On the evolution of cosmological adiabatic perturbations in the weakly non-linear regime

Details On the evolution of cosmological adiabatic perturbations in the weakly non-linear regime On the evolution of cosmological adiabatic perturbations in the weakly non-linear regime

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.197..931j&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 197, Dec. 1981, p. 931-940.

Astronomy and Astrophysics

Astrophysics

68

Adiabatic Equations, Astrophysics, Cosmology, Galactic Evolution, Gravitational Effects, Correlation, Equations Of Motion, Galactic Clusters, Many Body Problem, Mass Distribution, Tides

Scientific paper

The purpose of this paper is to investigate the weakly nonlinear stage in the evolution of adiabatic density fluctuations. It is shown that tidal processes may lead to the disruption of large scale inhomogeneities into smaller units. This phenomenon may change significantly the Doroshkevich, Sunyaev and Zeldovich scenario for development of structure in the expanding Universe. Accurate N-body experiments are necessary to decide whether the approach used in this paper is reasonable.

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