DYNAMICAL INSTABILITY OF GASEOUS MASSES APPROACHING SCHWARZSCHILD LIMIT IN GENERAL RELATIVITY
DYNAMICAL INSTABILITY OF GASEOUS MASSES APPROACHING SCHWARZSCHILD LIMIT IN GENERAL RELATIVITY
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DOI：
10.1086/147938
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发表时间：
1964-01-01
影响因子：
4.9
通讯作者：
CHANDRASEKHAR, S
中科院分区：
文献类型：
--
作者：
CHANDRASEKHAR, S
R & 1。125（2GM/c'）= 1。其中G是引力常数，c是光速，Rp是质量M的”引力半径”。在有关”准恒星”射电源的天文学发现中，施瓦茨希尔德极限的存在一直是最近讨论的主题。
R & 1. 125 (2GM/c')= 1. 125R „where G is the constant of gravitation, c is the velocity of light, and Rp is the" gravitational ra-dius" appropriateto the massM. The existence of the Schwarzschildlimit has been the subject of much recent discussion in the context of the astronomicaldiscoveries pertaining to the" quasistellar" radio sources.