why the current deuteron+au data from rhic are critical to decide if a qgp was formed in au+au
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Why the current Deuteron+Au data from RHIC are critical to decide if a QGP was formed in Au+Au. M. Gyulassy: BNL 3/8/03, LBNL 12/17/02. Two extremely different dynamical scenarios Claim to account for AA p T quenching Opaque QCD plasma leads to quenching - PowerPoint PPT PresentationTRANSCRIPT
BNL 3/6/03 Gyulassy 1
Why the current Deuteron+Au data from RHIC are critical to decide if a QGP was formed in
Au+Au
M. Gyulassy: BNL 3/8/03, LBNL 12/17/02
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AA RHIC Impass
Two extremely different dynamical scenarios Claim to account for AA pT quenching
1. Opaque QCD plasma leads to quenching and strong collective flow:=> AA provides info on equation of state
2. Transparent matter = No final state interactions But strong initial Wave function distortions CGC
=> eRHIC will provide precision measurements
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Pion Quenching at 200 AGeV
)
) (inelastic
ppT pp
2binary
TAA 2
eventsT AA
/ d /dp (d N
d /dp N d 1/Np R
PHENIX Preliminary
D. d’Enterria QM02
binary scaling
PHENIX
SPS – “Cronin” effect
RHIC – “Jet Quenching”
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• Jet Tomography via pions indicates that very high densityMatter was formed in Au+Au at 200 AGeV
• High pT Elliptic Flow consistent with highly opaque matter
The most powerfulProbe of the QCDEquation of state:
Mh dependence v2
• Kolb et al, Teany et al: Hydrodynamics of “soft” pT<2 GeV matter
•See R. Snellingsfor puzzling E dependence
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1. Nuclear Wavefunction a) pQCD: quark shadow, EMC; glue (anti?) shadow b) CGC : Saturated glue xGA< c Q2 R2 < A xGp
2. Initial State Interactions (Cronin)a) Glauber multiple collisions (target frame)b) None in CGC* (*KLMc flavor)
3. Final state Interactions a) dEg/dx , b) None in CGC*
Three Competing Nuclear EffectsIn A+A at RHIC
a/A a/pf (x,Q) A f (x,Q)¹
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What is CGC* prediction in 0.01< x < 0.1??
eA info on quark shadow EKS anti-shadow?
HIJING Q2 indepSuper Deep shadow ?
What is the Nuclear Parton Wave function?
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Cronin Initial State Interactions
Ivan Vitev, MG, PRL89 (02)
Alberto Accardi
Dumitru, Jalilian-Marian, Gelis
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Accardi, Treleani; GLV ; Wang
Kopeliovics et al; Dumitru,Gelis, Jalilian-Marian
Canonical Glauber Multiple Collision
Color Dipole Scattering
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QCD Bethe-Heitler
QGP Multiple Collision
Non-abelian Radiative Energy Loss
2 2
Lc 5fm
q Lc 2
E E 10GeV
E 60GeV
“Thick” Plasma Limit
Ivan Vitev NPB 595
gL / OpacityExpansion
“Thin” Plasma Limit
(1 x)ExE
g(1) 3s R 22
dN1L( )
R dy9
E CL
L4
2Eog
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to include medium induced energy loss
222 2 log(1 )
5^
^ ^= + +
pA pp
pk k L
ml
Intrinsic kT + Nuclear Cronin
EKS98 shadow/EMC SA
GRV98 pdf BKK ff
P() from GLV
GVW: PRL86(01)2537
geometry
Quenched pQCD Hadron Spectrum
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Single Hadron Tomography from SPS, RHIC, LHC
1. Cronin dominates at SPS
2. Cronin+Quench+Shadow
conspire to give ~ flat
R~Npart/Nbin at RHIC
dNg/dy ~ 1000 -> g ~100 0
3. Predicts sub Npart quench,
positive pT slope of R at LHC
and RLHC(40)~RRHIC(40)
Ivan Vitev and M.G, Phys.Rev.Lett. 89 (2002)
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Color Glass Model (KLMc flavor)
PHENIXAuAu(10%)=> hch
Claim no initial nor final state interaction canexplain quenching of charged pi+K+p due to saturation !
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Using gg g GLR formula
KLMc version of CGC
BNL 3/6/03 Gyulassy 150 5 10 15 20
0.0001
0.001
0.01
0.1
1
10
5 10 15 20
0.85
0.9
0.95
1.05
1.1
GLR with Classical Yang Mills
dNdyd2 k
µà0
1L dzz3
J0@kzDik1- ã14I-z2MQ2 LogB1Hz LL2Fy{2
k/Q
21/k
41/k
Q/
Teaser
BGdN / dN
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CGC dNg~1/pT4 tail and RHIC
p GeV^
2
dNdydp
p
^
pQCD (GRV,K=2,BKK)
g q g
CYM BKK+ ® p
0p 2=
0p 6=
CYM BKKpQCD(GRV BKK)
+ ®+ ®
pp
0p 2=
0p 6=
Large phenomenological modifications of CGC/GLRNeeded at RHIC because
Asymptotic Log1/x >>1, Log Qs/conditions are not reached at RHIC 0.01< x <0.1
p GeV^
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RHIC x>0.01 Large phenomenologicalModifications of CGC formulas required
2 2 2 2s s
4(x,p ) (p / Q (x)) (p / Q (x))(1 x)
s
2 2
0.3 0.52s
22
s42
s (1Q (x)
p(p /Q (x)) (p / )) x)Q (x
3) Neglect of q ~ g contributions, renormalize K
1)
2)
4) Ignore baryon anomaly and different quenching of pions
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d+Au essential to testwhich physical approximation
to Initial State Physics is closer to reality
This is the well learned lesson from J/Psi at SPS
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Jet Quenching
XN Wang, MG
Gluon Shadow
P0=2GeVBRAHMSPRL88(02)
No Cronin
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Shadow vs Cronin in d+Au : X.N. Wang
Old HIJING1… shadow
New HIJING2… shadow
Cronin only
dAuR (p )
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Ivan Vitev 03
Centrality Dependence Rapidity Dependence
Cronin systematics in D+Au at 200 AGeV
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GLR
Prediction of KLMc version of CGCfor d+Au
d Au Au AuR R 0.5 0.7
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Ivan Vitev 03
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Summary• Two extreme opposite interpretations of RHIC AA data exists
1. Evidence for opaque 100 x nuclear density matter2. Evidence for deep gluon shadowing (saturation)
• Ambiguity due to competition between initial nuclear wavefunction Shadowing, initial state (Cronin) interactions, and final state int.
as pointed out in 1992 p+A (or d+A) needed to isolate Initial State effects : shadowing and Cronin
• IF RHIC finds R(5 GeV) ~ 1.1-1.3 in d+Au , theninterpretation (1) QGP matter was produced in AA And RHIC AA Has chance to map out QCD EOS
• IF RHIC finds R(5 GeV)< 0.7 in d+Au , theninterpretation (2) and AA= shattered color glassNo QGP matter => go to eRHIC to map xGA.
• IF 0.7< R(5 GeV) < 1 ??? Back to the drawing board ???
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Phys.Rev.Lett.77 (96) 1222