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Astrophysics and Space Science

, Volume 69, Issue 2, pp 339–351 | Cite as

The primeval hadron: Origin of stars, galaxies and astronomical universe

  • R. M. Muradian
Article

Abstract

The relationship between mass and angular momentum for the known cosmic objects has been examined, and it is shown that they are described by the generalized Regge-like dependence of the formJ=(m/mp)1+1/nħ wheren=2 for galaxies, their clusters and superclusters, andn=3 for asteroids, planets and stars. It offers the possibility, that Ambartsumian's superdense proto-matter has hadronic nature. This allows us to give a realistic and quantitave explanation with a minimum number of arbitrary assumptions for the origin of cosmic angular momenta, cosmic magnetic fields and offers the framework for other cosmogonic implications. This approach incorporates in a natural way the fundamental quantum-mechanical parameters ħ andmp, besides the classical parametersG andc, and allows us to derive simple expressions for masses and spins of cosmic objects through fundamental constants, some of which coincide with Eddington-Dirac's ‘Large Number’ relations.

Keywords

Magnetic Field Angular Momentum Simple Expression Fundamental Constant Arbitrary Assumption 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Alfvén, H.: 1978, in L. V. Mirzoyan (ed.)Problems of Physics and Evolution of the Universe, p. 9. Acad. Sci. Armenian SSR, Yerevan.Google Scholar
  2. Alfvén, H. and Arrhenius, G.: 1976,Evolution of the Solar System, NASA, Washington.Google Scholar
  3. Allen, C. W.: 1973,Astrophysical Quantities, Athlone Press, London.Google Scholar
  4. Ambartsumian, V. A.: 1947,Stellar Evolution and Astrophysics, Acad. Sci. Armenian SSR, Yerevan.Google Scholar
  5. Ambartsumian, V. A.: 1956, in A. Beer (ed.),Vistas in Astronomy, Vol.2, p. 1708.Google Scholar
  6. Ambartsumian, V. A.: 1958, inLa Structure et l'Evolution de l'Universe, p. 241, Stoops, Bruxelles.Google Scholar
  7. Ambartsumian, V. A.: 1965, inThe Structure and Evolution of Galaxies, p. 1, Interscience Publishers, London.Google Scholar
  8. Ambartsumian, V. A.: 1971, in D. J. K. O'Connell (ed.),Nuclei of Galaxies, p. 9, North-Holland, Amsterdam.Google Scholar
  9. Ambartsumian, V. A.: 1975,Sitzungsberichte der Academie der Wissenschaften der DDR, 15N, p. 5, Akademie-Verlag, Berlin.Google Scholar
  10. Ambartsumian, V. A. and Saakyan, G. S.: 1960,Astron. Zh.,37, 193.Google Scholar
  11. Baluni, V.: 1978,Phys. Rev. D17, 2092.Google Scholar
  12. Baym, G. and Chin, S.: 1976,Phys. Lett. 62B, 241.Google Scholar
  13. Blackett, P. M. S.: 1947,Nature 159, 658.Google Scholar
  14. Chandrasekhar, S.: 1939,An Introduction to the Study of Stellar Systems, Univ. Press, Chicago.Google Scholar
  15. Chapline, G. and Nauenberg, M.: 1977,Phys. Rev. D16, 450.Google Scholar
  16. Chew, G. F. and Frautschi, S. C.: 1961,Phys. Rev. Lett. 7, 394.Google Scholar
  17. Collins, J. C. and Perry, M. J.: 1975,Phys. Rev. Lett. 34, 1353.Google Scholar
  18. Dethlefsen, J., Nielsen, H. and Tze, H. C.: 1974,Phys. Lett. 48B, 48.Google Scholar
  19. Dirac, P. A. M.: 1937,Nature 139, 323.Google Scholar
  20. Eddington, A. S.: 1926,Internal Constitution of the Stars, University Press, Cambridge.Google Scholar
  21. Freedman, B. and McLerran, L.: 1978,Phys. Rev. D17, 1109.Google Scholar
  22. Ginzburg, V. L. and Ozernoy, L. M.: 1977,Astrophys. Space Sci. 48, 401.Google Scholar
  23. Harrison, E. R.: 1970,Nature 228, 258.Google Scholar
  24. Harrison, E. R.: 1971,Monthly Notices Roy. Astron. Soc. 154, 167.Google Scholar
  25. Harrison, E. R.: 1972,Phys. Today 25, (12), 30.Google Scholar
  26. Harrison, E. R.: 1973, in E. Schatzman (ed.)Cargese Lectures in Physics, Gordon and Breach, New York.Google Scholar
  27. Harrison, E. R.: 1976,Nature 264, 525.Google Scholar
  28. Huntley, H. E.: 1967,Dimensional Analysis, Dover, New York.Google Scholar
  29. Jaffe, W. and Perola, G. C.: 1973,Astron. Astrophys. 26, 423.Google Scholar
  30. Kisslinger, M. B. and Morley, P. D.: 1978,Astrophys. J. 219, 1017.Google Scholar
  31. Lemaître, G.: 1950,The Primeval Atom, van Nostrand, New York.Google Scholar
  32. Miley, G. R. et al: 1972,Nature 237, 269.Google Scholar
  33. Minin, I. N.: 1979,Astrofisica,15, 121.Google Scholar
  34. Morrison, P.: 1969,Astrophys. J. 157, L73.Google Scholar
  35. Muller, R. A.: 1974, Preprint LBL-520/74.Google Scholar
  36. Muradian, R. M.: 1975,Astrofisica 11, 237.Google Scholar
  37. Muradian, R. M.: 1977a,Astrofisica 13, 63.Google Scholar
  38. Muradian, R. M.: 1977b,Proc. XVIII Int. Conf. on High Energy Physics, JINR, Tbilisi.Google Scholar
  39. Muradian, R. M.: 1977c, inProblems of Elementary Particle and Atomic Nucleus Physics, vol. 8, p. 175.Google Scholar
  40. Muradian, R. M.: 1978,Astrofisica 14, 439.Google Scholar
  41. Nordsieck, K. H.: 1973,Astrophys. J. 184, 735.Google Scholar
  42. Ozernoy, L. M.: 1974,Proc. IAU Symp. No. 58, D. Reidel Publ. Co., Dordrecht-Holland.Google Scholar
  43. Rood, H. J.: 1974,Astrophys. J. 188, 451.Google Scholar
  44. Saakyan, G. S.: 1974,Equilibrium Configurations of Degenerate Gaseous Masses, Plenum, New York.Google Scholar
  45. Sistero, R. F.: 1973,Astrophys. Space Sci. 24, 181.Google Scholar

Copyright information

© D. Reidel Publishing Co. 1980

Authors and Affiliations

  • R. M. Muradian
    • 1
    • 2
  1. 1.Joint Institute for Nuclear ResearchDubna
  2. 2.Byurakan Astrophysical ObservatoryByurakanU.S.S.R.

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