黑洞热力学

由于此引力场的普遍性，对Hawking热效应的研究以及对黑洞热力学性质的研究有着重要的物理意义。

Because the common of this grating field , the study of the Hawking therm effect and the Black Hole thermodynamics has a significant meaning .

这是由于Banerjee等人错误地假设了其中的待定函数H为多项式的形式，并且没有彻底运用黑洞热力学的麦克斯韦关系。

It is caused by that they made a wrong ansatz , that the undetermined function H is polynomial , and they did not apply the Maxwell relation in black hole thermodynamics in a good manner .

负能谱中的黑洞热力学

The Thermodynamics of Black Hole in Negative Energy Spectrum

随后，我们类比黑洞热力学的导出方法，推导出了全息屏的热力学第一定律。

Then we deduce the holographic screen thermodynamics analogously to black hole thermodynamics .

极端黑洞热力学研究的现状和未来黑洞热力学关系式

The Present Status and Future Development in the Study of Extreme Black Hole Thermodynamics

活动星系核中心黑洞热力学量的演化

The evolution of thermodynamical quantities of the central black holes in active galactic nuclei

关于黑洞热力学的四个定律

The four laws of black-hole thermodynamics

反之，裸奇性的出现必破坏黑洞热力学第三定律。

Conversely , the naked singularity appearing must destroy the third law of thermodynamics of black hole .

由此推断宇宙监督假设就是黑洞热力学第三定律。

Form here we infer that the cosmic censorship hypothesis is just the third law of thermodynamics of black hole .

概括了近年来极端黑洞热力学研究的主要结果、面临的挑战以及一些解决方案。

We review some main results , challenges and explanations that have appeared in the study of extreme black hole thermodynamics recently .

人们普遍相信，对黑洞热力学的深入研究会有助于我们建立引力的量子理论。

It is generally expected that a thorough understanding of the black hole thermodynamics will help us to establish the quantum theory of gravity .

现在，黑洞热力学的研究已经被推广到以视界为边界的时空热力学体系中，即：时空热力学。

It has extended the study of black hole thermodynamics to any spacetime with the horizon as the boundary of a thermodynamic system , viz .

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。

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 .

以黑洞热力学建立和热辐射研究为主线，简述了黑洞物理学研究中物理思想的发展轨迹。

The development of physical ideas is discussed briefly in the study of Black hole physics taking thermodynamics and heat radiation of Black hole as main line .

我们发现了目前的研究中存在的一些问题，其中一些问题在文章中已经被解决，另一些问题还有待研究。首先，我们研究了黑洞热力学的隧穿方法。

Some of them are resolved in this thesis , and others are still open questions . First , we investigate the tunneling method of black hole thermodynamics .

而且，如果认为量子隧穿过程为可逆过程，则量子隧穿效应中的结果与黑洞热力学第一、第二定律是一致的。

Moreover , if we consider the tunneling process as a reversible process , the result in Hawking radiation via tunneling is consistent with the first and second law of black hole thermodynamics .

具有内禀自旋的荷电稳态轴对称非Kerr-Newman黑洞的热力学性质

Thermodynamical properties of non-Kerr-Newman charged black hole with intrinsic spin

NUT-Kerr-Newman黑洞的热力学性质及其表面几何

Thermodynamical Properties and Surface Geometry of NUT Kerr Newman Black Holes

研究了一类具有质量四极矩的静态非Schwarzschild黑洞的热力学性质，这类黑洞存在热辐射，裸奇点处的视界温度受到强烈的影响。

The paper deals with the thermodynamic properties of a type of static non-Schwarzschild black holes with mass quadrupole moment . The black holes concerned have thermal radiation , affecting the event horizon temperature at singular points significantly .

最后，讨论了黑洞的热力学第三定律。

Lastly , the third law of thermodynamics of black-hole has been completely discussed .

经过我们的完善后，隧穿方法就可以得到黑洞相关热力学性质量子修正的正确结果。

We improve this method , and obtain the correct quantum correction of black hole entropy via tunneling method .

缓变动态Kerr-Newman黑洞的量子热力学性质

Quantum thermodynamical properties of the slowly changing nonstationary Kerr-Newman black hole

广义不确定关系与黑洞附近的热力学量

The generalized uncertainty relation and the thermodynamic quantities near the black holes

论文还研究了该黑洞的几何热力学的相变，发现相变在某些点是可以发生的。

We also study the phase transition and show that it can indeed take place at some points .

对具有双旋转参数的5维时空中，黑洞视界的热力学参量与宇宙视界的热力学参量进行了研究。

In this paper , in the two-parameter five-dimensional ( 5D ) rotating black hole , we discuss the thermodynamic parameters corresponding to the black hole 's horizon and the thermodynamic parameters corresponding to the cosmological horizon .

另外，我们构造了这些黑洞的整套①热力学度规，并计算分析了这些度规的Ricci标曲率。

The whole set of thermodynamical metrics for these black holes are also be constructed , their Ricci scalars are computed and analyzed .

欧氏作用量、配分函数与黑洞－整体单极热力学

Euclidean Action , Partition Function and Thermodynamics of a Black Hole-Global Monopole

同时，我们研究了一下黑洞的另外一些热力学性质。

At the same time , we study other thermodynamic charaters of the black hole .

Kerr-Newman黑洞的统计熵及黑洞热力学方程

Statistical Entropy and Thermodynamics Equations of the Black Hole of Kerr-Newman

将黑洞看作由裸黑洞和二维热力学面（黑洞的视界）组成的正则系综，利用量子统计方法给出黑洞Hawking辐射的能量谱。

When we take the black hole as a canonical ensemble composed of a naked black hole and the two-dimensional thermodynamic surface ( horizon of the black hole ), using the quantum statistical method , we derive the energy spectrum of the black hole Hawking radiation .