Abstract
We study the effect of the nucleon meson cloud on predictions of the Monte Carlo Glauber wounded nucleon model for AA, pA, and pp collisions. From the analysis of the data on the charged multiplicity density in AA collisions we find that the meson–baryon Fock component reduces the required fraction of binary collisions by a factor of ~2 for Au + Au collisions at √s = 0.2 TeV and ~1.5 for Pb + Pb collisions at √s = 2.76 TeV. For central AA collisions, the meson cloud can increase the multiplicity density by ~16–18%. We give predictions for the midrapidity charged multiplicity density in Pb + Pb collisions at √s = 5.02 TeV for the future LHC run 2. We find that the meson cloud has a weak effect on the centrality dependence of the ellipticity ϵ2 in AA collisions. For collisions of the deformed uranium nuclei at √s = 0.2 TeV, we find that the meson cloud may improve somewhat agreement with the data on the dependence of the elliptic flow on the charged multiplicity for very small centralities defined via the ZDCs signals. We find that the meson cloud may lead to a noticeable reduction of ϵ2 and the size of the fireball in pA and pp collisions.
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References
P. Huovinen, Int. J. Mod. Phys. E 22, 1330029 (2013); arXiv:1311.1849.
R. Derradi de Souza, T. Koide, and T. Kodama, Prog. Part. Nucl. Phys. 86, 35 (2016); arXiv:1506.03863.
U. Heinz and R. Snellings, Ann. Rev. Nucl. Part. Sci. 63, 123 (2013); arXiv:1301.2826.
H. Song, S. A. Bass, U. Heinz, and T. Hirano, Phys. Rev. C 83, 054910 (2011); Phys. Rev. C 86, 059903(E) (2012); arXiv:1101.4638.
B. Schenke, P. Tribedy, and R. Venugopalan, Phys. Rev. Lett. 108, 252301 (2012); arXiv:1202.6646.
B. Schenke, P. Tribedy, and R. Venugopalan, Phys. Rev. C 86, 034908 (2012); arXiv:1206.6805.
A. Bialas, M. Bleszynski, and W. Czyz, Nucl. Phys. B 111, 461 (1976).
D. Kharzeev and M. Nardi, Phys. Lett. B 507, 121 (2001); nucl-th/0012025.
L. D. McLerran and R. Venugopalan, Phys. Rev. D 49, 2233 (1994); hep-ph/9309289.
N. N. Nikolaev and B. G. Zakharov, Z. Phys. C 49, 607 (1991); Z. Phys. C 53, 331 (1992).
V. Barone, M. Genovese, N. N. Nikolaev, E. Predazzi, and B. G. Zakharov, Z. Phys. C 58, 541 (1993).
N. N. Nikolaev and B. G. Zakharov, Phys. Lett. B 332, 184 (1994); hep-ph/9403243.
F. E. Low, Phys. Rev. D 12, 163 (1975).
E. V. Shuryak, Rev. Mod. Phys. 65, 1 (1993).
A. Casher, H. Neuberger, and S. Nussinov, Phys. Rev. D 20, 179 (1979).
E. Gotsman and S. Nussinov, Phys. Rev. D 22, 624 (1980).
N. N. Nikolaev, B. G. Zakharov, and V. R. Zoller, JETP Lett. 59, 6 (1994); hep-ph/9312268.
N. N. Nikolaev and B. G. Zakharov, Phys. Lett. B 327, 149 (1994); hep-ph/9402209.
R. Fiore, N. N. Nikolaev, and V. R. Zoller, JETP Lett. 99, 363 (2014); arXiv:1403.1950.
A. Bialas and M. Jezabek, Phys. Lett. B 590, 233 (2004); hep-ph/0403254.
A. Bialas, A. Bzdak, and R. Peschanski, Phys. Lett. B 665, 35 (2008); arXiv:0804.2364.
A. Bzdak, Acta Phys. Polon. B 41, 2471 (2010); arXiv:0906.2858.
B. Alver, M. Baker, C. Loizides, and P. Steinberg, arXiv:0805.4411.
W. Broniowski, M. Rybczynski, and P. Bozek, Comput. Phys. Commun. 180, 69 (2009); arXiv:0710.5731.
M. Rybczynski, G. Stefanek, W. Broniowski, and P. Bozek, Comput. Phys. Commun. 185, 1759 (2014); arXiv:1310.5475.
B. B. Back et al. (PHOBOS Collab.), Phys. Rev. C 70, 021902 (2004); nucl-ex/0405027.
B. I. Abelev, et al. (STAR Collab.), Phys. Rev. C 79, 034909 (2009); arXiv:0808.2041.
M. Rybczynski and W. Broniowski; arXiv:1510.08242.
L. Adamczyk et al. (STAR Collab.), Phys. Rev. Lett. 115, 222301 (2015); arXiv:1505.07812.
P. Filip, R. Lednicky, H. Masui, and N. Xu, Phys. Rev. C 80, 054903 (2009).
S. A. Voloshin, Phys. Rev. Lett. 105, 172301 (2010); arXiv:1006.1020.
J. S. Moreland, J. E. Bernhard, and S. A. Bass, Phys. Rev. C 92, 011901 (2015); arXiv:1412.4708.
S. Chatterjee et al., Phys. Lett. B 758, 269 (2016); arXiv:1510.01311.
A. Bialas, W. Czyz, and W. Furmanski, Acta Phys. Polon. B 8, 585 (1977).
A. Bialas and W. Czyz, Acta Phys. Polon. B 10, 831 (1979).
P. Bozek, W. Broniowski, and M. Rybczynski; arXiv:1604.07697.
A. Bialas and A. Bzdak, Phys. Rev. C 77, 034908 (2008); arXiv:0707.3720.
S. Eremin and S. Voloshin, Phys. Rev. C 67, 064905 (2003); nucl-th/0302071.
C. Loizides, arXiv:1603.07375.
S. S. Adler et al. (PHENIX Collab.), Phys. Rev. C 89, 044905 (2014); arXiv:1312.6676.
J. Speth and A. W. Thomas, Adv. Nucl. Phys. 24, 83 (1997).
S. D. Drell and K. Hiida, Phys. Rev. Lett. 7, 199 (1961).
R. T. Deck, Phys. Rev. Lett. 13, 169 (1964).
A. B. Kaidalov, Phys. Rep. 50, 157 (1979).
M. L. Good and W. D. Walker, Phys. Rev. 120, 1857 (1960).
K. G. Boreskov, A. B. Kaidalov, and L. A. Ponomarev, Sov. J. Nucl. Phys. 17, 669 (1973); Sov. J. Nucl. Phys. 19, 514 (1974).
K. G. Boreskov, A. A. Grigorian, and A. B. Kaidalov, Sov. J. Nucl. Phys. 24, 411 (1976).
B. G. Zakharov and V. N. Sergeev, Sov. J. Nucl. Phys. 38, 947 (1983).
B. G. Zakharov and V. N. Sergeev, Sov. J. Nucl. Phys. 28, 689 (1978).
V. N. Gribov, Sov. Phys. JETP 29, 483 (1969).
A. Kaidalov, Nucl. Phys. A 525, 39 (1991).
K. Aamodt et al. (ALICE Collab.), Phys. Rev. Lett. 106, 032301 (2011); arXiv:1012.1657.
B. G. Zakharov, JETP Lett. 104, 6 (2016); arXiv:1605. 06012.
V. R. Zoller, Z. Phys. C 60, 141 (1993).
V. R. Zoller, Z. Phys. C 53, 443 (1992).
W. Melnitchouk, J. Speth, and A. W. Thomas, Phys. Rev. D 59, 014033 (1998); hep-ph/9806255.
H. Holtmann, A. Szczurek, and J. Speth, Nucl. Phys. A 596, 631 (1996); hep-ph/9601388.
J. D. Sullivan, Phys. Rev. D 5, 1732 (1972).
A. Szczurek and J. Speth, Nucl. Phys. A 555, 249 (1993).
A. B. Kaidalov and M. G. Poghosyan, Eur. Phys. J. C 67, 397 (2010); arXiv:0910.2050.
A. Capella and E. G. Ferreiro, Eur. Phys. J. C 72, 1936 (2012); arXiv:1110.6839.
B. Müller and K. Rajagopal, Eur. Phys. J. C 43, 15 (2005); hep-ph/0502174.
W. Broniowski and W. Florkowski, Phys. Rev. C 65, 024905 (2002); nucl-th/0110020.
D. Teaney and L. Yan, Phys. Rev. C 83, 064904 (2011); arXiv:1010.1876.
E. Retinskaya, M. Luzum, J.-Y. Ollitrault, Nucl. Phys. A 926, 152 (2014); arXiv:1401.3241.
C. Albajar et al. (UA1 Collab.), Nucl. Phys. B 335, 261 (1990).
J. Adam et al. (ALICE Collab.); arXiv:1509.07541.
B. Abelev et al. (ALICE Collab.), Eur. Phys. J. C 73, 2456 (2013); arXiv:1208.4968.
R. E. Ansorge et al. (UA5 Collab.), Z. Phys. C 43, 357 (1989).
M. Rybczynski, W. Broniowski, and G. Stefanek, Phys. Rev. C 87, 044908 (2013); arXiv:1211.2537.
A. Goldschmidt, Z. Qiu, C. Shen, and U. Heinz; arXiv:1502.00603.
H. Niemi, G. S. Denicol, H. Holopainen, and P. Huovinen, Phys. Rev. C 87, 054901 (2013); arXiv:1212.1008.
Z. Qiu and U. W. Heinz, Phys. Rev. C 84, 024911 (2011); arXiv:1104.0650.
A. Goldschmidt, Z. Qiu, C. Shen, and U. Heinz, Phys. Rev. C 92, 044903 (2015); arXiv:1507.03910.
A. J. Kuhlman and U. W. Heinz, Phys. Rev. C 72, 037901 (2005); nucl-th/0506088.
E. V. Shuryak, Phys. Lett. B 78, 150 (1978).
S. Chatrchyan et al. (CMS Collab.), Phys. Lett. B 718, 795 (2013); arXiv:1210.5482.
B. Abelev et al. (ALICE Collab.), Phys. Lett. B 719, 29 (2013); arXiv:1212.2001.
G. Aad et al. (ATLAS Collab.), Phys. Rev. Lett. 110, 182302 (2013); arXiv:1212.5198.
S. Chatrchyan et al. (CMS Collab.), J. High Energy Phys. 1009, 091 (2010); arXiv:1009.4122.
B. G. Zakharov, Phys. Rev. Lett. 112, 032301 (2014); arXiv:1307.3674.
B. G. Zakharov, J. Phys. G 41, 075008 (2014); arXiv:1311.1159.
W. Broniowski, P. Bozek, M. Rybczynski, and E. R. Arriola, Acta Phys. Polon. Supp. 8, 301 (2015); arXiv:1506.04362.
P. Bozek, Acta Phys. Polon. B 41, 837 (2010); arXiv:0911.2392.
M. Habich, G. A. Miller, and P. Romatschke, Eur. Phys. J. C 76, 408 (2016); arXiv:1512.05354.
J. Adam et al. (ALICE Collab.), Phys. Rev. C 91, 064905 (2015); arXiv:1412.6828.
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Published in Russian in Zhurnal Eksperimental’noi i Teoreticheskoi Fiziki, 2017, Vol. 151, No. 6, pp. 1011–1030.
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Zakharov, B.G. Monte Carlo Glauber wounded nucleon model with meson cloud. J. Exp. Theor. Phys. 124, 860–876 (2017). https://doi.org/10.1134/S1063776117050089
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DOI: https://doi.org/10.1134/S1063776117050089