Skip to main content

Part of the book series: Graduate Texts in Mathematics ((GTM,volume 60))

Abstract

In most cases (for example, in the three-body problem) we can neither solve the system of differential equations nor completely describe the behavior of the solutions. In this chapter we consider a few simple but important problems for which Newton’s equations can be solved.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 74.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Here we assume for simplicity that the solution φ is defined on the whole time axis .

    Google Scholar 

  2. For a definition, see, e.g., p. 155 of Ordinary Differential Equations by V. I. Arnold, MIT Press, 1973.

    Google Scholar 

  3. The only exception is the case when the period does not depend on the energy.

    Google Scholar 

  4. With the usual limitations.

    Google Scholar 

  5. Including reflections.

    Google Scholar 

  6. Let a drop of tea fall into a glass of tea close to the center. The waves collect at the symmetric point. The reason is that, by the focal definition of an ellipse, waves radiating from one focus of the ellipse collect at the other.

    Google Scholar 

  7. By planets we mean here points in a central field.

    Google Scholar 

  8. This problem is taken from V. V. Beletskii’s delightful book, “Notes on the Motion of Celestial Bodies,” “Nauka,” 1972.

    Google Scholar 

  9. The case M = 0 is left to the reader.

    Google Scholar 

  10. The moment of force is also called the torque [Trans. note].

    Google Scholar 

  11. Here we are assuming that U does not depend on m. In the field of gravity, the potential energy U is proportional to m, and therefore the acceleration does not depend on the mass m of the moving point.

    Google Scholar 

  12. J. M. Smith, Mathematical Ideas in Biology, Cambridge University Press, 1968.

    Book  Google Scholar 

  13. Ibid.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

Copyright information

© 1978 Springer Science+Business Media New York

About this chapter

Cite this chapter

Arnold, V.I. (1978). Investigation of the equations of motion. In: Mathematical Methods of Classical Mechanics. Graduate Texts in Mathematics, vol 60. Springer, New York, NY. https://doi.org/10.1007/978-1-4757-1693-1_2

Download citation

  • DOI: https://doi.org/10.1007/978-1-4757-1693-1_2

  • Publisher Name: Springer, New York, NY

  • Print ISBN: 978-1-4757-1695-5

  • Online ISBN: 978-1-4757-1693-1

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics