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Non-equilibrium aspects of the black hole-thermal state correspondence in string theory.

机译:弦论中黑洞-热态对应的非平衡方面。

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摘要

This dissertation contains the author's contributions to the study of non-equilibrium aspects of the correspondence between thermal states of quantum gauge field theories and black holes in string theory. This correspondence is contained in the larger holographic gauge/gravity duality, or AdS/CFT correspondence of string theory and M-theory. The work herein is divided into six fairly independent components. (1) We present results of a numerical simulation of the classical evolution of the plane-wave matrix model, which is dual to M-theory in a plane-wave background. We find evidence for rapid thermalization of the matrix model, related by the duality to the formation of a black hole. (2) We relate classical entropy production to the growth of entanglement entropy in a simple closed quantum system, in agreement with previous results for open quantum systems, and briefly investigate the dependence on the choice of coarse-graining. (3) We study the dynamics of a simple quantum system of two coupled degrees of freedom, one of which is undergoing non-adiabatic evolution. We study the resulting velocity dependent forces and quantum back-reaction. (4) We study the evolution of entanglement entropy due to local quenches in the D1--D5 conformal field theory (CFT), deformed away from the orbifold point, and discuss how this is one stage in a thermalization process, dual to the formation of a stringy black hole. (5) We investigate the holographic dual of a local quench of a CFT, and argue that it should be interpreted as a superposition of geometries. (6) We propose a quantum field theory state dual to a small anti-de Sitter (AdS) black hole. Finally, we discuss how all these various investigations fit into the larger context of black hole physics and non-equilibrium dynamics.
机译:本论文包含了作者对量子力学领域理论的热态与弦理论中的黑洞之间的非平衡性研究的贡献。此对应关系包含在较大的全息规格/重力对偶性中,或弦论和M理论的AdS / CFT对应关系中。本文的工作分为六个相当独立的部分。 (1)我们提出了平面波矩阵模型经典演化的数值模拟结果,该模型对平面波背景下的M理论是双重的。我们发现基质模型快速热化的证据,其与黑洞形成的对偶关系有关。 (2)我们将经典熵的产生与简单封闭量子系统中纠缠熵的增长联系起来,与先前的开放量子系统结果相一致,并简要研究了对粗粒度选择的依赖。 (3)我们研究具有两个耦合自由度的简单量子系统的动力学,其中一个正在经历非绝热演化。我们研究所得的速度相关力和量子反作用。 (4)我们研究了D1-D5共形场理论(CFT)中局部淬灭引起的纠缠熵的演化,该纠缠熵远离圆点变形,并讨论了这是一个热化过程的一个阶段,对形成是双重的的黑洞。 (5)我们研究了CFT局部淬灭的全息对偶,并认为应将其解释为几何形状的叠加。 (6)我们提出了对小反德西特(AdS)黑洞对偶的量子场论状态。最后,我们讨论所有这些不同的研究如何适应黑洞物理学和非平衡动力学的更大范围。

著录项

  • 作者

    Asplund, Curtis Tor.;

  • 作者单位

    University of California, Santa Barbara.;

  • 授予单位 University of California, Santa Barbara.;
  • 学科 Physics Astrophysics.;Physics Theory.
  • 学位 Ph.D.
  • 年度 2012
  • 页码 197 p.
  • 总页数 197
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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