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Black holes, entropy functionals, and topological strings.

机译:黑洞,熵函数和拓扑字符串。

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摘要

This thesis is devoted to study of the connection between extremal black holes and topological strings. Important ingredient of this connection is the relation between Hartle-Hawking wave function associated to black holes and topological string partition function. This leads to a natural entropy functional defined on the moduli space of string compactifications. We discuss several examples of such entropy functionals.; We start by proposing a wave function for scalar metric fluctuations on S3 embedded in a Calabi-Yau. This problem maps to a study of non-critical bosonic string propagating on a circle at the self-dual radius. This can be viewed as a stringy toy model for a quantum cosmology. Then we formulate an entropy functional on the moduli space of Calabi-Yau compactifications. We find that the maximization of the entropy is correlated with the appearance of asymptotic freedom in the effective field theory. The points where the entropy is maximized correspond to points on the moduli which are maximal intersection points of walls of marginal stability for BPS states. We then turn to study of the entropy functional on the moduli space of two dimensional conformal field theories captured by the gauged WZW model whose target space is an abelian variety. This gives rise to the effective action on the moduli space of Riemann surfaces, whose critical points are attractive and correspond to Jacobian varieties admitting complex multiplication. The partition function is a generating function for the number of conformal blocks in rational conformal field theories. Finally, we study non-supersymmetric, extremal 4 dimensional black holes which arise upon compactification of type II superstrings on Calabi-Yau threefolds. We propose a generalization of the OSV conjecture for higher derivative corrections to the non-supersymmetric black hole entropy, in terms of the one parameter refinement of topological string introduced by Nekrasov. We also study the attractor mechanism for non-supersymmetric black holes and show how the inverse problem of fixing charges in terms of the attractor value of Calabi-Yau moduli can be explicitly solved.
机译:本文致力于研究极端黑洞与拓扑弦之间的联系。这种连接的重要组成部分是与黑洞相关的Hartle-Hawking波函数与拓扑字符串分配函数之间的关系。这导致在弦压缩的模空间上定义的自然熵泛函。我们讨论了这种熵函数的几个例子。我们首先针对嵌入在Calabi-Yau中的S3提出标量度量波动的波动函数。该问题映射到对非临界玻色弦在自对角半径的圆上传播的研究。这可以看作是量子宇宙学的严格模型。然后,我们在Calabi-Yau紧致化的模量空间上构造一个熵泛函。我们发现,在有效场论中,熵的最大值与渐近自由的出现有关。熵最大化的点对应于模上的点,该点是BPS状态的边际稳定性壁的最大交点。然后,我们研究由目标空间为阿贝尔变种的规范WZW模型捕获的二维共形场理论的模空间上的熵泛函。这引起了对黎曼曲面模量空间的有效作用,其临界点很吸引人,并且对应于允许复数乘法的雅可比变量。分区函数是有理保形场理论中保形块数量的生成函数。最后,我们研究了在Calabi-Yau上三倍型II型超弦压实后出现的非超对称,极角4维黑洞。根据Nekrasov引入的拓扑字符串的一个参数细化,我们提出了OSV猜想的一般化,以对非超对称黑洞熵进行更高的导数校正。我们还研究了非超对称黑洞的吸引子机制,并展示了如何根据Calabi-Yau模的吸引子值来明确解决固定电荷的反问题。

著录项

  • 作者单位

    Harvard University.;

  • 授予单位 Harvard University.;
  • 学科 Physics Theory.
  • 学位 Ph.D.
  • 年度 2007
  • 页码 192 p.
  • 总页数 192
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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