微惑星のランダム速度と統計的性質
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Bibliographic Information
- Title
-
微惑星のランダム速度と統計的性質
- Author
-
長谷川, 正樹
- Author(Another name)
-
ハセガワ, マサキ
- University
-
東京大学
- Types of degree
-
博士 (理学)
- Grant ID
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甲第9210号
- Degree year
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1991-06-24
Note and Description
博士論文
Table of Contents
- Contents / (0005.jp2)
- Chapter1 Introduction / p1 (0006.jp2)
- Chapter2 Gravitational interaction between planetesimals and their statistical behavior / p4 (0009.jp2)
- §2.1 Previous works and unsolved problems / p4 (0009.jp2)
- §2.2 The scattering matrices of gravitational encounter between planetesimals / p6 (0011.jp2)
- §§2.2.1.Hill's equation / p7 (0012.jp2)
- §§2.2.2.The scattering matrices / p17 (0022.jp2)
- §§2.2.3.Distant encouter between planetesimals / p19 (0024.jp2)
- §§2.2.4.Close encouter between planetesimals / p23 (0028.jp2)
- §2.3 The kinetic equation: Basic formulation / p28 (0033.jp2)
- §2.4 Random velocities of protoplanets in the late stage planetary accumulation / p34 (0039.jp2)
- §§2.4.1.The late stage of planetary accumulation / p34 (0039.jp2)
- §§2.4.2.Distribution function of protoplanets / p35 (0040.jp2)
- §§2.4.3.Coefficients of the Fokker-Planck equation / p40 (0045.jp2)
- §§2.4.4.Statistical behavior of protoplanets / p49 (0054.jp2)
- Chapter3 Enhancement of random motion of planetesimals due to density wave on the solar nubula / p63 (0068.jp2)
- §3.1 Influence of the solar nebula on the motion of planetesimals / p63 (0068.jp2)
- §3.2 Gravitational influence due to density wave of the solar nebula / p64 (0069.jp2)
- §§3.2.1.Perturbation equation / p64 (0069.jp2)
- §§3.2.2.Solutions to the perturbation equations / p72 (0077.jp2)
- Chapter4 Conclusion and remarks / p79 (0084.jp2)
- Acknowledgements / p83 (0088.jp2)
- Appendix A Changes of orbital elements for the case of the large impact parameter / p84 (0089.jp2)
- Appendix B Changes of orbital elements for the case of the small impact parameter / p89 (0094.jp2)
- Appendix C Functions [数式], [数式], [数式], [数式], [数式] [数式]and [数式] / p95 (0100.jp2)
- References / p102 (0107.jp2)