| 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 radiation spectrum and wien ' s displancement law of schwarzschild black hole
黑洞的辐射谱及辐射定律 |
| 3. | 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。 |
| 4. | The schwarzschild solution 1916
史瓦西解 |
| 5. | Electromagnetic energy - momentum tensor in external region of schwarzschild black hole in melvin ' s magnetic universe
黑洞外部区域的电磁场能量动量张量 |
| 6. | 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。 |
| 7. | 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。 |
| 8. | 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。 |
| 9. | 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。 |
| 10. | 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。 |
