Schwarzschild himself thought it not to be physical.
史瓦西他自己认为它不是物质的。
For any object, there is a critical radius, called the Schwarzschild radius, at which its mass will form a black hole.
对于任何一个物体，都存在一个被称为史瓦西半径的临界半径，在这个半径以内的质量将形成一个黑洞。
In this paper we turn out the coherent-state expression of energy-momentum stress tensor in two dimensional Schwarzschild black holes.
讨论了一个二维黑洞的能量应力张量的相干态表示，并将这样得到的结果与已有的结果进行比较和讨论。
The entropy of the non-stationary and slowly changing spherically symmetric Schwarzschild space-time is calculated under local thermal balance.
研究了在视界附近局部热平衡下缓变动态球对称时空的熵。
The simplest type of black holes is the known as Schwarzschild black holes, named after the scientist who discovered this solution of General Relativity.
最简单的一种黑洞叫做希瓦兹凯尔德黑洞，以一个发现了广义相对论解答的科学家的名字命名。
The X-rays are sent off into space before the matter crosses the Schwarzschild radius and crashes into the singularity. Thus we can see this X-ray emission.
在物质穿过希瓦兹凯尔德半径，被压挤成单一体之前；x射线会进人太空，因而我们能够发现这种x射线辐射。
In this paper we turn out the coherent-state expression of energy-momentum stress tensor in two dimensional Schwarzschild black holes. The results have been discussed as well.
讨论了一个二维黑洞的能量应力张量的相干态表示，并将这样得到的结果与已有的结果进行比较和讨论。
A few months later, Karl Schwarzschild gave the solution for the gravitational field of a point mass, showing that something we now call a black hole could theoretically exist.
几个月之后，卡尔·史瓦西给出了点质量引力场解决方法，表明我们现在称做黑洞某物理论上可以存在。
Most physicists believed that they were a peculiar feature of the highly symmetric solution found by Schwarzschild, and that objects collapsing in nature would not form black holes.
大多数物理学家相信它们是史瓦西创立的高度相称性解的一个奇特的特征，而认为自然坍塌的物体就不形成黑洞。
This paper derives in detail the gravitational field of the sun by using the Schwarzschild metric, and expounds the advance of the Mercury's perihelion with the general theory of relativity.
用史瓦西度规详尽地推导了太阳引力场，用广义相对论解释了水星近日点的进动。
Using radiant exitance of Schwarzschild black hole, the radiation spectrums of Fermion field and Boson field of black hole are calculated out, and Wien's displacement laws are also obtained.
利用史瓦西黑洞的辐出度，导出了黑洞费米子场和玻色子场的辐射谱及其对应的维恩位移定律，并且得出二者的辐射谱及定律略有不同。
An object approaching simple Schwarzschild-type (non-rotating) black hole's center will appear to distant observers as having an increasingly slow descent as the object approaches the event horizon.
接近简单的史瓦西类型(非旋转)黑洞中心的物体将会对远距离的观察者当物体接近活动视界时候存在日益增加的慢降落。
An object approaching simple Schwarzschild-type (non-rotating) black hole's center will appear to distant observers as having an increasingly slow descent as the object approaches the event horizon.
接近简单的史瓦西类型(非旋转)黑洞中心的物体将会对远距离的观察者当物体接近活动视界时候存在日益增加的慢降落。
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