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Quantum Fluctuations in Cosmology and Galaxy Formation

  • G. V. Chibisov
  • V. F. Mukhanov

Abstract

The quantum theory of scalar perturbations in the isotropicly expanding Universe is discussed. Zero-point initial fluctuations can result in galaxies only if the Universe when near a cosmological singularity evolves through a de-Sitter stage of sufficient duration.

Keywords

Vacuum Energy Quantum Fluctuation Galaxy Formation Cosmological Singularity Friedmann Universe 
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

  • G. V. Chibisov
    • 1
  • V. F. Mukhanov
    • 1
  1. 1.P.N. Lebedev Physical InstituteMoscowUSSR

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