Skip to main content
Log in

Shear-free Perfect Fluids in General Relativity: Gravito-magnetic Spacetimes

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

Abstract

We investigate shear-free, perfect fluid solutions of Einstein's field equations in which the perfect fluid satisfies a barotropic equation of state p = p(w) such that w + p ≠ 0. We find that if the electric part of the Weyl tensor (with respect to the fluid flow) vanishes and the spacetime is not conformally flat then the fluid volume expansion is zero but the vorticity is necessarily nonzero. In addition, we show that if p = −w/3 then necessarily either the fluid expansion is zero or the fluid vorticity is zero.

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.

Institutional subscriptions

Similar content being viewed by others

REFERENCES

  1. Collins, C. B. (1984). J. Math. Phys. 25, 995.

    Google Scholar 

  2. Maartens, R., Lesame, W. M., and Ellis, G. F. R. (1998). Class. Quantum Grav. 15, 1005.

    Google Scholar 

  3. Trümper, M. (1965). J. Math. Phys. 6, 584.

    Google Scholar 

  4. Arianrhod, R., Lun, A. W.-C., McIntosh, C. B. G., and Perjes, Z. (1994). Class. Quantum Grav. 11, 2331.

    Google Scholar 

  5. Kramer, D., Stephani, H., MacCallum, M. A. H., and Herlt, E. (1980). Exact Solutions of Einstein's Field Equations (Cambridge University Press, Cambridge).

    Google Scholar 

  6. Treciokas, R., and Ellis, G. F. R. (1971). Commun. Math. Phys. 23, 1.

    Google Scholar 

  7. Ellis, G. F. R. (1967). J. Math. Phys. 8, 1171.

    Google Scholar 

  8. Ellis, G. F. R. (1971). In Relativistic Cosmology, General Relativity and Cosmology. Proc. Int. School of Physics 'Enrico Fermi' (Course XLVIII, 1969), R. K. Sachs, ed. (Academic, London).

    Google Scholar 

  9. Carminati, J. (1987). J. Math. Phys. 28, 1848.

    Google Scholar 

  10. Carminati, J., and Cyganowski, S. O. (1997). Class. Quantum Grav. 14, 1167.

    Google Scholar 

  11. Bonnor, W. B., and Davidson, W. (1985). Class. Quantum Grav. 2, 775.

    Google Scholar 

  12. Whittaker, J. M. (1968). Proc. Roy. Soc. London A 306, 1.

    Google Scholar 

  13. Kramer, D. (1984). Class. Quantum Grav. 1, L3.

    Google Scholar 

  14. Carminati, J., and Cyganowski, S. O. (1996). Class. Quantum Grav. 13, 1805.

    Google Scholar 

  15. Collins, C. B. (1986). Can. J. Phys. 64, 191.

    Google Scholar 

  16. Carminati, J. (1990). J. Math. Phys. 31, 2434.

    Google Scholar 

  17. Cyganowski, S. O., and Carminati, J. (1998). Comp. Phys. Commun. 115, 200.

    Google Scholar 

  18. Van den Bergh, N. (1999). Class. Quantum Grav. 16, 117.

    Google Scholar 

  19. Oleson, M. (1972). Ph.D. Thesis, University of Waterloo.

  20. White, A. J., and Collins, C. B. (1984). J. Math. Phys. 25, 332.

    Google Scholar 

  21. Lang, J. M., and Collins, C. B. (1988). Gen. Rel. Grav. 20, 683.

    Google Scholar 

  22. Newman, E. T., and Penrose, R. (1962). J. Math. Phys. 3, 566.

    Google Scholar 

  23. Czapor, S. R., McLenaghan, R. G., and Carminati, J. (1992). Gen. Rel. Grav. 24, 911.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Cyganowski, S., Carminati, J. Shear-free Perfect Fluids in General Relativity: Gravito-magnetic Spacetimes. General Relativity and Gravitation 32, 221–233 (2000). https://doi.org/10.1023/A:1001823208111

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1023/A:1001823208111

Navigation