1. Numerical Simulation in Astrophysics : Smoothed Particle Methods (III. General Applications)

スポンサーリンク

概要

著者

関連論文

The Surface Wave Instability of Stratified Incompressible Cylinders with Differential Rotation : Astrophysics and Relativity
Numerical Simulation of Viscous Flow by Smoothed Particle Hydrodynamics : Astrophysics and Relativity
Chapter 23 Gas Capture by Proto-Jupiter and Proto-Saturn : Part VI Growth of the Planets : Origin of the Solar System
Chapter 8 Efficiency of Angular Momentum Transfer by Shear Instability : Part II Formation Processes of Protostars : Origin of the Solar System
Chapter 7 Stability of the Primordial Solar Nebula : Part II Formation Processes of Protostars : Origin of the Solar System
Chapter 5 Collapse and Fragmentation of Isothermal Clouds : Part II Formation Processes of Protostars : Origin of the Solar System
Chapter 4 The Equilibrium and the Stability of Rotating Isothermal Clouds : Part II Formation Processes of Protostars : Origin of the Solar System
Fragmentation of Isothermal Sheet-Like Clouds. II : Full Nonlinear Numerical Simulations
Fragmentation of Isothermal Sheet-Like Clouds. I : Solutions of Linear and Second-Order Perturbations Equation
1. Numerical Simulation in Astrophysics : Smoothed Particle Methods (III. General Applications)
Characteristics of Collapse of Rotating Isothermal Clouds : Astrophysics and Relatively
Analytic Solutions for Equilibrium of Rotating Isothermal Clouds : One-Parameter Family of Axisymmetric and Conformal Configurations
Fission of a Massive Elongated Gas Cloud Rotating at the Galactic Center
3次元自己重力系における構造発生(基研短期研究会『天体現象と非線形・非平衡物理』報告,研究会報告)
3-D Numerical Hydrodynamics of Self-Gravitating Gas : Collisions and Fragmentations
Three-Dimensional Numerical Simulation of Interstellar Cloud-Cloud Collisions and Triggered Star Formation. I : Head-On Collisions
ポリトロープ星の三次元爆発(基研短期研究会「SN1987A」,研究会報告)
Wave Excitation in Isothermal Disks by External Gravity
Criteria for the Collapse and Fragmentation of Rotating Clouds
Three-Dimensional Hydrodynamical Simulations of Type 2 Supernova--Mixing and Fragmentation of Ejecta
Time Evolution of Pure Gravitational Waves
Fragmentation of Clouds(Proceedings of Japan-France Seminar on Chemical Evolution of Galaxies with Active Star Formation)
Is the Conventional Big Bang Compatible with the Discovery of the Quarks?
An Upper Bound on the Number Density of Primordial Black Holes from the Big Bang Nucleosynthesis
General Relativistic Collapse of an Axially Symmetric Star. I : The Formulation and the Initial Value Equations
A Method of Determining Apparent Horizons in [(2+1)+1]-Formalism of the Einstein Equations
An Analytic Solution of Initial Data for Slowly Rotating Dust Sphere under Maximal Slicing Condition
A New Formalism of the Einstein Equations for Relativisitic Rotating Systems
Constraints on Lifetime and Mass of Heavy Lepton Neutrinos Imposed by Big Bang Nucleosynthesis
Characteristics of Collapse of Rotating Isothermal Clouds

もっと見る

スポンサーリンク