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Special Issue of the 4th Workshop on Quarks and Compact Stars (QCS2023)
Chengjun XIA, Renxin XU, Jinchuan WANG
2024, 41(3): 1-4.
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A Study of Effects from a0(980) Meson to Asymmetric Matter Based on a Parity Doublet Model
KONG Yukkei, HARADA Masayasu
2024, 41(3): 787-793. DOI: 10.11804/NuclPhysRev.41.QCS2023.04
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Parity Doublet Model for Baryon Octets Based on the Quark-line Diagram
GAO Bikai, KOJO Toru, HARADA Masayasu
2024, 41(3): 794-800. DOI: 10.11804/NuclPhysRev.41.QCS2023.03
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Equation of State Based on Color-Spin-Molecular Dynamics
YASUTAKE Nobutoshi, MARUYAMA Toshiki
2024, 41(3): 801-805. DOI: 10.11804/NuclPhysRev.41.QCS2023.06
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Molecular Dynamics for Spin Systems
MARUYAMA Toshiki, YASUTAKE Nobutoshi
2024, 41(3): 806-810. DOI: 10.11804/NuclPhysRev.41.QCS2023.07
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Pasta Phases in Dense Matter
SHEN Hong, HU Jinniu, JI Fan, WU Xuhao, JU Min
2024, 41(3): 811-817. DOI: 10.11804/NuclPhysRev.41.QCS2023.02
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Elastic Properties of Nuclear Pasta in Neutron-star Crusts
XIA Chengjun, MARUYAMA Toshiki, YASUTAKE Nobutoshi, TATSUMI Toshitaka, ZHANG Yingxun
2024, 41(3): 818-827. DOI: 10.11804/NuclPhysRev.41.QCS2023.12
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Effects of Three-Baryon Forces Constrained by Causality Condition on the Equation of State with Kaon Condensation
MUTO Takumi
2024, 41(3): 828-833. DOI: 10.11804/NuclPhysRev.41.QCS2023.08
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Is There a “hyperon puzzle” Problem in Neutron Star Study?
LI Ang
2024, 41(3): 834-838. DOI: 10.11804/NuclPhysRev.41.QCS2023.09
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Investigations on the Equation of State of Neutron Star Matter with Density-dependent Relativistic Mean-field Model
HUANG Kaixuan, HU Jinniu
2024, 41(3): 839-853. DOI: 10.11804/NuclPhysRev.41.QCS2023.10
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Study of Three-Baryon Systems in a Quark Model for Solution of Hyperon Puzzle
NAKAMOTO Choki
2024, 41(3): 854-857. DOI: 10.11804/NuclPhysRev.41.QCS2023.14
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Revisiting Effects of Hyperonization and Core-crust Transition on Tidal Deformability of Neutron Stars
LI Niu, YE Jing, WEI Sina, YANG Rongyao, JIANG Weizhou
2024, 41(3): 858-862. DOI: 10.11804/NuclPhysRev.41.QCS2023.16
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Rutherford’s Atomic Nucleus versus Landau’s Gigantic Nucleus: Does Nature Favor Flavor Symmetry?
XU Renxin
2024, 41(3): 863-871. DOI: 10.11804/NuclPhysRev.41.QCS2023.19
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寻找由奇异夸克物质构成的天体
邹泽城, 黄永锋, 张晓黎
2024, 41(3): 872-879. DOI: 10.11804/NuclPhysRev.41.QCS2023.05
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Strangelets at Finite Temperature
YOU Haosong, CHEN Huaimin, XU Jianfeng, XIA Chengjun, XU Renxin, PENG Guangxiong
2024, 41(3): 880-889. DOI: 10.11804/NuclPhysRev.41.QCS2023.18
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Compact Stars in F(R) Gravity Theory
KATSURAGAWA Taishi, NUMAJIRI Kota, CUI Yongxiang, NOJIRI Shin’ichi
2024, 41(3): 890-899. DOI: 10.11804/NuclPhysRev.41.QCS2023.11
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强磁化中子星磁场演化与自转演化的研究
李永宏, 李志兵, 高志福, 王辉
2024, 41(3): 900-909. DOI: 10.11804/NuclPhysRev.41.QCS2023.20
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Effect of Nucleon Superfluidity and Its Uncertainty on the Neutron Star Cooling
WANG Yanping, DONG Jianmin, BAO Xiaojun, WU Puxun
2024, 41(3): 910-916. DOI: 10.11804/NuclPhysRev.41.QCS2023.21
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原子核质量模型对预言新超重元素合成截面的影响
耿畅, 陈鹏辉, 牛菲, 冯兆庆
2024, 41(3): 917-925. DOI: 10.11804/NuclPhysRev.41.QCS2023.13
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