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Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

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Page 1: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Collective Flow in Heavy-Ion Collisions

Kirill Filimonov (LBNL)

Page 2: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

What is Flow in Heavy-Ion Collisions?

• Collective motion characterized by space-momentum correlation of dynamic origin

• Concept from Hydrodynamics: - hot and compressed matter

behaves like a compressible fluid

• axially symmetric radial flow• azimuthally anisotropic transverse flow

Types of Flow:

Page 3: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Collective Behavior in non-central Heavy Ion Collisions

b – impact parameter

Low energy heavy-ion collisions: E/A=25 MeV

Page 4: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Collective Behavior in non-central Heavy Ion Collisions

Relativistic heavy-ion collisions: E/A~0.4-10 GeV

b – impact parameter

“spectators”

“spectators”

“participants”

Page 5: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Collective Behavior in non-central Heavy Ion Collisions

Passage time: 2R/(βcmγcm)

“spectators”

“spectators”

“participants”

REACTION PLANE

• 15 fm/c at 1 GeV/nucleon• 5.4 fm/c at 10 GeV/nucleon• 1.4 fm/c at 160 GeV/nucleon

Page 6: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

View in transverse plane

TARGET PROJECTILE

Spectator blocking

x

y

Azimuthal anisotropy in momentum space (directed flow)

px

py

Page 7: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Directed (sideward) FlowExample: E877 (AGS, 11 AGeV)

<px> ≠0

px

py protons deuterons

Page 8: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Out-of-plane squeeze-out (spectator blocking)

x

y

Azimuthal anisotropy in momentum space (elliptic flow)

px

py

dN/d

-/2 0 /2

Page 9: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

In-plane elliptic flow (due to pressure gradient)

x

y

Azimuthal anisotropy in momentum space (elliptic flow)

px

py

dN/d

-/2 0 /2

Page 10: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Interplay of passage/expansion times

Passage time: 2R/(βcmγcm)Expansion time: R/cs cs=c√dp/dε - speed of sound

Page 11: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Sensitivity to nuclear EOSScience, Vol 298, Issue 5598, 1592-1596, 22 November 2002Determination of the Equation of State of Dense Matter Pawel Danielewicz, Roy Lacey, William G. Lynch

Directed Flow: Elliptic flow:

Page 12: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Elliptic flow at RHIC

b – impact parameter

“spectators”

“spectators”

Longitudinal and transverse expansion => no influence of spectator matter at midrapidity

Page 13: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Elliptic flow at RHIC

Reactionplane

In-planeOu

t-o

f-p

lan

e

Y

X

Re-interactions FLOW Re-interactions among what? Hadrons, partons or both?

In other words, what equation of state?

Flow

Flow

Page 14: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Azimuthal distributions at RHIC

STAR, PRL90 032301 (2003)

b ≈ 4 fm

“central” collisions

b ≈ 6.5 fm

midcentral collisions

Page 15: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Azimuthal distributions at RHIC

STAR, PRL90 032301 (2003)

b ≈ 4 fmb ≈ 6.5 fmb ≈ 10 fm

peripheral collisions

“v2”

Page 16: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

v2 Excitation Function

Rich structure

Transition from in-plane to out-of-plane and back to in-plane emission

Geometry effect in addition to (smooth?) change in pressure

Page 17: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

v2 vs Energy Density

Steady increase with energy density

Close to hydrodynamic limit for most central collisions at RHIC

Page 18: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Elliptic flow => sensitivity to early system

“Elliptic flow”

• evidence ofcollective motion

• sensitive to early pressure

• evidence for• early thermalization

• QGP in early stage

Hydrodynamiccalculation ofsystem evolution

Page 19: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Quark-number scaling

At intermediate pT v2 appears to depend on quark-number

For pT/n > 0.6 GeV/c, v2 scales with the number of quarks n, as predicted for hadron formation by quark coalescence

v2hadron (pT

hadron ) nv2quark (pT

quark )

pThadron npT

quark

Pions deviate: perhaps because they are goldstone bosons but also because of resonance decay contributions.

Page 20: Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)

Conclusions and Outlook

• Elliptic flow at RHIC => Evidence for early pressure

• First time hydro works in heavy ion collisions!

• Indications of re-interaction between constituent quarks

• Will charm flow at RHIC?