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Evolution and simulation of spacetime structure in quantum inflationary universe

量子暴胀宇宙时空结构的演化与模拟

基本信息

批准号：
15540265
负责人：
NAMBU Yasusada
金额：
$ 1.47万
依托单位：
Nagoya University
依托单位国家：
日本
项目类别：
Grant-in-Aid for Scientific Research (C)
财政年份：
2003
资助国家：
日本
起止时间：
2003 至 2005
项目状态：
已结题

项目摘要

As a preparation to incorporate the quantum effect into spacetime structure, we investigated the gradient expansion approach which is a method to realize a model of inhomogeneous universes. This approach constructs the perturbative solution of the Einstein equation using expansion about the order of the spatial derivative. We succeeded to re-construct the lowest order solution of the gradient expansion by applying the renormalization group method to the cosmological perturbation about a Friedmann-Robertson-Walker universe. As a direct application of this result, we found that only non-adiabatic mode of fluctuation can back react a Friedmann-Robertson-Walker universe and modify its expansion law.Then using the lowest order gradient expansion, we investigated the dynamics of preheating stage after inflation numerically. In this stage, the metric fluctuation is amplified by the parametric resonance caused by the coherent oscillation of the inflaton field. For a model with two scalar fields, we obtained the evolution of the power spectrum of fluctuations. As the considering model is essentially chaotic system, the spatial correlation of the fields is lost as the system evolves and the spatial pattern evolves to that of the White noise. We found that the evolution of the power spectrum of metric perturbation depends on the initial power index of fluctuation and non-linear effect strongly affects the small scale structure while the large scale structure of which wave length is larger that the horizon scale is not affected by the back reaction effect caused by the parametric resonance.

作为将量子效应引入时空结构的准备工作，我们研究了梯度展开方法，这是一种实现非均匀宇宙模型的方法。该方法利用空间导数阶的展开构造了爱因斯坦方程的微扰解。我们将重整化群方法应用于关于friedman - robertson - walker宇宙的宇宙学扰动，成功地重建了梯度展开的最低阶解。作为这一结果的直接应用，我们发现只有非绝热涨落模式才能反反应一个friedman - robertson - walker宇宙并修正它的膨胀定律。然后采用最低阶梯度展开法，对膨胀后预热阶段的动力学进行了数值研究。在这个阶段，度量波动被膨胀场相干振荡引起的参数共振放大。对于具有两个标量场的模型，我们得到了波动功率谱的演化。由于考虑的模型本质上是混沌系统，随着系统的演化，场的空间相关性丢失，空间格局演化为白噪声的空间格局。我们发现度量摄动功率谱的演化依赖于波动的初始功率指数，非线性效应强烈地影响小尺度结构，而波长大于视界尺度的大尺度结构则不受参数共振引起的反反应效应的影响。