Energy Dependence of ϕ -meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim...

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Energy Dependence of ϕ-meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim (for the STAR collaboration) NISER, Bhubaneswar, India Critical Point and Onset of Deconfinement 11 – 15 March 2013, Napa Outline: Motivation STAR Experiment Results Summary

Transcript of Energy Dependence of ϕ -meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim...

Page 1: Energy Dependence of ϕ -meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim (for the STAR collaboration) NISER, Bhubaneswar, India.

Energy Dependence of ϕ-meson Production and Elliptic Flow in Au+Au

Collisions at STAR

Md. Nasim(for the STAR collaboration)NISER, Bhubaneswar, India

Critical Point and Onset of Deconfinement11 – 15 March 2013, Napa Valley, USA

Outline: Motivation STAR Experiment Results Summary

Page 2: Energy Dependence of ϕ -meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim (for the STAR collaboration) NISER, Bhubaneswar, India.

Motivation

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LHC Experiments

The RHIC Beam Energy Scan (BES)

BES Motivations • Search for phase boundary• Search for Critical point

Observables of de-confinement a) Strange hadron dynamics

N(Ω)/N(ϕ) and RCP(ϕ)

b) Strange hadron collectivity

Elliptic flow (v2) of ϕ

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Page 3: Energy Dependence of ϕ -meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim (for the STAR collaboration) NISER, Bhubaneswar, India.

Why -meson ?

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J. Phys. G 36, 064022 (2009),

AMPT model

In the hadronic case, no number-of-quark scaling and v2() << v2 of hadrons

Phy

s. R

ev. C

79,

067

901

(200

9)P

hys.

Rev

. C 8

7, 0

1490

3 (2

013)

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STAR Collaboration : Nuclear Physics A 757 (2005)

Page 4: Energy Dependence of ϕ -meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim (for the STAR collaboration) NISER, Bhubaneswar, India.

STAR Experiment

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ToF ToF

BBC

PMD

EMC Barrel EMC End

Cap

TPCHLT

FTPC

√sNN (GeV)

Good MB events in Million

7.7 ~ 4 M

11.5 ~ 12 M

19.6 ~ 36 M

27 ~ 70 M

39 ~ 130 M

62.4 ~ 67 MdNev

t / (

Nev

t dN

ch)

Uncorrected Nch

Collisions: Au+Au

Collisions centrality from

uncorrected dNch/dη in |η| < 0.5

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Page 5: Energy Dependence of ϕ -meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim (for the STAR collaboration) NISER, Bhubaneswar, India.

Particle Identification and v2 measurement

method

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η-sub event plane method: STAR, Phys. Rev. C 77, 054901 (2008)3/13/13 CPOD 2013

Au+Au 39 GeV

|η| < 0.9

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ϕ-meson pT spectra

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• meson transverse momentum distribution can be well described by a

Levy function

STAR preliminary

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Statistical error

Page 7: Energy Dependence of ϕ -meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim (for the STAR collaboration) NISER, Bhubaneswar, India.

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RCP ≥ 1 at intermediate pT for

√sNN ≤ 19.6 GeV.→ no suppression

K0S RCP : 0-05%/40-60%

RCP: 0-10%/40-60% and 0-05%/40-60% for 200 GeV

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Nuclear Modification Factor (RCP)

Statistical error

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Strange Quark Dynamics

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Intermediate pT Ω/ϕ ratios: Indication of separation between ≥ 19.6 and 11.5 GeV. Derived strange quark pT distributions show a trend of separation between ≥ 19.6

and 11.5 GeV. Change of Ω production mechanism ? Parton recombination fails at 11.5 GeV ?

Hwa & Yang, Phys. Rev. C 75, 054904 (2007), Phys. Rev. C 78, 034907 (2008).

STAR preliminary

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STAR preliminary

Statistical + Systematic error

STAR preliminary STAR preliminary

Page 9: Energy Dependence of ϕ -meson Production and Elliptic Flow in Au+Au Collisions at STAR Md. Nasim (for the STAR collaboration) NISER, Bhubaneswar, India.

Strange Quark Collectivity

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• Mass: proton ~ • At low pT, v2()/v2(p) decreases with

decreasing beam energies→ Indicating less partonic

collectivity with decreasing beam energy.

STAR Collaboration: arXiv: 1301.2348 and arXiv:1301.2347, Phys. Rev C 87, 014903 (2013)

STAR preliminary

• Au+Au , √sNN = 200 GeV

• At low pT, v2()/v2(p) > 1.0→ strange quark collectivity comparable to light quark. → proton v2 possibly affected by

hadronic re-scattering.

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Statistical error only

Au+Au 200 GeV

Hydro + cascade

Phys

. Rev

. C 7

7, 0

4490

9 (2

008)

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NCQ scaling: ϕ-meson v2

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ϕ meson v2 deviates from other particles ~ 2σ at the highest pT data in 7.7 and 11.5 GeV collisions.

→ Small or zero v2 for ϕ meson implies hadronic interactions are more important at lower energies.

More data for 7.7 and 11.5 GeV are needed for clear conclusion.Ref: B. Mohanty and N. Xu: J. Phys. G 36, 064022(2009) and Md. Nasim, B. Mohanty, N. Xu , Phys. Rev C 87, 014903 (2013)STAR Collaboration: arXiv: 1301.2348 and arXiv:1301.2347 ( PRL in press)

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Statistical error only

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Summary

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STAR preliminary ϕ meson spectra and elliptic flow in Au+Au collisions at √sNN= 7.7-62.4 GeV have been presented.

RCP ≥ 1 at intermediate pT for √sNN ≤ 19.6 GeV. → No suppression.

Intermediate pT Ω/ϕ ratios and derived strange quark pT distribution show a indication of separation between ≥ 19.6 GeV and 11.5 GeV. → Suggests change of production mechanism. Indication of phase transition?

At low pT, v2()/v2(p) decreases with decreasing beam energies. → Indicating less partonic collectivity with decreasing beam energy. Top RHIC Energy (√sNN =200GeV): At low pT, v2()/v2(p) > 1.0 . → Could be the effect of hadronic re-scattering.

ϕ meson v2 deviates from other particles ~ 2σ at the highest pT data in 7.7 and 11.5 GeV collisions. → It may indicate hadronic interactions are more important at lower

energies. 3/13/13 CPOD 2013

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Back-Up

123/13/13 CPOD 2013

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ϕ and proton v2 v2(p)/v2(ϕ) > 1 ~ mass effect

< 1 ~ hadronic re-scattering effect

Hydro + cascadeHydro

T. Hirano et al. Phys. Rev. C 77, 044909 (2008)