Skip to main content
SpringerLink
Log in

Stationary cosmological solution with torsion

  • Published:
Il Nuovo Cimento B (1971-1996)

Summary

The role of torsion and spin has been studied in the case of stationary universe with Weyssenhoff fluid under rigid rotation. It is shown that, when the pressure bears a linear relation with the density, there exist closed timelike lines. Only when the space-time isS-T homogeneous, the spin can avoid closed timelike lines.

Riassunto

Il ruolo della torsione e dello spin è stato studiato nel caso dell'universo stazionario con fluido di Weyssenhoff sottoposto a rotazione rigida. Si mostra che, quando la pressione ha una relazione lineare con la densità, esistono linee chiuse tipo tempo. Solo quando lo spazio tempo è omogeneo secondoS-T, lo spin può evitare linee chiuse di tipo tempo.

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

Access this article

Log in via an institution

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. K. Gödel:Rev. Mod. Phys.,21, 447 (1949).

    Article  ADS  Google Scholar 

  2. I. Ozsvath andE. Schucking:Ann. Phys. (Leipzig),55, 166 (1969).

    Article  MathSciNet  ADS  Google Scholar 

  3. W. J. van Stockum:Proc. R. Soc. Edinburgh,57, 135 (1937).

    Article  Google Scholar 

  4. S. C. Maitra:J. Math. Phys. (N.Y.),7, 1025 (1966).

    Article  MathSciNet  ADS  Google Scholar 

  5. E. P. Vasconcellos Vaidya, M. L. Bedran andM. M. Som:Prog. Theor. Phys.,72, 857 (1984).

    Article  MathSciNet  ADS  MATH  Google Scholar 

  6. J. R. Ray andL. L. Smalley:Phys. Rev. D,26, 2619 (1982).

    Article  MathSciNet  ADS  Google Scholar 

  7. J. R. Ray andL. L. Smalley:Phys. Rev. Lett.,49, 1059 (1982).

    Article  MathSciNet  ADS  Google Scholar 

  8. J. R. Ray:J. Math. Phys. (N. Y.),13, 1451 (1972).

    Article  ADS  Google Scholar 

  9. D. Tsoubelis:Phys. Rev. Lett.,51, 2235 (1983).

    Article  MathSciNet  ADS  MATH  Google Scholar 

  10. F. W. Hehl, P. von der Heyde, G. D. Kerlick andJ. M. Nester:Rev. Mod. Phys.,48, 393 (1976).

    Article  ADS  Google Scholar 

  11. W. Arkuszewski, W. Kopczynski andV. N. Ponomariev:Ann. Inst. Henri Poincaré,21, 89 (1974).

    MathSciNet  Google Scholar 

Download references

Author information

Authors and Affiliations

  1. Instituto de Física, Universidade Federal do Rio de Janeiro, Cidade Universitária, Ilha do Fundão, CEP 21.944, Rio de Janeiro, RJ, Brasil

    M. L. Bedran, E. P. Vasconcellos Vaidya & M. M. Som

Authors
  1. M. L. Bedran
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. E. P. Vasconcellos Vaidya
    View author publications

    You can also search for this author in PubMed Google Scholar

  3. M. M. Som
    View author publications

    You can also search for this author in PubMed Google Scholar

Additional information

Traduzione a cura della Redazione.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Bedran, M.L., Vasconcellos Vaidya, E.P. & Som, M.M. Stationary cosmological solution with torsion. Nuov Cim B 87, 101–108 (1985). https://doi.org/10.1007/BF02721532

Download citation

  • Received:

  • Revised:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02721532

PACS

Search

Navigation