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Title: Brookhaven National Laboratory


1
Resonance Production in AuAu and pp Collisions
at ?sNN200 GeV
  • Patricia Fachini
  • Brookhaven National Laboratory

Motivation Data Analysis Results Conclusions
2
Motivation - 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
3
Motivation - 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 ?

4
Resonance 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

5
Raw 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

7
Phase 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2000, unpublished E.V. Shuryak and G.E. Brown,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 ?

12
ltpTgt 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
14
Conclusions
  • 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
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