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  4. Strange and multistrange particle production in Au + Au collisions at [sqrt]sNN=62.4 GeV

Strange and multistrange particle production in Au + Au collisions at [sqrt]sNN=62.4 GeV

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Author(s)
Betancourt, Michael Joseph
•
Corliss, Ross Cameron
•
Hays-Wehle, James Prewitt
•
Leight, William Axel
•
Sakuma, Tai
•
Seele, Joseph Patrick
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Surrow, Bernd
•
Balewski, Jan T.
•
Milner, Richard G
•
Redwine, Robert P
more
Alternative Title
Strange and multistrange particle production in Au + Au collisions at √sNN=62.4 GeV
Date Issued
February 2011
Journal
Physical Review C
Publisher
American Physical Society
Citation
Aggarwal, M. et al. (Star Collaboration). “Strange and multistrange particle production in Au + Au collisions at sqrt[s_{NN}]=62.4 GeV.” Physical Review C 83 (2011). ©2011 American Physical Society.
Version
Final published version
Abstract
We present results on strange and multistrange particle production in Au + Au collisions at [sqrt]sNN=62.4 GeV as measured with the STAR detector at RHIC. Midrapidity transverse momentum spectra and integrated yields of KS0, Lambda, Xi, and Omega and their antiparticles are presented for different centrality classes. The particle yields and ratios follow a smooth energy dependence. Chemical freeze-out parameters, temperature, baryon chemical potential, and strangeness saturation factor obtained from the particle yields are presented. Intermediate transverse momentum (pT) phenomena are discussed based on the ratio of the measured baryon-to-meson spectra and nuclear modification factor. The centrality dependence of various measurements presented show a similar behavior as seen in Au + Au collisions at [sqrt]sNN=200 GeV.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/66109
DOI of Published Version
https://doi.org/10.1103/PhysRevC.83.024901
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