Skip to main content
Log in

Stationary Riemannian space-times with self-dual curvature

  • Research Articles
  • Published:
General Relativity and Gravitation Aims and scope Submit manuscript

Abstract

Riemannian space-times with self-dual curvature and which admit at least one Killing vector field (stationary) are examined. Such space-times can be classified according to whether a certain scalar fieldψ (which is the difference between the Newtonian and NUT potentials) reduces to a constant or not. In the former category (called here KSD) are the multi-TaubNUT and multi-instanton space-times. Nontrivial examples of the latter category have yet to be discovered. It is proved here that the static self-dual metrics are flat. It is also proved that each stationary metric for which the Newtonian and nut potentials are functionally related admits a Killing vector field relative to which the metric is KSD. It has also been proved that the regularity of theψ field everywhere implies that the metric is KSD. Finally it is proved that for non-KSD space-times every regular compact level surface of theψ field encloses the total NUT charge, which must be proportional to the Euler number of the surface.

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

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. Atiyah, M. F., Hitchin, N. J., Drinfeld, V. G., and Manin, Yu. I. (1918).Phys. Lett. A,65, 185.

    Google Scholar 

  2. Eguchi, T., Gilkey, P. B., and Hanson, A. J. (1980).Phys. Reps.,66, 213.

    Google Scholar 

  3. Hawking, S. W. (1979).Recent Developments in Gravitation (ed. M. Levy and S. Deser), Plenum, New York.

    Google Scholar 

  4. Boyer, C. P., and Finley III, J. D. (1981).J. Math. Phys.,23, 1126.

    Google Scholar 

  5. Kloster, S., Som, M. M., and Das, A. (1974).J. Math. Phys.,15, 1096.

    Google Scholar 

  6. Gibbons, G. W., and Hawking, S. W. (1978).Phys. Lett. B,78, 430.

    Google Scholar 

  7. Hawking, S. W. (1977).Phys. Lett. A,60, 81 (1977).

    Google Scholar 

  8. Tod, K. P., and Ward, R. S. (1979).Proc. R. Soc. London Ser. A,368, 411.

    Google Scholar 

  9. Gibbons, G. W. and Hawking, S. W. (1979).Commun. Math. Phys.,66, 291.

    Google Scholar 

  10. Eisenhart, L. P. (1950).Riemannian Geometry, Princeton University Press, Princeton, New Jersey.

    Google Scholar 

  11. Atiyah, M. F., Hitchin, N., and Singer, I. M. (1978).Proc. R. Soc. London Ser. A,362, 425.

    Google Scholar 

  12. Gibbons, G. W., and Perry, M. J. (1980).Phys. Rev. D,22, 313.

    Google Scholar 

  13. Prasad, M. K. (1979).Phys. Lett. B,83, 310.

    Google Scholar 

  14. Eguchi, T., and Hanson, A. J. (1978).Phys. Lett. B,74, 249.

    Google Scholar 

  15. Yano, K., and Bochner, S. (1953).Curvature and Betti Numbers, Princeton University Press, Princeton, New Jersey.

    Google Scholar 

  16. Hicks, N. J. (1965).Notes on Differential Geometry, Van Nostrand Reinhold, New York.

    Google Scholar 

  17. Spivak, M. (1970).A Comprehensive Introduction to Differential Geometry, Vol. I, Publish or Perish Press, Boston.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Additional information

The research reported here was done while the author was an NSERC Postdoctoral Fellow at Simon Fraser University.

The author is also a member of the Theoretical Science Institute at Simon Fraser University, and preparation for publication was partially assisted NSERC Research Grant No. 3993.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Gegenberg, J.D., Das, A. Stationary Riemannian space-times with self-dual curvature. Gen Relat Gravit 16, 817–829 (1984). https://doi.org/10.1007/BF00762935

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00762935

Keywords

Navigation