Kinetic Field Theory: Second-order perturbation theory

动场论：二阶微扰理论

• 批准号: 418152809
• 负责人: Professor Dr. Matthias Bartelmann
• 金额: --
• 依托单位: Institut für Theoretische Physik
• 依托单位国家: 德国
• 项目类别: Research Grants
• 财政年份: 2019
• 资助国家: 德国
• 起止时间: 2018-12-31 至 2020-12-31
• 项目状态: 已结题
• 来源: https://gepris.dfg.de/gepris/projekt/418152809?language=en
• 关键词: Kinetic; Field; Theory; Second; order

Astoundingly successful as it is, the cosmological standard model leaves us with two difficult and fundamentally important puzzles, viz. the dark matter and the dark energy, whose origin, composition, and place in the framework of physics are enigmatic. Large cosmological surveys are being and are about to be undertaken with the major goals of mapping and quantifying the dark-matter distribution and finding out about a possible evolution of the dark-energy density with time. Precise cosmological inference from these surveys hinges on the depth and precision of our understanding of the late-time, non-linear evolution of cosmic structures. While numerical simulations have returned a wealth of impressive and important results, calculating higher-order statistical properties of large-scale cosmic structures at late times is still a forbiddingly time-consuming task.Recently, we have developed a novel analytic approach to non-linear cosmic structure formation, based on a non-equilibrium kinetic field theory (KFT). This theory has several important advantages compared to more conventional approaches. In particular, it operates on the microscopic degrees of freedom of classical particles in phase space. Since the Hamiltonian flow in phase space is bijective and diffeomorphic, the notorious shell-crossing problem is absent from our approach. In its present form, the theory is free of adjustable parameters. We have shown in earlier work that even first-order perturbation theory applied to KFT reproduces the non-linear power spectrum of cosmic density fluctuations very well to wave numbers of k ~ 10 h/Mpc at the present cosmic epoch. We could further show how the central mathematical object of KFT, its generating functional, can be fully factorized into terms of a standard form.Based on this factorization, a diagrammatic approach to perturbation theory developed therefrom, and a first version of a symbolic computer code for constructing these diagrams, we propose here to calculate the second-order perturbation terms for the non-linear power spectrum of cosmic density fluctuations. Main challenges will be the reliable and fast numerical integration of the generic expressions appearing in the factorization of the generating functional, and the calculation of the one- and two-loop integrals appearing in the perturbation series. The essential goals of the proposed research are to finalize and test our symbolic computer code for perturbation diagrams, to supply it with a code for numerical integration of perturbation terms, and to evaluate, analyze and compare the contributions of these terms to the non-linearly evolved cosmic power spectrum. Based on the quality of the first-order perturbation theory in KFT, we are confident that we can analytically calculate accurate non-linear power spectra reaching wave numbers of k ~ 20-50 h/Mpc at the present epoch.

尽管宇宙学标准模型取得了惊人的成功，但它给我们留下了两个困难而又根本上重要的谜题，即。暗物质和暗能量的起源、组成和在物理学框架中的位置都是谜。大型宇宙学调查正在进行，并即将进行，主要目标是绘制和量化暗物质分布，并找出暗能量密度可能随时间演变的情况。从这些调查中得出的准确的宇宙学推断取决于我们对宇宙结构的后期、非线性演化的理解的深度和精确度。虽然数值模拟已经得到了大量令人印象深刻和重要的结果，但计算后期大规模宇宙结构的高阶统计性质仍然是一项令人望而生畏的耗时任务。最近，我们基于非平衡动力场理论(KFT)发展了一种新的分析方法来研究非线性宇宙结构的形成。与更传统的方法相比，这一理论有几个重要的优势。特别是，它对相空间中经典粒子的微观自由度起作用。由于相空间中的哈密顿流是双射的和微分同胚的，所以我们的方法中不存在著名的穿壳问题。在目前的形式下，该理论没有可调整的参数。我们在早期的工作中已经表明，即使一阶微扰理论应用于KFT，也很好地再现了宇宙密度涨落的非线性功率谱，在本宇宙纪元，波数为k~10h/Mpc。我们可以进一步展示KFT的中心数学对象，它的生成泛函，可以完全分解成标准形式的项。基于这种因式分解，发展了一种微扰理论的图解方法，以及用于构建这些图的符号计算机代码的第一个版本，我们在这里建议计算宇宙密度涨落的非线性功率谱的二阶微扰项。主要挑战将是生成泛函的因式分解中出现的类属表达式的可靠和快速的数值积分，以及出现在微扰级数中的单圈和双圈积分的计算。这项研究的基本目标是最终确定和测试我们的微扰图的符号计算机代码，为它提供一个微扰项的数值积分代码，并评估、分析和比较这些项对非线性演化的宇宙功率谱的贡献。基于KFT中一阶微扰理论的性质，我们有信心解析地计算出目前波数为k~20-50h/mpc的精确的非线性功率谱。