Patricia Fachini for the STAR collaboration
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Transcript of Patricia Fachini for the STAR collaboration
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 1
Patricia Fachini
for the STAR collaboration
Motivation
Measurements
Results
Conclusions
ρ0 Production in Cu+Cu Collisions at √sNN = 200 and 62.4 GeV in STAR
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 2
Motivation - I
• In-medium modification of mass and/or width Chiral Symmetry Restoration?
• Leptonic decay channel probes all stages of the collision.• Hadronic decay channel probes only late stages of the collision.
ρ0 ρ0π-
π+
π+
π-
ρ0 c = 1.3 fm
ρ0
ρ0
+
+
-
-
π- π+
ρ0
-
+
π- π+
ρ0
π+
π-
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 3
• Hadrons scale number constituent quarks v2/n• ρ0 v2 scale number constituent quarks?• ρ0(770) production mechanism scale NCQ v2/n
– ππ ρ0 n = 4 – qq ρ0 n = 2
• Difference between two limiting cases 30%
Motivation - II
C. Nonaka et al., Phys.Rev. C69 (2004) 031902
Hadron Gas
QGP
Hadron Gas + QGP
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 4
Motivation - III
• If ρ0 decays before kinetic freeze-out not reconstructed due to rescattering of daughters
• Chemical freeze-out elastic interactions π+π- ρ0 π+π- regenerate ρ0 until kinetic freeze-out
• Is the regeneration and rescattering driven by the hadron cross-sections?
Chemical freeze-out
Kinetic freeze-out
ρ0 measured
ρ0
π+π-
π+ π-ρ0
measured
ρ0
ρ0 lostρ0
π-
π+
ρ0
π-
π+
π-
π+
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 5
Motivation - IV
• ρ0 regeneration σ(ππ)
• ρ0 daughter rescattering σ(πp) and σ(Kπ)
• σ(ππ) >> σ(Kπ)
• σ(πp) > σ(ππ)
Probe dynamics between chemical and kinetic freeze-outs
Chemical freeze-out Kinetic freeze-out
K*π
K
Δ++p
π
πρ
π
π
πρ
π
π
σ(ππ)
K*
π
K
π
σ(Kπ)
π p
π
π p
π
σ(πp)
Δ++
Δ++
π
π
σ(ππ)
π
ρ
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 6
• HIJING events with a realistic simulation of detector response
• Use ω and K*0 shape from HIJING to fit the data
• K*0 signal is fixed using STAR measurement
ρ0(770) π+ π-
STAR Preliminary
ρ0
sNN = 200 GeV
K0S
π+ π-
K0S
ω(782) (π+ π-) π0 and π+ π-
ω η (π+ π-) π0 and (π+ π-)
η’ (π+ π-) η and (π+ π-) ρ0η + η’K*(892)0 K π with K misidentified as πK*0 + K*0
misidentified
π+π- Invariant Mass Distribution from Monte Carlo
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 7
Invariant Mass Distribution - Cocktail
• Background subtracted like-sign technique.• ρ0 and f0 widths fixed according PDG.
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 8
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.
ρ0
π-
π+
π-
π+
• M = Invariant Mass; pT = transverse momentum; T = Temperature
• 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
e- M2 + pT
2
TM
M2 + pT2
Phase Space =
BW(M) = Γ(M)
(M2 – M2)2 + M
2 Γ(M)2Γ(M) = Γρ
M2 – 4mπ2
Mρ2 – 4mπ
2
32 Mρ
M
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 9
Mass
• Mass shift ~45 MeV/c2 observed possible explanations– Medium modifications
– Bose-Einstein correlations
R. Rapp, Nucl.Phys. A725, 254 (2003), E.V. Shuryak and G.E. Brown, Nucl. Phys. A 717 (2003) 322
G.D. Lafferty, Z. Phys. C 60, 659 (1993); R. Rapp, Nucl.Phys. A725 (2003) 254-268
S. Pratt et al., Phys.Rev. C68 (2003) 064905
Statistical errors only Statistical errors only
J. Adams et al., Phys. Rev. Lett. 92 (2004) 92301
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 10
Spectra
• ρ0 measured in four different centralities in Cu+Cu.• Statistical and systematic errors added in quadrature.• Small signal to background ratio prevents the measurement in
central collisions (~1/1000).• Solid lines exponential fits.
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 11
Mean pT
• Statistical and systematic errors added in quadrature.
• ρ0 mean pT slightly increases with Npart.
• ρ0 mean pT comparable with proton mean pT.
B. I. Abelev et al., Phys. Rev. C 78 (2008) 44906J. Adams et al., Phys. Rev. C 71 (2005) 64902J. Adams et al., Phys. Rev. Lett. 92 (2004) 92301
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 12
M. Bleicher et al. J. Phys. G 25 (1999) 1859
Particle Ratios
σ(Kπ)
σ(ππ)
σ(πp)• Cross-section regeneration or rescattering. • K* rescattering of the daughters.
• ρ0 regeneration compensating rescattering of
the daughters.
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 13
M. Bleicher et al. J. Phys. G 25 (1999) 1859
Particle Ratios
σ(Kπ)
σ(ππ)
σ(πp)• Cross-section regeneration or rescattering. • K* rescattering of the daughters.• ρ0 regeneration compensating rescattering of
the daughters.
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 14
Particle Ratios – Transport Model M. Bleicher et al. J. Phys. G 25 (1999) 1859
σ(Kπ)
σ(ππ)
σ(πp)
• UrQMD long expansion time π+π- scattering will not have enough energy to produce ρ0.
STAR
• Significant ρ0 v2 measured pT > 1.2 GeV/c v2 ~ 13 ± 4%.
Elliptic Flow
15QM2009, Knoxville, March 30 - April 4 Patricia Fachini
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 16
Elliptic Flow
• Resonance v2 ρ0(770) production mechanism scale NCQ v2/nππ ρ0 n = 4 or qq ρ0 n = 2
a, b, c, and d constants extracted using KS0 and Λ v2 ρ0 v2 n= 4.7 ± 2.9
pT range covered not sufficient for conclusive statement on the ρ0 production mechanism.
v2(pT,n) = - dn1 + exp[-(pT/n – b)/c]
anX. Dong et al., Phys.Lett. B597 (2004) 328
n=2 n=4
STAR
• Significant ρ0 production measured in Cu+Cu collisions at √sNN= 200 and 62.4 GeV.
• Production measured in 20-60% of hadronic cross-section.• Mass shift ~45 MeV/c2 observed
– Medium modifications.– Bose-Einstein correlations.
• Regeneration and rescattering driven by hadron cross-sections.
• K* rescattering of the daughters.
• ρ0 regeneration compensating rescattering of the daughters.
• First measurement of the ρ0 v2 significant ρ0 v2 measured.
• pT range covered not sufficient for conclusive statement on the ρ0 production mechanism.
See the poster by Prabhat Pujahari for details on the analysis of the results presented in this talk.
QM2009, Knoxville, March 30 - April 4 Patricia Fachini 17
Conclusions
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 18
Elliptic Flow
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 19
• Significant ρ0 v2 measured pT > 1.2 GeV/c v2 ~ 13 ± 4%.
Elliptic Flow
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 20
• 1. Dynamical effect ρ0
interactions at late stages of the collision– nucleons, hyperons and
baryon resonances– pions, kaons and ρ0-mesons– t-channel exchanges
Distortion of the ρ0 spectral shape mass shift and/or broadening
-23 MeV/c2 shift in the ρ0 mass
-38 MeV/c2 shift in the ρ0 mass due to t-channel attraction
R. Rapp, hep-ph/0305011
E.V. Shuryak and G.E. Brown, Nucl. Phys. A 717 (2003) 322
Possible Explanations for Mass Shift - I
STAR QM2009, Knoxville, March 30 - April 4 Patricia Fachini 21
• 2. Interference between various π+π- scattering channels can effectively distort the line shape of resonances R. Longacre, nucl-exp/0305015
• 3. Bose-Einstein correlations between ρ0 decay daughters and pions in the surrounding matter can also distort the resonance shape G.D. Lafferty, Z. Phys. C 60, 659 (1993); R. Rapp, hep-ph/0305011; S. Pratt et al., nucl-th/0308087.
Possible Explanations for Mass Shift - II
ρ0
π-
π+
Dπ-
π+
Aρ0
π-
π+
A Interference