Symmetry energy of strange quark matter and tidal deformability of strange quark stars

Xu, J.; Xia, Caichu; Lù, Zhongwen; Peng, Guang-Xiong; Zhao, Ya-Peng

doi:10.1007/s41365-022-01130-x

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Cited by 10 publications

(1 citation statement)

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“…One way to generally characterize dense nuclear matter is using nuclear empirical parameters defined from a series expansion around the isospin asymmetry. [23,[51][52][53] Among them, nuclear symmetry energy is critical in encoding the energy cost to make the matter more neutron rich. It is thus intriguing to obtain effective constraints over the nuclear symmetry energy with measurements in HICs.…”

Section: -3mentioning

confidence: 99%

Phase Transition Study Meets Machine Learning

Ma 马,

Pang 庞,

Wang 王

et al. 2023

Chinese Phys. Lett.

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Section: -3mentioning

confidence: 99%

Phase Transition Study Meets Machine Learning

Ma 马,

Pang 庞,

Wang 王

et al. 2023

Chinese Phys. Lett.

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Effects of sequential decay on collective flows and nuclear stopping power in heavy-ion collisions at intermediate energies

Xiao¹,

Li²,

Wang³

et al. 2023

NUCL SCI TECH

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In this study, the rapidity distribution, collective flows, and nuclear stopping power in $$^{197}$$ 197 Au+$$^{197}$$ 197 Au collisions at intermediate energies were investigated using the ultrarelativistic quantum molecular dynamics (UrQMD) model with GEMINI++ code. The UrQMD model was adopted to simulate the dynamic evolution of heavy-ion collisions, whereas the GEMINI++ code was used to simulate the decay of primary fragments produced by UrQMD. The calculated results were compared with the INDRA and FOPI experimental data. It was found that the rapidity distribution, collective flows, and nuclear stopping power were affected to a certain extent by the decay of primary fragments, especially at lower beam energies. Furthermore, the experimental data of the collective flows and nuclear stopping power at the investigated beam energies were better reproduced when the sequential decay effect was included.

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