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Structure of Rotating Neutron Stars in Uniform Strong Magnetic Field
  • ISSN号：0253-6102
  • 期刊名称：《理论物理通讯：英文版》
  • 时间：0
  • 分类：P145.6[天文地球—天体物理;天文地球—天文学]
  • 作者机构：[1]Department of Physics, South China University of Technology, Guangzhou 510641, China, [2]Department of Physics, Jinan University, Guangzhou 510632, China, [3]The Faculty of Information Technology, Macau University of Science and Technology, Macao, China
  • 相关基金：The project supported by National Natural Science Foundation of China under Grant Nos. 10647116 and 10575140 and the China Postdoctoral Science Foundation under Grant No. 2005037175
作者： WEN De-Hua[1], CHEN Wei[2], LIU Liang-Gang[3]
关键词： 旋转中子星, 均匀强磁场, 结构方程, 状态方程, structure, neutron star, strong magnetic field
中文摘要：

在一致强壮的磁场的旋转中子星的性质和变丑是计算的。磁场将弄软中子星物质的状态的方程并且在旋转中子星的结构上做明显的效果。如果磁场是超级的强壮(B = 10 ~(17 ) T ) ，团，半径，和变丑将有效地变得更小。

英文摘要：

Properties and deformations of the rotating neutron stars in uniform strong magnetic field are calculated. The magnetic field will soften the equation of state of the neutron star matters and make an obvious effect on the structure of the rotating neutron star. If the magnetic field is superstrong （B=10^17 T）, the mass, radius, and the deformation will become smaller effectively.

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期刊信息
  • 《理论物理通讯：英文版》
  • 中国科技核心期刊
  • 主管单位:中国科学院
  • 主办单位:中科院理论物理所 中国物理学会
  • 主编：孙昌浦
  • 地址：北京2735邮政信箱 中国科学院理论物理研究所编辑部
  • 邮编：100190
  • 邮箱：ctp@itp.ac.cn
  • 电话：010-62551495 62541813 62550630
  • 国际标准刊号：ISSN：0253-6102
  • 国内统一刊号：ISSN：11-2592/O3
  • 邮发代号:
  • 获奖情况:
  • 首届国家期刊奖,中国科学院优秀期刊特别奖,国家期刊奖百种重点期刊,中国期刊方阵“双高”期刊
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  • 被引量:342