Magnetic field and EoS of neutron star matter at finite temperature
Wang, QW; Lu, XF
刊名INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS
2015
卷号24期号:7页码:1550051
关键词Photon mass neutron star matter magnetic field
通讯作者Wang, QW (reprint author), Sichuan Univ, Coll Phys Sci & Technol, Chengdu 610064, Peoples R China.
英文摘要In this paper, magnetic field and equation of state (EoS) of neutron star matter are studied under relativistic mean field theory. A nonzero mass term of magnetic field in the Lagrangian is introduced, which depends on baryon density of charged particles. The magnetic field has not been treated as external as usual and the calculations of magnetic field strength at finite temperature reveal the existence of inflection points in certain densities.
学科主题Physics
类目[WOS]Physics, Nuclear ; Physics, Particles & Fields
关键词[WOS]ASYMMETRIC NUCLEAR-MATTER ; HEAVY-ION COLLISIONS ; PHOTON MASS ; EQUATION ; SURFACE
收录类别SCI
语种英语
内容类型期刊论文
源URL[http://ir.itp.ac.cn/handle/311006/20940]  
专题理论物理研究所_理论物理所1978-2010年知识产出
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GB/T 7714
Wang, QW,Lu, XF. Magnetic field and EoS of neutron star matter at finite temperature[J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS,2015,24(7):1550051.
APA Wang, QW,&Lu, XF.(2015).Magnetic field and EoS of neutron star matter at finite temperature.INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS,24(7),1550051.
MLA Wang, QW,et al."Magnetic field and EoS of neutron star matter at finite temperature".INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS 24.7(2015):1550051.
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