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RHIC HBT in a larger context

RHIC HBT in a larger context. Zbigniew Chaj ę cki, OSU for the Experiment. Outline. HBT in Heavy-Ion Collisions at RHIC Multiplicity as universal scaling R(m T ) - direct probe of flow scenario Femtoscopy in p+p [reminder]

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RHIC HBT in a larger context

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  1. RHIC HBT in a larger context Zbigniew Chajęcki, OSUfor the Experiment Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  2. Outline • HBT in Heavy-Ion Collisions at RHIC • Multiplicity as universal scaling • R(mT) - direct probe of flow scenario • Femtoscopy in p+p [reminder] • mT scaling of HBT radii (AA/pp) [reminder] • Energy and Momentum Conservation Induced Correlations in p+p • STAR results from p+p (all fits) • world systematics : Rinv(N,mT), Ro,s,l(mT) • How different is pp from AA at the end? Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  3. Heavy ions at RHIC Multidimensional analysis at RHICR(√SNN, mT, b, Npart, A, B, PID) ... but is there a scaling variable? Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  4. Multiplicity scaling of HBT radii at RHIC Radii scale with multiplicity Lisa, Pratt, Soltz, Wiedemann, Ann.Rev.Nucl.Part.Sci. 55 (2005) 357-402 Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  5. mT dependence of pion HBT radii Au+Au@19.6GeV 0-10% centrality • Flow is the most important bulk feature at RHIC • mT-dependence of femtoscopy probes flow the most directly • quantitative agreement w/p-only observables Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  6. Femtoscopy - direct evidence of flow Spectra v2 R (fm) space-momentum substructure mapped in detail STAR PRL 91 262301 (2003) HBT mT (GeV/c)  K Flow-dominated “Blast-wave” toy models capture main characteristics e.g. PRC70 044907 (2004) Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008 6

  7. Id-pion correlations in p+p STAR preliminary mT [GeV/c2] mT [GeV/c2] • p+p and A+A measured in thesame experiment • great opportunity to compare physics • what causes pT-dependence in p+p? • same cause as in A+A? Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  8. Femtoscopy in pp vs heavy ions Ratio of (AuAu, CuCu, dAu) HBT radii by pp HBT radii scale with pp Scary coincidence or something deeper? pp, dAu, CuCu - STAR preliminary Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  9. Non-femto correlations / SH representation d+Au: peripheral collisions STAR preliminary Z.Ch., Gutierrez, Lisa, Lopez-Noriega, [nucl-ex/0505009] Pratt, Danielewicz [nucl-th/0501003] STAR preliminary Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  10. Decomposition of CF onto Spherical Harmonics Au+Au: central collisions C(Qout) C(Qside) C(Qlong) Z.Ch., Gutierrez, Lisa, Lopez-Noriega, [nucl-ex/0505009] Pratt, Danielewicz [nucl-th/0501003] Qx<0.03 GeV/c Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  11. Non-femtoscopic correlations in STAR N-dep. of non-femtoscopic correlations in p+p STAR preliminary Baseline problem is increasing with decreasing multiplicity STAR preliminary Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  12. EMCICs in other experiments Multiplicity increases Qx<0.2 GeV/c E766, PRD 49 (1994) 4373 OPAL, Eur. Phys. J. C52 (2007) 787-803 Qx<0.04 GeV/c NA23, Z. Phys. C43 (1989) 341 CLEO PRD32 (1985) 2294 NA22, Z. Phys. C71 (1996) 405 Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  13. Common approaches to „remove” non-femtoscopic correlations b |Q| |Q| z |Q| • MC simulations • ‘ad-hoc’ parameterizations • OPAL, NA22, … • “zeta-beta” fit by STAR [parameterization of non-femtoscopic correlations in Alm’s] • An alternative explanation:Energy and Momentum Conservation Induced Correlations, Z.Ch. and Mike Lisa [ArXiv:0803.022, sub. to PRC] Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  14. How do EMCICs look? GenBod calculations Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008 mike lisa - Nuclear Physics & RIKEN Theory Seminar 8 Aug 2008 14

  15. EMCIC fit to STAR p+p data λ = 0.38 ± 0.01 Ro = 0.65 ± 0.01 fm Rs = 0.85 ± 0.02 fm Rl = 1.42 ± 0.02 fm λ = 0.69 ± 0.01 Ro = 0.98 ± 0.03 fm Rs = 0.94 ± 0.02 fm Rl = 1.46 ± 0.03 fm N = 15 <E> = 0.39 GeV <E2> = 0.19 GeV2 <pT2> = 0.5 GeV2 <pz2> = 0.25 GeV2 STAR preliminary standard fit 15 15 Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  16. EMCIC fit to STAR p+p data λ = 0.38 ± 0.01 Ro = 0.65 ± 0.01 fm Rs = 0.85 ± 0.02 fm Rl = 1.42 ± 0.02 fm λ = 0.69 ± 0.01 Ro = 0.96 ± 0.04 fm Rs = 0.98 ± 0.03 fm Rl = 1.26 ± 0.02 fm N = 10.3 <E> = 0.61 GeV <E2> = 0.43 GeV2 <pT2> = 0.2 GeV2 <pz2> = 0.4 GeV2 STAR preliminary 16 Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  17. Various fits to STAR p+p data STAR preliminary STAR preliminary Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  18. mT scaling of HBT radii STAR preliminary Various fits give different radii but mT scaling of HBT radii is preserved in all fits p+p HBT looks like flow! Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  19. Multiplicity dependence in p+p STAR preliminary 200 GeV Rinv [fm] Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  20. p+p vs heavy ions - R(N,mT) STAR preliminary Similar mT and multiplicity dependence of HBT radii in p+p and heavy ions in STAR Is STAR p+p unique? Let’s look at world’s results on HBT in elementary particle collisions … Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  21. Femtoscopy in small systems R ≈ 0.5 - 1.5 fm Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  22. My first impression Can we do a direct comparison between experiments? Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  23. Parameterizations of 1D CF used in comparision b/w experiments RB≈2·RG Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008

  24. Femtoscopy similar in p+p as in Au+Au @ STAR “World results” show both pT and N dependence! EMCICs seen in small systems differences observed in pT spectra consistent with EMCIC “distortion” of unchanging parent distribution (soft sector) - talk by Mike Lisa & arXiv:0807.3569 Same physics in p+p as in Au+Au and the only difference due to phase-space effects? possibilities: spectra and HBT are insensitive to underlying physics (flow etc) they are sensitive & the very different physics of A+A and p+p look coincidentally identical they are sensitive, and driving physics is the same Summary Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008 24

  25. www.femtoscopy.org Database of talks/proceedings on particle correlations and related topics Femtoscopy.org in numbers Meetings : 24 records Speakers : 117 records Talks : 248 records Files : 295 records Z. Ch. - WPCF 2008, Krakow, Poland, Sep. 11-14 2008 25

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