2006
DOI: 10.1556/aph.25.2006.2-4.18
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Extraction of Kinetic Freeze-out Properties and Effect of Resonance Decays

Abstract: Abstract. We present STAR results from identified particle spectra measured in √ s N N = 62.4 GeV Au-Au collisions. Particle production and system dynamics are compared to results at √ s N N = 200 GeV. We extract kinetic and chemical freeze-out parameters using blast wave model parameterization and statistical model. We discuss the effect of resonance decays on the extracted kinetic freeze-out parameters.

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Cited by 1 publication
(5 citation statements)
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“…5 with results from most central 200-GeV Cu + Cu data. The π ± data points for p T < 0.5 GeV/c are excluded from the blast-wave fits to reduce the effects of resonance-decay contributions as done in previous works [5][6][7]. Including this low-p T region in the fit leads to a poorer description of proton and kaon shapes; however, the resultant modification of the extracted parameters remains well within their systematic uncertainty.…”
Section: Resultsmentioning
confidence: 99%
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“…5 with results from most central 200-GeV Cu + Cu data. The π ± data points for p T < 0.5 GeV/c are excluded from the blast-wave fits to reduce the effects of resonance-decay contributions as done in previous works [5][6][7]. Including this low-p T region in the fit leads to a poorer description of proton and kaon shapes; however, the resultant modification of the extracted parameters remains well within their systematic uncertainty.…”
Section: Resultsmentioning
confidence: 99%
“…These 0%-60% minimum-bias events, with 24 M and 10 M events recorded at 200 and 62.4 GeV, respectively, were divided into six centrality bins, each corresponding to a 10% interval of the geometric cross section. Transverse mass distributions for charged pions, charged kaons, protons, and antiprotons, previously reported by STAR for √ s NN = 200 GeV pp collisions and Au + Au collisions at 62.4 and 200 GeV [5][6][7], are used for comparison. The STAR time projection chamber (TPC) [12] tracks particle trajectories over a wide range of momentum at midrapidity (|η| < 1.8).…”
Section: The Star Experimentsmentioning
confidence: 99%
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