In the chapter three a low dimensions non-stationary black hole entropy is calculates.
在第三章中，我们计算了一个低维动态黑洞的熵。
The origins of black hole entropy and the black hole information paradox have long been puzzled problems to most theoretical physicists.
黑洞熵的微观起源和黑洞信息佯谬一直是大多数理论物理学家困惑的问题。
We gave a new equation of state density by the generalized uncertainty relation, studied black hole entropy on degenerate background of sphere symmetry.
采用由广义不确定关系得到的新的态密度方程，研究了球对称退化背景下黑洞的熵。
With the density of entropy of curved space-time, we have calculated black hole entropy directly, and avoided the difficulty of solving the field equation.
用弯曲时空的熵密度对黑洞熵进行了直接计算，避免了求解场方程的困难。
This result indicates that the conclusion that black hole entropy is proportional to its area can be applied to horizon not only globally, but also locally.
这一结果表明，熵与视界面积成正比的结论，不仅适用于整个视界，也适用于视界面上的局部；
This thesis is devoted to investigating black hole entropy by using the membrane method, and trying to find a possible way of solving the black hole information problem.
本篇论文致力于通过膜模型研究黑洞的统计熵，并尝试寻找解决信息佯谬的办法。
We overcome some difficulty in mathematics and calculate the free energy and the entropy of black hole in high dimensions space-time.
我们克服了数学上的一些困难，在高维情形里计算了动态黑洞的自由能和熵。
Classically, one could violate the second law of thermodynamics by material entering a black hole disappearing from our universe and resulting in a decrease of the total entropy of the universe.
经典地，一个靠材料进入黑洞从我们的宇宙消失而且造成宇宙总熵减少就违反了热力学第二定律。
Using the first law of black hole mechanics, it follows that the entropy of a black hole is one quarter of the area of the horizon.
使用黑洞力学第一定律，它遵守黑洞熵是活动视界区域中的四分之一。
It was later suggested that black holes are maximum-entropy objects, meaning that the maximum entropy of a region of space is the entropy of the largest black hole that can fit into it.
它是后来提出的黑洞是最大熵的物体，意味空间的一个区域最大熵是固定它的最大黑洞熵。
A comparison with the total entropy of Black Hole shows that the two have the same order of magnitude.
结果表明，视界的熵与黑洞的总熵可达到同一数量级。
It is by now well known that one of the outstandingly unsolved questions in gravitational theory is the microscopic origin of black-hole thermodynamic entropy.
另外众所周知，在引力理论中一个还没有解决的重要问题是黑洞热力学特性的微观起源。
Therefore, we find the quantum states density becomes finite near the horizon of black hole and the divergence of entropy in the brick wall model is removed without any unnatural cutoff.
这样我们发现黑洞视界附近的量子态密度变得有限，从而消除了砖墙模型中熵的发散而不需要采取任何不自然的截断。
It is shown that the entropy of the black hole is proportional to the area of event horizon at any time.
结果表明，任一时刻黑洞熵都与黑洞事件视界面积成正比。
The extreme black hole is investigated and it is pointed out that the topological entropy only has the classical meaning and is not a quantum viewpoint.
还讨论了极端黑洞熵，指出拓扑熵只有经典意义而不是量子的观点。
In this paper, using the generalized uncertainty relation, we calculated the Numbers of quantum state and further the entropy of Vaidya-Bonner black hole was also obtained.
本文，利用广义测不准关系对黑洞熵的修正值进行了计算，给出了由广义测不准关系而引起的修正项。
In this paper, using the generalized uncertainty relation, we calculated the Numbers of quantum state and further the entropy of Vaidya-Bonner black hole was also obtained.
本文，利用广义测不准关系对黑洞熵的修正值进行了计算，给出了由广义测不准关系而引起的修正项。
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