Full-text resources of PSJD and other databases are now available in the new Library of Science.
Visit https://bibliotekanauki.pl

PL EN


Preferences help
enabled [disable] Abstract
Number of results

Journal

2012 | 10 | 6 | 1238-1241

Article title

Highlights of the beam energy scan from STAR

Content

Title variants

Languages of publication

EN

Abstracts

EN
The first part of the beam energy scan (BES) program at RHIC was successfully completed in the years 2010 and 2011. First STAR results from particle yield measurements are in good agreement with previously published data from SPS and AGS experiments whereas other results like azimuthal HBT and K/π event-by-event fluctuations differ at some energies. In addition, new observations like the centrality dependence of chemical freeze-out parameters (T
ch and µB) or the smoothly increasing difference with decreasing energy in the elliptic flow v
2 between particles and corresponding anti-particles, are discussed.

Publisher

Journal

Year

Volume

10

Issue

6

Pages

1238-1241

Physical description

Dates

published
1 - 12 - 2012
online
4 - 12 - 2012

Contributors

  • Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA, 94720, USA

References

  • [1] Y. Aoki, G. Endrodi, Z. Fodor, S. D. Katz, K. K. Szabo, Nature 443, 675 (2006) http://dx.doi.org/10.1038/nature05120[Crossref]
  • [2] M. M. Aggarwal et al. (STAR Collaboration) arXiv:1007.2613
  • [3] S. Wheaton, J. Cleymans, M. Hauer, Comp. Phys. Comm. 180 (2009)
  • [4] L. Kumar for the STAR Collaboration, Cent. Eur. J. Phys., DOI:10.2478/s11534-012-0097-9 [Crossref]
  • [5] J. Cleymans, H. Oeschler and K. Redlich, Phys. Rev. C 59, 1663 (1999) http://dx.doi.org/10.1103/PhysRevC.59.1663[Crossref]
  • [6] J. Adams et al. (STAR Collaboration), Phys. Rev. Lett. 92, 052302 (2004) http://dx.doi.org/10.1103/PhysRevLett.92.052302[Crossref]
  • [7] S. Shi for the STAR Collaboration, Cent. Eur. J. Phys., DOI:10.2478/s11534-012-0081-4 [Crossref]
  • [8] J. C. Dunlop, M. A. Lisa, and P. Sorensen, Phys. Rev. C 84, 044914 (2011) http://dx.doi.org/10.1103/PhysRevC.84.044914[Crossref]
  • [9] J. Xu, L. -W. Chen, C. M. Ko, and Z. -W. Lin, Phys. Rev. C 85, 041901 (2012) http://dx.doi.org/10.1103/PhysRevC.85.041901[Crossref]
  • [10] C. Anson for the STAR Collaboration, arXiv:1107.1527
  • [11] V. Koch, A. Majumder and J. Randrup, Phys. Rev. Lett. 95, 182301 (2005) http://dx.doi.org/10.1103/PhysRevLett.95.182301[Crossref]
  • [12] S. V. Afanasiev et al., Phys. Rev. Lett. 86, 1965 (2001) http://dx.doi.org/10.1103/PhysRevLett.86.1965[Crossref]
  • [13] C. Alt et al. (NA49 Collaboration), Phys. Rev. C 79, 044910 (2009) http://dx.doi.org/10.1103/PhysRevC.79.044910[Crossref]
  • [14] J. Tian for the STAR Collaboration, Cent. Eur. J. Phys., DOI:10.2478/s11534-012-0145-5 [Crossref]
  • [15] X. Luo for the STAR Collaboration, arXiv:1111.5671

Document Type

Publication order reference

Identifiers

YADDA identifier

bwmeta1.element.-psjd-doi-10_2478_s11534-012-0149-1
JavaScript is turned off in your web browser. Turn it on to take full advantage of this site, then refresh the page.