Nonlinear Limit on Primeval Adiabatic Perturbations

Details Nonlinear Limit on Primeval Adiabatic Perturbations Nonlinear Limit on Primeval Adiabatic Perturbations

Jan 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970phrvd...1..397p&link_type=abstract

Physical Review D, vol. 1, Issue 2, pp. 397-399

Mathematics

Logic

37

Scientific paper

The amplitude of adiabatic perturbations that might have existed in the early universe is limited by the nonlinear transfer of energy to high frequencies. For flat cosmological models, this limit, together with the effect of linear dissipation, yields a residual perturbation in the matter distribution comparable with the semiempirical estimate of what is needed to produce massive galaxies.

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