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Gravity and black holes in four and five dimensions.

机译:重力和黑洞有四个维度和五个维度。

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摘要

In this thesis we study several aspects of gravitational physics and black holes. We particularly focus on two areas of current research. The first involves finding a statistical description of black hole entropy within the gravitational picture. In this direction we work with the Mathur fuzzball proposal. The second area of study involves the construction and classification of black hole geometries in higher dimensional space-times.;In the second half of this work we investigate solution generating techniques for five dimensional space-times. We present a general method to add KK-monopole charge to any asymptotically flat, stationary, and axisymmetric solution of five dimensional General Relativity. The technique exploits the Maison formalism and the associated underlying SL(3, R ) invariance of the system. The key step involves identifying a particular element of the symmetry group which has the special property that its action changes asymptotically flat boundary conditions to KK-monopole asymptotics. Furthermore, we also develop a set of technical tools which allow us to apply the SL(3, R ) transformations to solutions produced by the Inverse Scattering method. As an example of our methods, we construct a new exact solution describing a static black ring in a KK-monopole background.;In the first half of this thesis we construct a family of asymptotically flat solutions carrying D1, D5 and momentum charges. These geometries describe the spectral flow of all the ground states of the D1-D5 system. After applying the spectral flow transformation in the near horizon region, the geometries are extended to asymptotically flat infinity by utilizing the general form of minimal supergravity solutions in six dimensions. By construction the solutions are a priori known to correspond to bound states of the three charges and as such can be interpreted as gravitational microstates of the 3-charge black hole. After giving the general form of the solution, we give an explicit example of the construction by considering in detail the geometry corresponding to a particular profile function.
机译:在本文中,我们研究了引力物理学和黑洞的几个方面。我们特别关注当前研究的两个领域。首先涉及在引力图中找到黑洞熵的统计描述。在这个方向上,我们将处理Mathur的模糊建议。研究的第二个领域涉及在高维时空中黑洞几何的构造和分类。在本工作的后半部分,我们研究五维时空的解生成技术。我们提出一种将KK单极电荷添加到任何五维广义相对论的渐近平坦,固定和轴对称解的通用方法。该技术利用了Maison形式主义和相关的系统底层SL(3,R)不变性。关键步骤涉及确定对称组的特定元素,该元素具有以下特殊性质:其作用将渐近平坦的边界条件变为KK单极渐近。此外,我们还开发了一套技术工具,使我们可以将SL(3,R)转换应用于通过逆散射方法生成的解。作为我们方法的一个例子,我们构造了一个新的精确解,它在KK单极背景下描述了一个静态黑环。在本论文的上半部分,我们构造了一个带有D1,D5和动量电荷的渐近平解族。这些几何形状描述了D1-D5系统所有基态的光谱流。在近地平线区域中应用频谱流变换后,通过利用六维中最小超重力解的一般形式,将几何形状扩展为渐近平坦的无穷大。通过构造,该解决方案是先验已知的,其对应于三个电荷的束缚状态,因此可以解释为3-电荷黑洞的重力微状态。在给出了解决方案的一般形式之后,我们通过详细考虑与特定轮廓函数相对应的几何结构,给出了结构的明确示例。

著录项

  • 作者

    Ford, Jonathan.;

  • 作者单位

    University of Toronto (Canada).;

  • 授予单位 University of Toronto (Canada).;
  • 学科 Physics Elementary Particles and High Energy.
  • 学位 Ph.D.
  • 年度 2009
  • 页码 140 p.
  • 总页数 140
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

  • 入库时间 2022-08-17 11:38:30

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