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Constraints on the symmetry energy from PREX-II in the multimessenger era

Tong-Gang Yue1, Lie-Wen Chen1,*, Zhen Zhang2, and Ying Zhou3

  • 1School of Physics and Astronomy, Shanghai Key Laboratory for Particle Physics and Cosmology, and Key Laboratory for Particle Astrophysics and Cosmology (MOE), Shanghai Jiao Tong University, Shanghai 200240, China
  • 2Sino-French Institute of Nuclear Engineering and Technology, Sun Yat-sen University, Zhuhai 519082, China
  • 3Quantum Machine Learning Laboratory, Shadow Creator Inc., Shanghai 201208, China

  • *Corresponding author: lwchen@sjtu.edu.cn

Nontrivial features in the speed of sound inside neutron stars

D. Mroczek, M. C. Miller, J. Noronha-Hostler, and N. Yunes

Phys. Rev. D 110 123009 (2024)

Correlation between the symmetry energy slope and the deconfinement phase transition

Luiz L. Lopes, Debora P. Menezes, and Mateus R. Pelicer

Phys. Rev. C 109 045801 (2024)

Extended Skyrme effective interactions for transport models and neutron stars

Si-Pei Wang, Rui Wang, Jun-Ting Ye, and Lie-Wen Chen

Phys. Rev. C 109 054623 (2024)

Estimation of the slope of nuclear symmetry energy via charge radii of mirror nuclei

Sakshi Gautam, Anagh Venneti, Sarmistha Banik, and B.K. Agrawal

Nuclear Physics A 1043 122832 (2024)

Tensor and isovector–isoscalar terms of relativistic mean field model: Impacts on neutron-skin thickness, charge radius, and nuclear matter

N. Liliani, A.M. Nugraha, J.P. Diningrum, and A. Sulaksono

Nuclear Physics A 1042 122812 (2024)

Constraining a relativistic mean field model using neutron star mass–radius measurements I: nucleonic models

Chun Huang, Geert Raaijmakers, Anna L Watts, Laura Tolos, and Constança Providência

Monthly Notices of the Royal Astronomical Society 529 4650 (2024)

Relativistic description of dense matter equation of state and neutron star observables constrained by recent astrophysical observations

Raj Kumar, Sunil Kumar, Mukul Kumar, Queena, Gaurav Thakur, Mittal, and Shashi K. Dhiman

J. Phys. G: Nucl. Part. Phys. 51 085201 (2024)

Constraining equations of state for massive neutron star within relativistic mean field models

Raj Kumar, Anuj Sharma, Mukul Kumar, Sunil Kumar, Virender Thakur, and Shashi K. Dhiman

Eur. Phys. J. A 60 17 (2024)

Bayesian inference of the symmetry energy and the neutron skin in Ca48 and Pb208 from CREX and PREX-2

Zhen Zhang and Lie-Wen Chen

Phys. Rev. C 108 024317 (2023)

Neutron star matter based on a parity doublet model including the a0(980) meson

Yuk Kei Kong, Takuya Minamikawa, and Masayasu Harada

Phys. Rev. C 108 055206 (2023)

Statistical analysis of the effect of the symmetry energy on the crust-core transition density and pressure in neutron stars

Ilona Bednarek, Jan Sładkowski, Jacek Syska, and Wiesław Olchawa

Phys. Rev. C 108 055801 (2023)

Implications of isoscalar and isovector scalar meson mixed interaction on nuclear and neutron star properties

Sunil Kumar, Mukul Kumar, Raj Kumar, and Shashi K. Dhiman

Phys. Rev. C 108 055802 (2023)

α clustering in nuclei and its impact on the nuclear symmetry energy

Shuo Yang, Ruijia Li, and Chang Xu

Phys. Rev. C 108 L021303 (2023)

Correlation between the difference of charge radii in mirror nuclei and the slope parameter of the symmetry energy

Y. N. Huang, Z. Z. Li, and Y. F. Niu

Phys. Rev. C 107 034319 (2023)

Bayesian inference of neutron-star observables based on effective nuclear interactions

Jia Zhou, Jun Xu, and Panagiota Papakonstantinou

Phys. Rev. C 107 055803 (2023)

Observational constraint from the heaviest pulsar PSR J0952-0607 on the equation of state of dense matter in relativistic mean field model

Raj Kumar, Mukul Kumar, Virender Thakur, Sunil Kumar, Pankaj Kumar, Anuj Sharma, B. K. Agrawal, and Shashi K. Dhiman

Phys. Rev. C 107 055805 (2023)

New equations of state for dense nuclear matter properties

Anuj Sharma, Mukul Kumar, Sunil Kumar, Virender Thakur, Raj Kumar, and Shashi K. Dhiman

Nuclear Physics A 1040 122762 (2023)

Bayesian analysis of a relativistic hadronic model constrained by recent astrophysical observations

Bruno A de Moura Soares, César H Lenzi, Odilon Lourenço, and Mariana Dutra

Monthly Notices of the Royal Astronomical Society 525 4347 (2023)

A three-ranged Gogny interaction in touch with pion exchange: promising results to improve infinite matter properties

L. Batail, D. Davesne, S. Péru, P. Becker, A. Pastore, and J. Navarro

Eur. Phys. J. A 59 173 (2023)

Impact of symmetry energy on sound speed and spinodal decomposition in dense neutron-rich matter

Nai-Bo Zhang and Bao-An Li

Eur. Phys. J. A 59 86 (2023)

Decoding the nuclear symmetry energy event-by-event in heavy-ion collisions with machine learning

Yongjia Wang, Zepeng Gao, Hongliang Lü, and Qingfeng Li

Physics Letters B 835 137508 (2022)

Constraining equation of state of nuclear matter by charge-changing cross section measurements of mirror nuclei

Jun-Yao Xu, Zheng-Zheng Li, Bao-Hua Sun, Yi-Fei Niu, Xavier Roca-Maza, Hiroyuki Sagawa, and Isao Tanihata

Physics Letters B 833 137333 (2022)

Probing the high-density nuclear symmetry energy with the Ξ−/Ξ0 ratio in heavy-ion collisions at sNN≈3 GeV

Gao-Chan Yong, Bao-An Li, Zhi-Gang Xiao, and Zi-Wei Lin

Phys. Rev. C 106 024902 (2022)

Effects of an isovector scalar meson on the equation of state of dense matter within a relativistic mean field model

Virender Thakur, Raj Kumar, Pankaj Kumar, Vikesh Kumar, Mukul Kumar, C. Mondal, B. K. Agrawal, and Shashi K. Dhiman

Phys. Rev. C 106 045806 (2022)

Regression analysis of the nuclear symmetry energy for relativistic mean-field models

Ilona Bednarek, Wiesław Olchawa, Jan Sładkowski, and Jacek Syska

Phys. Rev. C 106 055805 (2022)

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