2005
DOI: 10.1088/0954-3899/31/4/012
|View full text |Cite
|
Sign up to set email alerts
|

Bulk properties at RHIC: systematic study

Abstract: A variety of particle species measured by the STAR experiment in 200 GeV Au+Au collisions yielded rich information about freeze-out dynamics at RHIC. The results on chemical and kinetic freeze-out properties and their centrality dependences appeared to be consistent with QGP formation in the early stage of the collision. To further advance our understanding of the collision evolution, lower energy 62.4 GeV Au+Au collisions were measured. Here, we present a review of freeze-out dynamics in 200 GeV collisions at… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
2
1

Citation Types

1
23
0

Year Published

2005
2005
2011
2011

Publication Types

Select...
8
1

Relationship

2
7

Authors

Journals

citations
Cited by 15 publications
(24 citation statements)
references
References 19 publications
1
23
0
Order By: Relevance
“…According to these results, the thermal parameters are different for two experiments, PHENIX and STAR, in spite of the same collision energy. Fits to mostly PHENIX ratios gave the lower freeze-out temperature [20] than fits to STAR data only [21]. This observation has been confirmed in the present analysis: fits to the PHENIX spectra with substitution of the STAR freeze-out thermal parameters (T = 160.0 MeV and µ B = 24.0 MeV [21]) and fits to the STAR spectra with the use of the PHENIX freeze-out thermal parameters (T = 155.2 MeV and µ B = 26.4 MeV [20]) have proven to be much worse than the fits done within the same experiment and finally reported in this work (here "worse fit" means that its χ 2 /NDF is greater).…”
Section: A Determination Of Geometric Parametersmentioning
confidence: 88%
See 1 more Smart Citation
“…According to these results, the thermal parameters are different for two experiments, PHENIX and STAR, in spite of the same collision energy. Fits to mostly PHENIX ratios gave the lower freeze-out temperature [20] than fits to STAR data only [21]. This observation has been confirmed in the present analysis: fits to the PHENIX spectra with substitution of the STAR freeze-out thermal parameters (T = 160.0 MeV and µ B = 24.0 MeV [21]) and fits to the STAR spectra with the use of the PHENIX freeze-out thermal parameters (T = 155.2 MeV and µ B = 26.4 MeV [20]) have proven to be much worse than the fits done within the same experiment and finally reported in this work (here "worse fit" means that its χ 2 /NDF is greater).…”
Section: A Determination Of Geometric Parametersmentioning
confidence: 88%
“…The data points with p T > 3 GeV have been excluded in the χ 2 analysis. The thermal parameters for the three cases of the maximal RHIC collision energy have been taken from the newer studies of the particle abundance ratios [20,21]. According to these results, the thermal parameters are different for two experiments, PHENIX and STAR, in spite of the same collision energy.…”
Section: A Determination Of Geometric Parametersmentioning
confidence: 99%
“…This is the case considered in Ref. [7]: the statistical parameters (T = 160.0 MeV, µ B = 24.0 MeV) are fitted to the STAR particle yield ratios [19] and the geometric parameters to the p T spectra of identified hadrons delivered by the STAR Collaboration in Ref. [20].…”
Section: B Identified Hadron Spectramentioning
confidence: 99%
“…We have studied the magnitude of the corrections using various model assumptions as input to the BRAG simulations. Assuming primary Λ/p ratios at √ s N N = 200 GeV similar to those measured at the lower energy [25] and a constant behavior with rapidity, we take these ratios and measured spectra shapes as input to the BRAG code for feed down correction from Λ decays. The simulated tracks are generated for the full phase space, digitized, and go through the real data analysis algorithm, as is done to determine the other correction factors.…”
Section: Centralitymentioning
confidence: 99%