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Geometrical effective action: Gauge field theory without ghosts.

机译:几何有效作用:无鬼影的量具场论。

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摘要

Ghosts were invented by Feynman (1) in 1962 while trying to construct a quantum theory of gravity. Having convinced himself that there was no way in which the gravitational field could consistently escape quantization in a universe where everything else is subject to the laws of quantum mechanics, he was trying to see how these laws would work when applied to spacetime curvature. The first obstacle he faced was the non-Abelian character of the diffeomorphism group (the gauge group of gravity) which forces the gravitational field to act partly as its own source. In the language of Feynman graphs this means that gravitational charge (stress-energy) is carried by graviton lines as well as by all other lines and hence leaks all over every graph.;Feynman's key idea for solving the problem was to replace every Feynman propagator by its equivalent, an advanced Green's function minus a positive-frequency Wightman function, and to throw away all noncausal loops of advanced Green's functions;Feynman's discovery, and the work that it stimulated, made it seem as if the quantum theory of gauge fields cannot even be formulated without ghosts. It is the purpose of this dissertation to show that ghosts are in fact not needed, even in a manifestly covariant quantum theory, and that a gauge invariant quantum effective action can be introduced which, like the classical action from which one starts, is independent of ghosts and gauge-breaking terms.;In this dissertation a quantum effective action for gauge field theories is constructed that is gauge invariant and independent of the choice of gauge breaking terms in the functional integral that defines it. The loop expansion of this effective action leads to new Feynman rules, involving new vertex functions but without diagrams containing ghost lines. The new rules are given in full for the Yang-Mills field, both with and without coupling to fermions, and renormalization procedures are described. No BRST arguments are needed. (Abstract shortened by UMI.) ftn
机译:Feynman(1)于1962年尝试建立重力量子理论时发明了鬼魂。他已经使自己确信,万有引力场无法始终逃避量子化,而宇宙中的其他所有事物都受量子力学定律的约束,他试图了解这些定律在应用于时空曲率时将如何工作。他面临的第一个障碍是非同构群(重力标距群)的非阿贝尔性,这迫使重力场部分充当其自身的来源。用费曼图的语言来说,这意味着引力线(所有其他线)都承载着引力电荷(应力能量),因此在每个图上都会泄漏。费曼解决问题的关键思想是替换每一个费曼传播器等效地,高级格林函数减去正频率Wightman函数,并抛弃了高级格林函数的所有非因果循环;费曼的发现以及它所激发的工作使表观场的量子理论似乎无法甚至没有鬼魂。本文的目的是表明,即使在明显的协变量子理论中,实际上也不需要重影,并且可以引入轨距不变的量子有效作用,就像经典的起步作用一样,它独立于本论文构建了一种规范场理论的量子有效作用,该规范具有规范不变性,并且与定义其的功能积分中规范断裂项的选择无关。此有效动作的循环扩展会导致新的费曼规则,其中涉及新的顶点函数,但没有包含幻影线的图表。对于Yang-Mills场,无论是否耦合到费米子,都将完全给出新规则,并描述重归一化过程。不需要BRST参数。 (摘要由UMI缩短。)ftn

著录项

  • 作者

    Paris, Carmen Molina.;

  • 作者单位

    The University of Texas at Austin.;

  • 授予单位 The University of Texas at Austin.;
  • 学科 High energy physics.
  • 学位 Ph.D.
  • 年度 1996
  • 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

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