k*(892) resonance production in au+au and cu+cu collisions at s nn = 200 gev & 62.4 gev

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K*(892) Resonance Production in Au+Au and Cu+Cu Collisions at s NN = 200 GeV & 62.4 Ge Motivation Analysis and Results Summary 1 Sadhana Dash Institute of Physics, Bhubaneswar (For STAR Collaboration) Outline:

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K*(892) Resonance Production in Au+Au and Cu+Cu Collisions at  s NN = 200 GeV & 62.4 GeV. Motivation Analysis and Results Summary. 1. Sadhana Dash Institute of Physics, Bhubaneswar (For STAR Collaboration). Outline:. Features of K* Meson. Charged   - meson : - PowerPoint PPT Presentation

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Page 1: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

K*(892) Resonance Production in Au+Au and Cu+Cu Collisions at sNN = 200 GeV & 62.4 GeV

Motivation

Analysis and Results

Summary

1

Sadhana DashInstitute of Physics, Bhubaneswar

(For STAR Collaboration)

Outline:

Page 2: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

Neutral K* -meson :

Mass : 896.10 +/- 0.27 MeV Width : 50.70 +/- 0.60MeVDecay Modes : K ~ 100 %Decay Modes for present study K+

K-

BR ~ 66% ……….. Life time : ~ 4 fm Quark Structure : d s d s

Features of K* Meson

2

Charged -meson :

Mass : 891.66 +/- 0.26 MeV Width : 50.80 +/- 0.90 MeVDecay Modes : K ~ 100 %Decay Modes for present study K0

S

K0 S

BR ~ 23% ……….. Life time : ~ 4 fm Quark Structure : K*+ u s K*- u s

Page 3: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

Importance of K* studies

3

K*/, /K* information on interplay of rescattering and regeneration effects .

Modification in K* Mass , Width and pT

spectra in-medium dynamical effects

v2 and RCP

measurements of K* provide important information on its production mechanism in the hot/dense phase of heavy ion collisions.

K* lifetime ~4fm/c, sensitive to the properties of hot and dense medium created.

Page 4: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

K* thermally produced at the chemical freeze-out stage

K*lost

K

K*

K*

K K K*

reconstructed

Regeneration Effect compensatesagainst lost K* yield

Chemical freeze-out

Thermal freeze-out

K*

time

K*

K

Daughter particles’ Rescattering Effect destroys part of K* signal

K

Regeneration and Rescattering Effects

4

We study K*/K ratio in p+p and A+A collisions to understand rescattering effect.

K*

reconstructed

Page 5: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

5

STAR Time Projection Chamber was used to select kaons and pions.

STAR Experiment

STAR DATA (Run IV & V)Au+Au 62.4 GeV ~ 7e+6 eventsAu+Au 200 GeV ~ 13e+6 eventsCu+Cu 62.4 GeV ~ 10e+6 eventsCu+Cu 200 GeV ~ 8e+6 events

Page 6: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

The signal was obtained by subtracting the combinatorialbackground distribution (generated using mixed event technique) from the kaon-pion invariant mass distribution.

K* Invariant Mass Spectrum

0

02

02/4] Signal : Simple Breit-Wigner

6

Background : Linear functionM0 and Gamma

Phys. Rev. C 71 (2005) 064902

MinBiasMinBias

Page 7: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

K*0 Mass and Width Distribution

7

K* mass and width are consistent with PDG values

Page 8: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

Centrality Dependence of Transverse Mass Spectra

Exponential Fit function:

8

d2N dN/dy 2πmT dmTdy 2 πmT(m0+T)

1exp {-(mT-m0)/T}

Page 9: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

K*0 dN/dy and <pT>

The integrated yields of K* scale with charged particle multiplicityfor Au+Au and Cu+Cu collisions at 62.4 GeV and 200 GeV.

9

K* 200GeV (Run II) : Phys. Rev. C 71 (2005) 064902

No significant centrality dependence of <pT> for both Au+Au and Cu+Cu collisions at a given energy.

Page 10: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

There is a suppression of (K*/K-)A+A

/(K*/K-)p+p

ratio with centrality => rescattering effect predominates over regeneration . 10

Rescattering crosssection> 5 times the regeneration cross-section,

Phys. Rev.D 9, 1872(1974)

Particle Ratio (K*/K-)

Page 11: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

(/K*)

A+A/ (/K*)

p+p ratio increases with centrality favouring

rescattering effect: more K* are destroyed than regenerated.

Particle Ratio (Φ/K*)

11

Page 12: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

Nuclear Modification Factor

Baryon-meson effect is favored in particle production

12

Run IV

RCP

of K* is smaller than and K

S at lower p

T => strong

rescattering of daughter particles.

Page 13: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

K* v2

13

Scaled particle momentum elliptic flow is same for different species.

Number of quarks is found to be 2.0 +- 0.3 which implies hadronic regeneration process contributes little to the final observed K*

Phys. Rev Lett.92(2004)052302

Number of quarks from v2 scaling = 4 => K*regenerationPhys.Rev.C69 ,031902(2004)

Au+Au at 200 GeV

STAR Preliminary

Page 14: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

K*(896) resonance production has been measured at sNN=62.4 GeV and sNN=200 GeV in both Au+Au and Cu+ Cu collisions by STAR at RHIC.

Measurements of K*0/K and /K*0 ratio, v2, and K* R

CP at low pT are primarily

formed at hadronization.

K*0 integrated yield scales with dNch

/d in both Au+Au and Cu+Cu collision systems.

<pT> shows no significant centrality or system size dependence in Au+Au and Cu+Cu collisions.

Summary

14

Page 15: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV
Page 16: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

At intermediate pT , RCP measurements support

baryon -meson effect over mass effect of particle production .A non-zero K* elliptic flow v2 was measured in Au+Au collisions at 200 GeV .

At intermediate pT , the number of quark constituents is found to be 2.0+-0.3 which suppports quark recombination model of particle production.

Summary (contd)

15

Page 17: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV
Page 18: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

Typical Invariant Mass Spectrum

The signal was obtained by subtracting the combinatorialbackground distribution (through mixed event technique) from the kaon-pion invariant mass distribution.

0

02

02/4]

Fit function :

0

: K* width

0 : K*

massSTAR PRELIMINARY

Au+Au 62GeV

Signal : Simple Breit-Wigner

Background : Linear functionSTAR PRELIMINARY

18

STAR TPC was used to selectkaons and pions.

STAR DATA (Run IV & V)Au+Au 62.4 GeV ~ 7e+6 eventsAu+Au 200 GeV ~ 13e+6 eventsCu+Cu 62.4 GeV ~ 10e+6 eventsCu+Cu 200 GeV ~ 8e+6 eventsQM-08 Sadhana Dash Jaipur, Feb 04 - 10

Page 19: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV

K* <pT> in comparison with other species

19

Page 20: K*(892) Resonance Production in  Au+Au and   Cu+Cu  Collisions at   s NN  = 200 GeV & 62.4 GeV