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Number of results

Journal

2012 | 10 | 6 | 1230-1233

Article title

Measurements of heavy flavor and di-electron production at STAR

Authors

Content

Title variants

Languages of publication

EN

Abstracts

EN
Heavy quarks are produced early in the relativistic heavy ion collisions, and provide an excellent probe into the hot and dense nuclear matter created at RHIC. In these proceedings, we will discuss recent STAR measurements of heavy flavor production, to investigate the heavy quark interaction with the medium. Electromagnetic probes, such as electrons, provide information on the various stages of the medium evolution without modification by final stage interactions. Di-electron production measurements by STAR will also be discussed.

Keywords

Publisher

Journal

Year

Volume

10

Issue

6

Pages

1230-1233

Physical description

Dates

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

Contributors

author
  • Department of Physics and Astronomy, University of California, Los Angeles, USA

References

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  • [2] P. Kolb, U. Heinz, arXiv:nucl-th/0305084
  • [3] P. Huovinen, P.V. Ruuskanen, Annu. Rev. Nucl. Part. Sci. 56, 163 (2006) http://dx.doi.org/10.1146/annurev.nucl.54.070103.181236[Crossref]
  • [4] Z. Tang (STAR Collaboration), J. Phys. G 38, 124107 (2011) http://dx.doi.org/10.1088/0954-3899/38/12/124107
  • [5] J. Kapitan (STAR Collaboration), Eur. Phys. J. C 62, 217 (2009) http://dx.doi.org/10.1140/epjc/s10052-009-0992-4[Crossref]
  • [6] R. Reed (STAR Collaboration), J. Phys. G 38, 124185 (2011) http://dx.doi.org/10.1088/0954-3899/38/12/124185
  • [7] L. Ruan et al. (STAR Collaboration), arXiv:0805.4638
  • [8] Y. Zhang (STAR Collaboration), J. Phys. G 38, 124142 (2011) http://dx.doi.org/10.1088/0954-3899/38/12/124142
  • [9] J. Adams et al. Phys. Rev. Lett. 94, 062301 (2005) http://dx.doi.org/10.1103/PhysRevLett.94.062301[Crossref]
  • [10] B. I. Abelev et al. (STAR Collaboration), Phys. Rev. Lett. 106, 159902(E) (2011) http://dx.doi.org/10.1103/PhysRevLett.106.159902[Crossref]
  • [11] G. Wang (STAR Collaboration), Nucl. Phys. A 855, 319 (2011) http://dx.doi.org/10.1016/j.nuclphysa.2011.02.069[Crossref]
  • [12] M.M. Aggarwal et al. (STAR Collaboration), Phys. Rev. Lett. 105, 202301 (2010) http://dx.doi.org/10.1103/PhysRevLett.105.202301[Crossref]
  • [13] R. Rapp, Phys. Rev. C 63, 054907 (2001) http://dx.doi.org/10.1103/PhysRevC.63.054907[Crossref]
  • [14] J. Zhao (STAR Collaboration), J. Phys. G 38, 124134 (2011) http://dx.doi.org/10.1088/0954-3899/38/12/124134
  • [15] L. Ruan et al. (STAR Collaboration), Nucl. Phys. A 855, 269 (2011) http://dx.doi.org/10.1016/j.nuclphysa.2011.02.056[Crossref]
  • [16] L. Ruan et al. (STAR Collaboration), J. Phys. G: Nucl. Part. Phys. 36, 095001 (2009) http://dx.doi.org/10.1088/0954-3899/36/9/095001
  • [17] Z. Tang, XXII International Conference on Relativistic Nucleus-Nucleus Collisions (2011)
  • [18] M.M. Aggarwal et al. (STAR Collaboration), arXiv:1007.2613

Document Type

Publication order reference

Identifiers

YADDA identifier

bwmeta1.element.-psjd-doi-10_2478_s11534-012-0052-9
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