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Identified charged hadron production in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4 GeV with the STAR detector

The STAR Collaboration

TL;DR

This study measures identified charged-hadron (π^{±}, K^{±}, p, bar{p}) production at mid-rapidity in Au+Au collisions at √s_NN = 54.4 GeV with the STAR detector. By analyzing transverse-momentum spectra across nine centrality classes, it extracts bulk observables dN/dy, ⟨p_T⟩, particle ratios, and kinetic freeze-out parameters T_{kin} and ⟨β_T⟩ using blast-wave fits, as well as the Bjorken energy density product ε_{BJ} × τ. The results reveal mass-dependent spectral shapes and centrality trends consistent with radial flow, along with antiparticle–particle ratios approaching unity for pions and showing energy-dependent behavior for kaons and protons. Comparisons to AMPT and HIJING highlight strengths and limitations of current heavy-ion collision models in reproducing yields, mean transverse momenta, and energy-density scaling, offering constraints on the interplay between initial conditions and medium evolution. The observed ε_{BJ} × τ values exceed lattice-predicted phase-transition thresholds, indicating high initial energy density at formation time across energies and system sizes studied.

Abstract

We present results on the production of $π^{\pm}$, $K^{\pm}$, $p$, and $\bar{p}$ in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4 GeV using the STAR detector at RHIC, at mid-rapidity ($|y| <$ 0.1). Invariant yields of these particles as a function of transverse momentum are shown. We determine bulk properties such as integrated particle yields ($dN/dy$), mean transverse momentum ($\langle p_{T} \rangle$), particle ratios, which provide insight into the particle production mechanisms. Additionally, the kinetic freeze-out parameters ($T_\text{kin}$ and $\langle β_{T} \rangle$), which provide information about the dynamics of the system at the time of freeze-out, are obtained. The Bjorken energy density ($ε_{BJ}$), which gives an estimate of the energy density in the central rapidity region of the collision zone at the formation time $τ$, is calculated and presented as a function of multiplicity for various energies. The results are compared with those from the models such as A Multi-Phase Transport (AMPT) and Heavy Ion Jet INteraction Generator (HIJING) for further insights.

Identified charged hadron production in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4 GeV with the STAR detector

TL;DR

This study measures identified charged-hadron (π^{±}, K^{±}, p, bar{p}) production at mid-rapidity in Au+Au collisions at √s_NN = 54.4 GeV with the STAR detector. By analyzing transverse-momentum spectra across nine centrality classes, it extracts bulk observables dN/dy, ⟨p_T⟩, particle ratios, and kinetic freeze-out parameters T_{kin} and ⟨β_T⟩ using blast-wave fits, as well as the Bjorken energy density product ε_{BJ} × τ. The results reveal mass-dependent spectral shapes and centrality trends consistent with radial flow, along with antiparticle–particle ratios approaching unity for pions and showing energy-dependent behavior for kaons and protons. Comparisons to AMPT and HIJING highlight strengths and limitations of current heavy-ion collision models in reproducing yields, mean transverse momenta, and energy-density scaling, offering constraints on the interplay between initial conditions and medium evolution. The observed ε_{BJ} × τ values exceed lattice-predicted phase-transition thresholds, indicating high initial energy density at formation time across energies and system sizes studied.

Abstract

We present results on the production of , , , and in Au+Au collisions at = 54.4 GeV using the STAR detector at RHIC, at mid-rapidity ( 0.1). Invariant yields of these particles as a function of transverse momentum are shown. We determine bulk properties such as integrated particle yields (), mean transverse momentum (), particle ratios, which provide insight into the particle production mechanisms. Additionally, the kinetic freeze-out parameters ( and ), which provide information about the dynamics of the system at the time of freeze-out, are obtained. The Bjorken energy density (), which gives an estimate of the energy density in the central rapidity region of the collision zone at the formation time , is calculated and presented as a function of multiplicity for various energies. The results are compared with those from the models such as A Multi-Phase Transport (AMPT) and Heavy Ion Jet INteraction Generator (HIJING) for further insights.

Paper Structure

This paper contains 7 sections, 6 equations, 16 figures, 2 tables.

Figures (16)

  • Figure 1: The transverse momentum spectra for (a) $\pi^{+}$, (b) $K^{+}$, (c) $p$, (d) $\pi^{-}$, (e) $K^{-}$ and (f) $\bar{p}$ at mid-rapidity ($|y| < 0.1$) in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4 GeV for nine centrality classes. The spectra for all the centralities other than 0-5% are scaled for clarity. The curves represent the Bose-Einstein functional fit to pions, Levy-Tsallis fit to kaons, and double-exponential fit to protons and anti-protons for 0-5% centrality. The statistical and systematic uncertainties are added in quadrature.
  • Figure 2: The $\langle \rm{N_{part}}\rangle$ dependence of the normalized integrated particle yield ($dN/dy/(\langle \rm{N_{part}}\rangle/2$) for (a) $\pi^{+}$, (b) $K^{+}$, (c) $p$, (d) $\pi^{-}$, (e) $K^{-}$, (f) $\bar{p}$ at mid-rapidity ($|y| < 0.1$) in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4 GeV. The results are compared with the published results at other STAR energies BESSTAR:2008med. The statistical and systematic uncertainties are added in quadrature where the latter dominates. $\rm \langle N_{part}\rangle$ uncertainties are not combined in quadrature for clarity of plots.
  • Figure 3: The $\langle \rm{N_{part}}\rangle$ dependence of mean transverse momentum ($\langle p_{T} \rangle$) of (a) $\pi^{+}$, (b) $K^{+}$, (c) $p$, (d) $\pi^{-}$, (e) $K^{-}$, (f) $\bar{p}$ at mid-rapidity ($|y| < 0.1$) in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4 GeV. The results are compared with the published results at other STAR energies BESSTAR:2008med. The statistical and systematic uncertainties are added in quadrature where the latter dominates.
  • Figure 4: The $\langle \rm{N_{part}}\rangle$ dependence of the antiparticle to particle ratios (a) $\pi^{-}$/$\pi^{+}$, (b) $K^{-}$/$K^{+}$ and (c) $\bar{p}$/$p$ at mid-rapidity ($|y| <$ 0.1) in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4 GeV. The results are compared with the published results at other STAR energies BESSTAR:2008med. The statistical and systematic uncertainties are added in quadrature where the latter dominates.
  • Figure 5: The $\langle \rm{N_{part}}\rangle$ dependence of mixed ratios (a) $K^{+}$/$\pi^{+}$, (b) ${p}$/$\pi^{+}$, (c) $K^{-}$/$\pi^{-}$ and (d) $\bar{p}$/$\pi^{+}$ at mid-rapidity ($|y| <$ 0.1) in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4 GeV. The results are compared with the published results at other STAR energies BESSTAR:2008med. The statistical and systematic uncertainties are added in quadrature where the latter dominates.
  • ...and 11 more figures