Skip to main content
Log in

The Mesofractal Universe Driven by Rayleigh-Lèvy Walks

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

Abstract

The report is devoted to the description of the observed non-homogeneous structure of the Universe in terms of the walk model with a transition probability of the inverse power type called the Rayleigh-Lèvy (RL) walk. This model contains four free parameters. An appropriate choice of them yields the mesofractal structure, revealing fractal properties on small scales and looking like a homogeneous medium on large scales. This approach can be considered as some kind of descriptive statistics allowing to extract necessary characteristics of the structure using a few parameters.

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. Zwicky, F. (1957). Morphological Astronomy, Springer-Verlag, Berlin.

    Google Scholar 

  2. Pilkington, J. D. H., and Scott, P. F. (1965). Mem. Roy. Astron. Soc. 69, 183.

    Google Scholar 

  3. Peebles, P. J. E. (1980). The Large-Scale Structure of the Universe, Princeton University Press, Princeton, NJ.

    Google Scholar 

  4. Bertschinger, E. (1992). In New Insights into the Universe, Lecture Notes in Physics, 408, Martinez, V. J., Portille, M., and Saez, D. (Eds.), Springer-Verlag, Berlin, p. 88.

    Google Scholar 

  5. Webster, A. S. (1976). Mon. Not. R. Ast. Soc. 175, 61.

    Google Scholar 

  6. Melott, A. L. (1990). Phys. Rep. 193, 1.

    Google Scholar 

  7. Martinez, V. J., Paredes, S., and Saar, E. (1993). Mon. Not. R. Ast. Soc. 260, 365.

    Google Scholar 

  8. Klypin, A., and Shandarin, S. F. (1993). Astrophys. J. 413, 48.

    Google Scholar 

  9. Borgani, S. (1995). Phys. Rep. 251, 1–152.

    Google Scholar 

  10. Coleman, P. H., and Pietronero, L. (1992). Phys. Rep. 213, 313.

    Google Scholar 

  11. Weinberg, S. (1972). Gravitation and Cosmology, Wiley, New York.

    Google Scholar 

  12. Mandelbrot, B. B. (1975). Comptes Rendus, 280A, 1551–1554.

    Google Scholar 

  13. Mandelbrot, B. B. (1983). The Fractal Geometry of Nature, W. H. Freeman, New York.

    Google Scholar 

  14. Stell, G. (1991). Lect. Appl. Math. 27, 109–137.

    Google Scholar 

  15. Balescu, R. (1975). Equilibrium and Non-Equilibrium Statistical Mechanics, Wiley, New York.

    Google Scholar 

  16. Uchaikin, V. V., and Ryzhov, V. V. (1988). The Stochastic Theory of High Energy Particles Transport, Nauka, Novosibirsk (in Russian).

    Google Scholar 

  17. Coles, P. (1992). In Statistical Challenges in Modern Cosmology, Feigelson, E., and Babu, G. J. (Eds.), Spinger, New York, pp. 57–81.

    Google Scholar 

  18. Fry, J. N., and Peebles, P. J. E. (1978). Astrophys. J. 221, 19.

    Google Scholar 

  19. Martinez, V. T., and Jones, B. J. T. (1990). Mon. Not. R. Ast. Soc. 242, 517–521.

    Google Scholar 

  20. Longair, M. S., and Einasto, J. (Eds.) (1978). The Large Scale Structure of the Universe,D. Reidel, Dordrecht, The Netherlands.

    Google Scholar 

  21. Groth, E. J., and Peebles, P. J. E. (1977). Astrophys. J. 217, 385.

    Google Scholar 

  22. Davis, M., and Peebles, P. J. E. (1983). Astrophys. J. 267, 465.

    Google Scholar 

  23. Sharp, N. A., Bonometto, S. A., and Lucchin, F. (1984). Ast. Astrophys. 130, 7.

    Google Scholar 

  24. Szapudi, I., Szalay, A., and Boschan, P. (1992). Astrophys. J. 390, 350.

    Google Scholar 

  25. Fry, J. N. (1984). Astrophys. J. 279, 499.

    Google Scholar 

  26. Davis, M., and Peebles, P. J. E. (1988). Astrophys. J. 35(Suppl.), 425.

    Google Scholar 

  27. Hamilton, A. J. S. (1988). Astrophys. J. 332, 67.

    Google Scholar 

  28. Saslaw, W. C., and Hamilton, A. J. S. (1984). Astrophys. J. 276, 13.

    Google Scholar 

  29. Saslaw, W. C., Chitre, S. M., Iton, M., and Inagaki, S. (1990). Astrophys. J. 365, 419.

    Google Scholar 

  30. Shane, C. D., and Wirtanen. (1967). Publ. Lick. Obs. 22(Pt. 1).

  31. Fry, J. N. (1994). Phys. Rev. Lett. 73(2), 215–219.

    Google Scholar 

  32. Slobodenyuk, V. A., and Uchaikin, V. V. (1998). J. Math. Sci. 89, 1570.

    Google Scholar 

  33. Zolotarev, V. M. (1986). One-Dimensional Stable Distributions, American Mathematical Society, Providence, RI.

    Google Scholar 

  34. Uchaikin, V.V., and Zolotarev, V. M. (1999). Chance and Stability, VSP, Utrecht, The Netherlands.

    Google Scholar 

  35. Samorodnitzky, G., and Taqqu, M. (1994). Stable Non-Gaussin Random Processes, Chapman & Hall, New York.

    Google Scholar 

  36. Chandrasekhar, S., and von Neumann, J. (1941). Astrophys. J. 95, 489, Chandrasekhar, S., and von Neumann, J. (1943). Astrophys. J. 97, 1.

    Google Scholar 

  37. Chandrasekhar, S. (1944). Astrophys. J. 99, 25; 99, 47.

    Google Scholar 

  38. Kanter, M. (1975). Ann. Probab. 3, 697.

    Google Scholar 

  39. Uchaikin, V. V., and Korobko, D. A. (1998). Proc. 3rd St. Petersburg Simulat. Workshop, 310.

  40. Uchaikin, V., Gismjatov, I., Gusarov, G., and Svetukhin, V. (1998). Int. J. Bifurcation Chaos 8(5), 977–984.

    Google Scholar 

  41. Carruthers, P., and Mint, D.-V. (1983). Phys. Lett. B 131, 116.

    Google Scholar 

  42. Fry, J. N. (1986). Astrophys. J. 306, 358.

    Google Scholar 

  43. Messina, A., Moscardini, L., Lucchin, F., and Matarrese, S. (1990). Mon. Not. R. Ast. Soc. 245, 244.

    Google Scholar 

  44. Martinez, V. J., and Jones, B. J. T. (1990). Mon. Not. R. Astr. Soc. 242, 517.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Uchaikin, V.V. The Mesofractal Universe Driven by Rayleigh-Lèvy Walks. General Relativity and Gravitation 36, 1689–1717 (2004). https://doi.org/10.1023/B:GERG.0000032161.40474.80

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1023/B:GERG.0000032161.40474.80

Navigation