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  3. The Gravitational Million–Body Problem
  • Cited by 452
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    • Publisher:
      Cambridge University Press
      Publication date:
      05 June 2012
      23 January 2003
      ISBN:
      9781139164535
      9780521773034
      9780521774864
      DOI:
      https://doi.org/10.1017/CBO9781139164535
      Dimensions:
      (247 x 174 mm)
      Weight & Pages:
      0.94kg, 372 Pages
      Dimensions:
      (247 x 174 mm)
      Weight & Pages:
      0.793kg, 372 Pages
      • Subjects:
      Physics and Astronomy, Astrophysics
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    Subjects:
    Physics and Astronomy, Astrophysics
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    Book description

    The globular star clusters of the Milky Way contain hundreds of thousands of stars held together by gravitational interactions, and date from the time when the Milky Way was forming. This 2003 text describes the theory astronomers need for studying globular star clusters. The gravitational million-body problem is an idealised model for understanding the dynamics of a cluster with a million stars. After introducing the million-body problem from various view-points, the book systematically develops the tools needed for studying the million-body problems in nature, and introduces the most important theoretical models. Including a comprehensive treatment of few-body interactions, and developing an intuitive but quantitative understanding of the three-body problem, the book introduces numerical methods, relevant software, and current problems. Suitable for graduate students and researchers in astrophysics and astronomy, this text also has important applications in the fields of theoretical physics, computational science and mathematics.

    Reviews

    ‘The book contains lucid and concise descriptions of most of the important tools in the subject, with only a modest bias towards the authors’ own interests.’

    Source: Classical and Quantum Gravity

    ‘Enhanced by exercises for the reader, this book is a comprehensive preparation for cutting edge research in the field of stellar dynamics.’

    Source: Orion

    'What they did, covers many aspects of the problem: a historical overview, analytical details for the solvable cases, numerical solutions including computer codes for others, applications for astrophysical examples like star clusters, and a reference list covering twenty pages.'

    Source: Zentralblatt MATH

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