Title: Brookhaven National Laboratory
1Resonance Production in AuAu and pp Collisions
at ?sNN200 GeV
- Patricia Fachini
- Brookhaven National Laboratory
Motivation Data Analysis Results Conclusions
2Motivation - I
- In-medium modification of mass and/or width ?
Chiral Symmetry Restoration, Collision Broadening
or Phase Space? - ?0(770) ? Leptonic decay channel ? probes all
stages of the collision. Hadronic decay channel ?
probes only late stages of the collision - F ? Information from early time ?
- f0(980) ? KK molecule (bound state) ? insight
strangeness behavior in relativistic collisions - K0(892) ? Regeneration and daughter rescattering
? time scale ?
?0 c? 1.3 fm
F c? 44 fm
3Motivation - II
- If resonance decays before kinetic freeze-out ?
not reconstructed due to rescattering of
daughters - K0 (c? 4 fm) survival probability ? time
between chemical and kinetic freeze-out, source
size and pT of K0 - Chemical freeze-out ? elastic interactions pK ?
K0? pK regenerate K0(892) until kinetic
freeze-out - K0/K may reveal time between chemical and
thermal freeze-out - ?/?, ?0/p, f0/p ?
4Resonance Production at RHIC
- ?0(770) ? p p- B.R. 1 c? 1.3 fm
- K0(892) ? p K B.R. 2/3 c? 4 fm
- f0(980) ? p p- B.R. 2/3 c? 2.6 fm
- F(1020) ? K K- B.R. 0.492 c? 44 fm
- F(1020) ? e e- B.R. 0.000296 c? 44 fm
- ?(1520) ? p K B.R. 0.45 c? 12.6 fm
- y 0.5
- Mixed Event or Like Sign Technique
5Raw Invariant Mass Distribution from Data
P. Fachini, L. Gaudichet, J. Ma, C. Maguire, H.
Zhang SQM2003
Statistical error only
pp
pp
40-80 AuAu
K0
STAR Preliminary
J. Adams et al. nucl-exp/0307023
J. Adams et al. nucl-exp/0307023
STAR
STAR
pp
AuAu
AuAu
F
STAR Preliminary
STAR Preliminary
?sNN 200 GeV
K0
F
ylt0.5
STAR Preliminary
AuAu
AuAu
pp
60-80 AuAu
PHENIX Preliminary
STAR Preliminary
PHENIX Preliminary
STAR Preliminary
F?KK-
F?ee-
?(1520)
?(1520)
Invariant Mass (GeV/c2)
Invariant Mass (GeV/c2)
Invariant Mass (GeV/c2)
Invariant Mass (GeV/c2)
6 K0 Mass and Width
H. Zhang, SQM2003
STAR Preliminary
STAR Preliminary
?sNN 200 GeV
ylt0.5
- K0 mass ? shifted in pp and AuAu at low pT
- K0 width ? agrees with the MC (GEANT)
calculation - Systematic and statistical error added in
quadrature
7Phase Space
P. Braun-Munzinger et.al., CERES Int. Note, March
2000, unpublished E.V. Shuryak and G.E. Brown,
Nucl. Phys. A 717 (2003) 322 P.K. Kolb and M.
Prakash, nucl-th/0301007 H.W. Barz et al., Phys.
Lett. B 265, 219 (1991) R. Rapp, hep-ph/0305011.
- M Invariant Mass pT transverse momentum T
Temperature - pp ? particle composition reasonably reproduced
by statistical model ? T 160 MeV - F. Becattini, Nucl. Phys. A 702, 336 (2002) Z.
Phys. C 69, 485 (1996) F. Becattini and U.
Heinz, Z. Phys. C 76, 269 (1997) - AuAu ? between chemical and kinetic freeze-out ?
resonances formed until particles too far apart ?
resonances emitted T 120 MeV - E.V. Shuryak and G.E. Brown, Nucl. Phys. A 717
(2003) 322
8 ?0 Mass
J. Adams et al. nucl-exp/0307023
- pp at ?s 27.5 GeV ? M? 762.6 2.6 MeV/c2
- PDG average hadroproduced ?0 ? M? 769.0 0.9
MeV/c2 - PDG average ee- ? ? M? 775.9 0.5 MeV/c2
- ?0 mass pt dependent and lower than previous pp
measurement in both pp and peripheral AuAu
collisions - ?0 mass high multiplicity pp lower than minimum
bias pp ? multiplicity dependent - Systematic errors ? common and correlated between
pp and peripheral AuAu - ?0 width ? no sensitivity for systematic study
10 of minimum bias pp for ?lt0.5
?sNN 200 GeV
ylt0.5
9 Mass Shift
- Dynamical Effect
E.V. Shuryak and G.E. Brown, Nucl. Phys. A 717
(2003) 322 R. Rapp, hep-ph/0305011. - ?0 interactions at late stages of the collision
- nucleons, hyperons and baryon resonances
- pions, kaons and ?0-mesons
- t-channel exchanges
- ? Distortion of the ?0 spectral shape ?
mass shift and/or broadening - Interference between various pp- scattering
channels R. Longacre,
nucl-exp/0305015 - Bose-Einstein correlations between ?0 decay
daughters and pions in the surrounding matter
G.D. Lafferty, Z. Phys. C 60, 659
(1993) R. Rapp, hep-ph/0305011 S. Pratt et al.,
nucl-th/0308087.
-23 MeV/c2 shift in the ?0 mass
-38 MeV/c2 shift in the ?0 mass due to t-channel
attraction
10 Spectra
J. Adams et al. nucl-exp/0307023
J. Ma, SQM2003
H. Zhang, SQM2003
P. Fachini, SQM2003
K0
F
?0 f0
STAR Preliminary
STAR Preliminary
STAR Preliminary
Statistical error only
?sNN 200 GeV
ylt0.5
L. Gaudichet, SQM2003
- AuAu ? spectra fit to exponential in mT-m0
- pp ? spectra fit to power-law ? contribution
pQCD processes larger than soft processes ?
?(1520)
pp
STAR Preliminary
11 Particle Ratios
M. Bleicher et al. J. Phys. G 25 (1999) 1859
J. Adams et al. nucl-exp/0307023
P. Fachini SQM2003
J. Ma SQM2003
L. Gaudichet, SQM2003
H. Zhang SQM2003
STAR Preliminary
Statistical and systematic errors added in
quadrature
- F/K- independent of centrality ? F not produced
via kaon coalescence ? - Cross-section ? regeneration or rescattering ?
12ltpTgt Charged Particle Dependence
H. Zhang, SQM2003
J. Ma, SQM2003
H. Zhang, SQM2003
J. Ma, SQM2003
Statistical and systematic errors added in
quadrature
STAR Preliminary
STAR Preliminary
- F and K0 ? No centrality dependence
- F ? Flows differently ?
- K0 ? Rescattering dominates at peripheral
collisions and regeneration becomes significant
for central collisions ?
13 Thermal Models
Chemical freeze-out
Kinetic freeze-out
Chemical kinetic freeze-out
m?770MeV
m?700MeV
?sNN 200 GeV
- Short-lived resonances ? Kinetic freeze-out ?
Statistical and systematic errors added in
quadrature
14Conclusions
- Significant resonance production measured from
hadronic interactions from RHIC data at ?sNN
200 GeV - ?0 and K0 ? mass shift observed even after phase
space correction in pp and AuAu collisions - Lower mass expected due to in-medium
modifications, interference and Bose-Einstein
correlations ? - F/K- independent of centrality ? F not produced
via kaon coalescence ? - Short-lived resonances ? Regeneration and
rescattering ? driven by hadronic cross sections
? - Resonances can provide information on the
collision dynamics