Laying the groundwork at the AGS: Recent results from E895 Mike Lisa, for the E895 Collaboration
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Transcript of Laying the groundwork at the AGS: Recent results from E895 Mike Lisa, for the E895 Collaboration
Mike Lisa, Quark Matter 2001 1E895
Laying the groundwork at the AGS:Recent results from E895
Mike Lisa, for the E895 Collaboration
N.N. Ajitanand, J. Alexander, D. Best, P. Brady, T. Case, B. Caskey, D. Cebra,J. Chance, P. Chung, B. Cole, K. Crowe, A. Das, J. Draper, S. Gushue, M. Gilkes,
M. Heffner, H. Hiejima, A. Hirsch, E. Hjort, L. Huo, M. Justice, M. Kaplan,J. Klay, D. Keane, J. Kintner, D. Krofcheck, R. Lacey, J. Lauret, E. LeBras,M. Lisa, H. Liu, Y. Liu, B. McGrath, Z. Milosevich, D. Olson, S. Panitkin,C. Pinkenburg, N. Porile, G. Rai, H.-G. Ritter, J. Romero, R. Scharenberg,
L. Schroeder, B. Srivastava, N. Stone, J. Symons, S. Wang, R. Wells, J. Whitfield, T. Wienold, R. Witt, L. Wood, X. Yang, Y. Zhang, W. Zhang
Auckland - BNL - CMU - Columbia - UC Davis - Harbin - KSU - LBL - St. Mary’s College - OSU - Purdue - Stony Brook
Mike Lisa, Quark Matter 2001 2E895
Reminder: why AGS is (still) interesting
sets baseline systematics“your systematics deviate from what?”
the “other” extreme condition - maximum baryon density probe medium & bulk effects
transition region for bulk properties
before E895pp
Fy
v2
T
Ebeam
Mike Lisa, Quark Matter 2001 3E895
This talkNot a “final wrap-up” of E895, which is still alive. Since QM99:
• PRL 83 1295 (1999) Transition from out-of-plane to in-plane elliptic flow• PRL 84 2798 (2000) Bombarding energy dependence of - HBT at the
AGS• PRL 84 5488 (2000) Sideward flow in Au+Au collisions at 2-8 AGeV• PRL 85 940 (2000) Anti-flow of K0 mesons in 6 AGeV Au+Au collisions• PLB 496 1 (2000) Azimuthal dependence of pion interferometry• PRL accepted (2000) flow in 2-6AGeV Au+Au collisions•Published E895 flow
•Beyond proton flow - collective flow of strange particles
•Geometrical dependence of flow
•HBT Beyond “R = 5 fm”
•geometric aspects of collective flow•6D phasespace density-p correlations
•Summary
Mike Lisa, Quark Matter 2001 4E895
Measurement with the EOS TPC
• Up to ~350 particles/event measured over large phase space
• Good reaction plane resolution p/p 3% (dominated by MCS)
“Grandfather of STAR TPC”
Mike Lisa, Quark Matter 2001 5E895
The Four Fundamental Corners of E895
space-time geometry& dynamics
PRL 84 2798 (2000)
pre-equilibrium dynamicscollective bulk response
equation of statePRL 83 1295 (1999)PRL 84 5488 (2000)
thermal/chemicalproperties
poster by J. Klay
talk by C. Pinkenburg
early thermochemistrystrange potentials
strange/nonstrangeradial flow
distinct freezeout?talk by C. Pinkenburg
tilted sourcesgeometry of
anisotropic flowPLB 496 1 (2000)poster by U. Heinz
phasespace density
poster by D. Cebra
thermal population?multiparticle effects?
p correlationsbaryon source geometry
two-hadron potential
, K0 flow
PRL 85 940 (2000)PRL, in press
strange potentials
talk by C. Pinkenburg
Mike Lisa, Quark Matter 2001 6E895
Reminder from QM99: Proton Flow
Elab (AGeV)1 101 10
F (
GeV
/c)
0
0.1
0.2
0.3
PRL 83 1295 (1999)PRL 84 5488 (2000)
n
x
dy
pdFsideward flow
elliptic flow 2cosv2
(Beam)Reaction plane
px
py
pz
F
Momentum space
Transition region for flow mappedF drops as resonances dominateStrong sensitivity to medium contributions to pressureNo single parameterization reproduces flow detailsNo sudden drops in pressure (flow) signaling phase transition
Elab (AGeV)
0.04
-0.08
-0.04
0
1 10
v 2
Mike Lisa, Quark Matter 2001 7E895
Beyond protons...
see talk of Chris Pinkenburg today
neural networks identifydecays of neutral strange
particles
• (p+p)•179
1.08 1.10 1.12 1.14Minv (GeV/c2)
0sK
Minv (GeV/c2)
p
production excitation function
Mike Lisa, Quark Matter 2001 8E895
flow
PRL accepted (2000) see talk of Chris Pinkenburg today
•“positive” flow
•decreases with Eb (more than
p)
•RQMD (without potential) underpredicts effect
•probe potential at high (complements hypernuclei studies) astrophysical models
“quark counting”
NNN32
p
x
(G
eV
/c)
y/ycm
2 AGeV
6 AGeV
4 AGeV
Mike Lisa, Quark Matter 2001 9E895
K0S (anti-)flow
PRL 85 940 (2000) see talk of Chris Pinkenburg today
0-0.5-1.0 0.5 1.0
6 GeV
0
0.1
-0.1
px
(GeV
/c)
RQMD (2.3)data
4 GeV data
y/ycm
Surprise— strong antiflow•grows with collision energy
Transport models:•rescattering insufficient (results in positive flow)
•strong repulsive vector potential required
S. Pal et al, PR C62 061903 (2000)
Mike Lisa, Quark Matter 2001 10E895
proton elliptic flow - varying the geometry
“min-bias” flow measurements do not constrain models
geometry provides another handle on flow
increasing spatial asymmetry produces larger signal
Can HBT give geometrical information on flow??
2 AGeV
4 AGeV
6 AGeV
2 4 6 80
0
.02
-.02
-.01
.01
0
-.02
-.04
v2
b (fm)
Mike Lisa, Quark Matter 2001 11E895
HBT: probing freeze-out space-time structure I - Cylindrical sources
K
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
RoutRside
y,xx,x sideout
HBT @ AGS mappedby E895 (QM99)
PRL 84, 2798 (2000)NPA 661, 444c (1999)
Mike Lisa, Quark Matter 2001 12E895
HBT: probing freeze-out space-time structure II - Collisions at b0
•Source in b-fixed system: (x,y,z)•Space/time entangled in
pair system (xO,xS,xL)
out
b
K
side
x
y
U. Wiedemann, PRC 57, 266 (1998)MAL, U. Heinz, U. Wiedemann PLB 489, 287 (2000)See Poster by U. Heinz
(several terms vanish @ pT = y = 0)
sinz~x~R
cosz~x~R
t~z~R
2sinx~y~R
x~y~2cosx~y~R
t~x~y~2cosx~y~R
2sl
2ol
22L
22l
22212
os
222122
212
s
22222122
212
o
Mike Lisa, Quark Matter 2001 13E895
1st-harmonic oscillations: spatial tilt
angle S
(Beam)
Coordinate space!
x
y
z
s
2nd-harmonic oscillations fromelliptical transverse shape
b
2y~
2x~
x
y
sinz~x~R
cosz~x~R
t~z~R
2sinx~y~R
x~y~2cosx~y~R
t~x~y~2cosx~y~R
2sl
2ol
22L
22l
22212
os
222122
212
s
22222122
212
o
First-order information in HBT()
Mike Lisa, Quark Matter 2001 14E895
Data: - correlation functionsAu(4 AGeV)Au, b4-8 fm
• 6 components to radius tensor: i, j = o,s,l
1D projections, =45°
2D projections
2ijji Rqqe1),q(C
lines: projections of 3D Gaussian fit
out side long
C(q
)
E895, PLB 496 1 (2000)
Mike Lisa, Quark Matter 2001 15E895
Cross-term radii Rol, Ros, Rsl quantify “tilts” in correlation functions
fit results to correlation functions
Lines: Simultaneous fit to HBT radiito extract underlying geometry
Mike Lisa, Quark Matter 2001 16E895
Images of --emitting sources (scaled ~ x1014)
3 fm
x ’
y
2 AGeV
x
zS=47°
x ’
y
4 AGeV
x
zS=37°
x ’
y
6 AGeV
x
zS=33°
Large, positivetilt angles
35.1x~
y~
2
2
similar to naïveoverlap: b~5 fm
Mike Lisa, Quark Matter 2001 17E895
Opposing average tilts in p, x and the physics of
flow• “antiflow” (negative tilt in p-space)
• x-space tilt in positive direction non-hydro nature of flow
B. Caskey
RQMD transport model:•Antiflow reflects dense region z~0•(dilute large-|z| show positive flow)
RQMD Au(2GeV)Au
z (f
m)
x (fm)
+ 6 AGeV
pion momentum anisotropies due toreflection from flowing baryons
(N N)
tilt reflects x-space structureof proton flowBass et al [PLB 302 381 (93)]:
Mike Lisa, Quark Matter 2001 18E895
Tomography in 6 Dimensions
y
x’
z
x
Flow analysis and HBT relative to the reaction plane allow a complete characterization of the final state in phase space, get space-momentum correlations
6 dimensional Tomography of proton flow
py
px
pz
px
Momentum Space (Flow) Coordinate Space (HBT)
6 AGeV
Tiny flow angle positive v2 Large tilt Out-of-plane
Mike Lisa, Quark Matter 2001 19E895
f = occupation of 6-D positionmomentum cell, volume h3
•determines magnitude of multi-particle correlations (lasers)•provides a test of thermalization/consistency
1e
1)p,x(f
)x(T/)x(up
T determines number of , as well as spectral shape
More on position - momentum space relationshipthe phasespace density
G. Bertsch, PRL 72 2349 (94)D. Ferenc et al, PL B457 347 (99)
Experimental access to spatially averaged density
longsideout
TT
3
3T RRR
ddppdyNd
E1
y,pf
volume in p-space
volume in x-space
•observation @ SPS, AGS: “Universal” freeze-out density
• breaks down at lower energies?
Mike Lisa, Quark Matter 2001 20E895 midrapidity
central collisions
•non-universal growth of f with collision energy
•f<1 no condensate
preliminary
Measured phasespace densities
Mike Lisa, Quark Matter 2001 21E895 midrapidity
central collisions
•non-universal growth of f with collision energy
•f<1 no condensate
•low-pT saturation of f as Ebeam 8 AGeV
•same occupancy as STAR!
preliminary
Measured phasespace densities
Mike Lisa, Quark Matter 2001 22E895 midrapidity
central collisions
•non-universal growth of f with collision energy
•f<1 no condensate
•low-pT saturation of f as Ebeam 8 AGeV
•same occupancy as STAR!
•Rough agreement with thermal Bose-Einstein
•high-pT excess @ high Eb
preliminary
Measured phasespace densities
Mike Lisa, Quark Matter 2001 23E895 midrapidity
central collisions
•non-universal growth of f with collision energy
•f<1 no condensate
•low-pT saturation of f as Ebeam 8 AGeV
•same occupancy as STAR!
•Rough agreement with thermal Bose-Einstein
•high-pT excess @ high Eb
•Better description by inclusion of radial flow[B. Tomasik, Ph.D. thesis]
•Substantial experimental & theoretical uncertainties
preliminaryalso see poster of D. Cebra
Measured phasespace densities
Mike Lisa, Quark Matter 2001 24E895
Baryon correlations
2 AGeV 4 AGeV 6 AGeVO 8 AGeV
k (GeV/c)0 0.4 0.8 0.12
0
0.6
0.8
1.0
1.2
0.2
0.4
C2
pp correlation function(central collisions, yycm)
• pp correlations ~ Ebeam independent
• another handle on baryon source?k (MeV/c)
0 20 40
0.8
0.2
0.6
0.4
1.0
1.2
1.6
1.4
1.0
1.2
1.8
C2
F. Wang & S. Pratt PRL 83 3139 (1999)
• p more sensitive than pp?• Correct p potential?
-p
p-p
Mike Lisa, Quark Matter 2001 25E895
Another E895 first: -p correlation function
•positive correlation observed
•qualitatively different shape than expected from Urbana p- potential
input to the particle physics
•work in progress… 100806040200
C(k
)
1.4
1.0
0.6
1.4
1.0
0.6
k (MeV/c)
Mike Lisa, Quark Matter 2001 26E895
Summary I•continuing to push the envelope…
•directed and elliptic flow excitation function•continue input to bulk parameterization
•strange particle flow•positive flow
• does not scale with proton flow (naïve 2/3 rule broken)
• potential important to describe flow
•strong antiflow of K0’s• strong, repulsive vector potential indicated
•Varying geometry (impact parameter): another handle
•increased x asymmetry larger p asymmetry
Mike Lisa, Quark Matter 2001 27E895
Summary II•azimuthally-sensitive HBT
• almond-shaped source, (~ entrance-channel geometry)• large positive spatial tilt angles• non-hydro nature of flow• coordinate-space structure of proton flow
•6-D phasespace density• non-universal growth of <f> with energy• saturation to “universal” behaviour at 8 AGeV• after 8 AGeV, increased yield pushed to high pT flow
• first p- signal observed• significant positive correlation• inconsistent with shape expected by Urbana potential
Mike Lisa, Quark Matter 2001 28E895
More E895 @ QM01
Production & Collective Behaviour of Strange Particles Parallel session today: Chris Pinkenburg
Phasespace Density & Source Charge DensityP063 Dan Cebra
Directed, Elliptic, Radial, & Longitudinal FlowP069 Jenn Klay
Azimuthally-sensitive HBT and the Tilt of the Source
P018 Ulrich Heinz*
* honorary E895 member
Mike Lisa, Quark Matter 2001 29E895
Pion and proton elliptic flow
• Ellitpic flow of both positive and negative pions follows the trends of the protons
W. C
askey,
DN
P98