Nonlinear growth of density fluctuations in the 3-dimensional self-gravitating systems

三维自引力系统中密度涨落的非线性增长

• 批准号: 62460039
• 负责人: SATO Humitaka
• 金额: $ 3.97万
• 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 (B)
• 财政年份: 1987
• 资助国家: 日本
• 起止时间: 1987 至 1989
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/en/grant/KAKENHI-PROJECT-62460039/
• 关键词: density fluctuation; galaxy formation; instability; general relativity; gramitational wave; pulsar; supnernova; nonlinear system; インフレーション宇宙; 重力不安定; 非線型過程; 宇宙の大局構造; 星形成; 自己重力系; 超新星爆発; 中性子星

Structure formations in the hierarchy of the universe are all related with the nonlinear growth of density fluctuations in the 3-dimensional self-gravitating system. In this research project, the characteristics of gravity in the structure formation was studied numerically as well as analytically. The subject is classified to the following three:1. Cloud and Stars Stability and fragmentation of an isothermal cloud was analyzed extensively by the 3-dimensional simulation code and the linear theory. Angular momentum transportation in the toras was analyzed by the quasi-nonlinear method. Effect of magnetic field in the evolution of cloud was systematically analyzed.2. Collapse and Supernova The code to compute the 3-dimensional gravitational collapse has been developed. Gravitational waves emission in the process of nertron stars coalescence was firstly computed by the post Newtonian approximation and the wave form was extensively studied. Supernova explosion was firstly computed by the 3-dimensional code and suggested the formation of clumpiness in the ejects. Propagation of X and gamma ray in the supernova ejecta was also studied.3. Cosmology Dynamical feature of 1-dimensional sheetlike self-gravitating system was studied in relation to the catastrophy theory. Various problems of cosmology were also studied.

宇宙层次结构的形成都与三维自引力系统中密度涨落的非线性增长有关。本研究计画以数值与解析的方式，探讨构造形成过程中的重力特性。本课题分为以下三个方面：1.用三维数值模拟程序和线性理论对等温云的稳定性和碎裂进行了详细的分析。用准非线性方法分析了Toras中的角动量输运。系统地分析了磁场在云演化过程中的作用.坍缩和超新星三维引力坍缩的计算程序已经开发完成。首次采用后牛顿近似计算了中子星并合过程中的引力波辐射，并对其波形进行了深入研究。首次用三维程序计算了超新星爆发过程，并提出了团簇的形成。研究了X射线和γ射线在超新星喷出物中的传播.利用灾变理论研究了一维片状自引力系统的动力学特征。宇宙学的各种问题也被研究。

项目成果

Y.Suto: "Microwave Background Anisotropies and the Primordial Spectrum of Cosmological Density Fluctuations" Astrophys.J.(in press).

Y.Suto：“微波背景各向异性和宇宙密度涨落的原始光谱”Astrophys.J.（出版中）。

T.Nakano: "Magnetic braking of the rotation of molecularc cloud cores" Mon.Not.R.astr.Soc.241(1989)241(1989)495-505.

T.Nakano：“分子云核心旋转的磁制动”Mon.Not.R.astr.Soc.241(1989)241(1989)495-505。

N.Gouda: "Evolution of Perturbations in a Baryon-Dominated Universe:Gauge-Invariant Analysis" Astrophys.J.341(1989)557-574.

N.Gouda：“重子主导宇宙中的扰动演化：规范不变分析”Astrophys.J.341(1989)557-574。

H.Kubotani: "The Surface Wave Instability of Stratifie k Incommpressible Cylinders with Differential Rotation" Prog.Theor.Phys.82. 523-534 (1989)

H.Kubotani：“具有差动旋转的分层不可压缩圆柱体的表面波不稳定性”Prog.Theor.Phys.82。

S.Tadaki: "Cosmological Domain Walls Coupled to Gravity" Phys.Rev.D(in press).

S.Tadaki：“与重力耦合的宇宙域壁”Phys.Rev.D（正在出版）。