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Strangeness production and Cronin effect in - PPT Presentation

d Au collisions at s NN 200 GeV in STAR Xianglei Zhu Tsinghua U UCLA For the STAR Collaboration 1 Motivation I Strangeness enhancement Strangeness enhancement in A A collisions at RHIC energy ID: 636344

effect star strangeness cronin star effect cronin strangeness enhancement central particle dependence data preliminary type k0s factor tpc collisions

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Slide1

Strangeness production and Cronin effect in d+Au collisions at √sNN = 200 GeV in STAR

Xianglei Zhu (Tsinghua U / UCLA)For the STAR Collaboration

1Slide2

Motivation I : Strangeness enhancementStrangeness enhancement in A+A collisions at RHIC energy, a

s a QGP signature (see. A. Timmins’ talk)d+Au strangeness data will connect peripheral A+A and p+p, supplying the baseline for the study of strangeness enhancement in the deconfined matter.

2

Redlich

, JPG27

Redlich&Tounsi

, 02

From A. TimminsSlide3

Motivation II : Cronin effect

Cronin effect in p+A, d+Au collision

[Cronin1975], seen in nuclear

m

odification

factor R

AA

or

R

CP

< 1 for

p

T < Px > 1 for pT > Px approach 1 again when pT →

3

p

q

h

A

Traditional

models

[

Accardi

hep

-ph/0212148]

:

Multiple

parton

/

hardon

scatterings in initial state

Recombination/Coalescence

:

[

Hwa&Yang

03, 04]

Final state effect, modification of hadronization

What is the mechanism of Cronin effect?

traditional models: do not explicitly predict particle type dependence, but centrality dependence.

final state models: predict particle species dependence of Cronin effect

Measurements of particle type and centrality dependence of Cronin effect seem helpful to understand the effect.Slide4

Cronin effect in d+Au STAR

4 Cronin effect seen with identified particle RdAu

For 2<pT

<5GeV/c, R

dAu

of proton seems higher than

pions

.

With topological reconstruction, strange hadrons have good PID up to high p

T! Suitable for the study of particle type dependence of Cronin effect.

STAR, PLB637, PLB616Slide5

OutlineK

0s, L, X spectra in most central

d+Au

200GeV

Strangeness enhancement in most central

d+Au

Baryon enhancement at intermediate

p

T

(

L

/ K

0s)Cronin effect, particle type dependence of RdAu in most central d+AuSummary5Slide6

STAR Run 08 d+Au Experiment Setup

Time Projection Chamber

Forward TPCs

Vertex Position Detector to confine primary vertex within ±30 cm, together with east ZDC as minimum bias trigger

No inner silicon detectors

pion

,

kaon

, proton and electron : identified using ionization energy loss

in TPC.

6Slide7

The data set

STAR Run 8 d+Au

200GeV Minimum Bias data

Event Selection:

|

VertexZ

| < 30cm

~

32

M

events after the cuts.

Centrality definition in

d+Au

:

Provided by uncorrected # of

charged particles @ east

Forward TPC

(

Au side, -3.8<

<-2.8),

refMult

’ in the

right plot

Currently, only the most central

(0-20%) events are well defined

by East FTPC.

7

STAR PreliminarySlide8

Strangeness reconstruction in STARStrange particles are reconstructed with their secondary TPC tracks through weak decay topology, thanks to TPC full

azimuthal coverage.

8

K

0

s

, |

y|<1

0.4 <pt<

0.6

Λ, |

y|<1

0.4 <pt< 0.6

Ξ

, |y

|<1

0.6 <pt<

1.0

STAR PreliminarySTAR Preliminary

STAR PreliminarySlide9

Spectra of K0s, Λ, Ξ

Λ(Λbar) corrected for weak decay feed-down from Ξ’sSpectra can be fitted with Levy function [Wilk&Wlodarczyk 00]

, low p

T

– exponential

high

p

T

– power law

fitting parameters:

percentage of

dN

/dy from extrapolation at low pT:K0s 10% ; Λ 17.5%; Ξ 29%9

d+Au 200 GeV

, 0-20%

dN

/

dyn

Tχ2/ndf

K0s

1.21±0.02

11.7±0.20.215±0.002

34.86/12Λ

0.402±0.00820.9±1.3

0.270±0.00510.81/10

Ξ0.058±0.003

14.0±1.30.275±0.011

3.52/5

STAR Preliminary

statistical error onlySlide10

Strangeness enhancement

Λ and K0s enhancement factor is almost the same in most central d+Au, lie in a trend with peripheral Cu+Cu and Au+AuΞ yield is consistent with that from most peripheral

Cu+Cu.strangeness enhancement factor is proportional to the strangeness content in

d+Au

too

10

dN

/

dy

/ <Npart> relative to pp

STAR Preliminary

statistical error only for

d+Au dataNumber of Participants NpartSlide11

Λ/K0s

Baryon enhancement at intermediate pT at STAR measured with Λ/K0sMost central

d+Au data is close to peripheral Au+Au

11

STAR Preliminary

p+p

data is from STAR PRC75Slide12

Nuclear modification factor RdAu

12STAR Preliminaryπ

,K,p

data is from STAR, PLB616, 637, statistical error only;

φ

data is from STAR arXiv:0809.4737;

p+p

K

0

s and

Λ

is from STAR PRC75

K0s agree with charged K at low pTΛ agrees with proton at intermediate pT (2 – 4GeV/c).Particle type (baryon/meson) dependence of RdAu for pT from 2.0 to 4 GeV/c; φ meson RdAu also falls into the meson band, for high statistical φ data, see C. Jena and X. Zhang’s postersSlide13

Summary

Measured productions for 3 identified particles(K0s

,

L

,

Ξ

) in most

central (0-20%)

d+Au

collisions at RHIC

Strangeness (

K

0s, L, Ξ) enhancement

in central

d+Au

.

Especially, we see

Ξ enhancement factor is also large in most central d+Au

L

/K

0

s

ratio

in

dAu

is close to

Au+Au

most peripheral (60-80%)

d+Au

Nuclear modification factor

seems

to show particle type (baryon/meson) difference (

K0s

,,φ vs. p, L), indicating that the hadronization scheme may have an impact on the Cronin effect13Slide14

backups14Slide15

Comparison of K0 to charged K spectraGood agreement of K0s

and charged K (from TPC dEdx) spectra at low pT.15

STAR PreliminarySlide16

RAA in low energy p+A collisions

s =27.4GeV

P.B Straub,PRL 68, 452(1992)

R

w/Be

in p+A collisions

W: tungsten Be: beryllium

s =38.8GeV

R

w/Be

:

Mesons

(2 quarks):

kaon and pion

~ 1.5;

Baryons

(3 quarks):

proton

~ 2.5

Particle-type dependence ??

~1.4

~1.5

~2.5

16