Abstract
The flavor dependence of the medium modification factor R pp for pp collisions has been studied for a scenario with formation of a small-size quark-gluon plasma (QGP) for RHIC (\(\sqrt s \)= 0.2 TeV) and LHC (\(\sqrt s \)= 2.76 TeV) energies. It has been found that at p T ~ 10 GeV the pion spectrum is suppressed by ~20–30 (25–35)% for RHIC (LHC), for D (B) mesons the suppression effect is smaller by a factor of ~0.7–0.8 (0.5). The flavor hierarchy R π pp < R D pp < R B pp is held at p T ≲ 20 GeV for RHIC and at p T ≲ 70 GeV for LHC. This gives a significant reduction of the heavy-to-light ratios of the nuclear modification factors R AA as compared to that in the standard scenario without the QGP production in pp collisions.
Similar content being viewed by others
References
B. G. Zakharov, Phys. Rev. Lett. 112, 032301 (2014); arXiv:1307.3674.
P. Bozek, Acta Phys. Polon. B 41, 837 (2010); arXiv:0911.2392.
J. Casalderrey-Solana and U. A. Wiedemann, Phys. Rev. Lett. 104, 102301 (2010); arXiv:0911.4400.
R. Campanini, G. Ferri, and G. Ferri, Phys. Lett. B 703, 237 (2011); arXiv:1106.2008.
V. Topor Pop, M. Gyulassy, J. Barrette, C. Gale, and A. Warburton, Phys. Rev. C 86, 044902 (2012); arXiv:1203.6679.
A. Bzdak, B. Schenke, P. Tribedy, and R. Venugopalan, Phys. Rev. C 87, 064906 (2013); arXiv:1304.3403.
E. Shuryak and I. Zahed, Phys. Rev. C 88, 044915 (2013); arXiv:1301.4470.
V. Khachatryan et al. (CMS Collab.), J. High Energy Phys. 1009, 091 (2010).
R. Field, Acta Phys. Polon. B 42, 2631 (2011); arXiv:1110.5530.
H. L. Vargas et al. (ALICE Collab.), J. Phys.: Conf. Ser. 389, 012004 (2012); arXiv:1208.0940.
B. G. Zakharov, J. Phys. G 41, 075008 (2014); arXiv:1311.1159.
B. G. Zakharov, JETP Lett. 88, 781 (2008).
B. G. Zakharov, JETP Lett. 93, 683 (2011); arXiv:1105.2028.
B. G. Zakharov, JETP Lett. 96, 616 (2013); arXiv:1210.4148.
B. G. Zakharov, J. Phys. G 40, 085003 (2013); arXiv:1304.5742.
B. G. Zakharov, JETP Lett. 63, 952 (1996), JETP Lett. 65, 615 (1997), JETP Lett. 70, 176 (1999), Phys. At. Nucl. 61, 838 (1998).
T. Renk, J. Phys.: Conf. Ser. 509, 012022 (2014); arXiv:1309.3059.
S. S. Adler et al. (PHENIX Collab.), Phys. Rev. Lett. 96, 032301 (2006).
B. I. Abelev et al. (STAR Collab.), Phys. Rev. Lett. 98, 192301 (2007); arXiv:nucl-ex/0607012; Phys. Rev. Lett. 106, 159902(E) (2011).
S. Sakai et al. (ALICE Collab.), http://qm2012.bnl.gov/default.asp.
B. Abelev et al. (ALICE Collab.), J. High Energy Phys. 1209, 112 (2012); arXiv:1203.2160.
Y. L. Dokshitzer and D. E. Kharzeev, Phys. Lett. B 519, 199 (2001).
P. Aurenche and B. G. Zakharov, JETP Lett. 90, 237 (2009); arXiv:0907.1918.
B. A. Kniehl, G. Kramer, and B. Potter, Nucl. Phys. B 582, 514 (2000).
T. Sjostrand, L. Lonnblad, S. Mrenna, and P. Skands, Nucl. Phys. B 582, 514 (2000). arXiv:hep-ph/0308153.
B. G. Zakharov, JETP Lett. 80, 617 (2004); hepph/0410321.
B. G. Zakharov, JETP Lett. 86, 444 (2007); arXiv:0708.0816.
P. Lévai and U. Heinz, Phys. Rev. C 57, 1879 (1998).
O. Kaczmarek and F. Zantow, Phys. Rev. D 71, 114510 (2005).
N. N. Nikolaev and B. G. Zakharov, Phys. Lett. B 327, 149 (1994).
Yu. L. Dokshitzer, V. A. Khoze, and S. I. Troyan, Phys. Rev. D 53, 89 (1996).
B. Müller and K. Rajagopal, Eur. Phys. J. C 43, 15 (2005); arXiv:hep-ph/0502174.
L. McLerran, M. Praszalowicz, and B. Schenke, arXiv:1306.2350.
S. Borsanyi, Nucl. Phys. A 904–905, 270c (2013); arXiv:1210.6901.
B. I. Abelev et al. (STAR Collab.), Phys. Rev. C 79, 034909 (2009).
S. Chatrchyan et al. (CMS Collab.), J. High Energy Phys. 1108, 141 (2011).
P. Aurenche, M. Fontannaz, J. P. Guillet, B. A. Kniehl, and M. Werlen, Eur. Phys. J. C 13, 347 (2000); hepph/9910252.
M. Cacciari, P. Nason, and R. Vogt, Phys. Rev. Lett. 95, 122001 (2005); hep-ph/0502203.
M. Cacciari, S. Frixione, N. Houdeau, M. L. Mangano, P. Nason, and G. Ridolfi, J. High Energy Phys. 1210, 137 (2012); arXiv:1205.6344.
Author information
Authors and Affiliations
Corresponding author
Additional information
The article is published in the original.
Rights and permissions
About this article
Cite this article
Zakharov, B.G. Flavor dependence of jet quenching in pp collisions and its effect on R AA for heavy mesons. Jetp Lett. 103, 363–368 (2016). https://doi.org/10.1134/S0021364016060126
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S0021364016060126