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Multi-strange Hadron v2 and Partonic Collectivity

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Presentation on theme: "Multi-strange Hadron v2 and Partonic Collectivity"— Presentation transcript:

1 Multi-strange Hadron v2 and Partonic Collectivity
Markus Oldenburg Lawrence Berkeley National Laboratory STAR Heavy Flavor Workshop October 13−15, 2005 M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

2 STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL
Overview Motivation on why to measure v2 of multi-strange hadrons Analysis details and technique Data and results Discussion Conclusion Outlook: from multi-strange to heavy flavor M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

3 Timeline of a heavy-ion collision
hadronization Ξ, ,  hadronic stage , K, p direct photons initial collisions hard scatterings, jet production partonic stage thermal photons Time by S. Bass M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

4 Flow of strange hadrons
(GeV) freeze-out of multi-strange hadrons - at higher temperature Tfo - with lower collective velocity T small cross section of strange hadrons with non-strange hadrons sensitivity to the early, partonic stage STAR: Nucl. Phys. A715, 458c (2003) Phys. Rev. Lett. 92, (2004) Phys. Rev. Lett. 92, (2004) M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

5 STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL
Importance of  v2 STAR: Phys. Rev. C65, (R) (‘02) Phys. Lett. B612, 181 (2005) Kaon coalescence effectively ruled out as a dominant channel for  production at these energies.  is a true signal from the early stage of the collision! anisotropic flow measurement of  will conclude: type of the system at an early stage partonic vs. hadronic origin of observed scaling at intermediate pT mass vs. particle type M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

6 STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL
Elliptic flow v2 x z y px py y x non-central collisions: azimuthal anisotropy in coordinate-space interactions  asymmetry in momentum-space sensitive to early time in the system’s evolution Measurement: Fourier expansion of the azimuthal pT distribution M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

7 STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL
Dataset system: Au+Au collisions energy: sNN = 200 GeV event sample: ~11 M events centrality: 0–80 % event plane resolution ~75 % correction: M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

8 Particle identification and mass spectra
identified via decay topology:  K+ + K- background estimation by event mixing > 10,000,000 particles identified Ξ- and (anti- Ξ)+ identified via decay topology: Ξ  Λ +  and Λ  p +  background estimated by rotating the Λ by 180° in the transverse plane > 450,000 particles identified Ω- and (anti-Ω)+ identified via decay topology:   Λ + K and   p +  background estimated by rotating the Λ by 180° in the transverse plane > 13,000 particles identified  results by Sarah Blyth M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

9 New analysis technique
analysis method: v2 vs. minv motivated by Borghini et al. [nucl-th/ ] advantages over standard method: only one fit per pT bin smaller systematic uncertainties new method used for K0S, Λ, Ξ, , and  analysis standard method and v2 vs. minv method give consistent results SIG + BG BG BG (SIG+BG) SIG (SIG+BG) v2TOT(minv) M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

10 v2 of multi-strange hadrons
_ common fit to K and Λ n = number of constituent quarks [X. Dong et al., Phys. Lett. B597 (2004)] v2 Ξ+Ξ Ω+Ω _ baryons mesons pT/n > 0.75 GeV/c 2/ndf for NCQ=2 2/ndf for NCQ=3 Ξ+Ξ 82.7/6 27.4/6 Ω+Ω 4.1/3 2.1/3 2.0/5 7.4/5 _ 200 GeV Au+Au _  results by Sarah Blyth M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

11 Discussion of strange hadron v2 results
K0S and Λ results by Yan Lu STAR preliminary  results by Sarah Blyth Hydro: P. Huovinen, priv. comm. (2004) The strange baryons Ξ and Ω show strong elliptic flow. The Ξ v2 clearly follows the baryon v2(pT).  flows as strongly as other mesons. Collective flow is generated during the partonic stage already. M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

12 Conclusions from the measurements
v2 of multi-strange hadrons: , Ξ, and  show strong elliptic flow. Their behavior is similar to the other mesons and baryons. They flow as strongly as the other particles. NCQ scaling of v2 : observed scaling is a meson↔baryon, not a mass effect! Collectivity develops early among partons! = Partonic Collectivity at RHIC Thermalization? M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

13 Timeline of a heavy-ion collision
production of heavy quarks hadronization Ξ, ,  hadronic stage , K, p direct photons initial collisions hard scatterings, jet production partonic stage thermal photons Time by S. Bass M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL

14 STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL
Heavy-Flavor Quarks B. Mueller, nucl-th/ Mass (MeV/c2) 106 105 104 103 102 10 1 Even in a QGP with chiral restoration, the c, b (and t) quarks stay heavy. If charm quarks show collective behavior (= flow) the must have suffered frequent interactions with the light quarks u, d, s. The light quarks u, d, s must be thermalized. M. Oldenburg STAR Heavy Flavor Workshop — October 13–15, 2005, LBNL


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