event anisotropy measurement in high-energy heavy-ion collisions at rhic
DESCRIPTION
Event anisotropy measurement in high-energy heavy-ion collisions at RHIC ShinIchi Esumi Univ. of Tsukuba Contents flow measurements in PHENIX identified hadron v 2 - PowerPoint PPT PresentationTRANSCRIPT
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 1
Event anisotropy measurement in high-energy heavy-ion collisions at RHIC
ShinIchi Esumi Univ. of Tsukuba
Contents
(1) flow measurements in PHENIX(2) identified hadron v2
(3) charmed and photon v2
(4) relation of v2 and jets(5) azimuthal angle dependent HBT
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 2
Au+Au collisions in sqrt(sNN)=200GeV with
Relativistic Heavy Ion Collider (RHIC) at BNL
PHENIXmid-rapidity hadron/electron/ photon spectrometer
Forward-rapidity muon spectrometer
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 3
BBC/ZDC : centralityDch/PC1,2,3 : trackingTof : hadron PIDRich : electron PIDEmcal : electron/photon PID
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 4
Target
Projectile
b:impact parameter
Reacti
on pl
ane Reaction plane
initial geometryfinal momentum anisotropy
parton
parton
hadrons
A+A
p+pExperimentally, the R.P. is defined by the event anisotropy by itself, when one uses participants.
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 5
Reaction plan
e
x
y
Reaction plan
e
x
y
Σ wi*sin(2i) tan(22) =
Σ wi*cos(2i)
21
Σ wi*sin(i) tan(1) =
Σ wi*cos(i)
Reaction plane definition
plane with the directed moment
plane with the elliptic moment
(wi: 1 or pT or ET)
i
i
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reaction plane based analysis (geometrical origin / smeared by resolution)
dN / d(-true) = C (1 + 2vncos(n(-true))) : azimuthal angle for particles true (or meas.) : true (or measured) reaction plane angle vn
’ = <cos(n(-meas.))> : measured anisotropy parameter vn = <cos(n(-true))> = vn
’/R.P.: corrected anisotropy parameter R.P. = <cos(n(meas.-true))> : reaction plane resolution
pair wise correlation analysis (no resolution / larger non-flow effect)
Nreal () / Nmixed() = C (1 + 2vn2cos(n()))
ij
F() = A exp(-0.5( /width)2) + B (1+2v22cos(2))
Gauss term is to account for some of the non-flow contribution.
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 7
Beam-beam counter(BBC) ||=3~464pmts in each BBC charged particles
two central arms (CNT) ||<0.35Dch,PCs,TOF,EMCALtracking, momentum, PID
collision point
beam line
dNch
/d
-6 -3 0 3 6
Zero Degree CalorimeterShower-Max DetectorSpectator neutron energyBeam position
BBC
CNT
ZDC/SMD
MuonMuon arm +Silicon multiplicity(MVD) endcap
MVD
Reaction plane detectors in PHENIX
South North
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MIP calibration for each pmtRing gain correctionAverage sin/cos shift correctionremoving 4 special pmtsNormalized sumx/y distribution correctionConventional flattering (shifting angle) correction
Beam-Beamcounter
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Measurement with the MVD
• The MVD is currently configured as a silicon pad detector covering a 1.8<||<2.6 for collisions at z==0. Effective range (with vertex smearing) is 1.1<||<3.3 .
collisionvertex
• Geometry:Each end (North/South) has 12 wedges. Each wedge has 12 columns of 21 pads.
(6048 channels total)
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BBC
“Beam’s eye” view of ZDC
ZDC – Zero Degree CalorimeterBBC – Beam Beam CountersFHC – Forward Hadron Calorimeter
ZDC location in RHIC tunnel
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“Naked” ZDC module
Clear PPMA fibers
Tungsten absorber plates
Schematic of ZDC module assy
LED flasher
Scintillator strips
WLS fibers
16ch. PMT “M16”
Shower Maximum Detector (SMD)
ZeroDegreeCalorimeter (ZDC)
horizontal-strips
vertical-strips
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SMD1 (South) SMD2 (North)
Y (c
m)
X (cm) X (cm)
(X-CX)/X
(Y-C
Y)/
Y
(X-CX)/X
SMD1 SMD2
beam spot distribution
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SMD1vsSMD2BBC1vsBBC2 SMDvs BBC
BBC1vs
BBC2
back-to-back back-to-back spectator neutrons vss from participants are flowing opposite.
MVD1vs
MVD2 BBCvs
MVD
directed plane
elliptic plane
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mid-rapidity hadron, electron, and photon spectrometer
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STAR large acceptance hadron tracking chambersecondary vertex
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large acceptancewith full tracking
reaction plane method2 particle correlation method4th order cumulant method
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particleR.P. (rad)
beam linereaction plane
neutron spectatorcharged particles(pions) at mid
beam
pT cut
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PHOBOS : nucl-ex/0406021
PHENIX Preliminary
indication of v2 saturation at RHIC energy
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Thermal model with blast-wave
hydro is really good to be truth!!What will happen with resonances?
Resonance effects are important in single spectra, but not too much in v2, because of pT shift of heavy particles having smaller v2 and linear pT dependence of v2.
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 20
Phys
.Lett
. B59
7 (20
04) 3
28-33
2, X. D
ong e
t.al.
Phys
.Rev
. C70
(200
4) 02
4901
, V. G
reco e
t.al
Pion deviation is explained by resonance decays
pT shift is the dominant effect compared to the smearing given by the opening angle.
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stat. error onlysys. error <20% (62GeV) 15% (200GeV)
v 2 /n
quar
k
pT /nquark [GeV/c]
62.4 GeV Au+Au: preliminary
200 GeV Au+Au, charged ,K,p : PRL91, 182301 (2003)
0 : preliminary
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hydro + jet
quark coalescence
recombination + fragmentation
Data prefer “quark coalescence / recombination” based picture rather than “hydro + jet” picture at intermediate pT.
QGP
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minimum bias Au+Au at sNN = 200 GeV
PHENIX preliminary
some remainingmass ordering
PHENIX preliminary
quark + hadron flow
Tfo
early freeze-out
SPS
Similar effect from the time-difference is seen in v2
Almost NOmass ordering
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Hadronic cascade fails in magnitude (too small, it needs a big push from QGP), but it shows clear meson / baryon difference.
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hydro + jet
Jets dominate the high pT part of spectra.
recombination + fragmentation
PHENIX STAR
And they (jets) are suppressed.
v2
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Charm quarks are binary scaled (lower pT) or suppressed (high pT) w.r.t light quarks, but it could be enhanced and suppressed (looked like binary scaled). The v2 of charm would give a hint for the answer to the question.
Converter method Cocktail subtraction method
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PHENIX Preliminary
RAA (2.5<pT<5.0 GeV/c)
Nuc
lear
mod
ifica
tion
fact
or
Converter method
Cocktail subtraction method
pT (GeV/c)
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inclusive ee v2
charmed ee v2
If charm quarks also flow, charm quarks are thermalized and / or suppressed (interact with matter) similarly to the light quarks.
STAR SQM04
nucl-ex/0502009
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run2 Au+Au ~10 J/’sin PHENIX central arm (ee)
run4 Au+Au ~100 times in statisticscompared with run2
Single muon and muon pair in PHENIX muon arm …
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Inclusive Single
PHENIX Preliminary
Run2 AuAu 200 GeV
Direct photons are enhanced w.r.t. production, but it’s just because is suppressed, and the direct photons are in fact binary scaled.
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vertical bar : stat. errorcurves, gray box : sys. error
phenix preliminary
Note : Inclusive photon = including all of the decay effect from hadrons
phenix preliminary phenix preliminary
pT [GeV/c]
, 200 GeV Au+Au , 200 GeV Au+Au , 200 GeV Au+Au
Direct photons should not have any flow by definition, but …Alternatively ratio can be measured by assuming v2
=0.
The difference here and the ratio will give us a measure of direct v2.
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 32
STAR2
part
icle
cor
rela
tion
(v2 +
non
-flow
)The difference here is given by the real flow (v2).
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STAR : nucl-ex/0409033 non-flow reduced
v2{2}
v2{RP}
v2{4}STAR Preliminary
charged particle v2
v2{2}
v2{RP}
If jet suppression ends somewhere, should v2 go to zero?
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PHENIX Preliminary
Reac. plane v2 does have less non-flow because of the gap.Non-flow are removed in 2 part. corr. 2nd cumulant …
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recombination + fragmentation
semi-old STAR data
old STAR data
no jet-quenching
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phenix preliminary
}nucl-ex/0305013
Au+Au 200 GeV Au+Au 200 GeV
v2 reduction of charged particles in the previous page could be enlarged by the baryon/meson ratio.
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1<p T
(ass
ocia
te) <
1.5G
eV2.
5<p T
(ass
ocia
te) <
3GeV
hadron-hadron correlation (full pT reference)
(rad)
pure harmonic function fit
1.1
1.0
0.91.1
1.0
0.9
harmonic +near-side Gaussfunction fit
0. 0. 0.
harmonic +near-side +Far-side Gaussfunction fit
harmonic function fixed to themeasured v2
Au+Au 200GeV PHENIX preliminary
Another way to get the v2 : (v2)2 is given by the pair correlation
Ways to reduce the jet correlation with additional Gauss terms
A{1+2 (v2)2 cos(2)} + Gauss term
QM04
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4 < pT(trig.) < 6 GeV/c
Is the away-side jet-like?
Away-side looks jet like in p+p,but not in central Au+Au.
nucl-ex/0404010 0501016
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Associated particles pT distributions
0.15<pT(asso.)<4 GeV/c
nucl-ex/0501016
STAR preliminary
re-distributed lost energy 4 < pT(trig.) < 6 GeV/c0.15 < pT(asso.) < 4 GeV/c
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leading parton
hadrons
Q: Are jets source of v2?Q: Does reaction zone make flowing jets?
20-60%
STAR preliminary
20-60%
track1 - track2|
r.p.
in-plane pair
out-of-plane pair
in between
trigger particlein the selected angular window
Proof of the jet quenchingand the source of v2 at high pT
4 < pT(trig.) < 6 GeV/c 2 GeV/c< pT(asso.) < pT(trig.)
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trigger hadron pT>3GeV/c
hadron-hadron correlation
0<pT<1 1<pT<2 2<pT<5
0-20%
20-40%
40-90%
associated hadron pT window
in-planemiddleout-of-plane
Fitted line shape is given by :
with fixed(1)v2(trigger)(2)v2(associated)(3)R.P. resolution(4)in/out bin width (nucl-ex/0311007)
and one freenormalization parameter fit is done in a limited range shown
Au+Au 200GeV PHENIX preliminary
c(
) [ar
b. u
nit]
QM04
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 44
flow subtracted hadron-hadroncorrelation data
trigger hadron pT>3GeV/c
hadron-hadron correlation
0<pT<1 1<pT<2 2<pT<5
0-20%
20-40%
40-90%
associated hadron pT window
c(
) [ar
b. u
nit]
Au+Au 200GeV PHENIX preliminary
QM04
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 45photon-hadron correlation
associated hadron pT window
0<pT<1 1<pT<2 2<pT<5
0-20%
20-40%
40-90%
trigger photon pT>2GeV/c
in-planemiddleout-of-plane
Au+Au 200GeV PHENIX preliminary
c(
) [ar
b. u
nit]
Fitted line shape is given by :
with fixed(1)v2(trigger)(2)v2(associated)(3)R.P. resolution(4)in/out bin width (nucl-ex/0311007)
and one freenormalization parameter fit is done in a limited range shown
QM04
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associated hadron pT window
trigger photon pT>2GeV/c
photon-hadron correlation
0<pT<1 1<pT<2 2<pT<5
0-20%
20-40%
40-90%
flow subtracted photon-hadroncorrelation data
c(
) [ar
b. u
nit]
Au+Au 200GeV PHENIX preliminary
QM04
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 47
in-plane pairin between pairout-of-plane pair
h - h
0 0 (rad) (rad)
real
/mix
ed flow subtractedpT
trigger(h) > 3GeV/c1< pT
associated(h) <2GeV/c
three curves are fixed bymeasured v2 and resolution
coalescence of jet-fragmentation could be one of the source of v2
PHENIX preliminary PHENIX preliminary
flow subtractedpT
trigger() > 2GeV/c1< pT
associated(h) <2GeV/c
PHENIX preliminary
in-plane pairin between pairout-of-plane pair
- h
PHENIX preliminary
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• The correction for R.P was applied
• Sinyukov’s fit• Fitting by cos and s
in function
)2sin(RRR
)2cos(RRR
)2cos(RRR
)2cos(RRR
22,os
20,os
2os
22,l
20,l
2l
22,o
20,o
2o
22,s
20,s
2s
expected tendencies of sin or cos are seen !
A
B
In-plane
Out-Of-plane
Reaction Plane
Au Au
RsideRout
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– Rs,2/Rs,0, Ro,2/Rs,0 and Ros,2/Rs,0 are larger at mid-central than at central.– Ro,2/Rs,0 , Ros,2/Rs,0 seem to be larger than Rs,2/Rs,0
– Rl,2/Rl,0 and the difference (Ro,2/Rs,0 - Rs,2/Rs,0 ) seem to be possitive? – anisotropy in geometry or (maybe more) in time/expansion
geo. geo. + time
cross term (geo. + time)/geo.
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Summary
quark number scaling in v2 and Rcpquark degree of freedom / partonic flow
jet quenching / away side jet suppressionbinary scaling of direct photon / heavy quark?
chemical equilibrium in hadron yieldstrangeness saturation factor s ~ 1
thermal equilibrium in momentum spectralarge hadronic expansion and cooling
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STAR preliminary
RCP for and K0s in d-Au
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||ηη|<0.7|<0.7
preliminary
<Npart>
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d+Au, 40-100%
Au+Au, 0-5%
STAR preliminary
3 < pT(trig.) < 6 GeV/c2 < pT(asso.) < pT(trig.)
correlation width
correlated yield3 < pT(trig.) < 4 GeV/c2 < pT(asso.) < pT(trig.)
|| < 1.0
STAR preliminary
Seminor at LANL, 29/Mar/2005 ShinIchi Esumi, Univ. of Tsukuba 54
• Pairs are divided into 4 Δφbins (width=45degree)
q_ot
her<
40M
eV/c
qα(GeV/c)