黑洞熵

广义测不准关系与没有Brick-wall的黑洞熵

The Generalized Uncertainty Relation and Black Hole Entropy without Brick Wall

没有brick-wall的黑洞熵

Black hole entropy without brick-wall

新Tortoise坐标变换与任意加速带电动态黑洞熵

A new Tortoise coordinate transformation and entropy of arbitrarily accelerating charged black hole

探讨了黑洞熵与Hawking辐射的关系。

And also the relation between entropy of black hole and Hawking radiation is discussed .

利用brickwall模型研究具有高自旋的引力场和电磁场对Schwarzschild黑洞熵的量子修正。

Quantum correction to the entropy of a Schwarzschild black hole due to high spin fields of gravitation and electromagnetism was studied by brick wall model .

高自旋场对Schwarzschild黑洞熵的量子修正

Quantum correction to the entropy of Schwarzschild black hole due to high spin fields

在文〔1〕的基础上，进一步论证了黑洞熵可能是量子化的，其量子单位为2πKB；

A further investigation on the quantization of black-hole entropy which is of quantum unit , 2 π KB , is given baed on ref. [ 1 ] .

Atorus-like黑洞熵与能斯特定理

The Nernst Theorem and the Entropy of the A Torus-like Black Hole

把广义不确定原理引入黑洞熵的计算，采用薄膜brickwall模型，对一般静态黑洞外部标量场的熵进行了计算，得到了熵计算公式。

Taking into account the effect of the generalized uncertainty principle on the entropy of black hole and adopting the thin film brick-wall model , the entropy of the quantum scalar field in generalized static black holes is calculated . The general formula for the entropy is obtained .

利用改进的brick-wall模型推导出自旋为2的引力场对动态Vaidya-Bonner黑洞熵的贡献，在自然单位制中其值为A/2；

The contribution of gravitational field of spin 2 to the entropy of Vaidya-Bonner black hole is calculated by using thin film brick-wall model proposed by Zhao Zheng et al .

利用改进后的计算黑洞熵的brick-wall模型，计算了带电非稳态黑洞Vaidya-Bonner黑洞的熵，得到它的熵仍然与其世界面积成正比。

Via the improved brick-wall model proposed by t ' Hooft in 1985 , we calculate the entropy of charged non-stationary Vaidya-Bonner black hole and conclude that the entropy is proportional to its horizons .

广义不确定原理对一般静态黑洞熵的影响

Generalized uncertainty principle influences the entropy of generalized static black hole

视界邻域的几何与黑洞熵

Geometry of the neighborhood nearby the horizon and black hole entropy

中微子的自旋对黑洞熵的影响

Effect of spin on the black hole entropy due to neutrinos

广义测不准关系与黑洞熵的修正值

Generalized Uncertainty Principle and Correction Value to the Black Hole Entropy

也简短讨论了弦理论中的黑洞熵。

Black hole entropy in string theory is also briefly discussed .

第二部分介绍黑洞熵；

The second part is about the origins of black hole entropy ;

黑洞熵无截断薄层模型的改进与推广

Improvement and extension of the thin film brick wall model without cut-off

黑洞熵，黑洞信息佯谬及弯曲时空中的量子通讯

Black Hole Entropy , Black Hole Information Paradox & Quantum Teleportation in Curved Space-time

黑洞熵应该满足能斯特定理

Black hole entropy should satisfy Nernst theorem

计算结果表明所得到的黑洞熵与其视界面积成正比。

The result showed that this entropy is proportion to the area of event horizon .

高自旋场对静态球对称黑洞熵的贡献

The contribution of the high spinning gravitation field to the static black hole entropy with spherical-symmetry

从中揭示了黑洞熵与视界面积之间的内在联系，也进一步表明了黑洞熵是视界面上量子态的熵，是一种量子效应。

It is found that there is an internal relation between the event horizon and the entropy .

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。

The origins of black hole entropy and the black hole information paradox have long been puzzled problems to most theoretical physicists .

结果表明，任一时刻黑洞熵都与黑洞事件视界面积成正比。

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，通过适当选取截断因子，仍可得出黑洞熵与视界面积成正比的结论。

The re-sult shows that the entropy of the R-N black hole is still proportional to its surface area if we choose proper cut-off .

当取适当的贯穿系数时，得到黑洞熵与视界面积成正比的结论。

When we take an appropriate impenetrate coefficient , we can derive that the entropy of black hole is proportional to the area of horizon .

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。

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 .

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。

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 .

对于黑洞熵取不同修正时，我们建立了数值模型来模拟黑洞蒸发率的形式。

After that , we try to build a numerically applicable model for modification of the black hole entropy to simulate the formation of a black hole evaporation rate .