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MODELING OF HADRON CHARGE CORRELATIONS IN HEAVY ION COLLISIONS AT NICA ENERGIES
- Authors: Zabrodin E.E.1, Korotkikh V.L.1, Lokhtin I.P.1, Petrushanko S.V.1, Snigirev A.M.1, Chernyshov A.S.1, Eyyubova G.K.1
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Affiliations:
- Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
- Issue: Vol 166, No 3 (2024)
- Pages: 340-346
- Section: Articles
- URL: https://bakhtiniada.ru/0044-4510/article/view/268162
- DOI: https://doi.org/10.31857/S0044451024090050
- ID: 268162
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Abstract
The model analysis of hadron charge correlations in heavy ion collisions was performed for energies available at NICA collider. The balance functions are considered as characteristics of such charge correlations. They represent the probability densities for oppositely charged particles to fall within a certain rapidity and azimuthal angle intervals. It has been shown that observed at STAR experiment at RHIC collider dependences of rapidity widths on centrality of gold-gold collisions at center-of-mass energies √SNN = 7.7 and 11.5 GeV per nucleon pair are reproduced by HYDJET++ model in the case of taking into account event-by-event conservation of electric charge for direct hadrons and finite values of isospin, strange and baryon chemical potentials.
About the authors
E. E. Zabrodin
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: lokhtin@www-hep.sinp.msu.ru
Russian Federation, 119991, Lenisnkie Gory, Moscow
V. L. Korotkikh
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: lokhtin@www-hep.sinp.msu.ru
Russian Federation, 119991, Lenisnkie Gory, Moscow
I. P. Lokhtin
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: lokhtin@www-hep.sinp.msu.ru
Russian Federation, 119991, Lenisnkie Gory, Moscow
S. V. Petrushanko
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: lokhtin@www-hep.sinp.msu.ru
Russian Federation, 119991, Lenisnkie Gory, Moscow
A. M. Snigirev
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: lokhtin@www-hep.sinp.msu.ru
Russian Federation, 119991, Lenisnkie Gory, Moscow
A. S. Chernyshov
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: lokhtin@www-hep.sinp.msu.ru
Russian Federation, 119991, Lenisnkie Gory, Moscow
G. Kh. Eyyubova
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Author for correspondence.
Email: lokhtin@www-hep.sinp.msu.ru
Russian Federation, 119991, Lenisnkie Gory, Moscow
References
- J. W. Harris and B. Muller, arXiv: 2308.05743.
- I. Arsene et al. (BRAHMS Collaboration), Nucl. Phys.A 757, 1 (2005).
- B.B. Back et al. (PHOBOS Collaboration), Nucl. Phys.A 757, 28 (2005).
- J. Adams et al. (STAR Collaboration), Nucl. Phys. A 757, 102 (2005).
- K. Adcox et al. (PHENIX Collaboration), Nucl. Phys. A 757, 184 (2005).
- B. Muller, J. Schukraft, and B. Wyslouch, Ann. Rev. Nucl. Part. Sci. 62, 361 (2012).
- N. Armesto and E. Scomparin, Eur. Phys. J. Plus 131, 52 (2016).
- ALICE Collaboration, arXiv: 2211.04834.
- D. Drijard et al., Nucl. Phys. B 155, 269 (1979).
- S. Bass, P. Danielewicz, and S. Pratt, Phys. Rev. Lett. 85, 2689 (2000).
- V. Vechernin, Symmetry 14, 21 (2022).
- C. Alt et al. (NA49 Collaboration), Phys. Rev. C 71, 034903 (2005).
- M. M. Aggarwal et al. (STAR Collaboration), Phys. Rev. C 82, 024905 (2010).
- B. I. Abelev et al. (STAR Collaboration), Phys. Lett. B 690, 239 (2010).
- L. Adamczyk et al. (STAR Collaboration), Phys. Rev. C 94, 024909 (2016).
- B. Abelev et al. (ALICE Collaboration), Phys. Lett. B 723, 267 (2013).
- J. Adam et al. (ALICE Collaboration), Eur. Phys. J. C 76, 86 (2016).
- S. Acharya et al. (ALICE Collaboration), Phys. Rev. C 100, 044903 (2019).
- A. Tumasyan et al. (CMS Collaboration), arXiv: 2307.11185.
- V. Abgaryan et al. (MPD Collaboration), Eur. Phys. A 58, 140 (2022).
- I. P. Lokhtin, L. V. Malinina, S. V. Petrushanko et al., Comput. Phys. Commun. 180, 779 (2009).
- И. П. Лохтин, Л. В. Малинина, С. В. Петрушанко и др., ЯФ 73, 2196 (2010).
- A. S. Chernyshov, G. Kh. Eyubova, V. L. Korotkikh et al., Chin. Phys. C 47, 084107 (2023).
- D. Drijard et al., Nucl. Phys. B 166, 233 (1980).
- J. Fu, J. Phys. G: Nucl. Part. Phys. 38, 065104 (2011).
- S. Pratt and C. Plumberg, Phys. Rev. C 104, 014906 (2021).
- I. P. Lokhtin and A. M. Snigirev, Eur. Phys. J. C 45, 211 (2006).
- T. Sjostrand, S. Mrenna, and P. Skands, JHEP 0605, 026 (2006).
- T. Sjostrand, S. Mrenna, and P. Skands, Comput. Phys. Commun. 178, 852 (2008).
- N. S. Amelin, R. Lednicky, T. A. Pocheptsov et al., Phys. Rev. C 74, 064901 (2006).
- N. S. Amelin, R. Lednicky, I. P. Lokhtin et al., Phys. Rev. C 77, 014903 (2008).
- G. Torrieri, S. Steinke, W. Broniowski et al., Comput. Phys. Commun. 167, 229 (2005).
- L. Adamczyk et al. (STAR Collaboration), Phys. Rev. C 96, 044904 (2017).
- A. V. Belyaev, L. V. Bravina, A. S. Chernyshov et al., J. Phys.Conf.Ser. 1690, 012117 (2020).
- O. Kodolova, M. Cheremnova, I. Lokhtin et al., Phys. Part. Nucl. 52, 658 (2021).
- M. Cheremnova, A. Chernyshov, Ye. Khyzhniak et al., Symmetry 14, 1316 (2022).
- S. A. Bass, M. Belkacem, M. Bleicher et al., Prog. Part. Nucl. Phys. 41, 255 (1998).
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