论文标题

双曲重力的仪表理论公式

Gauge Theory Formulation of Hyperbolic Gravity

论文作者

Ferrari, Frank

论文摘要

我们根据$ \ text {psl}(2,\ mathbb r)_ \ partiale $ circile demage ogguge ogguge ogguge ogguge ogguge of Flat Flat Connections的最通用的引力模型在任意定向的二维表面上具有恒定的负曲率(“双曲重力”)。这包括常规的JT重力,作为特殊情况的Dilichlet边界条件具有Dirichlet边界条件。一个关键要素是要意识到正确的量规组不是完整的$ \ text {psl}(2,\ mathbb r)$,而是一个子组$ \ text {psl}(2,\ mathbb r)_ {\ mathbb r)_ {。我们找到了具有相关边界项的四个可能的边界条件类别,可以独立应用于每个边界组件。 I类具有五个不相等的变体,对应于固定长度,尖端,固定角度的圆锥形缺陷或大缸形渐近区域的圆锥形缺陷,具有固定长度和外部曲率一个或大于一个。 II类精确地再现了通常的JT重力。特别是,通常的二阶公式的至关重要的外部曲率边界项是由仪表理论边界项自动生成的。 III类是更奇特的可能性,集成的外部曲率固定在边界上。 IV级是II类的Legendre转型;固定长度的约束被边界宇宙常数项所取代。

We formulate the most general gravitational models with constant negative curvature ("hyperbolic gravity") on an arbitrary orientable two-dimensional surface of genus $g$ with $b$ circle boundaries in terms of a $\text{PSL}(2,\mathbb R)_\partial$ gauge theory of flat connections. This includes the usual JT gravity with Dirichlet boundary conditions for the dilaton field as a special case. A key ingredient is to realize that the correct gauge group is not the full $\text{PSL}(2,\mathbb R)$, but a subgroup $\text{PSL}(2,\mathbb R)_{\partial}$ of gauge transformations that go to $\text{U}(1)$ local rotations on the boundary. We find four possible classes of boundary conditions, with associated boundary terms, that can be applied to each boundary component independently. Class I has five inequivalent variants, corresponding to geodesic boundaries of fixed length, cusps, conical defects of fixed angle or large cylinder-shaped asymptotic regions with boundaries of fixed lengths and extrinsic curvatures one or greater than one. Class II precisely reproduces the usual JT gravity. In particular, the crucial extrinsic curvature boundary term of the usual second order formulation is automatically generated by the gauge theory boundary term. Class III is a more exotic possibility for which the integrated extrinsic curvature is fixed on the boundary. Class IV is the Legendre transform of class II; the constraint of fixed length is replaced by a boundary cosmological constant term.

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