Study of a quantum inhomogeneous universe

量子非均匀宇宙的研究

• 批准号: 02640231
• 负责人: SASAKI Misao
• 金额: $ 1.28万
• 依托单位: KYOTO UNIVERSITY
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for General Scientific Research (C)
• 财政年份: 1990
• 资助国家: 日本
• 起止时间: 1990 至 1992
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-02640231/
• 关键词: Inflationary Universe; Large scale structure of the universe; Quantum tunneling with dissipation; False vacuum decay; 量子重力; マトリックス模型; インフレ-ション宇宙; 量子トンネル現象; 量子重力理論; 量子宇宙論

In order to understand the quantum origin of inhomogeneous structures of the universe, the relation between quantum fluctuations of the spacetime metric and those of matter fields has been investigated in this project. (1)Quantum fluctuations in the power-law inflationary universe It was shown that the infrared quantum fluctuations in a power-law inflation model are more unstable than those in exponential inflation. Using this instability, the baryon spectrum in a unified model with majoron is found to be exactly what one needs for the minimal isocurvature scenario of the structure formation. Further, the probability distribution is found to be highly non-Gaussian on small scales but is Gaussian on large scales. (2)Quantum tunneling in the early universe To understand quantum tunneling in the universe, it is important to analyze the effect of dissipative environment, as well as to know the role of gravity. As a first step, a canonical formulation of quantum tunneling with dissipation was given and it was shown that dissipative interactions may not necessarily suppress the tunneling rate. Then, false vacuum decay under the presence of gravity was investigated and it was found that the existence of gravitational modes changes the previous naive picture significantly.

为了了解宇宙不均匀结构的量子起源，已经研究了该项目的时空度量标准与物质场的量子波动之间的关系。 （1）幂律通货膨胀宇宙中的量子波动表明，幂律通货膨胀模型中的红外量子波动比指数膨胀的量子波动更不稳定。使用这种不稳定性，发现与Maparon的统一模型中的重子光谱正是结构形成最小的同化场景所需的。此外，发现概率分布在小尺度上是高度非高斯，但在大尺度上是高斯。 （2）早期宇宙中的量子隧道以了解宇宙中的量子隧穿，分析耗散环境的效果以及了解重力的作用很重要。第一步，给出了随着耗散的量子隧穿的规范公式，并表明耗散相互作用可能不一定会抑制隧道率。然后，研究了重力存在下的假真空衰变，发现重力模式的存在显着改变了先前的天真图像。

项目成果

M.Sasaki: "Matrix Realization of Random Surfaces" Phys.Rev.D43. 4015-4028 (1991)

M.Sasaki：“随机表面的矩阵实现”Phys.Rev.D43。

M. Sasaki: "Matrix Realization of Random Surfaces" Phys. Rev.D43. 4015-4028 (1991)

M. Sasaki：“随机表面的矩阵实现”物理。

K.Yamamoto: "Statistics of Baryons Isocurvature Perturbations in the Inflationary Universe" Phys.Rev.D46. 4206-4217 (1992)

K.Yamamoto：“暴胀宇宙中重子等曲率扰动的统计”Phys.Rev.D46。

M.Sasaki: "Non ScaleーInvariant Isocurvature Perturbations Produced in the PowerーLaw Inflation" Mod,Phys.Lett.6. 2935-2945 (1991)

M.Sasaki：“幂律膨胀中产生的非标度-不变等曲率扰动” Mod，Phys.Lett.6 (1991)。

K.FUJIKAWA: "Quantum Tunneling with Dissipation-Possible Enhancement by Dissipative Interactions-" Phys.Rev.B46. 10295-10309 (1992)

K.FUJIKAWA：“耗散量子隧道-耗散相互作用可能增强-”Phys.Rev.B46。