上传用户：xkxiwypqqq资料价格：5财富值&&『』文档下载 ：『』&&『』学位专业：&关 键 词 ：&&&&&&&&权力声明：若本站收录的文献无意侵犯了您的著作版权，请点击。摘要:（摘要内容经过系统自动伪原创处理以避免复制，下载原文正常，内容请直接查看目录。）环绕黑洞的量子行动，本文重要做了两个方面的任务。一方面，我们应用协变标准失常和引力失常抵消办法研讨了(3+1)维和更高维渐近AdS的迁移转变带电黑弦的霍金辐射，分离导出了它们的霍金辐射电荷流、角动量流和能动张量流。分歧于黑洞，这些黑弦的拓扑构造可所以柱状或环状。在我们的剖析中，约化后的二维有用度规的行列式不须要限制在(？)=1的情况，全部剖析异常具有普通性，而且支撑霍金辐射是来源于视界上的一种量子效应的广泛意见。别的一方面，我们把Kerr/CFT对应性推行到五维迁移转变(带电)极端黑洞的对偶描写，详细包含五维视界被压扁的迁移转变极端Kerr黑洞和迁移转变带电的极端Cvetic一Youm黑洞，和五维哥德尔宇宙直达动的极端Kerr一Godel黑洞和迁移转变带电的极端EMCS一Godel黑洞。盘算注解，这些极端黑洞的远视界量子态对偶于二维的手征性共形场论，该共形场论与时空的迁移转变对称性有关。借助Cardy公式，获得对偶共形场论的与Bekenstein一Hawking熵分歧的微不雅熵，给出了这些极端黑洞熵的统计说明。因为五维黑洞有两个迁移转变，我们获得了两个彼此对易的二维Virasoro(？)代数。虽然视界被压扁的极端Cvetic一Youm黑洞和极端EMCS一Godel黑洞含有U(1)的标准场，但经由过程详细的盘算发明，这些标准场对Virasoro代数的中间荷没有进献。接上去，我们把极端Kerr一Godel黑洞的对偶描写推行到非极端情况。基于普通非极端Kerr一Godel黑洞配景上无质量标量场方程的低频径向波方程在接近视界的内部区域具有SL(2，R)L×SL(2，R)R的共形对称性，我们料想普通非极端Kerr一Godel黑洞对偶于一个二维无限温度的共形场论。为了支撑这个料想，我们分离盘算了对偶共形场论的熵和无质量标量场的接收截面，前者与Bekenstein一Hawking熵分歧，后者与尺度的二维含化学势的无限温度共形场论的接收截面雷同。相似的剖析和结论异样实用于普通非极端EMCS一Godel黑洞。另外，我们还研讨了黑弦和普通非极端情况下这些黑洞的热力学性质。重要成果包含：给出了(3+1)维和更高维黑弦的将宇宙学常数视为热力学变量的热力学第必定律；盘算了普通非极端视界被压扁的Cvetic一Youm黑洞的狭义Abbott一Deser质量和角动量，引力张力，偶极荷和偶极势，这些量知足热力学第必定律的积分情势和微分情势；我们在阁下两个体系中从新界说Kerr一Godel黑洞的角速度、静电势、温度和熵，把Kerr一Godel黑洞表里视界上的热力学第必定律改写成共形热力学情势。Abstract:Quantum operations around the black hole, this paper has done two aspects of the task. On the one hand, we use the standard covariant arrhythmia and discuss measures to offset the gravitational aberration (3+1) Hocking radiation and higher dimensional asymptotic AdS transition of charged black string, derived from the Hocking radiation charge separation flow, their angular momentum and energy momentum tensor flow. Different from black holes, the topological structure of these black strings can be so cylindrical or circular. In our analysis, the reduced dimension of the two dimensional useful metric is not required to limit the determinant in (? In the case of =1, all of the analysis of the anomaly is common, and it is a broad view of the quantum effect that is derived from the perspective of Hocking's radiation. The other hand, we put the implementation of Kerr/CFT corresponding to 5D transition (charged) dual extreme black holes contain a detailed description of five horizon was extreme Cvetic compressed transition extreme Kerr black hole and the transition of a charged Youm black hole, the extreme EMCS black hole and a Godel change of extreme Kerr migration and charged five dimensional Godel moving to the universe a Godel black hole. Computer notes, the quantum state of these dual hyperopia circles of extreme black holes in two-dimensional chiral conformal field theory, the conformal field theory and space related symmetry transition. By means of the Cardy formula, get the micro entropy dual conformal field theory and Bekenstein Hawking entropy differences, given that these extreme statistical entropy of black hole. Because there are two five dimensional black hole transition, we obtained two of the 2D Virasoro (to each other? Algebra. Although the horizon was extreme Cvetic squashed a Youm black hole and the extreme EMCS Godel black hole with U (1) standard, but through calculating the detailed process of invention, these standard field of Virasoro Algebra with no charge. Then we take the extreme Kerr Godel black hole's dual description into non extreme cases. Based on the ordinary non extreme Kerr Godel black hole background on the massless scalar field equation of radial wave equation with low frequency SL in the internal region near the horizon (2, R) L * SL (2, R) conformal symmetry R, we expect the ordinary non extreme Kerr Godel black hole is dual to a two-dimensional infinite the temperature of the conformal field theory. In order to support the expected, we isolated brooding dual conformal field theory and entropy without receiving section of massive scalar field, and the former Bekenstein Hawking entropy differences, the latter with infinite temperature scale with two-dimensional chemical potential conformal field theory similar to receiving section. Similar analysis and conclusions are also useful for ordinary non extreme EMCS a Godel black hole. In addition, we have studied the thermodynamic properties of these black holes in the case of black string and ordinary non extreme cases. Important results include: given (3+1) and higher dimensional black string will be regarded as the cosmological constant thermodynamic variable ther calculating common non extreme horizon is flattening of the Cvetic Youm Abbott Deser black hole in the mass and angular momentum, gravity load and tension, dipole dipole potential, the amount of content the thermodynamic law and differential integral will we in two from the new territories in your system of angular velocity, Kerr Godel black hole, the electrostatic potential temperature and entropy, put a Godel black hole in Kerr horizon thermodynamics first law of thermodynamics to rewrite the conformal situation.目录:摘要5-7Abstract7-8前言11-15第一章 绪论15-37&&&&1.1 黑洞热力学性质17-21&&&&1.2 量子反常与霍金辐射21-28&&&&&&&&1.2.1 维数约化22-24&&&&&&&&1.2.2 规范反常24-25&&&&&&&&1.2.3 引力反常25-27&&&&&&&&1.2.4 霍金辐射流27-28&&&&1.3 Kerr/CFT对应性28-34&&&&&&&&1.3.1 极端Kerr黑洞近视界几何31-33&&&&&&&&1.3.2 Virasoro代数与中心荷33-34&&&&&&&&1.3.3 微观熵34&&&&1.4 本文结构34-37第二章 渐近AdS转动带电黑弦的霍金辐射与协变反常37-51&&&&2.1 引言37-38&&&&2.2 协变反常与(3+1)维黑弦的霍金辐射38-45&&&&2.3 协变反常与高维黑弦的霍金辐射45-48&&&&2.4 小结与讨论48-51第三章 五维具有压扁视界的转动(带电)黑洞的Kerr/CFT对应性51-69&&&&3.1 引言51-52&&&&3.2 五维具有压扁视界的极端Kerr黑洞和CFT对偶52-57&&&&&&&&3.2.1 具有压扁视界的Kerr黑洞的近视界几何53-54&&&&&&&&3.2.2 中心荷与对偶CFT熵54-57&&&&3.3 具有压扁视界的极端Cvetic-Youm黑洞和CFT对偶57-63&&&&&&&&3.3.1 具有压扁视界的Cvetic-Youm黑洞和近视界几何57-60&&&&&&&&3.3.2 当q=2a~2-m时的CFT熵60-62&&&&&&&&3.3.3 当q=m时的CFT熵62-63&&&&3.4 Cvetic-Youm黑洞的热力学与CFT温度63-67&&&&3.5 小结67-69第四章 五维Godel宇宙中极端转动(带电)黑洞的全息对偶69-79&&&&4.1 引言69-70&&&&4.2 极端Kerr-Godel黑洞与CFT对偶70-74&&&&4.3 极端EMCS-Godel黑洞与CFT对偶74-77&&&&4.4 小结77-79第五章 五维Godel宇宙中转动黑洞的隐共形对称性79-91&&&&5.1 视界热力学与共形热力学80-83&&&&5.2 标量场方程83-85&&&&5.3 隐共形对称性85-87&&&&5.4 CFT熵和吸收截面87-89&&&&5.5 小结89-91第六章 总结与展望91-95附录A 有效作用量与霍金辐射95-101附录B 维数约化的非唯一性101-103附录C 五维G(o|¨)del宇宙中转动带电黑洞的守恒荷103-107参考文献107-119攻读学位期间发表的论文119-121发表论文他引详情121-129致谢129分享到：相关文献|