energy dependence of the bose-einstein correlations
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Energy dependence of the Bose-Einstein Correlations. Sergey Panitkin RHIC/AGS User Meeting 2006. Outline. Introduction Energy dependence of pion correlations Azimuthally sensitive pion HBT Summary. Two-particle Correlations. Single particle spectrum is sensitive to momentum - PowerPoint PPT PresentationTRANSCRIPT
Sergey Panitkin
Sergey Panitkin
RHIC/AGS User Meeting
2006
Energy dependence of the Bose-Einstein Correlations
Sergey Panitkin
Outline
Introduction
Energy dependence of pion correlations
Azimuthally sensitive pion HBT
Summary
Sergey Panitkin
Two-particle Correlations
Single particle spectrum is sensitive to momentum distribution only
Relative momentum distribution of particle pairs is sensitive to space-time information
Basis for Identical and Non-identical particle femtoscopy
),(4 pp
xSdxddNE
),(|),(|)/)(/(
/)( 2
2111
2122 qrqrr
pppp
q SdddNddN
dddNC
Source functionFSI
System evolution encoded in S(r,q)
Sergey Panitkin
qout
qside
qlong
Hanbury Brown-Twiss interferometry
Rsi
de
R long
Rout
x1
x2
12 ppq
p1
p2
q
12 pp2
1k
Pratt-Bertsch parameterization
HBT: Quantum interference between identical particles
pairsevent mixed
pairsevent real
)(P)(P
),(P),(
21
2121
pp
ppppC
2long
2long
2side
2side
2out
2out)(1),(
RqRqRqekkqC
q (GeV/c)q (GeV/c)
C (
q)C
(q)
11
22R
1~
– Final-state effects (Coulomb, strong) also can cause correlations, need to be accounted for
Gaussian model (3-d):
Sergey Panitkin
HBT for Gaussian sources
Kt~x~KR
Kx~KR
Kt~x~KR
2llong
2l
2side
2s
2out
2o
xxx~
)K,x(Sxd
)x(f)K,x(Sxdf
4
4
Decompose q into components:qLong : in beam directionqOut : in direction of transverse momentum KT
qSide : qLong & qOut
222222
1),,( llssoo RqRqRqlso eqqqC
Radii are related to source variances:
221
21
ppk
ppq
In Longitudinally Co-Moving System (LCMS) l =0
Sensitive to emission time
Sensitive to transverse extent
Sensitive to longitudinal extent
Sergey Panitkin
Mt dependence
Charged pions, AuAu (PbPb) most central
Mt dependence is attributed to collective flow
Sergey Panitkin
Femtoscopic signature of QGP
3D 1-fluid Hydrodynamics
Rischke & Gyulassy, NPA 608, 479 (1996)
withtransition
“”
Long-standing signature of QGP:
• Lattice QCD -> Speed of sound goes to zero (pressure drop) at phase transition
• increase in , ROUT/RSIDE due to deconfinement confinement transition
• hoped-for “turn on” as QGP threshold is reached (“softest point”)
G. Boyd et al., , Nucl.Phys. B469 (1996) 419
Sergey Panitkin
Compilation of world BP 3D -HBT parameters as a function of s
• ~10% Central AuAu(PbPb) events
• y ~ 0
• kT 0.17 GeV/c
no significant rise in spatio-temporal size of the emitting source
STAR Preliminary
The HBT Excitation function circa 2001
QM 2001
Sergey Panitkin
Energy systematics 2006
•Many new measurements since 2001
•Same conclusions
Sergey Panitkin
<ßr> (RHIC) = 0.55 ± 0.1 cTKFO (RHIC) = 100 ± 10 MeV
• Rapid change in freeze-out temperature and flow velocity between 2-20GeV
• Explosive Transverse Expansion at RHIC High Pressure
•Almost constant freeze-out temperature above 20 GeV
Tth
[GeV
]< r
> [
c]
STA
R
Kinetic freezeout from AGS->RHIC
T. Nayak
Blast wave fits to spectra
Sergey Panitkin
Freeze-out volume vs. beam energy
• non-monotonic behaviour
• minimum between AGS and SPS
•Why there is a drop at AGS ?
√s(GeV)
<kt> ~ 0.16 GeV/c
CERES Phys. Rev. Lett. 90 (2003) 022301
H. Appelshauser
Freeze-out volume estimate: 2sidelong
3
f RR2V
•Not a simple concept for expanding sources with continuous emission•Because of flow the best “total volume” estimate is at low Kt•Ad hoc formula
Sergey Panitkin
????
Freeze-out volume
Freeze-out volume estimate: 2sidelong
3
f RR2V
0.15 < kt < 0.25 GeV/c
<Npart>
CERES Phys. Rev. Lett. 90 (2003) 022301 partf NV
Centrality dependence:
since
partch NN
.constf
only at given beam energy!!
2sidelong
3
f RR2V
Sergey Panitkin
Particle multiplicity vs. beam energy
CERES Phys. Rev. Lett. 90 (2003) 022301
• particle number increases monotonically freeze-out at constant density excluded
• chemical composition changes
• cross sections are very different try mean free path:
√s(GeV)
1
Sergey Panitkin
Mean free path
N
V1 f
ff
in a composed medium:
... NNN NN
mb mb, 1372N
CERES Phys. Rev. Lett. 90 (2003) 022301
√s(GeV)
also Nσ shows non-monotonic behaviour dominated by baryons at low energy and mesons at high energy
Sergey Panitkin
Universal pion freeze-out
N
V1 f
ff CERES Phys. Rev. Lett. 90 (2003) 022301
√s(GeV)
Nσ follows Vf
data are consistent with constant mean free path at freeze-out
fm 1f
independent of beam energy and centrality
Sergey Panitkin
Universal freeze-out II
universal pion freeze-out:
independent of beam energy and system size
in A-A: f << R
why no dependence on beam energy and system size? why so small?
fm 1f
sqrt(sNN) (GeV) f
(fm
)
NN
V
N
V1
NN
fff
..implies f.o. at constant density (R~(dNch/d)1/3) if particle ratios are constant!
H. Appelshauser
Sergey Panitkin
What is “true” scaling variable?
STAR Preliminary
Nch seems to be better
Sergey Panitkin
Multiplicity scaling of radii
STAR DATASTAR DATA (pp,dAu,CuCu,AuAu@62GeV - prelim.)
“Universal radii scaling”as a concequence of volume scaling
For different systems and energies at RHIC physics does not change!?
Multiplicity scaling seems to work at all measured Kt
Sergey Panitkin
HBT relative to reaction plane HBT()
• “Standard” HBT provides direct access to space-time (size) information about source, "HBT radii"
• Additionally, HBT() provides direct access to shape and orientation of source
• Source shape at freeze-out evolution of system"How much of initial spatial deformation still exists at freeze-out?"
later hadronic stage?
bx
beam into screen
Heinz & Kolb, Nucl.Phys. A702 (2002) 269-280
collective expansion of system
Sergey Panitkin
Elliptic geometry leads to oscillations of the radii
– For example Rside
b
Rsi
de2
(fm
2 )
Out-of-plane In-planeCircular
(degree)out-of-planeextended source
p=0°
p=90°
Rside (large)Reactionplane
Rside (small)
Naïve view with no flow
HBT with respect to reaction plane
Heinz, Hummel, Lisa, Wiedemann PRC 044903 (2002)
Sergey Panitkin
Predictions from hydro
• Hydrodynamics: initial out-of-plane anisotropy may become in-plane later hadronic stage?
in-plane-extended
out-of-plane-extended
Teaney, Lauret, & Shuryak, nucl-th/0110037Heinz & Kolb, hep-ph/0111075
kT dependence
Sergey Panitkin
Centrality Dependence of HBT()
12 -bin analysis (kT integrated)
15° bins, 72 CF's total 12 bins × 3 centrality bins × 2 pion signs
0.15 < kT < 0.65
Oscillations exist in transverse radii for all bins
Amplitudes weakest for 0-10%
• Lines represent fits to allowed oscillations:
out, side, long go as cos(2)out-side goes as sin(2)
STAR
Sergey Panitkin
Estimate of initial vs F.O. source shape
2x
2y
2x
2y
RR
RR
20,S
22,S
FO R
R2
• estimate INIT from Glauber
• from asHBT:
FO =
INIT
FO < INIT → dynamic expansion
FO > 1 → source always OOP-extended
• constraint on evolution time
RHIC1[Kolb & Heinz]
•Out of plane extended source •Short life time
Sergey Panitkin
• AGS: E895, RHIC: STAR• does it make sense? Is it related
to bulk dynamics? YES
sNN (GeV)
(approximately same centrality)
AGS: FO init
RHIC: FO < init
Exitation function
•AGS: E895, RHIC: STAR
•~200 GeV Gap in measurements
Sergey Panitkin
Summary
HBT is a valuable tool for studies of space-time structure of systems created in heavy ion collisions
Important additional constraint for spectra and v2 measurements Large systematic datasets are already collected from AGS, SPS and
RHIC Non-trivial energy dependence of HBT radii is observed
– No predicted signatures of 1st order phase transition are not (yet?) observed
– Non monotonic behaviour (dip) around 10 GeV – “CERES hypothesis” is tempting: Universal mean free path at f.o.?– Similar dynamics, hence chemistry drives freeze-out– Multiplicity scaling at SPS and RHIC
Azimuthally sensitive HBT provides additional unique information about reaction dynamics
Detailed measurements at RHIC (and AGS), no measurements at SPS– Out of plain extended sources observed, imply short (~10 fm)
source lifetime More measurements are needed Lower energy measurements around 10-20 GeV will be very interesting