The Composition of Baryon in the Proto Neutron Star PSR J0348+0432

被引:14
|
作者
Zhao, Xian-Feng [1 ]
机构
[1] Southwest Petr Univ, Sch Sci, Chengdu 610500, Sichuan, Peoples R China
关键词
Hyperon; Relativistic mean field thoery; Neutron star; MATTER;
D O I
10.1007/s10773-018-03997-2
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The effect of the mesons f(0)(975)(named as f ), phi(1020)(named as phi) and on the properties of the proto neutron star PSR J0348 + 0432 is studied in the framework of the relativistic mean field theory considering the baryon octet. We find the central particle number density will decrease considering the mesons but will increase as the mesons f, phi or mesons f, phi and all being considered. We also find that the mesons f, phi and have little effect on the field strengths of mesons sigma and but have a greater influence on those of mesons . For the chemical potential of neutrons, the influence of these mesons is relative small but for the chemical potential of electrons the meson effect is relatively large. It is also found that the relative particle number density of n will decrease while those of p and sigma(-) will increase considering the effect of the mesons , or f, phi, or f, phi and . The relative particle number density of , sigma(0), sigma(+), (-) and (0) will decrease considering the effect of the mesons but will increase as the mesons f, phi or the mesons f, phi and all being considered.
引用
收藏
页码:1060 / 1070
页数:11
相关论文
共 50 条
  • [21] Constraints on the properties of the massive neutron star PSR J0348+0432 from the f0(975) and φ(1020) mesons
    Zhao, Xian-Feng
    EUROPEAN PHYSICAL JOURNAL A, 2014, 50 (05): : 1 - 6
  • [22] Effect of the mesons on the baryons distribution in the massive NS PSR J0348+0432
    Xian-Feng Zhao
    Astrophysics and Space Science, 2019, 364
  • [23] Probing the physical and mathematical structure of f(R)-gravity by PSR J0348+0432
    De Laurentis, Mariafelicia
    De Martino, Ivan
    INTERNATIONAL JOURNAL OF GEOMETRIC METHODS IN MODERN PHYSICS, 2015, 12 (04)
  • [24] Examination of the influence of the f0(975) and φ(1020) mesons on the surface gravitational redshift of the neutron star PSR J0348+0432
    Zhao, Xian-Feng
    PHYSICAL REVIEW C, 2015, 92 (05):
  • [25] Analytical model of massive Pulsar J0348+0432
    Jafry, M. Abdul Kayum
    Molla, Sajahan
    Islam, Rabiul
    Kalam, Mehedi
    ASTROPHYSICS AND SPACE SCIENCE, 2017, 362 (10)
  • [26] Analytical model of massive Pulsar J0348+0432
    M. Abdul Kayum Jafry
    Sajahan Molla
    Rabiul Islam
    Mehedi Kalam
    Astrophysics and Space Science, 2017, 362
  • [27] 大质量中子星PSR J0348+0432原生星的组成与结构
    洪斌
    贾焕玉
    母雪玲
    周霞
    天文学报, 2015, 56 (06) : 531 - 540
  • [28] The pulsar PSR J0348-0432 and strange stars
    Yu. L. Vartanyan
    A. K. Grigoryan
    A. A. Shaginyan
    Astronomy Letters, 2015, 41 : 343 - 350
  • [29] The Pulsar PSR J0348-0432 and Strange Stars
    Vartanyan, Yu. L.
    Grigoryan, A. K.
    Shaginyan, A. A.
    ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS, 2015, 41 (07): : 343 - 350
  • [30] Properties of proto neutron star PSR J0737-3039A
    赵先锋
    钟水蓉
    霍建立
    Chinese Physics C, 2022, (10) : 211 - 218