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Number of results

Journal

2012 | 10 | 6 | 1282-1284

Article title

Scaling properties and charge dependence of particle ratio fluctuations at RHIC

Authors

Content

Title variants

Languages of publication

EN

Abstracts

EN
It has been suggested that the existence of a QCD phase transition would cause an increase and divergence of fluctuations. Thus event-by-event particle ratio fluctuations could be used to study strangeness and baryon number fluctuations near the critical point in the QCD phase diagram. In this paper, we present dynamical K/π, p/π, and K/p ratio fluctuations from Au+Au collisions at $\sqrt {s_{NN} } $ = 7.7 to 200 GeV. Charge dependent results as well as multiplicity scaling properties of these fluctuation results are discussed. The STAR data are compared to different theoretical model predictions and previous experimental results.

Publisher

Journal

Year

Volume

10

Issue

6

Pages

1282-1284

Physical description

Dates

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

Contributors

author
  • National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, MI, 48824-1321, USA

References

  • [1] V. Koch, A. Majumder, J. Randrup, Phys. Rev. Lett. 95, 182301 (2005) http://dx.doi.org/10.1103/PhysRevLett.95.182301
  • [2] S.V. Afanasiev et al. [NA49 collaboration], Phys. Rev. Lett. 86, 1965 (2001) http://dx.doi.org/10.1103/PhysRevLett.86.1965[Crossref]
  • [3] C. Pruneau, S. Gavin, S. Voloshin, Phys. Rev. C 66, 044904 (2002) http://dx.doi.org/10.1103/PhysRevC.66.044904
  • [4] V. Koch, T. Schuster, Phys. Rev. C 81, 034910 (2010) http://dx.doi.org/10.1103/PhysRevC.81.034910
  • [5] C. Alt et al., Phys. Rev. C 79, 044910 (2009) http://dx.doi.org/10.1103/PhysRevC.79.044910
  • [6] B.I. Abelev et al. (for the STAR Collaboration), Phys. Rev. Lett. 103, 092301 (2009) http://dx.doi.org/10.1103/PhysRevLett.103.092301
  • [7] T.J. Tarnowsky (for the STAR Collaboration), J. Phys. G: Nucl. Part. Phys. 38, 124054 (2011) http://dx.doi.org/10.1088/0954-3899/38/12/124054
  • [8] T.J. Tarnowsky (for the STAR Collaboration), J. Phys. G 38, 124054 (2011) http://dx.doi.org/10.1088/0954-3899/38/12/124054
  • [9] T.J. Tarnowsky (for the STAR Collaboration), Acta Phys. Polon. Supp. 5, 515 (2012) http://dx.doi.org/10.5506/APhysPolBSupp.5.515[Crossref]
  • [10] M.M. Aggarwal et al. (for the STAR Collaboration), arXiv:1007.2613v1 [nucl-ex]
  • [11] T. Anticic et al. [NA49 collaboration], Phys. Rev. C 83, 061902(R) (2011) http://dx.doi.org/10.1103/PhysRevC.83.061902
  • [12] D. Kresan, V. Friese, PoS(CFRNC2006)017

Document Type

Publication order reference

Identifiers

YADDA identifier

bwmeta1.element.-psjd-doi-10_2478_s11534-012-0095-y
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