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The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

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Page 1: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

The Re-Combinatorics of Thermal Quarks

LBNL School on

Twenty Years of Collective Expansion

Berkeley, 19-27 May 2005

Berndt Müller

Duke University

Page 2: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Re-Combinatorics of Thermal Quarks

• M. Asakawa• S.A. Bass• R.J. Fries• C. Nonaka

• PRL 90, 202303 • PRC 68, 044902• PLB 583, 73• PRC 69, 031902• PRL 94, 122301• PLB (in print)

Special thanks to: The Duke QCD theory group

Page 3: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Jet quenching seen in Au+Au, not in d+Au

PHENIX Data: Identified 0

d+Au

Au+Au

Page 4: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Suppression Pattern: Baryons vs. Mesons

What makes baryons different from mesons ?

…or what really came as a complete surprise…

Page 5: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Suppression: Baryons vs. mesons

baryons mesons

RC

P

pT (GeV/c)

behaves like meson ?

(also -meson)

Page 6: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Hadronization Mechanisms

qq

q

Baryon1

Meson

Fragmentation

q q

q q q

Baryon1

Meson

Recombination

M Q B Q2 3p p p p

Recombination was predicted in the 1980’s – Hwa, Ochiai, …

S. Voloshin

QM2002

Page 7: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Recombination is favored …

… for a thermal source

Baryons compete with mesons

Fragmentation wins out for a power law tail

Page 8: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Instead of a History ….

• Recombination as explanation for the “leading particle effect”:– K.P. Das & R.C. Hwa: Phys. Lett. B68, 459 (1977)

– Braaten, Jia, Mehen: Phys. Rev. Lett. 89, 122002 (2002)

• Fragmentation as recombination of fragmented partons:– R.C. Hwa, C.B. Yang, Phys. Rev. 024904 + 024905 (2004)

• Relativistic coalescence model– C.B. Dover, U.W. Heinz, E. Schnedermann, J. Zimanyi,

Phys. Rev. C44, 1636 (1991)

• Statistical recombination– ALCOR model (see T.S. Biro’s lecture)

• Quark recombination / coalescence– Greco, Ko, Levai, Chen, Rapp / Lin, Molnar / Duke group

– A. Majumder, E. Wang & X.N. Wang (in progress)

Page 9: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Recombination: The Concept

“fragmentation”

“recombination”REC

DER

1 2 p p P

“freeze-out”

Page 10: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Sudden recombination picture

q

qM

d

Transition time from QGP into vacuum (in rest frame of produced hadron) is:

/fT

md d

p

Not gradual coalescence from dilute system !!!

pT m

Allows to ignore complex dynamics in hadronization region; corrections O(m/pT)2

QGP

Page 11: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Tutorial: Non-Relativistic Recombination

Consider system of quarks and antiquarks (no gluons!) of volume V and phase-space distribution wa(p) = p,ap,a.

Quark-antiquark state vs. meson state:

1 1 2 2( )11 2

1

,

, ( )

i p x p x

iP RM

x p p V e

x P V r

Q

M e

11 22

1 2

( )

)

R x x

r x x

with

Probability for finding a meson with P and q = (p1-p2)/2 :3

2 231 2 1 22

(2 )ˆ, , ( ) ( )MQ p p M P P p p q

V

Number of produced mesons:3 2

3

3 3323 1 2

1 1 1 23 3 3

, ,(2 )

( ) ( ) , ,(2 ) (2 ) (2 )

M

abM a b

ab

d PN V M P M P

d p d pd PC V w p w p Q p p M P

Page 12: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Tutorial – page 2

3

21 12 23 3 3

ˆ ( )(2 ) (2 )

abMM a b M

ab

dN V d qC w P q w P q q

d P

The meson spectrum is given by:

Consider case P q, where q is of order M, and expand (for wa = wb):

21 1 1 1 1 1 12 2 2 2 2 2 2i j i j i j

ij

w P q w P q w P q q w P w P w P w P

Using only lowest order term:

3

2 221 12 23 3 3 3

ˆ ( )(2 ) (2 ) (2 )

MM M M

dN V d q VC w P q C w P

d P

Corrections are of order M2w/Pw = M

2/PT for thermal quarks.

Page 13: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Tutorial – page 3

The same for baryons:3

2 231 2 3 1 2 32

(2 )ˆ, , ( ) ( , )BQ p p p B P P p p p q s

V

where q, s are conjugate to internal coordinates

11 2 3 1 22 ( ) a d 'nr x x x r x x

The baryon spectrum is then:

3 321 1 1 1 1

3 2 3 2 33 3 3 3

3 2133

ˆ ( , )(2 ) (2 ) (2 )

1 ( / )(2 )

abcBM a b c B

abc

B B

dN V d q d sC w P q s w P q s w P q q s

d P

VC w P O PT

Page 14: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Tutorial - page 4

For a thermal Boltzmann distribution ( ) exp ( ) /w p E p T

we get

21 12 2

31 13 3

exp 2 / exp /

exp 3 / exp /

M

B

w P E P T E T

w P E P T E T

and therefore: 2( )1 ( / )

( )B B

M M

dN E CO PT

dN E C

Page 15: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Wigner function formulation

General formulation relies on Wigner functions:

1 2 2

3 31 21 1 1 1

1 1 2 2 1 1 2 2 1 2 1 22 2 2 2 3 3, , ( , ; , )

(2 ) (2 )p r p r

ab

d p d pr r r r r r r r e W r r p p

Meson number becomes:

3 33 3 3 1 1 1 1

2 2 2 23 3

*1 12 2

, ; ,(2 ) (2 )M ab

ab

iq rM M

d P d qN d Rd rd r W R r R r P q P q

e r r r r

Relativistic generalization (u = time-like normal of volume):

3 3 3P ud P d R d Pd

E

Page 16: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Relativistic formulation

2M

M3 3,

2B

B3 3, ,

( , ) ( , (1 ) ) ( )(2 )

' ( , ) ( , ' ) ( , (1 ') ) ( , ')(2 )

dN P uE d dxw R xP w R x P x

d P

dN P uE d dxdx w R xP w R x P w R x x P x x

d p

Relativistic formulation using hadron light-cone frame (P = P):

For a thermal distribution,

the hadron wavefunctions can be integrated out, eliminating the model dependence of predictions. This is true even if higher Fock space states are included!

( , ) exp( v / ) w r p p T

0

3 2 012

with and

k

d k dk d k k k k k xPk

Page 17: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Beyond the lowest Fock state1

2 21

0

12

2

0

; ( 1) ( , ; ) ( ) ( )

( 1) ( , , ; ) ( ) ( ) ( )

a b a b a b a b

a b c a b c a b c a b c

M Q dx dx x x x x Q q x q x

dx dx dx x x x x x x Q q x q x g x

12

2

0

12/

2

0

( ) ( ) (( 1) ( , , )

( , ,1 )

)q a qqqg a b c a b c a b c

P Ta b a b a b

a g cW dx dx dx x x x x x x

e

w x w x w

dx dx x x x x

x

/ / / ( ) /a b c a b cx P T x P T x P T x x x P Te e e e

1 12 2/

1 2

0

/

0

( ,1 ) ( , ,1 )P Tqq qqg a a

P Tb a b a a bM bW W e dx x x dx dx x x x xW e

12

1

0

1 12 2/

1 1

0 0

( 1) ( , )

( )

( ) ( ) ( ) ( )

( 1) ( , ) ( ,( ) 1 )

qq a b a b a b a b a b

P Ta b q a q aa b a b a a aw x w x

W dx dx x x x x q x q x q x q x

dx dx x x x x e dx x x

/ / ( ) /a b a bx P T x P T x x P Te e e For thermal medium

Page 18: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Statistical model vs. recombination

3

1

3

3 exp / 12

with

B s

i

ii i i iI

id NE P d

df P u

gf P u P u B S I T

P

In the stat. model, the hadron distribution at freeze-out is given by:

For pt , hadron ratios in SM are identical to those in recombination!

(only determined by hadron degeneracy factors & chem. pot.) recombination provides microscopic basis for apparent chemical equilibrium among hadrons at large pt BUT: Elliptic flow pattern is approximately additive in valence quarks, reflecting partonic, rather than hadronic origin of flow.

Page 19: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Recombination vs. Fragmentation

1h 1

h3 3 30

( , ) ( )(2 ) z

dN P u dzE d w r P D z

d P z

Fragmentation:

…always wins over fragmentation for an exponential spectrum (z<1):

… but loses at large pT, where the spectrum is a power law ~ (pT) -b

ee xxp p(v / )) v /( PP zTT

Recombination…

( , ) ( , (1 ) ) exp v /

( , ) ( , ' ) ( , (1 ') ) exp v /

w r xP w r x P P T

w r xP w r x P w r x x P P T

Meson

Baryon

2M

M3 3,

( , ) ( , (1 ) ) ( )(2 )

dN P uE d dxw R xP w R x P x

d P

Recombination:

Page 20: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Model fit to hadron spectrum

Teff = 350 MeV blue-shifted temperature

pQCD spectrum shifted by 2.2 GeV

R.J. Fries, BM, C. Nonaka, S.A. Bass (PRL )

Corresponds to ≥ 0.6 !!!

Recall:

G 0.5 ln(…)

Q 0.25 ln(…)

Page 21: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Hadron Spectra I For more details – see S.A. Bass’ talk tomorrow

Page 22: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Hadron Spectra II

Page 23: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Hadron dependence of high-pt suppression

• R+F model describes different RAA behavior of protons and pions

• Jet-quenching becomes universal in the fragmentation region

Page 24: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Hadron production at the LHC

r = 0.75

r = 0.85

r = 0,65

R.J. Fries

includes parton energy loss

Page 25: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Conclusions (1)

• Evidence for dominance of hadronization by quark recombination from a thermal, deconfined phase comes from:

– Large baryon/meson ratios at moderately large pT;

– Compatibility of measured abundances with statistical model predictions at rather large pT;

– Collective radial flow still visible at large pT.

• -meson is an excellent test case (if not from KK).

Page 26: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Parton Number Scaling of Elliptic Flow

In the recombination regime, meson and baryon v2 can be obtained from the parton v2 (using xi = 1/n):

3

2

2 2

2

2

22

2

2

3v 32v2

v

1 2 v

v3 3

v

1 6 v32

and

p pt t

B

p t

Mt t

p tp t

p p

p

p

pp p

Neglecting quadratic and cubic terms, a simple scaling law holds:

2 2 2 2an vv23

vd2

v 3M B ptt

tp tpp

pp

Originally poposed by S. Voloshin

Page 27: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Hadron v2 reflects quark flow !

Page 28: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Higher Fock states don’t spoil the fun

1 2

1 2

M C qq C qqg

B C qqq C qqqg

2

2

( )1

( ) 22

( )1

( ) 22

( , , )

( , ,

(

,

, )

( , , )

)

Ba b c a b c

Ba b c g

Ma b a b

Ma b g

a b c g

a b g

x x x

x x x x

x x x x x

x x x

x x x x x x x x

x

Page 29: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Conclusions (2)

• Recombination model works nicely for v2(p):

– v2(pT) curves for different hadrons collapse to universal curve for constituent quarks;

– Saturation value of v2 for large pT is universal for quarks and agrees with expectations from anisotropic energy loss;

– Vector mesons (, K*) permit test for influence of mass versus constituent number (but note the effects of hadronic rescattering on resonances!);

– Higher Fock space components can be accommodated.

Page 30: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Enough of the Successes…

Give us some Challenges!

Page 31: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Dihadron correlations

Data: A. Sickles et al. (PHENIX) Hadrons created by reco from a thermal medium should not be correlated.

But jet-like correlations between hadrons persist in the momentum range (pT 4 GeV/c) where recombination is thought to dominate!

( STAR + PHENIX data)

Page 32: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Hadron-hadron correlations

Near-side dihadron correlations are larger than in d+Au !!!

Far-side correlations disappear for central collisions.

d+Au

A. Sickles et al. (PHENIX)

Page 33: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Sources of correlations

• Standard fragmentation

• Fragmentation followed by recombination with medium particles

• Recombination from (incompletely) thermalized, correlated medium

• But how to explain the baryon excess?

• “Soft-hard” recombi-nation (Hwa & Yang). Requires microscopic fragmentation picture

• Requires assumptions about two-body cor-relations (Fries et al.)

Page 34: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

How serious is this?

• Original recombination model is based on the assumption of a one-body quark density. Two-hadron correlations are determined by quark correlations, which are not included in pure thermal model.

• Two- and multi-quark correlations are a natural result of jet quenching by energy loss of fast partons.

• Incorporation of quark correlations is straightforward, but introduces new parameters: C(p1, p2).

Page 35: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Diparton correlations

• Parton correlations naturally translate into hadron correlations.

• Parton correlations likely to exist even in the "thermal" regime, created as the result of stopping of suprathermal partons.

A plausible explanation?

Two-point velocity correlations among 1-2 GeV/c hadrons

away-side same-side

T. Trainor

Page 36: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Dihadron formation mechanisms

(1 )

( )(1 )

A Aa

A A A

A BA

A A

dz Pg E

z z z

z PD

F

z

F

z DP

12

1eff2

( )

exp2

a A B

A B

A B

g P P E

P PD

P P

S F

T

H

eff

exp A BSSP

TS

PS

A

A

A

B

B

B

Page 37: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Correlations - formalism

222211114

2

2

2

123

13

6

2

23

13 2

1,

2

1,

2

1,

2

1)()(

)2(qPqPqPqPWqqqdqd

V

PdPd

dNMM

Di-meson production:

)(),,( 1 in

nn pwppW 1 ,qq i ji j

C p p

Partons with pairwise

correlations2

2 21 2 0 1 23 3 6

1 2

1 1 1 11 2 4 ,

(2 ) 2 2 2 2MM

qq

dN Vw P w P C C P P

d Pd P

Meson-meson, baryon-baryon, baryon-meson correlations

9 , 6 , 4BB qq MB qq MM qqC C C C C C

First results of model studies are encouraging →

Page 38: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Dihadron correlations - results

Meson triggers Baryon triggers

by 100/Npart

Fixed correlation

volume

Page 39: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Comparison with Data

R.J. Fries, S.A. Bass, BM, nucl-th/0407102, acct’d in PRL

Page 40: The Re-Combinatorics of Thermal Quarks LBNL School on Twenty Years of Collective Expansion Berkeley, 19-27 May 2005 Berndt Müller Duke University

Conclusions – at last!

Evidence for the formation of a deconfined phase of QCD matter at RHIC:

Hadrons are emitted in universal equilibrium abundances;

Most hadrons are produced by recombination of quarks;

Hadrons show evidence of collective flow (v0 and v2);

Flow pattern (v2) is not universal for hadrons, but universal for the (constituent) quarks.

Hadron correlations from quasithermal quark correlations.