Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars-Reference-Cited by-同舟云学术

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Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars

Published:2011-09-23 Issue:4 Volume:312 Page:042006
ISSN:1742-6596
Container-title:Journal of Physics: Conference Series
language:
Short-container-title:J. Phys.: Conf. Ser.

Author:

Li Bao-An,Chen Lie-Wen,Gearheart Michael,Hooker Joshua,Ko Che Ming,Krastev Plamen G,Lin Wei-Kang,Newton William G,Wen De-Hua,Xu Chang,Xu Jun

Publisher

IOP Publishing

Subject

General Physics and Astronomy

Link

http://stacks.iop.org/1742-6596/312/i=4/a=042006/pdf

Reference107 articles.

1. Nuclear matter and its role in supernovae, neutron stars and compact object binary mergers

2. Neutron Star Structure and the Equation of State

3. The Physics of Neutron Stars

4. Neutron star observations: Prognosis for equation of state constraints

Cited by 13 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A Statistical Approach to Neutron Stars’ Crust–Core Transition Density and Pressure;Entropy;2023-12-13

2. Statistical analysis of the effect of the symmetry energy on the crust-core transition density and pressure in neutron stars;Physical Review C;2023-11-01

3. Regression analysis of the nuclear symmetry energy for relativistic mean-field models;Physical Review C;2022-11-17

4. Properties of Neutron stars with hyperon cores in parametrized hydrostatic conditions;International Journal of Modern Physics E;2018-11

5. Relativistic mean-field hadronic models under nuclear matter constraints;Physical Review C;2014-11-10

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