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Origin of The Primordial Inhomogeneities of the Universe

  • D. A. Kompaneets
  • V. N. Lukash
  • I. D. Novikov
Chapter

Abstract

We propose a general principle which enables us to determine the initial fluctuations of the metric in the hot Universe. We consider the recently discovered process of amplification of density perturbations near the cosmological singularity. The conclusions are applied to the problem of formation of the large-scale structure of the Universe.

Keywords

Density Perturbation Potential Perturbation Cosmological Expansion Cosmological Singularity Grand Unification Theory 
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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Copyright information

© Plenum Press, New York 1984

Authors and Affiliations

  • D. A. Kompaneets
    • 1
  • V. N. Lukash
    • 1
  • I. D. Novikov
    • 1
  1. 1.Space Research InstituteAcademy of SciencesUSSR

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