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Christina MarkertSQM2004, Cape Town

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Christina Markert SQM2004, Cape Town. 1. Production of Resonances in Heavy Ion Collisions ... Horst St cker .Phys.G30 (2004) 111. signal loss in low momentum region ... – PowerPoint PPT presentation

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Title: Christina MarkertSQM2004, Cape Town


1
Production of Resonances in Heavy Ion Collisions
Christina Markert, Yale University
Resonances in Medium Rescattering and
Regeneration Time Scale Contribution
to Particle Yields Conclusions
2
Resonances in Medium
Life-time fm/c ? 1.7
K(892) 4 S(1385) 5.7 L(1520)
13 ? (1020) 44
  • Measurements
  • Leptonic and hadronic channels
  • e.g. f ? ee-, mm- , KK-
  • Collision systems
  • pp and AA collisions

3
Resonance in dense Matter
STAR preliminary 30-50 AuAu
?
PDG
Minv pp GeV/c2
  • nucleon propagation in medium
  • fireball conditions (T, r )
  • (1232) from Tkin100 MeV
  • (1232)? width increase

Hendrik von Hees HotQuarks2004 (Hees and Rapp
nucl-th/0407050) Medium Modifications of the
Delta Resonance at RHIC
4
f Meson at SPS and RHIC
Talks at this conference A. Marin New results
from CERES f in KK- and ee-
(Talk on Sunday)
M. Kaneta PHENIX f in dAu
(future AuAu)

Hadronic channel less signal in low pt lower
yield (factor 2-4)
5
Hadronic Phase after Chemical Freeze-out
signal loss in low momentum region ? Increase of
inverse slope
  • Signal loss in UrQMD 26
  • Data yield factor of 2-4 difference
  • for hadronic to leptonic channel.
  • Additional in medium modification
  • of resonance at early stage ?
  • Theory describes data with
  • In-medium kaon potential
  • Rescattering of secondary kaons
  • ? width of f 30 MeV (Vacuum 4.5 MeV)
  • ? life time of fireball 20 fm/c

UrQMD Marcus Bleicher and Jörg Aichelin Phys.
Lett. B530 (2002) 81. M. Bleicher and Horst
Stöcker .Phys.G30 (2004) 111.
E. Kolomeitsev, SQM2001 J.Phys.G281697-1706,2002
6
Statistical Model for Particle Production in
AuAu Collisions
STAR Preliminary
Resonance ratios in AuAu are not are well
described with Tch 160?10 MeV, mB 24 ?5 MeV
(QM2004 Olga Barannikova)
7
Rescattering and Regeneration
UrQMD 2
Thermal model 1 T 177 MeV mB 29 MeV
Life-time fm/c ? 1.7
K(892) 4 S(1385) 5.7 L(1520)
13 ? (1020) 44
K rescattering gt regeneration D regeneration
gt rescattering S similar to D ,baryonmeson L
rescattering gt regeneration no regeneration
with p Regeneration cross section s(kp) lt s
(kp) lt s (pp), s (Lp) ? L K
D S
1 P. Braun-Munzinger et.al., PLB
518(2001) 41 D.Magestro, private
communication 2 Marcus Bleicher and Jörg
Aichelin Phys. Lett. B530 (2002) 81.
M. Bleicher and Horst Stöcker J.
Phys.G30 (2004) 111.
8
Signal Loss in low pT Region
Inverse slope increase from pp to AuAu
collisions. UrQMD predicts signal loss at low pT
due to rescattering of decay daughters. ?
Inverse slopes and mean pT are higher. UrQMD has
long lifetime (Dt 5-20fm/c)
9
Particle spectra from Thermal Model
Signal loss for K in low momentum region due to
rescattering
W. Florkowski, this conference
10
Temperature and Life-time fromK and L (STAR)

G. Torrieri and J. Rafelski, Phys. Lett. B509
(2001) 239
  • Model includes
  • Temperature at chemical freeze-out
  • Life-time between chemical and
  • thermal freeze-out
  • By comparing two particle ratios
  • (no regeneration)
  • results between
  • T 160 MeV gt ?? gt 4 fm/c
  • (lower limit !!!)
  • ?? 0 fm/c gt T 110-130 MeV

Does not work for S, D, f (STAR)
?(1520)/? 0.034 ? 0.011 ? 0.013
K/K- 0.20 ? 0.03 at 0-10 most central AuAu
11
Temperature, Life-time from Particle Spectra
p,K and p
Tch freeze-out
Tch from Thermal model, Tkin and b from
Blast-Wave-Fit to p, K and p
Tkin freeze-out
Life-time nearly constant in peripheral and
central AuAu collisions
Go to smaller systems volume ? Life-time dAu ,
SiSi , CuCu
12
Feed down from Resonances
  • J.Letessier, J.Rafelski,
  • Hadrons and Quark Gluon Plasma,
  • Cambridge Monographs

S
STAR
direct L
  • Thermal modelSTAR data
  • Tch160 MeV
  • 32 primary Lambdas
  • 26 primary Protons

S0
Tch 160 MeV
  • Large fraction of stable particles
  • come from resonance decays.
  • Rescattering and regeneration
  • Less primary particles
  • Momentum distribution changes

S0 Talk by G. Van Buren at this conference
13
Conclusions
  • Strong interacting hadronic medium after
  • chemical freeze-out.
  • ? Thermal models do not describe all resonance
    yields.
  • ? Rescattering and regeneration of resonances.
  • ? Regeneration probes hadronic cross sections
    of heavy baryons.
  • ? Life-time between freeze-outs gt 4 fm/c
  • Medium modification of resonances.
  • ? Width broadening of D observed at RHIC
    energies in
  • AuAu collisions ? medium modification.
  • ? f yield in leptonic and hadronic channel at
    SPS
  • give indication of width broadening of phi
    in medium.
  • Large fraction of particles coming from
  • resonance decays
  • ?Could affect kinematics of primordial
    particles.
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