t. csörgő with m. csanád, r. lacey et al
DESCRIPTION
The scenario of perfect fluid hydrodynamics in A+A collisions at RHIC. T. Csörgő with M. Csanád, R. Lacey et al. Introduction: RHIC Scientists serve up “Perfect Liquid”, April 18, 2005 BRAHMS, PHENIX, PHOBOS, STAR White Papers, NPA, 2005 AIP Top Physics Story 2005 - PowerPoint PPT PresentationTRANSCRIPT
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T. Csörgő @ GRC NuCh, 2006/6/71
T. Csörgőwith M. Csanád, R. Lacey et al.
The scenario of perfect fluid hydrodynamics
in A+A collisions at RHIC
•Introduction:
RHIC Scientists serve up “Perfect Liquid”, April 18, 2005
BRAHMS, PHENIX, PHOBOS, STAR White Papers, NPA, 2005
AIP Top Physics Story 2005
•Hydrodynamics and scaling of soft observables
• Exact (i.e. not numerical) integrals of fluid dynamics
• non-relativistic and relativistic solutions
• Evidence for hydrodynamic scaling in RHIC data
• Scaling of slope parameters
• Scaling of Bose-Einstein /HBT radii
• Universal scaling of elliptic and higher order flows
• Intermediate pt region: breaking of the hydro scaling
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T. Csörgő @ GRC NuCh, 2006/6/72
"In general we look for a new law by the following process. First we guess it. Then we compare the consequences of the guess to see what would be implied if this law that we guessed is right. Then we compare the result of the computation to nature, with experiment or experience, compare it directly with observation, to see if it works. If it disagrees with experiment it is wrong.
In that simple statement is the key to science. It does not make any difference how beautiful your guess is. It does not make any difference how smart you are, who made the guess, or what his name is — if it disagrees with experiment it is wrong.”
/R.P. Feynman/
Discovering New Laws
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T. Csörgő @ GRC NuCh, 2006/6/73
Quark Gluon Plasma“Ionize” nucleons with heat“Compress” them with density
New state(s?) of matter
Phases of QCD Matter, EoS
Z. Fodor and S.D. Katz:Tc = 164 ± 2 -> 189 ± 8 MeV, QM’05(?)
even at finite baryon density, Cross over like transition.
(hep-lat/0106002, hep-lat/0402006)
Most recent result:
Tc=176±3MeV (~2 terakelvin)(hep-ph/0511166)
Input for hydrodynamics
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T. Csörgő @ GRC NuCh, 2006/6/74
Nonrelativistic dynamics of perfect fluids
• Equations of nonrelativistic hydro:
• Not closed, EoS needed:
• Perfect fluid: definitions are equivalent, term used by PDG # 1: no bulk and shear viscosities, and no heat conduction.
# 2: energy-momentum tensor diagonal in the local rest frame.
• ideal fluid: ambiguously defined term, discouraged #1: keeps its volume, but conforms to the outline of its container
#2: an inviscid fluid
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T. Csörgő @ GRC NuCh, 2006/6/75
Exact, ellipsoidal, nonrelativistic solutions
• A new family of PARAMETRIC, exact, scale-invariant solutions • T. Cs. Acta Phys. Polonica B37 (2006) 1001, hep-ph/0111139
• Temperature scaling function is arbitrary, e.g. homogeneous temperature Gaussian density Buda-Lund profile: Zimányi-Bondorf-Garpman profile:
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T. Csörgő @ GRC NuCh, 2006/6/76
Exact integrals of fluid dynamics
Examples of density profiles- Fireball- Ring of fire- Embedded shells of fireExact integrals of hydroNo numerical viscosity
Time evolution of the scales (X,Y,Z)follows a classic potential motion.Scales at freeze out -> observables.info on history LOST!No go theorem - constraintson initial conditions (penetrating probels) indispensable.
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T. Csörgő @ GRC NuCh, 2006/6/77
Examples of exact hydro results
• Propagate the hydro solution in time numerically:
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T. Csörgő @ GRC NuCh, 2006/6/78
Solution of the “HBT puzzle”
HBT volumeHBT volumeFull volume
Geometrical sizes keep on increasing. Expansion velocities tend to constants. HBT radii Rx, Ry, Rz approach a direction independent constant.
Slope parameters tend to direction dependent constants.General property, independent of initial conditions - a beautiful exact result.
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T. Csörgő @ GRC NuCh, 2006/6/79
Geometrical & thermal & HBT radii
3d analytic hydro: exact time evolution
geometrical size (fugacity ~ const)
Thermal sizes (velocity ~ const)
HBT sizes (phase-space density ~ const)
HBT dominated by the smaller of the geometrical and thermal scales
nucl-th/9408022, hep-ph/9409327
hep-ph/9509213, hep-ph/9503494
HBT radii approach a constant of time
HBT volume becomes spherical
HBT radii -> thermal ~ constant sizes
hep-ph/0108067, nucl-th/0206051
animation by Máté Csanád
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T. Csörgő @ GRC NuCh, 2006/6/710
Scaling predictions of fluid dynamics
- Slope parameters increase linearly with mass- Elliptic flow is a universal function its variable w is proportional to transverse kinetic energy and depends on slope differences.
Inverse of the HBT radii increase linearly with massanalysis shows that they are asymptotically the same
Relativistic correction: m -> mt
hep-ph/0108067,nucl-th/0206051
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T. Csörgő @ GRC NuCh, 2006/6/711
Relativistic Perfect Fluids
• Rel. hydrodynamics of perfect fluids is defined by:
• A recent family of exact solutions: nucl-th/0306004
• Overcomes two shortcomings of Bjorken’s solution:• Yields finite rapidity distribution, includes transverse flow
• Hubble flow lack of acceleration. • Accelerating, new rel. hydro solutions: nucl-th/0605070
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T. Csörgő @ GRC NuCh, 2006/6/712
Solutions of Relativistic Perfect Fluids
• A new family of exact solutions: • T. Cs, M. I. Nagy, M. Csanád: nucl-th/0605070
• Overcomes two shortcomings of Bjorken’s solution:• Yields Finite Rapidity distribution, similarly to Landau’s solution• Includes relativistic acceleration of the matter• Works in 1+1 and 1+3 spherically symmetric expansions
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T. Csörgő @ GRC NuCh, 2006/6/713
Animation of the new exact solution
nucl-th/0605070dimensionless = 21+1 dboth internaland externallooks like A+A
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T. Csörgő @ GRC NuCh, 2006/6/714
nucl-th/0605070: advanced estimate of
• Width of dn/dy distribution is due to acceleration:• acceleration yields longitudinal explosion, thus• Bjorken estimate underestimates the initial energy density
t f0 Bj2
0 f 00
m ddn dy
d d dR
1
12
0 f f
Bj 0 0
2 12
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T. Csörgő @ GRC NuCh, 2006/6/715
• Let us fit BRAHMS dn/deta data• dn/deta width yields a correction factor of ~ 2.0 - 2.2• Yields inital energy density of 10- 30 GeV/fm^3
• a correction factor > 1 @ SPS!
nucl-th/0605070: advanced estimate of
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T. Csörgő @ GRC NuCh, 2006/6/716
Principles for Buda-Lund hydro model
• Analytic expressions for all the observables
• 3d expansion, local thermal equilibrium, symmetry
• Goes back to known exact hydro solutions:
• nonrel, Bjorken, and Hubble limits, 1+3 d ellipsoids
• but phenomenology, extrapolation for unsolved cases
• Separation of the Core and the Halo
• Core: perfect fluid dynamical evolution
• Halo: decay products of long-lived resonances
• Missing links: phenomenology needed
• search for accelerating ellipsoidal exact solutions
• first accelerating solution found, nucl-th/0605070
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T. Csörgő @ GRC NuCh, 2006/6/717
A useful analogy
• Core Sun• Halo Solar wind
• T0,RHIC ~ 210 MeV T0,SUN ~ 16 million K
• Tsurface,RHIC ~ 100 MeV Tsurface,SUN ~6000 K
Fireball at RHIC our Sun
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T. Csörgő @ GRC NuCh, 2006/6/718
Buda-Lund hydro model
The general form of the emission function:
Calculation of observables with core-halo correction:
Assuming profiles for
flux, temperature, chemical potential and flow
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T. Csörgő @ GRC NuCh, 2006/6/719
Buda-Lund hydro model
Invariant single particle spectrum:
Invariant Buda-Lund correlation function: oscillating, non-Gaussian prefactor!
Non-invariant Bertsch-Pratt parameterization, in a Gaussian approximation:
Non-Gaussian BL form Gaussian BP approximation:
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T. Csörgő @ GRC NuCh, 2006/6/720
The generalized Buda-Lund model
• The original model was for axial symmetry only, central coll.
• In its general hydrodynamical form:Based on 3d relativistic and non-rel solutions of perfect fluid dynamics:
• Have to assume special shapes:• Generalized Cooper-Frye prefactor:
• Four-velocity distribution:
• Temperature:
• Fugacity:
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T. Csörgő @ GRC NuCh, 2006/6/721
Scaling predictions of fluid dynamics
- Slope parameters increase linearly with mass- Elliptic flow is a universal function its variable w is proportional to transverse kinetic energy and depends on slope differences.
Inverse of the HBT radii increase linearly with massanalysis shows that they are asymptotically the same
Relativistic correction: m -> mt
hep-ph/0108067,nucl-th/0206051
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T. Csörgő @ GRC NuCh, 2006/6/722
Scaling predictions of Buda-Lund
- Slope parameters increase linearly with transverse mass- Elliptic flow is same universal function. - Scaling variable w is prop. to generalized transv. kinetic energy and depends on effective slope diffs.
Inverse of the HBT radii increase linearly with massanalysis shows that they are asymptotically the same
Relativistic correction: m -> mt
hep-ph/0108067,nucl-th/0206051
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T. Csörgő @ GRC NuCh, 2006/6/723
Some analytic Buda-Lund results
HBT radii widths
Slopes, effective temperatures
Flow coefficients
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T. Csörgő @ GRC NuCh, 2006/6/724
Buda-Lund hydro and Au+Au@RHIC
2/NDF = 126/208 (stat + syst errors added in quadrature)
Spectra
Spectra
v2
nucl-th/0311102, nucl-th/0207016, nucl-th/0403074
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T. Csörgő @ GRC NuCh, 2006/6/725
Femptoscopy signal of sudden hadronization
Buda-Lund hydro fit indicates
hydro predicted (1994-96)scaling of HBT radii
T. Cs, L.P. Csernai
hep-ph/9406365T. Cs, B. Lörstad
hep-ph/9509213
Hadrons with T>Tc :a hint for cross-over
M. Csanád, T. Cs, B. Lörstad and A. Ster,
nucl-th/0403074
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T. Csörgő @ GRC NuCh, 2006/6/726
Confirmation
see nucl-th/0310040 and nucl-th/0403074, R. Lacey@QM2005/ISMD 2005
A. Ster @ QM2005.
Universal scalingPHOBOS v2(->w)
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T. Csörgő @ GRC NuCh, 2006/6/727
• Exact non-rel. hydro solution:
Slope parametersBuda-Lund rel. hydro formula:
Experimental test: PHENIX, STAR
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T. Csörgő @ GRC NuCh, 2006/6/728
Similar scaling of Bose-Einstein/HBT radii
Rside/Rout ~ 1 Rside/Rlong ~ 1 Rout/Rlong ~ 1
1/R2side ~ mt 1/R2
out ~ mt 1/R2long ~ mt
same slopes ~ fully developed, 3d Hubble flow
1/R2eff=1/R2
geom+1/R2therm
and 1/R2therm ~mt
intercept is nearly 0, indicating 1/RG
2 ~0,
thus (x)/T(x) = const!
reason for success of thermal models @ RHIC!
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T. Csörgő @ GRC NuCh, 2006/6/729
Elliptic flow, limits
GG. Veres, PHOBOS data, proc QM2005
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T. Csörgő @ GRC NuCh, 2006/6/730
Universal scaling and dependence
PHOBOS, nucl-ex/0406021PHOBOS, nucl-ex/0406021PHOBOS, nucl-ex/0406021PHOBOS, nucl-ex/0406021
s
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T. Csörgő @ GRC NuCh, 2006/6/731
Universal scaling and v2(centrality,)
PHOBOS, nucl-ex/0407012PHOBOS, nucl-ex/0407012PHOBOS, nucl-ex/0407012PHOBOS, nucl-ex/0407012
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T. Csörgő @ GRC NuCh, 2006/6/732
Universal v2 scaling and PID dependence
PHENIX, PHENIX, nucl-ex/0305013nucl-ex/0305013
PHENIX, PHENIX, nucl-ex/0305013nucl-ex/0305013
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T. Csörgő @ GRC NuCh, 2006/6/733
Universal scaling and fine structure of v2
STAR, nucl-ex/0409033STAR, nucl-ex/0409033STAR, nucl-ex/0409033STAR, nucl-ex/0409033
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T. Csörgő @ GRC NuCh, 2006/6/734
Universal v2 scaling predicted in 2003
PHENIX and PHOBOSdata collapse to aPREDICTEDUniversal Scaling Lawof perfect fluid hydro
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T. Csörgő @ GRC NuCh, 2006/6/735
Summary on universal scaling of v2
Black scaling law:Theoretical
predictionfrom analytic perfect fluid hydrodynamics:
12
0
( )
( )
I wv
I w
hep-ph/0108067, nucl-th/0310040
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T. Csörgő @ GRC NuCh, 2006/6/736
Scaling and scaling violations
Universal hydro scaling breakswhere quark number scalingsets in, pt ~ 1-2 GeVFluid of QUARKS!!
R. Lacey and M. OldenburgProc. QM 2005
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T. Csörgő @ GRC NuCh, 2006/6/737
Summary
Au+Au elliptic flow data at RHIC satisfy theUNIVERSAL scaling laws
predicted (2001, 2003)
by the (Buda-Lund) hydro model, based on exact solutions of
PERFECF FLUID hydrodynamics
quantitative evidence for a perfect fluid in Au+Au at RHIC
scaling breaks in pt at ~ 1.5 GeV,
in rapidity at ~|y| > ymay - 0.5
Search for establishing the domain of applicability started.Scaling of HBT radii and spectra:
first tests passed, further tests going on.
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T. Csörgő @ GRC NuCh, 2006/6/738
ConclusionConclusion
Thank you for your attention !
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T. Csörgő @ GRC NuCh, 2006/6/739
Backup Slides from now onBackup Slides from now on
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T. Csörgő @ GRC NuCh, 2006/6/740
Buda-Lund rel. hydro formula:
Higher flow coefficientsExact non-relativistic result:
0 1 2 3 4 5
v 4 (%
)
0
1
2
3
4
5
6
h (STAR)v2 scaled
s 200 GeVNNAu Au
2( )fsTy
242
4 2 T
vv k y
242
4 2 T
vv k y
R. Lacey, Proc. QM 2005
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T. Csörgő @ GRC NuCh, 2006/6/741
Hamiltonian motion in heavy ion physics
• Direction dependent Hubble flow
• Late t -> v = H r, where H = 1/t. Spherical symmetry: R=X=Y=Z
• 2/3 in general: cs2, if T0 < 0, and cs
2 = 1/3 -> Friedmann
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T. Csörgő @ GRC NuCh, 2006/6/742
Friedmann eq. of heavy ion physics
• Scale invariant solutions of fireball hydro, hep-ph/0111139:
• From global energy conservation -> “Friedmann equation”
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T. Csörgő @ GRC NuCh, 2006/6/743
Scaling laws from hydro Exact non-rel. and Buda-Lund rel.
Single particle spectraSlopeRapidity widthElliptic flowHigher harmonicsHBT radius parametersasHBT
Au+Au data at RHIC satisfy thescaling laws that were predictedby the Buda-Lund hydro model.
v2(y,pt, ...) is mapped alreadyto a universal scaling function
-> compelling evidence for a perfect fluid at RHIC
scaling breaks between 1-2 GeV,where quark number scaling sets
in.
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T. Csörgő @ GRC NuCh, 2006/6/744
Hubble from numerical rel. hydro
Assume net barion-free, approx. boost invariant caseRel. Euler equation Entropy conservation4 independent eqs, 5 variables
Closed by thermodynamicalrelationships.key quantity:temperature dependent speed of soundcan be taken from lattice QCD
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T. Csörgő @ GRC NuCh, 2006/6/745
Some num. rel. hydro solutions
M. Chojnacki, W. Florkowski, T. Cs,nucl-th/0410036lattice QCD EOS (B=0)T0(r) ~ initial entropy (Glauber)H0 ~ initial Hubble flow
Support the quick development of the Hubble flowand the Blast-wave, Buda-Lund and Cracow etc models
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T. Csörgő @ GRC NuCh, 2006/6/746
Effects of pre-equilibrium flow
Hubble
Initial temperature gradient and initial flow have to be co-variedto get Hubble in a sufficiently short time. H0 > 0
Hubble
Hubble