Title: STAR: update on Strangeness and Heavy Flavor
1 STAR update on Strangeness and Heavy Flavor
- Olga Barannikova
- for the STAR Collaboration
2Outline
- Selected recent STAR results on strangeness and
heavy flavor production - Medium properties
- Thermalization
- Particle production and Parton propagation
- Energy density Energy loss
- Summary
2
3But first Hypernuclei at RHIC
Hypernucleus - Nucleus which contains at least
one hyperon in addition to nucleons.
Hypernucleus of lowest A - Hypertriton
Saito, HYP06
First discovery Danysz and Pniewski in 1952
Hypernucleus experiments SPHERE at
JINR Jlab HypHI at GSI/FAIR J-PARC
(2009) PANDA at FAIR (2012) .
No one has ever observed any antihypernucleus
3
4 observation
3LH mesonic decay, mass2.991 GeV, BR 0.25 200
GeV AuAu data
- Hypernucleus Discovery in HI at RHIC 6s
combined signal - First ever observation of an anti-hypernucleus
4s signal - The hypertriton and anti-hypertriton lifetime
4
5Strangeness studies Motivation
- Why bother?
- Produced in the collision
- Small rescattering cross-sections
- Phase-boundary/hadronization probes
- Equilibration?
- Enhancement of strangeness one of the earliest
QGP predictions - Flavor dependence of energy loss
5
6Strangeness production at RHIC
- Detailed systematic studies with multiple systems
- Evidence of s-quark equilibration in central
AuAu collisions - Enhancement of strangeness production in AuAu,
CuCu, dAu
STAR, PLB616 (2006) 637
6
7Thermalization studies strange particles V2
- Mass ordering in the low pT is well established
with common hadrons
- Multi-strange hadron v2 ?
- Partonic collectivity
- Hadronization via coalescence
Run 7
Open symbols PHENIX, PRL 98 (2007) 162301
7
8High pT strangeness
- Kaon production (wrt. pions) is enhanced up to
highest pT - Suggestive of jet-chemistry modifications
W. Liu and R. Fries, PRC 77, 054902 (2008)
- Partons conversions may be significant due to
interactions with the medium - Abundant QGP s-quarks result in boost of Kaon
production factor 2
8
9Jet flavor conversion
STAR Preliminary
W. Liu and R. Fries, PRC 77, 054902 (2008)
- Expectation from color charge dependence of
energy loss RAA(p) lt RAA(?) - Observation from central AuAu collisions
RAA(?) ltRAA(K) ltRAA(p) - Hierarchy consistent with jet flavor conversion
- parton ?medium interactions
9
Yichun Xu, 5A Anthony Timmins, 6C
Jörn Putschke for the STAR Collaboration, QM09,
Knoxville
9
10Heavy Flavor studies Motivation
- Why Heavy Flavor?
- Produced in the early stages
- Heavy quarks calculable (?) probes for medium
properties - Discriminating power for energy loss scenarios
- Open Heavy Flavor pQCD tests of thermalization
and energy loss mechanisms - Quarkonia production mechanisms
- deconfinement and thermalization
tests
10
11High pT suppression for HF
- Light flavor energy loss
- Strong suppression at high pT in RAA
- Jet studies via correlations softened spectra,
broadening - Radiative vs. collisional energy loss
- Open heavy flavor
- Smaller gluon bremsstrahlung for heavy quarks
? - Smaller suppression at high pT
RAA for non-photonic electrons (from heavy flavor
decays)
No decrease in suppression for non-photonic e
11
12Energy loss for beauty
- Heavy Flavor results from non-photonic
electrons - Strong suppression of heavy-flavor at high pT
in RAA light mesons - Inconsistent with radiative energy loss
prediction ? needs collisional too - What about beauty?
e D0 correlation using like-sign e-K pairs
- Significant contribution from b-decays
- 50 at pT5 GeV/c
mostly B
25B,75C
12
13Charm and Beauty in pp
e-hadron correlations
- Agreement on b- and c- fractions from e-h and
e-D0 correlation results - b-decays contribution to non-photonic electrons
50 at pT5 GeV/c - ? strong suppression in AA for both charm and
beauty!
13
14Quarkonia as temperature probes
- Systematic studies of multiple states (J/?, ?,
?C,?) could serve as a thermometer for QCD
matter - TD (?) 4Tc
- TD (?) TD (J/?) ?
- ?/ ?, J/? /? vs. pT very sensitive to system
temperature size
15J/? measurements at high pT
STAR Preliminary
CS Color Singlet CO Color Octet
STAR Preliminary
First high pT J/? measurements Constrains on
production mechanisms Direct QCD CSCO in
agreement with data, little room for
feed-down NNLO CS predicts steeper pT spectra
15
16J/? production mechanisms and RAA
pp collisions
CuCu collisions
J/?-h correlation
STAR Preliminary
- Small background at high-pT in pp? J/?- hadron
correlations - Use the correlation function to measure the B?J/?
fraction 13 5 - Contrast to AdS/CFT Hydro prediction (99 C.L.)
- RAA(pTgt5GeV/c) gt 0.6 (97 C.L.), indicating RAA
increases with pT
16
17J/? at forward rapidity
Invariant mass of ee- pairs (J/?) with a photon
requirement
Invariant mass of all cluster pairs
counts
?C ? J/? ? ? e e- ? Significance2.9s
J/? ? e e- Significance 4.5s
First observation of high-xF(0.4) J/? beyond ISR
energies
17
18Upsilon production in dAu
- Run8 dAu 200 GeV
- High luminosity 32nb-1
- Low material in front of TPC
- L0L2 Upsilon trigger
Recall Run 6 pp 200 GeV Signal significance 3s
18
19Nuclear modification factor
pp
dAu
RdAu 0.98 0.32 (stat.) 0.28 (sys.)
- Consistent with Nbin scaling
- Consistent with anti-shadowing calculations
First ? signal in AuAu
19
20Summary
- STAR Systematic studies of the partonic
medium - First observation of anti-hypernucleus
- Systematic studies of strangeness at RHIC
- - Precision PID v2, NCQ test
- - Strangeness enhancement in different systems
- - Color-charge effects / jet flavor conversion
- Ongoing heavy flavor program
- High pT suppression both Charm and Beauty?
- J/psi RCuCu consistent with unity at high pT
- Upsilon Nbin scaling in dAu
- - Prospective RAA for Upsilon to understand J/psi
(suppression vs. recombination)
20
21Back-Up
21
22 signal from the data
- Signal observed from the data (bin-by-bin
counting) 15730 - Mass 2.9890.0010.002 GeV Width (fixed)
0.0025 GeV. - Projection on anti-hypertriton yield
1572168/5810 5911
22
23 signal from the data
- Signal observed from the data (bin-by-bin
counting) 7017 - Mass 2.9910.0010.002 GeV Width (fixed)
0.0025 GeV.
23
24Heavy Flavor measurements
non-photonic electrons
D0 reconstruction
25J/Y Suppression at SPS