| 1. | Schwarzschild himself thought it not to be physical
史瓦西他自己认为它不是物质的。 |
| 2. | The schwarzschild radius of a solar mass black hole is about 3 km
太阳质量的黑洞的史瓦西半径约为3公里。 |
| 3. | The schwarzschild solution 1916
史瓦西解 |
| 4. | The region inside the event horizon is defined to be the region of space occupied by the black hole
在史瓦西半径以内的范围，被定义为黑洞所占有的空间。 |
| 5. | The schwarzschild radius is now known to be the radius of a non - rotating black hole , but was not well understood at that time
史瓦西半径就是现在知道的非旋转黑洞半径,但是在那时不是很好理解。 |
| 6. | In the second chapter we discuss the mass - defect in the schwarzshild field and r - n field , and if a = 0 the latter will reduce to the case in the former
第二章详细讨论了史瓦西场中及r - n场中的质量亏损效应，且当= 0时，后者就会退化为前者的情况。 |
| 7. | 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。 |
| 8. | 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。 |
| 9. | Soon after einstein published his general theory of relativity in the beginning of 20th century , karl schwarzschild found a mathematical solution of the theory to describe the spacetime structure of such object with spherical symmetry . that was the prelude to the study of black holes
爱因斯坦在二十世纪初发表了广义相对论后不久，史瓦西便利用广义相对论方程求得一个描述球对称天体附近时空结构的解，为黑洞的研究展开了序幕。 |
