Skip to main content
Log in

Apparent superluminal velocities due to the curvature of space

  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

Instead of the difficult concept of a three-dimensional curved space one can use two partial models of two-dimensional curved subspaces. If a two-dimensional subspace is curved the arbitrary angle of view must have a distorted shape which has in consequence an optical illusion. The distorted shape of ϕ must be corrected to the real angle1φ, valid in uncurved space according to the relation φ=1φf(ρ) where ρ is the central angle in theoretical sphere. If a two-dimensional subspace is just a spheric surface, the correction factor isf s (ρ)≅ρ/sin ρ, appropriate to the angle distance ρ from observer to the observed object.

In this way it is possible to explain why, in remote parts of the Universe, it was observed that their assumed components were receding at velocities larger than that of light, because the correction factorf(ρ) can change up to infinity for ρ=π. On the other hand there are many clustering of galaxies, because the correction factor for a hyperbolic spool space or internal part of annuloid is between zero and one: 0<f A (ρ))<1.

Conception considered explains the cause of polarizing effect and interference phenomenon of light without assuming of components, too, but it is in contradiction with the recent interpretation of the spectrum.

If we consider the Universe closed into itself due to curvature the existence of superluminal velocities is a undirect evidence for it. If we consider local hyperbolic spool spaces or that of annuloid, the existence of galaxies clustering is a needful but not sufficient condition for it.

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

  • Appenzeller, T. and Hiltner, W. A.: 1967,Astrophys. J. 149, L17.

    Google Scholar 

  • Blandford, R. D., McKee, C. F., and Rees, M. J.: 1977,Nature 267, 211.

    Google Scholar 

  • Burbidge, G. R., Crowne, A. H., and Smith, H. E.: 1977,Astrophys. J. Suppl. 33, 113.

    Google Scholar 

  • Chalupa, M.: 1982, private communication.

  • Chitre, S. M. and Narlikar, J. V.: 1979,Monthly Notices Roy. Astron. Soc. 187, 655.

    Google Scholar 

  • Cohen, M. H., Kellermann, K. I., Shaffer, D. B., Linfield, R. P., Moffet, A. T., Romney, J. D., Seielstad, G. A., Pauliny-Toth, I. I. K., Preuss, E., Witzel, A., Schilizzi, R. T., and Geldzahler, B. J.: 1977,Nature 268, 405.

    Google Scholar 

  • Cohen, M. H., Pearson, T. J., Readhead, A. C. S., Seielstad, G. A., Simon, R. S., and Walker, R. C.: 1979,Astrophys. J. 231, 293.

    Google Scholar 

  • Gearhart, M. R. and Pacht, E.: 1977,Nature 266, 819.

    Google Scholar 

  • Greenfield, P. E., Roberts, D. H., and Burke, B. F.: 1980,Science 208, 495.

    Google Scholar 

  • Hewish, A., Readhead, A. C. S., and Duffett-Smith, P. J.: 1974,Nature 277, 657.

    Google Scholar 

  • Hickson, P., Richstone, D. O., and Turner, E. L.: 1977,Astrophys. J. 213, 323.

    Google Scholar 

  • Hodge, P. E. and Aller, H. D.: 1977,Astrophys. J. 211, 669.

    Google Scholar 

  • Hyland, A. R. and Allen, D. A.: 1982,Monthly Notices Roy. Astron Soc. 199, 943.

    Google Scholar 

  • Impey, C. D., Brand, P. W. J. L., Wolstencroft, R. D., and Williams, P. M.: 1982,Monthly Notices Roy. Astron. Soc. 200, 19.

    Google Scholar 

  • Kinman, T. D.: 1967,Astrophys. J. 148, L53.

    Google Scholar 

  • Kinman, T. D.: 1977,Nature 267, 798.

    Google Scholar 

  • Marscher, A. P. and Broderick, J. J.: 1982,Astrophys. J. 255, L11.

    Google Scholar 

  • Möller, C.: 1955,Theory of Relativity, Clarendon Press, Oxford.

    Google Scholar 

  • Moore, R. L.: 1982, in D. S. Heeschen (ed.) ‘Extragalactic Radio Sources’,IAU Symp. 97, 345.

    Google Scholar 

  • Nicoll, J. F., Johnson, D., Segal, I. E., and Segal, W.: 1980,Proc. Nat. Acad. Sci. 77, 6275.

    Google Scholar 

  • Osmer, P. S. and Smith, M. G.: 1977,Astrophys. J. 215, L47.

    Google Scholar 

  • Pearson, T. J., Unwin, S. C., Cohen, M. H., Linfield, R. P., Readhead, A. C. S., Seielstad, G. A., Simon, R. S., and Walker, A. C.: 1981,Nature 290, 365.

    Google Scholar 

  • Peebles, P. J. E.: 1971,Physical Cosmology, Princeton University Press, Princeton.

    Google Scholar 

  • Phillips, R. B. and Mutel, R. L.: 1982,Astrophys. J. 257, L19.

    Google Scholar 

  • Porcas, R. W.: 1981,Nature 294, 47.

    Google Scholar 

  • Rashefski, P. K.: 1967,Riemannian Geometry and Tensor Analysis, Moscow, pp. 383–403.

  • Readhead, A. C. S., Pearson, T. J., Cohen, M. H., Ewing, M. S., and Moffet, A. T.: 1979,Astrophys. J. 231, 299.

    Google Scholar 

  • Rieke, G. H., Grasdalen, G. L., Kinman, T. D., Hintzen, P., Wills, B. J., and Wills, D.: 1976,Nature 260, 754.

    Google Scholar 

  • Sanders, R. H.: 1974,Nature 248, 390.

    Google Scholar 

  • Saslaw, W. C.: 1979,Nature 277, 266.

    Google Scholar 

  • Scheuer, P. A. G.: 1976,Monthly Notices Roy. Astron. Soc. 177, 1.

    Google Scholar 

  • Seaquist, E. R.: 1973,Astron. Astrophys. 22, 299.

    Google Scholar 

  • Segal, I. E.: 1975,Proc. Nat. Acad. Sci. 72, 2473.

    Google Scholar 

  • Seielstad, G. A., Cohen, M. H., Linfield, R. P., Moffet, A. T., Romney, J. D., Schilizzi, R. T., and Shaffer, D. B.: 1979,Astrophys. J. 229, 53.

    Google Scholar 

  • Smith-Haenni, A. L.: 1977,Astron. Astrophys. Suppl. 27, 205.

    Google Scholar 

  • Tolman, R. C.: 1969,Relativity, Thermodynamics, and Cosmology, Clarendon Press, Oxford.

    Google Scholar 

  • Walker, R. C., Seielstad, G. A., Simon, R. S., Unwin, S. C., Cohen, M. H., Pearson, T. J., and Linfield, R. P.: 1982,Astrophys. J. 257, 56.

    Google Scholar 

  • Whitney, A. R., Shapiro, I. I., Rogers, A. E. E., Robertson, D. S., Knight, C. A., Clark, I. A., Goldstein, R. M., Maradino, G. E., and Vandenberg, N. R.: 1971,Science 173, 225.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Souček, J. Apparent superluminal velocities due to the curvature of space. Astrophys Space Sci 94, 319–331 (1983). https://doi.org/10.1007/BF00653722

Download citation

  • Received:

  • Revised:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00653722

Keywords

Navigation