Abstract
The energy and centrality dependence of \(K_{S}^{0}\)-meson spectra measured by the STAR Collaboration at RHIC in \(\textrm{Au}+\textrm{Au}\) collisions over a wide range of \(\sqrt{s_{NN}}=7.7{-}200\) GeV was studied in the \(z\)-scaling approach. The scaling function \(\psi(z)\) was constructed and the self-similarity of \(K_{S}^{0}\)-meson production was confirmed. This observation is consistent with an abrupt decrease of the model parameter \(c_{\textrm{AuAu}}\) from the value of 0.16 at \(\sqrt{s}_{NN}=7.7\) and 11.5 GeV to about 0.09 at the top RHIC energy. The scaling parameter is interpreted as a specific heat of the produced medium. The non-trivial dependence of \(c_{\textrm{AuAu}}\) on the collision energy shows that \(K_{S}^{0}\) meson is much more sensitive to properties of nuclear medium than a non-identified negative hadron. The irregularities in the behavior of the specific heat parameter \(c_{\textrm{AuAu}}\) are considered as a possible indication of phase transition in nuclear matter.
REFERENCES
I. Arsene et al. (BRAHMS Collab.), Nucl. Phys. A 757, 1 (2005).
B. B. Back et al. (PHOBOS Collab.), Nucl. Phys. A 757, 28 (2005).
J. Adams et al. (STAR Collab.), Nucl. Phys. A 757, 102 (2005).
K. Adcox et al. (PHENIX Collab.), Nucl. Phys. A 757, 184 (2005).
STAR Collab., Studying the Phase Diagram of QCD Matter at RHIC, A STAR White Paper SN0598. https://drupal.star.bnl.gov/STAR/starnotes/public/ sn0598. Accessed June 1, 2014.
PHENIX Collab., The PHENIX Experiment at RHIC, Decadal Plan 2011–2020 (Brookhaven Natl. Labor., 2010).
G. Roland, K. Šafařík, and P. Steinberg, Prog. Part. Nucl. Phys. 77, 70 (2014).
P. Foka and M. A. Janik, Rev. Math. Phys. 1, 154 (2016).
M. S. Abdallah (STAR Collab.), Phys. Lett. B 827, 137003 (2022).
W. Busza, K. Rajagopal, and W. van der Schee, Ann. Rev. Nucl. Part. Sci. 68, 339 (2018).
J. Rafelski, Eur. Phys. J. Spec. Top. 229, 1 (2020).
J. Adam (STAR Collab.), Phys. Rev. C 102, 034909 (2020).
M. M. Aggarwal (STAR Collab.), Phys. Rev. C 83, 024901 (2011).
G. Agakishiev (STAR Collab.), Phys. Rev. Lett. 108, 072301 (2012).
C. Adler (STAR Collab.), Phys. Lett. B 595, 143 (2004).
H. E. Stanley, Introduction to Phase Transitions and Critical Phenomena (Oxford Univ. Press, London, 1971).
H. E. Stanley, Rev. Mod. Phys. 71, S358 (1999).
I. Zborovský and M. V. Tokarev, Phys. Rev. D 75, 094008 (2007).
M. V. Tokarev and I. Zborovský, Int. J. Mod. Phys. A 32, 1750029 (2017).
M. V. Tokarev, I. Zborovský, A. O. Kechechyan, and T. G. Dedovich, Phys. Part. Nucl. 51, 141 (2020).
I. Zborovský and M. Tokarev, Phys. Part. Nucl. Lett. 18, 302 (2021).
I. Zborovský and M. Tokarev, PoS (ICHEP2020), 575 (2021).
M. V. Tokarev (for the STAR Collab.), Int. J. Mod. Phys. Conf. Ser. 39, 1560103 (2015).
M. Tokarev, A. Kechechyan, and I. Zborovský, Nucl. Phys. A 993, 121646 (2020).
P. Koch, B. Müller, and J. Rafelski, Phys. Rep. 142, 167 (1986).
J. Rafelski, Eur. Phys. J. Spec. Top. 155, 139 (2008).
V. S. Stavinsky, Sov. J. Part. Nucl. 10, 949 (1979).
M. Tokarev and I. Zborovský, Nucl. Phys. A 1025, 122492 (2022).
J. Cleymans and K. Redlich, Phys. Rev. C 60, 054908 (1999).
S. Basu, S. Chatterjee, R. Chatterjee, T. K. Nayak, and B. K. Nandi, Phys. Rev. C 94, 044901 (2016).
ACKNOWLEDGMENTS
This work was partially supported by RVO61389005.
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Tokarev, M., Zborovský, I. Specific Heat of Nuclear Medium Probed by \({K_{S}^{0}}\) Mesons Produced in \(\textrm{Au}+\textrm{Au}\) Collisions at RHIC. Phys. Atom. Nuclei 85, 981–987 (2022). https://doi.org/10.1134/S1063778823010568
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DOI: https://doi.org/10.1134/S1063778823010568