计算物理 ›› 2011, Vol. 28 ›› Issue (6): 942-948.

• 研究论文 • 上一篇    

黑洞阴影在SSD中的位置和形状

潘彩娟1, 马游1,2, 朱云锋1   

  1. 1. 百色学院 物理与电信工程系, 广西 百色 533000;
    2. 广西大学 电气工程学院, 广西 530004
  • 收稿日期:2011-01-11 修回日期:2011-06-07 出版日期:2011-11-25 发布日期:2011-11-25
  • 作者简介:潘彩娟(1965-),女,广西百色,副教授,主要从事力学教学及天体物理研究,E-mail:pancaiiuan@163.com

Shape and Position of a Black Hole Shadow in SSD

PAN Caijuan1, MA You1,2, ZHU Yunfeng1   

  1. 1. Department of Physics and Telecommunication Engineering, Baise University, Baise, Guangxi 533000, China;
    2. College of Electrical Engineering, Guangxi University, Guangxi 530004, China
  • Received:2011-01-11 Revised:2011-06-07 Online:2011-11-25 Published:2011-11-25

摘要: 假设旋转的黑洞在标准吸积盘内,在吸积盘的内边界等于最后稳定轨道的情况下,画出黑洞阴影在吸积盘的图像.通过定性和定量分析黑洞的形状和位置,发现对于相同质量的黑洞,黑洞阴影的大小及形状与黑洞的自旋参量有关.旋转黑洞阴影的形状和位置与它的旋转轴是不对称的,通过研究旋转轴与黑洞阴影的位置关系来确定黑洞的质量中心的位置及黑洞的旋转参量.

关键词: 吸积盘, 黑洞物理

Abstract: A rotating black hole is supposed to lie in a standard acc.retion disk.Imaging of the black hole shadow in an accretion disk are drawn as accretion disk inner boundary is equal to the last stable orbit.With qualitative and quantitative analysis of shape and position of a black hole,it is found that the size and shape of a black hole shadow for black holes with same mass are relevant to black hole spin.Shape and position of n rotating black hole shadow are asymmetrical relative to its rotating axis.The center of mass and rotation parameters of a black hole are determinated with position between rotating axis and black hole shadow.

Key words: accretion disk, black hole physics

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