Czasopismo
Tytuł artykułu
Autorzy
Warianty tytułu
Języki publikacji
Abstrakty
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.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Numer
Strony
1230-1233
Opis fizyczny
Daty
wydano
2012-12-01
online
2012-12-04
Twórcy
autor
- Department of Physics and Astronomy, University of California, Los Angeles, USA, gwang@physics.ucla.edu
Bibliografia
- [1] J. Rafelski, B. Muller, Phys. Rev. Lett. 48, 1066 (1982) http://dx.doi.org/10.1103/PhysRevLett.48.1066[Crossref]
- [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
Typ dokumentu
Bibliografia
Identyfikatory
Identyfikator YADDA
bwmeta1.element.-psjd-doi-10_2478_s11534-012-0052-9