Stochastic Gravity: Theory and Applications

IF 26.3 2区 物理与天体物理 Q1 PHYSICS, PARTICLES & FIELDS
Bei Lok Hu, Enric Verdaguer
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引用次数: 214

Abstract

Whereas semiclassical gravity is based on the semiclassical Einstein equation with sources given by the expectation value of the stress-energy tensor of quantum fields, stochastic semi-classical gravity is based on the Einstein-Langevin equation, which has, in addition, sources due to the noise kernel. The noise kernel is the vacuum expectation value of the (operator-valued) stress-energy bitensor, which describes the fluctuations of quantum-matter fields in curved spacetimes. A new improved criterion for the validity of semiclassical gravity may also be formulated from the viewpoint of this theory. In the first part of this review we describe the fundamentals of this new theory via two approaches: the axiomatic and the functional. The axiomatic approach is useful to see the structure of the theory from the framework of semiclassical gravity, showing the link from the mean value of the stress-energy tensor to the correlation functions. The functional approach uses the Feynman-Vernon influence functional and the Schwinger-Keldysh closed-time-path effective action methods. In the second part, we describe three applications of stochastic gravity. First, we consider metric perturbations in a Minkowski spacetime, compute the two-point correlation functions of these perturbations and prove that Minkowski spacetime is a stable solution of semiclassical gravity. Second, we discuss structure formation from the stochastic-gravity viewpoint, which can go beyond the standard treatment by incorporating the full quantum effect of the inflaton fluctuations. Third, using the Einstein-Langevin equation, we discuss the backreaction of Hawking radiation and the behavior of metric fluctuations for both the quasi-equilibrium condition of a black-hole in a box and the fully nonequilibrium condition of an evaporating black hole spacetime. Finally, we briefly discuss the theoretical structure of stochastic gravity in relation to quantum gravity and point out directions for further developments and applications.

Abstract Image

随机重力:理论与应用
半经典引力基于半经典爱因斯坦方程,其源由量子场的应力-能量张量的期望值给出,而随机半经典引力基于爱因斯坦-朗之万方程,其源由噪声核给出。噪声核是描述弯曲时空中量子-物质场波动的(算符值)应力-能量位传感器的真空期望值。从这一理论的观点出发,还可以提出一种新的改进的半经典引力有效性判据。在这篇综述的第一部分,我们通过两种方法描述了这一新理论的基本原理:公理化和泛函。公理化方法有助于从半经典引力的框架来看理论的结构,显示了从应力-能量张量的平均值到相关函数的联系。泛函方法采用费曼-弗农影响泛函和Schwinger-Keldysh闭时路径有效作用方法。在第二部分中,我们描述了随机重力的三种应用。首先,我们考虑Minkowski时空中的度量微扰,计算这些微扰的两点相关函数,并证明Minkowski时空是半经典引力的稳定解。其次,我们从随机引力的观点讨论结构的形成,它可以超越标准的处理,通过纳入膨胀涨落的完整量子效应。第三,利用Einstein-Langevin方程,讨论了盒状黑洞的准平衡条件和蒸发黑洞时空的完全非平衡条件下,霍金辐射的反作用和度规涨落的行为。最后,我们简要地讨论了随机引力与量子引力的理论结构,并指出了进一步发展和应用的方向。
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来源期刊
Living Reviews in Relativity
Living Reviews in Relativity 物理-物理:粒子与场物理
CiteScore
69.90
自引率
0.70%
发文量
0
审稿时长
20 weeks
期刊介绍: Living Reviews in Relativity is a peer-reviewed, platinum open-access journal that publishes reviews of research across all areas of relativity. Directed towards the scientific community at or above the graduate-student level, articles are solicited from leading authorities and provide critical assessments of current research. They offer annotated insights into key literature and describe available resources, maintaining an up-to-date suite of high-quality reviews, thus embodying the "living" aspect of the journal's title. Serving as a valuable tool for the scientific community, Living Reviews in Relativity is often the first stop for researchers seeking information on current work in relativity. Written by experts, the reviews cite, explain, and assess the most relevant resources in a given field, evaluating existing work and suggesting areas for further research. Attracting readers from the entire relativity community, the journal is useful for graduate students conducting literature surveys, researchers seeking the latest results in unfamiliar fields, and lecturers in need of information and visual materials for presentations at all levels.
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