Chapter 16 Gravitational Scattering between Planetesimals and Their Statistical Behavior : Part V Physical Processes Relevant to the Planetary Growth : Origin of the Solar System

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概要

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• Mutual gravitational scattering between planetesimals is the elementary process which leads to the relaxation of their random motion. In most of studies made so far, the relaxation time and the magnitude of random velocity have been estimated by the two-body approximation in free space with neglect of the solar gravity. However, we will first show that we cannot neglect the solar gravity in those evaluations. Next we will review previous work in two alternative approaches by kinetic equations and by N-body numerical simulation, and also review a preliminary study of relaxation time of Keplerian particles without any two-body approximation.

• 理論物理学刊行会の論文
• 1989-03-10

著者

• Nakazawa Kiyoshi

  Department of Cardiology, St. Marianna University School of Medicine

• Nakagawa Y

  Department Of Earth And Planetary Sciences Faculty Of Science Kobe University

• Nakagawa Yoshitsugu

  Geophysical Institute University Of Tokyo

• Nakagawa Yoshitsugu

  Geophysical Institute Faculty Of Science University Of Tokyo

• OHTSUKI Keiji

  Geophysical Institute, University of Tokyo

• HASEGAWA Masaki

  Geophysical Institute, Faculty of Science, University of Tokyo

• Ohtsuki Keiji

  Geophysical Institute Faculty Of Science University Of Tokyo

• HASEGAWA Munetake

  Laboratory of Physics, Fukuoka Dental College

• Nakazawa Kiyoshi

  Department Of Applied Physics Tokyo Institute Of Technology

• HASEGAWA Munetaka

  Laboratory of Physics, Fukuoka Dental College

• Hasegawa Masaki

  Geophysical Institute Faculty Of Science University Of Tokyo

• NAKAZAWA Kiyoshi

  Department of Applied Physics, Tokyo Institute of Technology

• OHTSUKI Keiji

  Geophysical Institute, Faculty of Science, University of Tokyo

• NAKAGAWA Yoshitsugu

  Department of Physics, Kyoto University

• Nakazawa Kiyoshi

  Gifu University

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