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Conclusion

Published online by Cambridge University Press:  12 October 2009

A. V. Gurevich
Affiliation:
P. N. Lebedev Physics Institute, Moscow
V. S. Beskin
Affiliation:
P. N. Lebedev Physics Institute, Moscow
Ya. N Istomin
Affiliation:
P. N. Lebedev Physics Institute, Moscow
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Summary

The theory presented above provides insight into the basic physical processes proceeding in the magnetosphere of a neutron star. Within this theory we can describe the principal details of the dynamics and evolution of pulsars, clarify the nature of their activity, establish the origin of the electron–positron plasma, and describe the coherent generation mechanism of observed radio emission. The main predictions of the theory are in agreement with observations.

There are, of course, many questions requiring further theoretical investigations. For example, it is necessary to carry out a reliable calculation of free electron energy on the neutron star's surface (Section 2.5), to investigate the wave excitation processes in the boundary layer near the light surface and in an extensive region behind it (Chapter 4), to study the transition layer structure on the boundary between the open and closed regions of the magnetosphere (Chapter 4), and so on. It is noteworthy that only first steps have been made in the study of the nature of non-stationary processes in the pulsar magnetosphere (Section 7.7). Nevertheless, the physical picture of the basic processes in the pulsar magnetosphere seems on the whole to be clear.

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Publisher: Cambridge University Press
Print publication year: 1993

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  • Conclusion
  • A. V. Gurevich, P. N. Lebedev Physics Institute, Moscow, V. S. Beskin, P. N. Lebedev Physics Institute, Moscow, Ya. N Istomin, P. N. Lebedev Physics Institute, Moscow
  • Book: Physics of the Pulsar Magnetosphere
  • Online publication: 12 October 2009
  • Chapter DOI: https://doi.org/10.1017/CBO9780511564673.011
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  • Conclusion
  • A. V. Gurevich, P. N. Lebedev Physics Institute, Moscow, V. S. Beskin, P. N. Lebedev Physics Institute, Moscow, Ya. N Istomin, P. N. Lebedev Physics Institute, Moscow
  • Book: Physics of the Pulsar Magnetosphere
  • Online publication: 12 October 2009
  • Chapter DOI: https://doi.org/10.1017/CBO9780511564673.011
Available formats
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Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • Conclusion
  • A. V. Gurevich, P. N. Lebedev Physics Institute, Moscow, V. S. Beskin, P. N. Lebedev Physics Institute, Moscow, Ya. N Istomin, P. N. Lebedev Physics Institute, Moscow
  • Book: Physics of the Pulsar Magnetosphere
  • Online publication: 12 October 2009
  • Chapter DOI: https://doi.org/10.1017/CBO9780511564673.011
Available formats
×