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SQM 2004 Summary: SQM, a STAR Qollaboration Meeting

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Strange Quark Matter Cape Town September 2004. 2. S. Q. M. 2004 ... Strange Quark Matter Cape Town September 2004. 12. S. Q. M. 2004 'Jettiness': the ... – PowerPoint PPT presentation

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Title: SQM 2004 Summary: SQM, a STAR Qollaboration Meeting


1
SQM 2004 SummarySQM, a STAR Qollaboration
Meeting?
  • Paul Sorensen
  • Lawrence Berkeley National Laboratory

2
130 Participants
3
  • Charm was the centerpiece of the conference.
  • Bare charm quark from NLO matches STAR D
    measurements!
  • What about hadronization!?

4
  • STAR measurement in dAu is several sigma above
    NLO pQCD.
  • The charm mass used to match the shape of the
    spectrum does worse for the beam energy
    dependence of the cross section.
  • Something is not under control maybe charm is
    not massive enough for pQCD

5
PHENIX
M. Van Leeuwen
  • AuAu electron measurements insensitive so far
    to scaling or suppression.

6
F. Laue
  • Apparently large D v2 after corrections
  • Generated greatest interest of the conference.

7
  • NLO calculations fail to reproduce pp spectra
    for identified particles why?
  • Fragmentation functions are not under control.

8
Kaneta
Estienne
  • STAR and PHENIX interpretations of phi slopes
    differ.
  • The court of popular opinion sided with PHENIX
    because they wanted to see feed-down corrected
    STAR results.

9
  • CERES dilepton measurement disfavors the NA49
    observation of phis in the lepton channel
  • Within overlapping range in Npart , NA60 on ??µµ
    are close to those from NA49 on ? ?KK, but are
    higher than those from NA50 on ? ?µµ

10
  • Marcus Bleicher v2/ltptgt saturates at ltptgt0.37
  • UrQMD cannot reproduce the plateau this may be
    evidence for an initial QGP pressure

11
Moronga
Teaney
  • Hydro second order terms solve accausality and
    stability problems
  • Upper limit on viscosity is even lower than
    predicted minimum advertised by Gyulassy.

12
Quark-number scaling
  • How would a quark dependence manifest itself in
    v2 if v2 developed in a hadronic phase?
  • v2 is developed amongst quarks!
  • Isnt v2 a long range correlation?
  • ? to develop v2 quarks need to be deconfined
    (over distances greater than hadron length
    scales)!

13
Jettiness the odd man out?
Can jettiness be accommodated within the same
picture that explains less suppression of baryon
yields AND a larger baryon v2? The Test can the
baryon/meson correlation structure be traced to
one unique quark/gluon correlation structure
(not is there a structure)?
PHENIX arXivnucl-ex/0408007
PHENIX arXivnucl-ex/0408007
14
Jettiness at intermediate pT
Perhaps correlations amongst quarks and gluons
are mapped onto hadron correlations through
recombination.
15
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16
Thanks! -Paul Sorensen
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