Neutron Star Magnetic Field as for Nonzero Photon Mass

• 作者: Lue Xiaofu Wang Qingwu
• 来源期刊: 近代物理研究所和兰州重离子加速器实验室年报：英文版
• 学科: 物理学
• 关键词: 光子质量 表面磁场 中子星 非零 维里定理 脉冲星 科学家 标量
• 年，卷（期）: 2005,（1）
• 页码范围: 26-27
• 页数: 2页
• 分类号: O572.31

摘要

<正>After the discovered pulsars were identified as rotating magnetized neutron stars with an extremely large surface magnetic field of 1012-1014 G and - 1018 G could exist in the interior of star presumed from the scalar virial theorem, many scientists have investigated its origin and effects on the other properties of neutron star such as mass and radius. The neutron star is not of pure neutrons, it has a few percent protons as compared with neutrons. So, model, in which proton and neutron in dense nuclear matter behave