2020
DOI: 10.1016/j.physletb.2020.135452
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Light nuclei production in Au+Au collisions at sNN = 5–200 GeV from JAM model

Abstract: In relativistic heavy-ion collisions, the light nuclei production is sensitive to the baryon density fluctuations and can be used to probe the QCD phase transition. Based on the coalescence production of light nuclei, we can extract the neutron density fluctuation from the yield ratio of proton (p), deuteron (d) and triton (t), Np × Nt/N 2 d . In this work, we studied the production of proton, deuteron, triton in Au+Au collisions at √200 GeV from a transport model (JAM model). We presented the energy dependenc… Show more

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Cited by 44 publications
(26 citation statements)
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“…The following section presents comparisons of different experimental data (ALICE [33,36,37], STAR [38,39], E866 [39], E877 [39] and PHENIX [39] ) to the simulation results from UrQMD.…”
Section: Resultsmentioning
confidence: 99%
“…The following section presents comparisons of different experimental data (ALICE [33,36,37], STAR [38,39], E866 [39], E877 [39] and PHENIX [39] ) to the simulation results from UrQMD.…”
Section: Resultsmentioning
confidence: 99%
“…In this subsection, we study the multi-particle yield correlation tp/d 2 , which has recently attracted extensive attention [32,[59][60][61][62][63] and considered to be a probe for the structure of the QCD phase diagram [34]. Compared with other yield ratios discussed in the last subsection, it has been observed by the STAR experiment to show a nonmonotonic trend as the function of √ s NN in the most central Au-Au collisions as shown by the solid circles and squares with error bars in Fig.…”
Section: E Multi-particle Yield Correlation Tp/dmentioning
confidence: 99%
“…Such production mechanism possesses its unique characteristics. Many specific models and/or event-generators such as hybrid dynamical model (iEBE-MUSIC) [32], the Ultra-relativistic-Quantum-Molecular-Dynamics model (UrQMD) [33], Jet AA Mi-croscopic Transportation Model (JAM) [34], the parton and hadron cascade model (PACIAE) [35], etc., have been developed to include light nuclei formation via the nucleon coalescence and provided nice explanations for series of observables. Besides these two mechanisms, transport scenario is also proposed for light nuclei production, which assumes the existence of light nuclei in strongly-interacting hadronic matter and aims to study how light nuclei evolve during the hadronic system evolution [36][37][38][39].…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…Presently, there are many successful phenomenological models widely used to describe the production of hadrons and light nuclei in relativistic heavy-ion collisions 23 , 24 , such as the Ultra-relativistic Quantum Molecular Dynamics (UrQMD) approach 25 , a Multiphase Transport (AMPT) model 26 , and the Simulating Many Accelerated Strongly interacting Hadrons (SMASH) approach 27 . For the light (anti)nuclei production in terms of their yields, yield ratios, -spectra, flow, etc., either the coalescence models 28 35 or the statistical thermal approaches 36 39 are usually employed. The lightest nuclear cluster, i.e., deuterons, has been especially studied to shed light on the nuclei formation process.…”
Section: Introductionmentioning
confidence: 99%