude of fluctuations
moderate Scaling of relative fluctuations Increa
se in K/p fluctuations at low vs
Equilibrium evolution? Small latent
heat? Kinetic freeze-out far from critical
point? Connection to PT/CP?
23What can we learn from fluctuations?
Nature of the phase transition?
(How) Does matter thermalize?
How is entropy produced?
Properties of the medium?
How are hadrons made?
ca 2000
24Properties of the Medium
Net Charge/?y Fluctuations ? Charge/DoF
Flucs change from 1-2 (QGP) to 4 (Pion
Gas) Fluctuations frozen b/c charge
conservation Diffusion vs Expansion
timescale
Ratio N/N-
Jeon, Koch PRL (2000) hep-ph/0003168 Asakawa,
Heinz, Mueller PRL (2000) hep-ph/0003169
Event-by-event distribution of net charge ratio
Note Similar for net baryon number
Connection to quark number
susceptibilities Connection to Critical point
25Properties of the Medium
Net Charge Fluctuations
PHENIX PRL 89 (2002)
STAR PRC 68 (2003)
130 GeV AuAu
Ratio
? lt 0.7, 0.1 GeV/c lt pT
Stochastic Fluctuations
Charge Conservation
P130 GeV AuAu
HIJING
Quark- Coalescence
Net Charge
Bialas, 2003
Resonance Gas
QGP
Centrality
Centrality
Fluctuations agree with stochastic distributions
of Hadrons
26Net Charge Fluctuations
Quark- Coalescence
Bialas, 2003
QGP
Little (no) vs dependence of charge fluctuations
27What can we learn from fluctuations?
Nature of the phase transition?
(How) Does matter thermalize?
How is entropy produced?
Properties of the medium?
How are hadrons made?
28What can we learn from fluctuations?
Nature of the phase transition?
(How) Does matter thermalize?
How is entropy produced?
Properties of the medium?
How are hadrons made?
Quark coalescence? Property of
Hadronization? Diffusion? Bound states?
Net charge fluctuations large ( hadron
gas) Small/no vs dependence
29Forward/backward multiplicity correlations
Use variance s2C
30Forward/backward multiplicity correlations
effective cluster size 2-2.5 for 200 GeV AuAu
31Clusters in AA (and pp) collisions
effective cluster size 2-2.5 for 200 GeV AuAu
Cluster in ??,?f space via 2-particle
correlations (pythia pp _at_200 GeV, ?lt3)
32UA5 Phys.Lett.B123361,1983
Keff
PN
546 GeV
Clusters in AuAu reminiscent of results from pp
33Measuring global charge fluctuations
Clustersize ?y2
Acc. Clustersize Rapidity gap
SPS
NA49
Acc. Clustersize lt Rapidity gap
RHIC
STAR
Acc. gt Clustersize ltlt Rapidity gap
LHC
CMS
34Beyond global charge fluctuations
STAR 200 GeV pp
Pythia, 200 GeV pp, all pT , all charges
Like sign
Split sample
2-D angular correlation function
Unlike sign
Tom Trainor et al (STAR)
35Charge Dependent Correlations
STAR 200 GeV pp
Like sign
longitudinal charge ordering
gaussian
flat
subtract
Unlike sign
Charge Dependent (CD) correlations like sign
- unlike sign
Tom Trainor et al (STAR)
36Difference of like-sign and unlike-sign
2-particle correlations
?f
pp
37Difference of like-sign and unlike-sign
2-particle correlations
?f
??
pp
AuAu
STAR nucl-ex/0406035
Evolution of cluster properties/charge
correlations
38Correlations and Fluctuations, revisited
Net-charge Fluctuations
Global scaling, even though underlying
correlations change
Text
Central AA
pp
centrality ?
Net-charge correlations (c.f. Balance Function)
39What can we learn from fluctuations?
Nature of the phase transition?
(How) Does matter thermalize?
How is entropy produced?
Properties of the medium?
How are hadrons made?
Large multiplicity fluctuations Strong change in
underlying correlation structure
Particles produced in large clusters Understand
ing of hadronization essential Collision
dynamics reflected in correlation structure
40What can we learn from fluctuations?
Nature of the phase transition?
(How) Does matter thermalize?
How is entropy produced?
Properties of the medium?
How are hadrons made?
Some remarks on future measurements
41NA49 Horn
Strangeness Fluctuations vs vs
NA49 (Christof Roland QM04)
NA49
preliminary
Fluctuations in K/pi ratio
42Strangeness Fluctuations vs vs
Opportunity with possible low-E run at RHIC STAR
with ToF/Si-VTX upgrade is ideal place
43v2 near mid-rapidity
PHOBOS 200 GeV Statistical errors only
PHOBOS 200 GeV h
Statistical errors only
AuAu
preliminary
CuCu preliminary
Geometrical initial state eccentricity from
Glauber model
Surprisingly large flow signal in CuCu!
44Realign the coordinate system to maximize
ellipsoidal shape (a principal axis
transformation)
Participant eccentricity (versus standard
eccentricity)
45Hydro- Limit
Eccentricity Fluctuations provide additional
correlation strength Nuclear Physics!? ?
Measure v2 fluctuations
CuCu
AuAu
CuCu PHOBOS QM 2005
Participant Eccentricity provides universal
scaling Approach to equilibrium?
Low Density Limit STAR, PRC 66 034904
(2002) Voloshin, Poskanzer, PLB 474 27
(2000) Heiselberg, Levy, PRC 59 2716, (1999)
46Denes Molnar, BNL workshop June 05
47Analogy Cosmic Microwave Background
Cosmic microwave background
COBE 1992
Penzias, Wilson 1964
WMAP
?T/T 10-5
ltTgt3K
48Summary
- Rich existing data set on fluctuations
- Energy independence of global pT, charge
fluctuations - Energy dependence in K/p, p/p fluctuations
- limited statistical significance
- Non-trivial structure/change in charge
correlations - Low-vs scan at RHIC could confirm and improve
experimental results
49Excitation Function K/p Fluctuations
Normalized by dN/dy
RHIC
AGS?
SPS
Scaling by dN/dy or (dN/dy)1/2 does not work over
full energy range
50What can we learn from fluctuations?
Nature of the phase transition?
(How) Does matter thermalize?
How is entropy produced?
Properties of the medium?
How are hadrons made?
Look at the medium using 2-particle correlations
(untriggered) at high(er) pT
51Properties of the Medium
2-particle momentum correlations
0-5
Shape of near-side parton-fragmentation peak
evolves with centrality
52Properties of the Medium
2-particle momentum correlations
Subtract fragmentation peak to look at medium
AuAu 200 GeV 20-30
53What can we learn from fluctuations?
Nature of the phase transition?
(How) Does matter thermalize?
How is entropy produced?
Properties of the medium?
How are hadrons made?
Medium modification of pT correlation
shape Possible medium modification due to
partonic recoil
Interaction of partons with bulk medium (flow
field) Extract bulk properties (e.g. viscosity)?
54(No Transcript)
55Net Charge, and K/p Fluctuations
Instead of measuring the variance of a yield
ratio,
Study the dynamical fluctuations
Side Note
ltptgt Fluctuations