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Sonia Kabana SUBATECH, Nantes, France for the STAR Collaboration “Excited QCD 2010”, Slovakia Selected highlights from the STAR experiment at RHIC.

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Presentation on theme: "Sonia Kabana SUBATECH, Nantes, France for the STAR Collaboration “Excited QCD 2010”, Slovakia Selected highlights from the STAR experiment at RHIC."— Presentation transcript:

1 Sonia Kabana SUBATECH, Nantes, France for the STAR Collaboration “Excited QCD 2010”, Slovakia Selected highlights from the STAR experiment at RHIC

2 2 Sonia KabanaExcited QCD 2010 o Introduction and experimental set up o Strangeness and elliptic flow o (Anti-)hypertriton o Low energy scan o Future plans for spectroscopy with STAR o Summary and Outlook Outline

3 3 Sonia KabanaExcited QCD 2010 Introduction Heavy Ion collisions: exploring the QCD phases Formation of sQGP in central Au+Au collisions at sqrt(s)=200 GeV at RHIC Initial Bjorken energy density ~5 GeV/fm^3

4 4 Sonia KabanaExcited QCD 2010 RHIC BRAHMS PHOBOS PHENIX STAR AGS TANDEMS Animation M. Lisa Relativistic Heavy Ion Collider (RHIC)

5 5 Sonia KabanaExcited QCD 2010 STAR-TPC: NIMA 499 (2003) 659 STAR-detector: NIMA 499 (2003) 624 STAR Detector

6 6 Sonia KabanaExcited QCD 2010 MRPC ToF barrel BBC PMD FPD FMSFMS EMC barrel EMC End Cap DAQ1000 FGT Completed Ongoing MTD R&D HFT TPC FHC HLT STAR Detector

7 7 Sonia KabanaExcited QCD 2010 Strangeness and elliptic flow

8 8 Sonia KabanaExcited QCD 2010 Strangeness Production versus N(part)  Strange hadrons are enhanced relative to p+p  Relative enhancement seems to be slightly lower than in SPS for baryons, similar for anti- and higher for anti-.  Strangeness content “hierarchy”  Proposed to be linked to canonical suppression in p+p (e.g. J. Cleymans, A Muronga, Phys. Lett. B 388 (1996) 5). 8 STAR Collaboration, nucl-ex/0809.0823 Rich set of strange particle measurements at STAR. M Munhoz, SQM2009

9 9 Sonia KabanaExcited QCD 2010 Phi meson enhancement Phi meson enhancement indicates that strangeness enhancement is not due to canonical suppression. More enhancement seen at higher energy Phi enhancement does not follow enhancement hierarchy with number of s-quarks. STAR Coll., Phys. Lett. B 673 (2009) 183  strange quark enhancement in dense partonic medium formed in HI collisions - Not a baryon-meson effect, not mass effect. - “Corona” effect ? (J. Aichelin, K. Werner, arXiv:0810.4465, F. Becattini, J. Manninen, arXiv:0811.376.)

10 10 Sonia KabanaExcited QCD 2010 R. J. Fries et al, Phys. Rev., C68:044902, 2003 R. C. Hwa and C. B. Yang, Phys. Rev., C67:034902, 2003 V. Greco et al, Phys. Rev. Lett., 90:202302,2003. STAR Collaboration, J. Phys. G34, S933-936, 2007 Baryon to meson ratio Baryons are more abundantly produced than mesons at intermediate p T in Au+Au collisions at √s NN = 200 GeV ▫p/ π, Λ /K s 0, Ω / Φ This behavior can be qualitatively reproduced by models that assume the coalescence of partons M Munhoz, SQM2009

11 11 Sonia KabanaExcited QCD 2010 Azimuthal Anisotropy: Elliptic Flow Almond shape overlap region in coordinate space Anisotropy in momentum space Interactions/ Rescattering Important tool to probe the early stages of the collision dynamics

12 12 Sonia KabanaExcited QCD 2010 Elliptic Flow and Strangeness - Elliptic flow: reveal the early stage collision dynamics Good probe of the early medium Look at particle type dependence (K s 0, Λ, Ξ ) Low hadronic interaction ( Ω, ): probe partonic collectivity 12 partonic hadronic J/ Ψ, D , Ω, Ξ, Λ, K S 0 , K, p

13 13 Sonia KabanaExcited QCD 2010 No of quarks scaling of v 2 in Au+Au collisions  Hydro approach reproduces mass ordering  v 2 of strange hadrons shows baryon-meson difference. v2/n q scaling-> suggests coalescence/recombination scheme for hadronization of bulk partonic matter at low pT. v2 build up at partonic level Indications of a different behavior for higher p T 13 Hydro: P. Huovinen and P. V. Ruuskanen, Annu. Rev. Nucl. Part. Sci. 56, 163 (2006) M Munhoz, SQM2009 STAR preliminary

14 14 Sonia KabanaExcited QCD 2010 Elliptic Flow of Ω and  14  Ω and : low hadronic interaction --> partonic flow STAR preliminary PHENIX: nucl-ex/0604011v1 M Munhoz, SQM2009

15 15 Sonia KabanaExcited QCD 2010 Ideal hydrodynamic limit N. Li poster QM09. STAR preliminary Borghini & Ollitrault, PLB 642(2006)227 Au+Au 200 GeV 0 – 80% v 4 /v 2 2 results suggest that ideal hydro limit is not reached

16 16 Sonia KabanaExcited QCD 2010 Partial summary : flow, strangeness Elliptic flow develops early at partonic level - low pT (v2/n_q scaling) Hydrodynamics applicable in bulk - low pT (v2 vs pT) Ideal hydrodynamic limit not reached (v4/v2^2) Deviation from n_q scaling seen at high pT Quark coalescence/recombination dominant hadron production mechanism in heavy ion collisions at RHIC in the bulk - low pT (v2/n_q scaling, baryon/meson ratios)

17 17 Sonia KabanaExcited QCD 2010 (Anti-)hypertriton discovery

18 18 Sonia KabanaExcited QCD 2010 S=-1 S=-2 S=-0 Hypertriton: hypernucleus with lowest A Never observed before Observation of antihypertriton at RHIC

19 19 Sonia KabanaExcited QCD 2010 Observation of (anti)hypertriton Hypernuclei: ideal lab for YN and YY interaction – Baryon-baryon interaction with strangeness sector – Input for theory describing the nature of neutron stars No anti-hypernuclei have ever been observed up to now Coalescence mechanism for production: depends on overlapping wave functions of Y+N at final stage Anti-hypernuclei and hypernuclei ratios: sensitive to anti- matter and matter profiles in HIC – Extension of the nuclear chart into anti-matter with S [1] [1] W. Greiner, Int. J. Mod. Phys. E 5 (1995) 1 Jin Hui Chen QM09 and HypX 2009, Zhangbu Xu, RHIC-AGS meeting june 2009.

20 20 Sonia KabanaExcited QCD 2010 3  H mesonic decay, m=2.991 GeV, B.R. 0.25; Data-set used, Au+Au 200 GeV ~67M year 2007 minimum-bias ~22M year 2004 minimum-bias ~23M year 2004 central, |V Z |<30cm Tracks level: standard STAR quality cuts, i.e., not near edges of acceptance, good momentum & dE/dx resolution. Secondary vertex finding technique DCA of v0 to PV < 1.2 cm DCA of p to PV > 0.8 cm DCA of p to 3 He < 1.0 cm Decay length > 2.4 cm QM09 proceeding: arXiv:0907.4147 Data-set and track selection Jin Hui Chen QM09 and HypX 2009, Zhangbu Xu, RHIC-AGS meeting june 2009.

21 21 Sonia KabanaExcited QCD 2010 Select pure 3 He sample: 3 He: 5810 counts anti- 3 He: 2168 counts condition: -0.2 2 GeV/c… Theory curve: Phys. Lett. B 667 (2008) 1 3 He & anti- 3 He selection Jin Hui Chen QM09 and HypX 2009, Zhangbu Xu, RHIC-AGS meeting june 2009.

22 22 Sonia KabanaExcited QCD 2010 Signal observed from the data (bin-by-bin counting): 157±30; Mass: 2.989±0.001±0.002 GeV; Width (fixed): 0.0025 GeV. Projection on anti-hypertriton yield: =157*2168/5810= 59±11 Hypertriton inv. mass Jin Hui Chen QM09 and HypX 2009, Zhangbu Xu, RHIC-AGS meeting june 2009.

23 23 Sonia KabanaExcited QCD 2010 Signal observed from the data (bin-by-bin counting): 70±17; Mass: 2.991±0.001±0.002 GeV; Width (fixed): 0.0025 GeV. Antihypertriton inv. mass Jin Hui Chen QM09 and HypX 2009, Zhangbu Xu, RHIC-AGS meeting june 2009.

24 24 Sonia KabanaExcited QCD 2010 Combined hyperT and anti-hyperT signal : 225±35; It provides a >6  significance for discovery. Hypertriton+Antihypertriton inv. mass Jin Hui Chen QM09 and HypX 2009, Zhangbu Xu, RHIC-AGS meeting june 2009.

25 25 Sonia KabanaExcited QCD 2010 Measurement of the lifetime ps We measure   = 267±5 ps PDG value is   = 263±2 ps PDG: Phys. Lett. B 667 (2008) 1 Jin Hui Chen QM09 and HypX 2009, Zhangbu Xu, RHIC-AGS meeting june 2009.

26 26 Sonia KabanaExcited QCD 2010 Production rate Antiparticle/particle ratios favor coalescence Coalescence => 0.45 ~ 0.77*0.77*0.77 Jin Hui Chen QM09 and HypX 2009, Zhangbu Xu, RHIC-AGS meeting june 2009.

27 27 Sonia KabanaExcited QCD 2010 The measured lifetime is ps, consistent with free  lifetime (263 ps) within uncertainty. Consistency check has been done on hypertriton analysis; 157 candidates, with significance better than 5  Antihypertriton has been observed for first time; 70 candidates, with significance ~4 . The antihypertriton/hypertriton ratio is measured to be 0.49±0.18±0.07, and anti- 3 He / 3 He is 0.45±0.02 ±0.04, favoring coalescence. Summary : (anti)-hypertriton Jin Hui Chen QM09 and HypX 2009, Zhangbu Xu, RHIC-AGS meeting june 2009.

28 28 Sonia KabanaExcited QCD 2010 Lifetime: –data samples with larger statistics (~factor 10 more within a few years) 3  H  d+p+  channel measurement: d-identification via ToF. Search for other hypernucleus: 4  H, 4  He, 4  H, 3  H, Search for anti-   RHIC: best antimatter machine ever built AGS-E906, Phys. Rev. Lett. 87, 132504 (2001) Outlook - anti-(hyper)-nuclei

29 29 Sonia KabanaExcited QCD 2010 Future plans for spectroscopy with STAR at RHIC J. H. Lee, Hadron 2009 Search for glueball production in Double Pomeron Exchange processes - Roman Pots (used for pp2pp exp. at RHIC) for forward proton tagging - rapidity gap > 4 units for M_X < 3 GeV - polarized p+p collisions p1 p2 -> p1’ M_X p’2 M_X centrally produced Search for gb candidates in M_X M_X (1-3 GeV) --> pi+pi-, pi+pi-pi+pi-, K+K- Acceptance for decay pions from M-X -> pi+pi-pi+pi-

30 30 Sonia KabanaExcited QCD 2010 Low energy scan

31 31 Sonia KabanaExcited QCD 2010 Critical point search Key idea: study Phase Diagram throughout energy scan region Low energy scan happening this year ! Measurement of direct signatures of the critical point e.g. fluctuations Turn off sQGP signatures already established at RHIC

32 32 Sonia KabanaExcited QCD 2010 Pparticle ratios, v 2 and HBT results are comparable to SPS results at a similar energy. Unambiguous beam+beam events 4 hours and 40 minutes in year 2008: ~3000 good events (good≡ primary vertex along beam and within acceptance) STAR preliminary L. Kumar QM09 Energy scan: 9.2 GeV STAR coll., arXiv:0909.4131, acc. for publication in PRC

33 33 Sonia KabanaExcited QCD 2010 Summary Elliptic flow, B/M ratios, strangeness suggest --> Parton coalescence as dominant mechanism for hadron production in the bulk First observation ever of anti-hypertriton in Au+Au collisions at sqrt(s)=200 GeV. Data suggest production through coalescence. RHIC: best antimatter machine ever built Low  b, high number and energy density of partons at top RHIC energy --> RHIC: a unique source of exotics ?

34 34 Sonia KabanaExcited QCD 2010 N Z S Extension of the chart of the nuclides into anti-matter with Strangeness sector

35 35 Sonia KabanaExcited QCD 2010 see next talk of S. Margetis Key measurements: - v 2 and R cp of D 0 - Charm baryon Λ c - Bottom cross sections Heavy Flavour Tracker

36 36 Sonia KabanaExcited QCD 2010 ONE NO STAR-SLIDE

37 37 Sonia KabanaExcited QCD 2010 Thermal model prediction for the (anti) - hypertriton I. Kraus, S. Kabana, H. Oeschler Thermal model with parameters fixed by other hadron ratios in Au+Au collisions at RHIC: T = 170 MeV mu_B = 27 MeV (values from PRC 74 (2006) 034903 J Cleymans et al) gamma_s = 1 (GC), 0.8, 0.7 m(3He) = 2.809 GeV m(hypertriton)=2.991 GeV Antiparticle to particle ratios measured are compatible with thermal model prediction for both Helium3 and hypertriton Ratios between (anti-)hypetriton and (anti-)helium-3 are higher in the data than in the model. This is due -at least partially- (BR=0.25) to Helium-3 feeding uncorrected in the model. preliminary

38 38 Sonia KabanaExcited QCD 2010 BACK-UP SLIDES

39 39 Sonia KabanaExcited QCD 2010 Event display

40 40 Sonia KabanaExcited QCD 2010 Nr of Quarks scaling works with Cu+Cu collisions. STAR preliminary Nr of quarks scaling of v 2 in Cu+Cu collisions PHENIX π/K /p: arXiv:0805.4039 STAR preliminary G. Wang, QM2009

41 41 Sonia KabanaExcited QCD 2010 Λ /K s 0 ratio at 62.4 GeV versus pT, centrality and collision system  Same behavior of Λ /K s 0 ratio observed for Au+Au and Cu+Cu at √s NN = 62.4 GeV  Greater Λ /K s 0 ratio reached in central than in peripheral collisions. 41 STAR Preliminary Cu+Cu, √s NN = 62.4 GeV STAR Preliminary Au+Au, √s NN = 62.4 GeV M Munhoz, SQM2009

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