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Volume 41 Issue 1
Mar.  2024
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Ang LI. Astrophysical and Laboratory Studies on the Equation of State of Neutron Stars[J]. Nuclear Physics Review, 2024, 41(1): 308-317. DOI: 10.11804/NuclPhysRev.41.2023CNPC36
Citation: Ang LI. Astrophysical and Laboratory Studies on the Equation of State of Neutron Stars[J]. Nuclear Physics Review, 2024, 41(1): 308-317. DOI: 10.11804/NuclPhysRev.41.2023CNPC36
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Astrophysical and Laboratory Studies on the Equation of State of Neutron Stars

  • Department of astronomy, Xiamen University, 361005

Funds: National SKA Program of China (2020SKA0120300); National Natural Science Foundation of China (12273028)
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  • Author Bio:

    Ang LI: E-mail: liang@xmu.edu.cn

  • Received Date: July 19, 2023
  • Revised Date: January 26, 2024
  • Available Online: March 14, 2024
    Graphical Abstract
    • Abstract
  • The equation of state of dense matter in neutron stars holds significant research significance in nuclear astrophysics, astrophysics, and dense QCD phase structure. It plays a decisive role in the structure, formation, and evolution of these stars. The direct detection of gravitational waves by LIGO has ushered in a golden age of neutron star research. This article presents our research progress on neutron star strangeness phase transitions, hyperon puzzle, and the evolution of temperature and frequency. We combine nuclear physics and astronomy to analyze these phenomena and also discuss ways of distinguishing different types of neutron stars based on current multi-messenger observations and model calculations of microscopic parameters in the equation of state.
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    • References (45)
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