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黑洞吸积盘内边缘半径的演化
引用本文:汪定雄,杨兰田,何沙.黑洞吸积盘内边缘半径的演化[J].中国天文和天体物理学报,1995(2).
作者姓名:汪定雄  杨兰田  何沙
作者单位:中南民族学院物理系,华中师范大学物理系
基金项目:国家自然科学基金,国家攀登计划资助
摘    要:本文用广义相对论讨论了黑洞吸积盘内边缘半径r(ms)的演化规律。结果表明,吸积盘的中心黑洞在由Schwarzschild型向极端Kerr型演化的过程中,黑洞的角动量变化对r(ms)的影响始终比黑洞的质量变化对r(ms)的影响大。在此过程中r(ms)始终是连续、单调减小的。本文得出r(ms)对时间变化率的取值范围,并对其物理意义作了讨论。

关 键 词:黑洞吸积盘  内边缘半径

The Evolution of the Inner Marginal Radius of the Black-Hole Accretion Disk
WANG Ding-xiong,YANG Lan-tian,HE Sha.The Evolution of the Inner Marginal Radius of the Black-Hole Accretion Disk[J].Chinese Journal of Astronomy and Astrophysics,1995(2).
Authors:WANG Ding-xiong  YANG Lan-tian  HE Sha
Institution:WANG Ding-xiong;YANG Lan-tian;HE Sha(South-Central College for Nationalities)(Huazhong Normal Univertity)
Abstract:The evolution of the inner marginal radius r_(ms)of the black-hole accretion disk is investigated on the basis of general relativity. It is shown that r_(ms) is affected more strongly by the variation of black-hole angular momentum than that of blackhole mass during the whole evolution process from Schwarzschild black hole to extreme Kerr black hole. In addition,r_(ms) always decreases continuously and monotonously in this process. The range of values for the time derivative of r_(ms) is obtained and its physical meaning is discussed in this paper.
Keywords:black  hole accretion disk  inner marginal radius  
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